SEMINAR SERIES ON
STRING PHENOMENOLOGY
Past Talks
All talk videos can be found here. See below for individual talk information, slides, and video links.
Giorgio Leone
Title: Rigid Orientifold Vacua in 6d with Broken SUSY
Abstract: Brane Supersymmetry Breaking (BSB) is a phenomenon occurring in lower dimensional orientifold vacua in which supersymmetry is broken without admitting tachyonic instabilities. This feature is ascribed to the simultaneous presence of a tree-level supersymmetric closed string sector coupled with a non-supersymmetric open string one, which underlies a non-linear realisation of supersymmetry. After reviewing the original construction in six dimensions built on the T^4/Z_2 orbifold, I will present an almost rigid variation that can only be deformed via an overall D-branes recombination. Afterwards, I will describe the BSB orientifold built upon the T^4/Z_4 orbifold in which, in contrast to the previous case, the presence of fractional orientifold planes forbids any further continuous deformation. Finally, I will briefly comment on the structure of the gauge kinetic functions entering the low-energy effective action and the unitarity constraints arising from the presence of 2d defects coupled to the R-R 2-forms required by the Green-Schwarz-Sagnotti mechanism.
Antonia Paraskevopoulou
Title: Emergence of R^4 terms in M-theory
Abstract: In its original formulation, the Emergence Proposal postulates that terms in the low-energy effective action are emerging after integrating out towers of states becoming exponentially light in asymptotic regions of the moduli space, in agreement with the Swampland Distance Conjecture. In this talk, I will motivate an M-theoretic refinement of the Emergence Proposal by revisiting the computation of a particular higher derivative coupling in toroidal compactifications of M-theory. On a technical level, our calculations rely on employing an appropriate regularization method and demonstrate that integrating out the full towers of light states is crucial for reproducing the known amplitudes.
Joan Quirant
Title: Massive spin-2 particles and the Swampland
Abstract: In this talk, we will study swampland constraints on massive spin-2 particles coupled to gravity. We will start by considering an effective theory (EFT) with a single (interacting) massive spin-2 particle and a gap to the cutoff. We will show that this theory can never be made consistent with the so-called Classical Regge Growth conjecture (CRG), therefore being in the swampland. We will then move to the case in which there are several massive spin-2 particles in the EFT. We will see that the CRG demands an infinite tower, bounding the gaps between the masses of the different massive spin-2 particles.
Stefano Lanza
Title: Neural Network Learning and Quantum Gravity
Abstract: The landscape of low-energy effective field theories stemming from string theory is too vast for a systematic exploration. However, the meadows of the string landscape may be fertile ground for the application of machine learning techniques. In this talk, I will illustrate that Quantum Gravity effective field theories are naturally endowed with key statistical learnability properties due to their underlying tame structures. Consequently, several problems therein formulated can be concretely addressed with machine learning techniques, delivering results with sufficiently high accuracy.
Lorenzo Paoloni
Title: On the Moduli Space Curvature at Infinity
Abstract: Moduli spaces are a key feature of String Compactifications and play a central role in the Swampland Programme. In this talk, I will analyse the scalar curvature of the vector multiplet moduli space of type IIA string theory compactified on a generic Calabi–Yau manifold. While the volume of this space is known to be finite, cases have been found where the scalar curvature diverges positively along trajectories of infinite distance. I will discuss the asymptotic behaviour of the scalar curvature for a broad set of large volume limits, and provide the source of the divergence both in geometric and physical terms.
Bernardo Fraiman
Title: Rank Reduction in Non-supersymmetric String Theories
Abstract: The lack of experimental evidence for supersymmetry has recently fueled a resurgence of interest in non-supersymmetric heterotic strings. A detailed analysis was carried out on the possible gauge symmetries and the behavior of the one-loop potential for circle compactifications of these strings. However, no minima were found. Orbifold compactifications lead to theories with reduced-rank symmetries and fewer moduli, making them potentially easier to stabilize. Interestingly, part of the structure underlying the supersymmetric string landscape is retained in these non-supersymmetric variants, allowing us to study these rank-reduced theories in great detail. Furthermore, an analysis of infinite distance limits reveals a complex web that interrelates both known and previously unknown theories.
Margherita Putti
Title: Gravitational Axiverse Spectroscopy
Abstract: Among various predictions of string compactifications, axions hold a pivotal role, as they provide a unique avenue to tie UV physics to experiments. Most experimental setups aim to detect a signal using the direct coupling between the axion and the Standard Model. However, string axions do not necessarily need to couple to the Standard Model directly. In this talk I will describe how inflationary models with multiple “spectator" axions coupled dark gauge sectors via Chern-Simons coupling could source observable gravitational waves. If string axions coupled to Abelian gauge fields undergo slow-roll during inflation, they produce a multi-peak GW signal whose magnitude depends on the details of the compactification. I will discuss how to embed spectator axions into type IIB orientifold compactifications and the restrictions imposed on such models from consistency and control requirements, thereby motivating models that may live in the landscape as opposed to the swampland.
Veronica Collazuol
Title: A twist at infinite distance in the CHL string
Abstract: In this talk, I will analyse a space-time algebra of BPS states that emerges in the infinite distance limit in the moduli space of the nine-dimensional CHL string as the theory decompactifies to the ten-dimensional E8×E8 heterotic string, and compare it with the heterotic case. As expected, we find an affine algebra, but in a twisted version.
David H. Wu, Harvard
Title: Species scale in diverse dimensions
Abstract: In a quantum theory of gravity, the species scale can be defined as the scale at which corrections to the Einstein action become important due to the fact that the inverse of the species scale gives us the smallest size black hole described by the EFT involving only the Einstein term. In this talk, I will demonstrate the validity of this picture in diverse dimensions and with different amounts of supersymmetry and show that the species scale exhibits the expected behavior at the boundary of the moduli space. Furthermore, with this picture in mind, we can now evaluate the species scale in the interior of the moduli space along with computing the “desert point“ where the species scale is maximized, computing the diameter of the moduli space, and providing more evidence for a global bound on the gradient of the log of the species scale.
Ignacio Ruiz, IFT Madrid
Title: A Taxonomy of Infinite Distance Limits
Abstract: The Emergent String Conjecture constrains the possible types of light towers in infinite-distance limits in quantum gravity moduli spaces. In this talk we will explain how one can use these to put further restrictions on the convex hull of the scalar charge-to-mass vectors of these light towers, as well as the related convex hull that controls the asymptotic behavior of the species scale. Under certain assumptions, this enables a systematic classification in terms of a finite list of polytopes. Most of these polytopes arise in known string theory compactifications, while others may yet reside in either the landscape or the swampland.
Ethan Torres, CERN
Title: Generalized Symmetries, Gravity, and the Swampland
Abstract: In quantum gravity, it is generally expected that all global (generalized) symmetries are either gauged or broken. In this talk, I will discuss the UV fate of such global symmetries in the context of 7D and 5D vacua realized by compact Calabi-Yau spaces with localized singularities in M-theory. Conversely, I will also show how the emergence of (approximate) global symmetries in the IR coincides with the appearance of (approximately) topological operators realized from branes. Along the way we will see how the gluing conditions between local sectors of a Calabi-Yau lead to a preferred global structure of the non-abelian and higher-form gauge groups. In particular, we find that the 7D gauge groups always take a particular form which may suggest new swampland conditions.
Bjoern Friedrich, Heidelberg
Title: End-of-the-world branes in string theory and their implications in cosmology
Abstract: The existence of end-of-the-world (ETW) branes allows for the appearance of two phenomena relevant in cosmology: The decay of universes to nothing and the creation of universes from nothing. In this talk, we discuss both the existence of ETW branes in string theory and their effects in cosmology. We explicitly construct an ETW brane for type IIB compactifications on Calabi-Yau orientifolds and estimate the decay/creation rates of universes.
Gonzalo Villa, Cambridge
Title: String Thermodynamics In and Out of Equilibrium: Boltzmann Equations and Random Walks
Abstract: In this talk, we explore the Bolzmann equation approach to string thermodynamics and explore its inherent capability of studying out-of-equilibrium physics, with cosmological applications in mind. More concretely, after a short description of the phase space of string theory in a flat background, we consider the leading contribution to the decay and absorption rates of typical highly excited strings in a thermal ensemble, in an arbitrary number d of effectively non-compact dimensions (which we define in the talk). Using the random walk interpretation of these rates, which should apply in more general backgrounds, we infer more complicated contributions which at the moment lack a worldsheet computation. All these are then used to write down Boltzmann equations in such a way that the principle of detailed balance becomes manifest, and we use this principle to find equilibrium configurations and test our inferred rates. We conclude by studying perturbations out-of-equilibrium by computing equilibration rates and fully solve for the behaviour of the perturbations in simple cases. Time permitting, potential implications in cosmology will be outlined.
Calvin Yi-Ren Chen, Imperial
Title: Consistency Conditions from Causality
Abstract: In recent years, causality has emerged as a powerful criterion to distinguish between “physical” and “unphysical” low-energy effective field theories (EFTs). A direct way to ensure a given EFT is causal is to demand a lower bound on scattering time delays, which essentially imposes a speed limit averaged over a trajectory. In flat space, this is unambiguously dictated by the Minkowski light cones, but the situation is more subtle with dynamical gravity. I will make the case that the relevant notion is so-called infrared (IR) causality.
As the prototypical example, I will study the leading-order EFT of gravity in $D \geq 5$. IR causality imposes compact bounds on its Wilson coefficient, which is consistent with positivity bounds. Attempts to further sharpen this bound use specific configurations of shockwaves which enhance the amount of causality violation. In this talk I will emphasise that this is not possible.
This talk is based on arXiv:2112.05031 and 2309.04534 in collaboration with C. de Rham, A. Margalit, and A. J. Tolley.
Daniel Baldwin, King's College London
Title: Coulomb and Higgs Phases of $G_{2}$-Manifolds
Abstract: We will discuss the physics of M-theory compactifications onto $G_2$-orbifolds of the type that can be desingularised via the method of Joyce and Karigiannis i.e. orbifolds where one has a singular locus of A1 singularities that admits a nowhere-vanishing ($\textbf{Z}_2$-twisted) harmonic 1-form. Interestingly, there are topologically distinct desingularisations of such orbifolds which we show can be physically interpreted as different branches of the 4d vacuum moduli space of the arising gauge theories, known as ‘Coulomb’ and ‘Higgs’ branches. The results suggest generalisations of the results of Joyce and Karigiannis to $G_2$-orbifolds with more diverse ADE singularities and higher order twists.
As a bonus, we also get an isomorphism between the moduli space of flat connections on flat compact 3-manifolds and the moduli space of Ricci flat metrics on the $G_{2}$-orbifolds. We will briefly discuss this. Based on 2309.12869 and 2312.12311.
Jesús Huertas, IFT Madrid
Title: Aspects of Dynamical Cobordism in AdS/CFT
Abstract: The cobordism conjecture implies that consistent theories of Quantum Gravity must admit the introduction of boundaries. In this talk, we will present the dynamical realization of the cobordism conjecture in type IIB in AdS5 × S5, using the existing gravity duals of 4d N=4 SYM with Gaiotto-Witten superconformal boundary conditions (near-horizon limits of D3-branes ending on NS5- and D5-branes). We will show that these configurations are, from the 5d perspective, dynamical cobordism solutions which start from an asymptotic AdS5 vacuum and evolve until they hit an end of the world (ETW) brane with AdS4 worldvolume. The latter displays localization of gravity, and provide a string theory completion of the Karch-Randall AdS branes. Also, a novel double scaling limit will be presented, which zooms into the ETW brane and makes localization of gravity manifest, and which shows a tantalizing relation with wedge holography. Finally, we will briefly explain how to extend the picture to AdS5 theories with less (super)symmetry, via orbifolds and S-folds, leading to dynamical cobordisms for gravity duals of 4d theories with N=2 and N=3 supersymmetry.
Hamza Ahmed, Northeastern University
Title: T-duality and flavor symmetries of Heterotic Little String Theories(LSTs)
Abstract: 6D Heterotic Little String Theories(LSTs) are a subsector of every 6D SUGRA (with at least one tensor multiplet), after decoupling gravity. As such, while possessing usual QFT-like properties such as global symmetries, they also possess gravity-like properties such as T-duality, which makes them an interesting intermediate. Recently, a fruitful line of research has been to chart the landscape of T-dual LSTs, and establish certain invariants across this T-duality, which includes the 5D Coulomb branch dimension, and the 2-Group structure constants (mixed anomalies). In this talk, we will argue that the rank of the flavor algebra is another invariant across this duality. This involves using 6D anomaly cancellation conditions and carefully taking into account potential ABJ anomalies. We will then discuss some interesting novel LSTs with non-trivial flavor holonomies, focusing on their T-duality structure. Based on arXiv:2311.02168.
Filippo Revello, Utrecht University
Title: String Theory and the First Half of the Universe
Abstract: We perform a detailed study of stringy moduli-driven cosmologies between the end of inflation and the commencement of the Hot Big Bang, including both background and cosmological perturbations: a period that can cover half the lifetime of the universe on a logarithmic scale. Compared to the standard cosmology, stringy cosmologies motivate extended kination, tracker and moduli-dominated epochs involving significantly trans-Planckian field excursions. As conventional effective field theory is unable to control Planck-suppressed operators, such epochs require a stringy completion for a consistent analysis. Perturbation growth is substantially enhanced compared to conventional cosmological histories. The transPlanckian field evolution results in radical changes to Standard Model couplings during this history and we outline potential applications to baryogenesis, dark matter and gravitational wave production.
Jeroen Monnee, Utrecht University
Title: Complexity of the Flux Landscape
Abstract: The landscape of F-theory flux compactifications is expected to be remarkably constrained due to deep insights in Hodge theory and tame geometry. In this talk, I will first review known finiteness theorems for the landscape of self-dual flux vacua and provide additional insights on this matter using asymptotic Hodge theory. In the remainder of the talk, I will present and motivate three new mathematical conjectures on the enumeration, dimensionality, and geometric complexity of the flux landscape, including a reformulation of the tadpole conjecture. Based on Arxiv:2311.09295.
Muthusamy Rajaguru, Lehigh University
Title: Moduli stabilization in type IIB models with h^{1,1}=0
Abstract: The tadpole conjecture constrains the number of moduli that can be stabilized with fluxes in F-theory and type IIB flux compactifications. In this talk, I will discuss ongoing work that aims to test this assertion in non-geometric type IIB flux compactifications with no Kähler moduli. In particular, I will restrict to supersymmetric Minkowski vacua in orbifolds of the 1^9 and 2^6 Gepner models. Generically these Minkowski critical points have many massless directions. In principle, we are able to expand the flux superpotential around these Minkowski critical points upto arbitrary order. This allows us to ask if these massless directions are truly flat or if they get stabilized by some higher-than-quadratic order term in the superpotential. Furthermore, there exist powerful non-renormalization theorems for the flux superpotential that make such questions meaningful to ask in these non-geometric compactifications.
Rafael Álvarez-García, Hamburg University
Title: The Distance Conjecture in F-theory via Semi-stable Degenerations
Abstract: We study infinite-distance limits in the complex structure moduli space of six-dimensional F-theory as part of the ongoing efforts to understand the boundaries of moduli spaces in quantum gravity. Our work consists of two parts: an algebro-geometric analysis of the limits, corresponding to the recent paper arXiv:2310.07761, and their physical interpretation, to appear soon. We start by summarizing the first of these, explaining how the limits can be described as semi-stable degenerations of elliptic Calabi-Yau threefolds, leading to an asymptotic spacetime consisting of log Calabi-Yau spaces glued along their boundaries. We then center our attention on the physical interpretation of the infinite-distance trajectories as either emergent string limits or partial decompactification processes to theories with (non-perturbative) defects. The latter aspect is a novel feature of the six-dimensional scenario compared with its counterpart in compactifications of F-theory on elliptic K3 surfaces.
Alberto Castellano, IFT
Title: A Universal Pattern in Quantum Gravity
Abstract: The Distance Conjecture in the Swampland program famously predicts the breakdown of any low energy EFT description of a gravitational theory when probing infinite distance/weak coupling points in the moduli space due to the appearance of an infinite number of states with exponentially light masses. Such universal breakdown can be made more precise upon introducing the Quantum Gravity cut-off, which sets the maximal energy scale of any underlying field theoretic description, and which can be seen to also decrease exponentially with the traversed field space distance. In this talk, we will argue for a sharp and universal pattern linking these two quantities and which is moreover satisfied at any infinite distance boundary of moduli space, thus imposing non-trivial 'gluing' conditions for the different phases (or duality frames) of the theory. In addition, we will also explain what are the minimal sufficient conditions for it to hold from the bottom-up perspective, as well as the derived bounds that immediately follow from the pattern.
George Tringas, LAPTH
Title: On the robustness of scale-separated AdS4 from type IIA
Abstract: In this presentation, I will discuss an extension of the so called DGKT solution resulting from the O6 plane backreaction. Our focus will center on a well-established large N expansion method that allows us to identify corrections to fields and flux profiles due to backreaction, thereby refining the smeared DGKT solution. The parameter N represents the unbounded F4 flux parameter. We will investigate this extension within the framework of ten-dimensional massive type IIA supergravity and a four-dimensional effective theory, utilizing a warped compactification framework. Our analysis will encompass the generalization of flux scaling and the exploration of potential contributions from backreaction corrections, including axions. We will discuss the relevance of corrections to the DGKT scalar potential and determine whether they dominate over alpha prime corrections. Additionally, we will consider flux quantization, which imposes crucial constraints on flux corrections. Our investigation extends to the examination of next-to-next-to-leading-order corrections and their implications. This presentation will be based on the recent paper 2310.06115.
Daniel Panizo, Uppsala University
Title: A cosmological excursion to dark bubbles
Abstract: The Dark Bubble scenario proposes that an expanding four-dimensional cosmology, equipped with dark energy, can be realised on the boundary of a five-dimensional bubble mediating the decay between two non-supersymmetric anti-de Sitter vacua. In this express journey, I will be your guide to the bulk, where dark bubbles can nucleate and expand. We will depart from string theory at around 11:30 EST, all the way down to four dimensions. The required technology to appreciate the energy scale hierarchy of the model will be provided when crossing the junction conditions border (No need to bring small extra dimensions from home). Stringy corrections will ensure our safe landing on universes with positive cosmological constant. Here we will study the Gauss-Codazzi interplay between the bubble's boundary and bulk, which decorates the expanding cosmology with familiar energy densities, such as gravitational or electromagnetic radiation.
Salvatore Raucci, Scuola Normale Superiore Pisa
Title: A first-order formalism for non-supersymmetric strings
Abstract: The absence of supersymmetry in perturbative string theory usually leads to runaways arising from nonvanishing dilaton tadpoles. The spacetime manifestation is a scalar potential, the stringy counterpart of quantum vacuum energies in quantum field theory, which should be accounted for in geometric vacua. In this talk, I will discuss a first-order formalism that replaces supersymmetry as a vacuum-generating technique for non-supersymmetric strings. In its most basic form, this is known as fake supersymmetry. This strategy raises interesting observations on vacuum stability by employing a definition of energy inspired by the Witten-Nester approach.
Matilda Delgado, IFT
Title: Emergence of Species Scale Black Hole Horizons
Abstract: The scale at which quantum gravitational effects become manifest, the species scale, has recently been argued to take values parametrically lower than the Planck scale. It is therefore of interest to quantum gravity phenomenology to have a precise definition of how to compute this scale in any EFT that has a UV completion in quantum gravity. Two proposals have been made in the litterature, of different conceptual origin; one linked to the size of the smallest black hole that one can describe in an EFT and the other to the scale of higher-derivative corrections to the EFT. Arguably one of the most profound aspects of a theory of quantum gravity is that it should be background independent and that semi-classical spacetime should only "emerge" as a low-energy description. I will demonstrate how this notion of "emergence" unites the two definitions of the species scale. I will do so by studying small (singular) black hole solutions in string theory and illustrating how higher-derivative corrections obtained from emergence correct these solutions and generate a species scale sized horizon for these black holes. Based on arXiv:2310.04488.
Nicolò Petri, Ben Gurion U. of Negev
Title: Towards AdS Distances in String Theory
Abstract: Recent developments in high-energy physics have brought to light the need to formulate a consistent notion of distance between gravitational vacua. Specifically, within the Swampland program, the AdS Distance conjecture proposes to assign such a notion for AdS vacua in quantum gravity. Beginning with very basic AdS vacua in string theory, I will expand upon this concept, providing a more formal framework for it. Firstly, I will introduce a precise definition of a metric for the space of conformal variations of AdS. This metric, however, turns out to be negative, resulting in an ill-defined distance, a property related to the famous conformal factor problem in quantum gravity. Nonetheless, in string theory, variations in the AdS conformal factor are accompanied by variations in the internal dimensions and background flux. Interestingly, the inclusion of these variations can change the sign of the metric over the space of AdS vacua variations. I will propose a consistent procedure for deriving the distance between AdS vacua by introducing the notion of an "action metric", which accounts for all of these variations simultaneously. I will test this procedure by focusing on AdS4 and AdS7 Freund-Rubin vacua in M-theory and demonstrate that it yields a well-defined and positive distance.
Matteo Licheri, University of Bologna
Title: Higher Derivative Corrections to String Inflation
Abstract: We quantitatively estimate the leading higher derivative corrections to N=1 supergravity derived from IIB string compactifications and study how they may affect moduli stabilisation and LVS inflation models. Using the Kreuzer-Skarke database of 4D reflexive polytopes and their triangulated Calabi-Yau database, we present scanning results for a set of divisor topologies corresponding to threefolds with 1≤ h^1,1 ≤ 5. In particular, we find several geometries suitable to realise blow-up inflation, fibre inflation and poly-instantons inflation, together with a classification of the divisors topologies for which the leading higher derivative corrections to the inflationary potential vanish. In all other cases, we instead estimate numerically how these corrections modify the inflationary dynamics, finding that that they do not destroy the predictions for the main cosmological observables.
Muldrow Etheredge, UMass
Title: Dense Geodesics, Tower Alignment, and the Sharpened Distance Conjecture
Abstract: The Sharpened Distance Conjecture and Tower Scalar Weak Gravity Conjecture are closely related but distinct conjectures, neither one implying the other. Motivated by examples, I propose that both are consequences of two new conjectures: 1. The infinite distance geodesics passing through an arbitrary point φ in the moduli space populate a dense set of directions in the tangent space at φ. 2. Along any infinite distance geodesic, there exists a tower of particles whose scalar-charge-to-mass ratio (-∇ log m) projection everywhere along the geodesic is greater than or equal to 1/\sqrt(d-2). I perform several nontrivial tests of these new conjectures in maximal and half-maximal supergravity examples. I also use the Tower Scalar Weak Gravity Conjecture to conjecture a sharp bound on exponentially heavy towers that accompany infinite distance limits. Based on 2308.01331.
Carlo Branchina, Chung-Ang University
Title: UV-sensitivity in Kaluza Klein Theories: Naturalness and Dark Dimension
Abstract: When the Higgs potential or the vacuum energy are derived in the framework of Higher dimensional effective field theories on a multiply connected spacetime with compact dimensions and non-trivial boundary conditions (as in the case of the Scherk-Schwarz SUSY breaking), the usual calculations lead to the conclusion that these quantities are naturally UV-insensitive. By means of a thorough analysis of the assumptions on which these calculations are based, I will show that this paradigm actually misses a crucial source of UV-sensitivity, ultimately connected to the non-trivial topology of the spacetime in these theories. As a consequence, the conclusions on the UV-insensitivity of the Higgs mass, of the Higgs potential, and on the existence of a Dark Dimension (that crucially depends on the supposed UV-insensitivity of the vacuum energy in Kaluza-Klein theories) need to be seriously reconsidered. Our results were challenged in a note very recently posted online. If time allows, I will point out the flaws in these criticisms.
Junsei Tokuda, IBS
Title: Gravitational positivity bounds: implications for the swampland program
Abstract: In the context without gravity, it has been known that the S-matrix positivity bounds offer a useful tool to derive ultraviolet constraints on low-energy effective field theories. In this talk, we assume that the positivity bounds are approximately valid even in the presence of gravity, and discuss the implications of the bounds for phenomenological models. Interestingly, we obtain strong bounds on the simplest dark photon models which can be compared with experimental bounds, while the Standard Model easily satisfies the bounds. We also provide a scenario which gives rise to the approximate gravitational positivity bounds based on the Reggeization of graviton exchange.
Manki Kim, MIT
Title: Towards string loop corrections in Calabi-Yau orientifold compactifications
Abstract: Computation of string loop corrections to the effective action has been one of the main challenges in string phenomenology. One major complication for such computations is that the string loop corrections are sensitive to the spectrum of strings probing Calabi-Yau orientifolds, which is practically inaccessible. In this talk, I will claim that some terms in the string one loop corrections to the Kahler potential are computed by more computable crude details of the string spectrum. This result may pave a way to explicit computations of the string loop corrections in generic Calabi-Yau orientifold compactifications.
Houri-Christina Tarazi, Harvard
Title: Non-BPS path to the string lamppost
Abstract: We provide further motivation for the string lamppost principle in 9d supergravities. Using a blend of ideas which includes Swampland conjectures, finiteness of black hole entropy, and classification of SCFTs, we show that infinite distance limits that keep BPS states heavy must decompactify to type IIA supergravity on an interval. Without relying on string theory, we provide bottom-up explanations for various UV features of the theory, such as the physics near the orientifold branes and the worldvolume theories of different stacks of non-perturbative 8-branes. We also provide a Swampland argument for the countability of the number of inequivalent string limits up to dualities which is a strong result with applications beyond this work.
Christian Kneißl, Max Planck Institute Munich
Title: Dynamical Cobordism Conjecture: Solutions for End-of-the-World Branes
Abstract: Analyzing finite size solutions for a generalized D-dimensional Dudas-Mourad (DM) model reveals a dynamical cobordism configuration with neutral and charged end-of-the-world (ETW) defect branes. In this talk I will demonstrate an explicit construction of non-isotropic solutions of the corresponding codimension one ETW-branes. Consequently, I will show the appearance of a lower bound for the critical exponent in the scaling behavior of the distance and the curvature close to the defect. This allows us to make a connection to the (sharpened) Swampland Distance Conjecture and the (Anti-) de Sitter Distance Conjecture.
Héctor Parra de Freitas, IPhT
Title: Tadpoles and Gauge Symmetries
Abstract: The tadpole conjecture proposes that complex structure moduli stabilisation by fluxes that have low tadpole charge can be realised only at special points in moduli space, leading generically to (large) gauge symmetries. In this talk I will consider F-Theory flux compactifications on K3xK3 with fully stabilised complex structure moduli and show how lattice embedding techniques allow for a full characterization of their gauge symmetries. I will report on the results of a scan of these models, showing that all of them have non-abelian gauge symmetries whenever the tadpole bound is satisfied.
Min-Seok Seo, KNUE
Title: Uplift and towers of states in warped throat
Abstract: The difficulty in realizing the metastable de Sitter vacuum in the string model has been considered in light of the distance conjecture. In this talk, we investigate the Type IIB compactifications containing the warped throat and point out that the uplift potential produced by anti-D3 branes satisfies the scaling behavior with respect to the tower mass scale, hence can be directly connected to the distance conjecture. Unless the throat length is extremely close to zero, the tower mass scale corresponds to the Kaluza-Klein mass, the lowest tower mass scale.
Simon Schreyer, University of Heidelberg
Title: α' Corrections to KPV: An Uplifting Story
Abstract: In earlier work, the effect of $\alpha'^2$ curvature corrections on the NS5-brane responsible for the decay of anti-D3-branes in the set-up of Kachru, Pearson, and Verlinde (KPV) was considered. In this talk, I extend this analysis to include all known $\alpha'^2$ corrections to the action of an abelian fivebrane which involve not just curvature but also gauge fields and flux. This leads to the $\alpha'^2$ corrected potential for the NS5-brane at the tip of the Klebanov-Strassler throat. The resulting potential provides the explicit realization of a novel uplifting mechanism where one can obtain metastable vacua with an arbitrarily small positive uplifting potential by fine-tuning $\alpha'$ corrections against the tree-level potential. This mechanism works for small warped throats, both in terms of size and contribution to the D3-tadpole, thereby sidestepping the issues associated with a standard deep warped throat uplift which are deadly in KKLT and severely constraining in the Large Volume Scenario.
Flavio Tonioni, University of Wisconsin-Madison
Title: Late-time Accelerating Cosmologies
Abstract: I will characterize the late-time expansion rate of the universe in multi-scalar cosmologies with multi-exponential potentials, taking advantage of previously unobserved universal asymptotic features of the solutions to the cosmological equations. This provides a simple diagnostic of whether any given multi-exponential potential holds the necessary conditions for late-time cosmic acceleration. I will also discuss the conditions under which scaling solutions are inevitable late-time cosmological attractors for such theories. For scaling cosmologies, all field-space trajectories are known analytically, which allows one to characterize exactly any observable of interest. Multi-exponential potentials have been studied extensively as phenomenological models of quintessence and, moreover, they are ubiquitous in string-theoretic constructions. I will therefore sharpen several statements on the low-energy signatures of quantum gravity in this context. [based on hep-th/2303.03418 + upcoming preprint, in collaboration with G. Shiu and H.V. Tran]
Roberta Angius, IFT Madrid
Title: Small Black Hole Explosions
Abstract: 4d small black holes are powerful tools to pursue dynamical explorations of infinite distances in moduli space. Upon S2 compactification they show the features of a Dynamical Cobordism, with a singular core, located at finite distance in spacetime, at which some scalars run to infinity.
In this talk, I will discuss such setups in the presence of additional 4d scalar potentials growing exponentially near the black hole core with a characteristic exponent δ. I will show that the small black hole behavior is preserved for values of δ under a certain limit, while up to this bound the potential is too large, it obstructs the realisation of the Dynamical Cobordism, and the small black hole explodes into a puffed-up regular black hole or into a runaway configuration. I will emphasize as the 2d perspective puts the black hole and the scalar potentials on an equal footing, allowing us a direct analysis of their competition.
In order to describe an explicit realisation of this mechanism I will focus on the context of 4d N = 2 gauged supergravity theories where the 2d picture also allows a unified discussion of fluxes, domain walls and black holes.
Finally I will discuss the capability of small black holes to continue exploring infinite distance limits in moduli space, even in the presence of 4d potentials.
Ignacio Ruiz, UAM Madrid
Title: Asymptotic Accelerated Expansion in String Theory and the Swampland
Abstract: We study whether the universal runaway behaviour of stringy scalar potentials towards infinite field distance limits can produce an accelerated expanding cosmology à la quintessence. We identify a loophole to some proposed bounds that forbid such asymptotic (at parametric control) accelerated expansion in 4d $\mathcal{N}=1$ supergravities, by considering several terms of the potential competing asymptotically. We then analyse concrete string theory examples coming from F-theory flux compactifications on Calabi-Yau fourfolds, extending previous results by going beyond weak string coupling to different infinite distance limits in the complex structure moduli space. We find some potential candidates to yield asymptotic accelerated expansion with a flux potential satisfying $\gamma=\frac{\|\nabla V\|}{V}<\sqrt{2}$ along its gradient flow. However, whether this truly describes an accelerated expanding cosmology remains as an open question until full moduli stabilization including the Kahler moduli is studied. Finally, we also reformulate the condition for forbidding asymptotic accelerated expansion as a convex hull de Sitter conjecture which resembles a convex hull scalar WGC for the membranes generating the flux potential. This provides a pictorial way to quickly determine the asymptotic gradient flow trajectory in multi-moduli setups and the value of $\gamma$ along it.
Jacob Leedom, DESY
Title: Heterotic de Sitter Beyond Modular Symmetry
Abstract: I will discuss the vacua of 4d heterotic toroidal orbifolds using effective theories consisting of an overall Kähler modulus, the dilaton, and non-perturbative corrections to both the superpotential and Kähler potential that respect modular invariance. I will prove three de Sitter no-go theorems for several classes of vacua and thereby substantiate and extend previous conjectures. Additionally, I will provide evidence that extrema of the scalar potential can occur inside the PSL(2, Z) fundamental domain of the Kähler modulus, in contradiction of a separate conjecture. I will also illustrate a loophole in the no-go theorems and determine criteria that allow for metastable de Sitter vacua. Finally, I will identify inherently stringy non-perturbative effects in the dilaton sector that could exploit this loophole and potentially realize de Sitter vacua.
Niccolò Cribiori, Munich
Title: Swampland constraints on scale separation and de Sitter in 4D & 5D
Abstract: Swampland conjectures are meant to be consistency conditions for low energy effective theories to be compatible with quantum gravity. In the talk, I will argue that applying some of the most tested conjectures, such as the weak gravity conjecture, directly to gauged supergravity with at least eight supercharges leads to stringent constraints. In particular, one can argue for the absence of supersymmetric anti-de Sitter vacua with a separation of scales between the compact and the non-compact dimensions. At the cost of introducing an additional assumption on the gravitino mass, a similar analysis can be extended to de Sitter vacua as well.
Sebastian Rauch, UMass
Title: Symmetries and Structures of N=3 S-folds
Abstract: I will discuss the techniques and results of computing the global structures and symmetries of N=3 S-folds. We may treat a stack of D3 branes probing an S-fold holographically, and compute the symmetries of the N=3 SCFT via topological information in the bulk. I will proceed by reviewing S-folds and the role branes play as symmetry operators. I will then compute the possible global structures and symmetries of N=4 and 3 S-folds, the N=4 S-folds providing a check of our methods.
Lorenz Schlechter, Utrecht
Title: Tameness in QFT and CFT
Abstract: In this talk I will discuss tameness as a finiteness principle that can be applied to a variety of physical systems. Specifically, I will introduce the concept of tame geometry and explore its application to both perturbative and non-perturbative quantum field theories. Through an examination of solvable models, I will offer evidence to support tameness as a swampland criterion, and put forth precise conjectures regarding the tameness of amplitudes, as well as the spaces of QFTs and CFTs.
Saghar Sophie Hosseini, Durham
Title: Symmetry TFTs of geometrically engineered field theories
Abstract: (D+1)-dimensional topological field theories, known as SymTFTs, contain information about choices of generalised global symmetries and anomalies of D-dimensional QFTs. In this talk, I will introduce SymTFTs and explain how the BF theory, classifying higher-form symmetries, may be obtained from the dimensional reduction of a Chern-Simons action for self-dual fields in string theory.
Eduardo Garcia-Valdecasas, Harvard
Title: Non invertible symmetries in supergravity
Abstract: We revisit the symmetries of maximal supergravity in 10d and 11d, showing that there are non-invertible symmetries analog to the ones present in 4d theories with a U(1) symmetry with ABJ anomaly. As expected, these symmetries are explicitly broken by the UV completion, String Theory or M-theory. The way in which they are broken gives further support to the connection between the completeness hypothesis and the absence of global symmetries in gauge theories.
Alessandro Mininno, DESY
Title: The Asymptotic Weak Gravity Conjecture in M-theory
Abstract: In this talk, I will focus on five-dimensional compactifications of M-theory on Calabi-Yau 3-folds. In particular, for gauge groups with a weak coupling limit, I will show that there exist many super-extremal states along every ray in the charge lattice, as predicted by the tower Weak Gravity Conjecture, for any consistent quantum gravity theory.
I will first characterize the possible weak coupling limits, building on an earlier classification of infinite distance limits in the Kähler moduli space of M-theory compactifications.
The result is that weakly coupled gauge groups are associated to curves on the compactification space contained in generic fibers or in fibers degenerating at finite distance in their moduli space. These always admit an interpretation as a Kaluza-Klein or winding U(1) in a dual frame or as part of a dual perturbative heterotic gauge group, in agreement with the Emergent String Conjecture. Finally, the fact that every ray in the associated charge lattice either supports a tower of BPS or of non-BPS states, can be shown using the connection between Donaldson-Thomas invariants and Noether-Lefschetz theory, proving also that these states satisfy the super-extremality condition, at least in the weak coupling regime.Alberto Castellano Mora, Madrid
Title: How can Gravity Emerge?
Abstract: In the Emergence Proposal in QG it is conjectured that all light-particle kinetic terms are absent in the fundamental UV theory and are generated by quantum corrections in the IR. It has been argued that this proposal may provide for some microscopic understanding of the Weak Gravity and the Swampland Distance conjectures. In this talk, we will review the main motivations behind this surprising idea, elaborating on certain string/M-theory examples which exhibit this phenomenon along infinite distance corners of their moduli spaces. This renders support to the Emergence Proposal, and to the idea that infinite distance singularities may arise in QG as an intrinsic IR phenomenon.
Nicklas Ramberg, Mainz
Title: Bubbles from Dark Confinement with Holography
Abstract: Gravitational waves emitted from strongly coupled QFTs are, at present, a daunting task to accurately predict due to the strong coupling. In this talk, we demonstrate how to predict the gravitational wave spectra of such theories using holography and lattice data input for a pure SU(3) Yang-Mills theory with minor uncertainties. We will elaborate on how we obtain an effective potential using holography with the free energy landscape approach and formulate an effective action. Once the effective action is in our grasp, we will use this to study bubble nucleation to predict the gravitational wave spectra.
Shing Yan Li, MIT
Title: Large U(1) charges from flux breaking in 4D F-theory models
Abstract: We study the massless charged spectrum of U(1) gauge fields in F-theory that arise from flux breaking of a nonabelian group. The U(1) charges that arise in this way can be very large. In particular, using vertical flux breaking, we construct an explicit 4D F-theory model with a U(1) decoupled from other gauge sectors, in which the massless/light fields have charges as large as 657. This result greatly exceeds prior results in the literature. We argue heuristically that this result may provide an upper bound on charges for light fields under decoupled U(1) factors in the F-theory landscape.
Matilda Delgado, IFT Madrid
Title: Black Holes as Probes of Moduli Space Geometry
Abstract: We argue that supersymmetric BPS states can act as efficient finite energy probes of the moduli space geometry thanks to the attractor mechanism. We focus on 4d N=2 compactifications and capture aspects of the effective field theory near the attractor values in terms of physical quantities far away in moduli space. Furthermore, we illustrate how the standard distance in moduli space can be related asymptotically to the black hole mass. We also compute a measure of the resolution with which BPS black holes of a given mass can distinguish far away points in the moduli space. The black hole probes may lead to a deeper understanding of the Swampland constraints on the geometry of the moduli space.
Yichul Choi, Stony Brook
Title: Non-invertible Gauss Law and Axions
Abstract: In axion-Maxwell theory, there is no conserved, gauge-invariant, and quantized electric charge. This is related to the absence of the ordinary electric 1-form symmetry. Instead, I will explain that the theory has a non-invertible version of the electric 1-form symmetry and discuss a non-invertible Gauss law associated with it. This non-invertible 1-form symmetry leads to exact selection rules for correlation functions of extended operators, which are related to the Witten effect. Finally, I will comment on the implication of the non-invertible symmetry for the Completeness Hypothesis in quantum gravity.
Luca Nutricati, Durham
Title: On the running of gauge couplings in string theory
Abstract: String theories naturally give rise to infinite towers of states whose degeneracies grow exponentially as functions of mass. These infinite towers of states are ultimately responsible for many of the finiteness properties for which string theory is famous. Recently, a framework was developed in which the effects of all of these states can be incorporated in a self-consistent way when calculating quantities relevant for low-energy phenomenology, such as the masses of the Higgs fields that arise in such theories. This formalism also gives rise to an "on-shell'' effective field theory description in which the final results are expressed in terms of contributions from only the on-shell, level-matched physical string states, and in which these quantities also exhibit an EFT-like "running'' as a function of an effective spacetime mass scale. In this talk, I’ll discuss how to apply this formalism to calculate the running of the gauge couplings within closed string theories. Unlike previous calculations in the literature, our calculation fully respects the underlying closed-string modular invariance and expresses many of the final results in terms of contributions from only the on-shell physical string states. We find, however, that the calculation of the gauge couplings differs in one deep way from the calculation of the Higgs mass: while the latter results depend on the supertraces over only the on-shell string states, the former results have a different modular structure which causes them to depend on supertraces over the off-shell string states as well.
Taken together, our results yield the expected logarithmic running of the gauge couplings at certain energy scales. However, they also yield a number of intrinsically stringy behaviors that transcend what might be expected within an effective field theory approach.Muyang Liu, Uppsala
Title: Geometry and T-dualities between Heterotic ALE instantonic Little String Theories
Abstract: Recently, we revisited the properties of Heterotic string compactifications on ALE space in a series of papers. In particular, this talk focuses on the geometric counterpart of T-dualities between Heterotic ALE instantonic LSTs in F-theory. T-dualities are realized as inequivalent elliptic fibrations of the same geometry. Due to the Heterotic/F-theory duality, the elliptic fibered Calabi-Yau in our consideration admits a nested elliptic K3 fibration structure. This is crucial to our design: the K3 fibrations determine the flavor groups and their global forms, in addition to serving as the key to identifying various T-dualities. In the end, I will also comment on more generic LSTs originating from non-geometric Heterotic backgrounds: a particularly exotic class of LSTs formed from extremal K3 surfaces that allows flavor groups with a maximal rank of 18. We find that all models are related to a so-called T-hexality (i.e., a 6-fold family of T-dualities) that we anticipate from the inequivalent elliptic fibrations of the extremal K3.
Tuesday, Dec 13, 2022
11:00, EFT strings and emergence, Luca Melotti, IFT, Madrid
Luca Melotti, IFT, Madrid
Title: EFT strings and emergence
Abstract: We revisit the Emergence Proposal in 4d N = 2 vector multiplet sectors that arise from type II string Calabi–Yau compactifications, with emphasis on the role of axionic fun- damental strings, or EFT strings. We focus on large-volume type IIA compactifications, where EFT strings arise from NS5-branes wrapping internal four-cycles, and consider a set of infinite-distance moduli-space limits that can be classified in terms of a scaling weight w = 1, 2, 3. It has been shown before how one-loop threshold effects of an infinite tower of BPS particles made up of D2/D0-branes generate the asymptotic behaviour of the gauge kinetic functions along limits with w = 3. We extend this result to w = 2 limits, by taking into account D2-brane multi-wrapping numbers. In w = 1 limits the leading tower involves EFT string oscillations, and one can reproduce the behaviour of both weakly and strongly-coupled U(1)’s independently on whether the EFT string is critical or not, by assuming that charged modes dominate the light spectrum.
Nicolas Kovensky, IPhT, Saclay
Title: More on KKLT from ten dimensions
Abstract: Gaugino condensation on D-branes wrapping internal cycles give a mechanism to stabilize the associated moduli. According to the effective field theory, they can give rise, when combined with fluxes, to supersymmetric AdS$_4$ solutions. In this talk we provide a ten-dimensional description of these vacua. We first describe the supersymmetry equations for type II AdS$_4$ vacua non-perturbative sources in the framework of generalized complex geometry. We then solve them for type IIB compactifications with gaugino condensates on smeared D7-branes. The solution is remarkably simple. Supersymmetry requires a (conformal) Calabi-Yau manifold and self-dual three-form fluxes with an additional (0,3) component. The latter is proportional to the cosmological constant, whose magnitude is determined by the expectation value of the gaugino condensate and the stabilized volume of the cycle wrapped by the branes. This confirms, qualitatively and quantitatively, the results obtained using effective field theory. As for the localized solution, it requires going beyond SU(3)-structure internal manifolds. If time allows, we show that the action can nevertheless be evaluated on-shell without relying on the details of such complicated configuration, and discuss the issue of divergencies arising in this context.
Stefano Andriolo, Ben Gurion
Title: Self-Binding in AdS and the WGC,
Abstract: The Positive Binding Conjecture is a proposed formulation of the Weak Gravity Conjecture appropriate to Anti de-Sitter (AdS) space. It proposes that in a consistent gravitational theory, with a U(1) gauge symmetry, there must exist a charged particle with non-negative self-binding energy. In order to formulate this as a constraint on a given effective theory, we calculate the self-binding energy for a charged particle in AdS4 and AdS5. In particular, we allow it to couple to an additional scalar field of arbitrary mass. Unlike the flat-space case, even when the scalar field is massive it contributes significantly to the binding energy, and therefore is an essential component of the conjecture. In AdS5, we give analytic expressions for the self-binding energy for the cases when the scalar field is massless and when it saturates the Breitenlohner-Freedman (BF) bound, and in AdS4 when it is massless. We show that the massless case reproduces the flat-space expressions in the large AdS radius limit, and that both analytic cases lead to vanishing total self-binding energy for BPS particles in example supersymmetric models. For other masses of the scalar we give numerical expressions for its contribution to the self-binding energy.
Andriana Makridou, Munich Max Planck Inst.
Title: The dark dimension in a warped throat
Abstract: The smallness of the cosmological constant Λ, together with swampland ideas, lead to the recent Dark Dimension proposal, which postulates that there exists a single mesoscopic extra dimension with size of a few micrometers. In particular, a single tower of light states should appear, with masses scaling like m ~ Λ^{1/4}. In this talk, I will explain how a strongly warped throat with its redshifted KK tower provides a natural string-theoretical mechanism realizing this aforementioned scaling, with the dark dimension being the one along the throat. I will point out challenges that may arise when considering such a setup, in particular concerning the masses of other KK towers.
Antoine Pasternak, Stanford
Title: Dynamical supersymmetry breaking in string theory
Abstract: Realizing supersymmetry breaking in string theory is an essential step for connecting our best-understood theory of quantum gravity with phenomenology. In this talk, I will review how to embed supersymmetry breaking gauge dynamics into branes at singular geometries in the framework of type IIB string theory. The stability of this construction will be addressed in the decoupling limit of Maldacena. I will finally outline the potential realization of a new non-supersymmetric gauge/gravity duality.
Eduardo Gonzalo, Lehigh U.
Title: Dark Dimension Gravitons as Dark Matter
Abstract: We consider cosmological aspects of the Dark Dimension (a mesoscopic dimension of micron scale), which has recently been proposed as the unique corner of the quantum gravity landscape consistent with both the Swampland criteria and observations. In particular we show how this leads, by the universal coupling of the Standard Model sector to bulk gravitons, to massive spin 2 KK excitations of the graviton in the dark dimension (the "dark gravitons") as an unavoidable dark matter candidate. We explain the main features of the model and comment on future experiments that can probe the dark dimension scenario.
Patrick Jefferson, MIT
Title: Analyzing the non-perturbative superpotential in type IIB orientifold compactifications
Abstract: In 4D N=1 type IIB orientifold compactifications, non-perturbative contributions to the superpotential can be generated by D3-instantons or seven-brane gaugino condensation. Under M/F-theory duality, these contributions are known to have a common origin, namely Euclidean M5-instantons wrapping vertical divisors in an elliptic Calabi-Yau fourfold. Understanding the geometric properties of vertical divisors is essential to analyzing the moduli-dependence of the non-perturbative superpotential. I will discuss a newly-developed algorithm for computing the Hodge structure of vertical divisors, which only requires as input the geometric data of the corresponding type IIB orientifold compactification space. A key part of this algorithm is a conjectured formula for the Euler characteristic of vertical divisors that captures the contributions of O3-planes.
Hao Zhang, UPenn
Title: The Branes Behind Generalized Symmetry Operators
Abstract: Generalized global symmetries in a QFT are encoded in topological symmetry operators, which non-trivially link the defect operators. In QFTs engineered via string theory on a non-compact geometry X, these defects descend from branes wrapped on non-compact cycles which extend to the boundary \partial X. Yet the realization of symmetry operators via string construction has long been implicit. We construct the generalized symmetry operators linking these defects as arising from magnetic dual branes wrapped on cycles in \partial X. This provides a systematic way to study their worldvolume topological field theories, and the resulting fusion rules. We illustrate these general features in the context of 6D superconformal field theories constructed using the F-theory, and read off the worldvolume theory of the symmetry operators from wrapped branes. These systems generically have non-invertible 2-form symmetries whenever the duality bundle of the F-theory model is non-trivial. We conclude by remarking that our understanding in principle allows for identifying the full symmetry structure of general geometrically engineered QFTs as (higher) fusion categories. We also comment on the potential top-down understanding of such categorical structure in connection with D-branes in topological string theories.
Vincent Van Hemelryck, KU Leuven
Title: Scale-separated AdS3 vacua from G2-orientifolds using bispinors
Abstract: In this talk, I discuss minimal supersymmetric AdS3 solutions on G2-orientifolds of type IIA and IIB supergravity. Such solutions have been studied before and I show that they can easily be obtained by bispinor techniques. With this formalism, I show that AdS3 solutions in massless type IIA string theory do not exist on such G2-backgrounds. Moreover, I show that in massive type IIA, the vacua do admit a separation of scales, whereas the same cannot be said for the type IIB. Furthermore, I present a formula for the 3d superpotential in terms of the bispinors, valid for both type IIA and IIB configurations. Finally, I show that the supersymmetry conditions for this superpotential lead back to the bispinor equations.
Tuesday, Oct 4, 2022
11:00, Non-Invertible Symmetries from Outer-Automorphism Gaugings, Lea Bottini , University of Oxford. (Video)
Lea Bottini, University of Oxford.
Title: Non-Invertible Symmetries from Outer-Automorphism Gaugings
Abstract: In the past year, a lot of attention has been given to non-invertible symmetries in dimensions higher than 3. These are characterized by the fact that the associated topological defects obey more general, not group-like fusions. In this talk I will present a prescription for constructing non-invertible symmetries by gauging outer-automorphism 0-form symmetries and apply it to some concrete gauge theory examples.
Gerben Venken, University of Heidelberg.
Title: Curvature corrections to KPV: Do antibrane uplifts need deep throats?
Abstract: I discuss alpha'^2 curvature corrections to the action of the
NS5-brane which is central to the metastability analysis of warped
anti-D3-brane uplifts by Kachru, Pearson and Verlinde (KPV). These
corrections can dramatically alter the KPV analysis. For the
alpha'^2-corrections to be sufficiently small to recover essentially
the leading-order KPV potential one needs a surprisingly large radius
at the tip of the throat, corresponding to g_s M > 20. In the context
of the Large Volume Scenario (LVS) this implies a D3-tadpole of at
least O(10^3-10^4). However, large alpha'^2-corrections do not
necessarily spoil the uplift in KPV. Rather, as the curvature
corrections lower the tension of the brane, a novel uplifting
mechanism suggests itself where the smallness of the uplift is
achieved by a tuning of curvature corrections. A key underlying
assumption is the existence of a dense discretuum of g_s. This new
mechanism does not require a deep warped throat, thereby sidestepping
the main difficulty in uplifting KKLT and LVS. However, all of the
above has to be treated as a preliminary exploration of possibilities
since, at the moment, not all relevant corrections at the order
alpha'^2 are known.
Joseph McGovern, University of Oxford
Title: New examples of modular supersymmetric flux vacua
Abstract: We compute the zeta function for a number of multiparameter Calabi-Yau threefolds. This is a generating function for point counts of these manifolds over finite fields. When the complex structure moduli space of these manifolds possesses a suitable $\mathbb{Z}_{2}$ symmetry, we find supersymmetric flux vacua on the fixed loci of this involution. In accordance with the Flux Modularity Conjecture of Kachru, Nally, and Yang (KNY) we observe that for these supersymmetric flux vacua the zeta function exhibits modular behaviour, so that one can read off weight-two modular newforms. In the F-theory uplift these newforms are associated to the F-theory curve by the modularity theorem, again in agreement with KNY. By applying Deligne's conjecture, we can evaluate derivatives of the Calabi-Yau periods in terms of L-values related to those elliptic curves.
Tuesday, June 28, 2022
11:00, Sharpening the Distance Conjecture in Diverse Dimensions, Muldrow Etheredge, Massachusetts U. (Video)
Muldrow Etheredge Massachusetts U. (Video)
Title: Sharpening the Distance Conjecture in Diverse Dimensions
Abstract: The Distance Conjecture holds that any infinite-distance limit in the scalar field moduli space of a consistent theory of quantum gravity must be accompanied by a tower of light particles whose masses scale exponentially with the proper field distance. This exponential dependence depends on a constant that is order-one in Planck units. In this talk, I will propose a sharp lower bound for this constant for the lightest tower in a given infinite-distance limit in d-dimensions: 1/sqrt(d-2). In support of this proposal, I will argue that (1) it is exactly preserved under dimensional reduction, (2) it is saturated in many examples of string/M-theory compactifications, and (3) simple apparent counterexamples actually do satisfy the bound.
Jeroen Monnee, Utrecht U.
Title: Bulk Reconstruction in Moduli Space Holography
Abstract: In recent years, asymptotic Hodge theory has been an essential tool for understanding the properties of field spaces in string compactifications. One such property is the emergence of universal algebraic structures near every boundary in the moduli space, dubbed boundary data. A fascinating result of Cattani, Kaplan and Schmid shows that using this simple data one can algorithmically recover the bulk of the moduli space (to a large extent). In this talk we discuss this procedure in detail and show that it can be applied in concrete examples to compute the period mapping of all one-modulus Calabi-Yau threefolds near any boundary.
Juven Wang, Harvard U.
Title: Cobordism and Deformation Class of the Standard Model and Beyond
Abstract: 't Hooft anomalies of quantum field theories (QFTs) with an invertible global symmetry G (including spacetime and internal symmetries) in a d-dim spacetime are known to be classified by a d+1-dim cobordism group TPd+1(G), whose group generator is a d+1-dim cobordism invariant written as a d+1-dim invertible topological field theory. Deformation class of QFT is recently proposed to be specified by its symmetry G and a d+1-dim invertible topological field theory. Seemingly different QFTs of the same deformation class can be deformed to each other via quantum phase transitions. We ask which deformation class controls the 4d ungauged or gauged (SU(3)×SU(2)×U(1))/Zq Standard Model (SM) for q=1,2,3,6 with a continuous or discrete (B−L) symmetry and with also a compatible discrete baryon plus lepton Z_{2Nf} B+L symmetry. (The Z_{2Nf} B+L is discrete due to the ABJ anomaly under the BPST instanton.) We explore a systematic classification of candidate perturbative local and nonperturbative global anomalies of the 4d SM, including all these gauge and gravitational backgrounds, via a cobordism theory, which controls the SM's deformation class. While many Grand Unified Theories violating the discrete B+L symmetry suffer from the proton decay, the SM and some versions of Ultra Unification (constrained by Z_{16} class global anomaly that replaces sterile neutrinos with new exotic gapped/gapless topological or conformal sectors) can have a stable proton. Dictated by a Z_2 class global mixed gauge-gravitational anomaly, there can be a gapless deconfined quantum critical region between Georgi-Glashow and Pati-Salam models -- the Standard Model and beyond occur as neighbor phases. We will also comment on a new mechanism to give the neutrino mass via topological field theories and topological defects. Work based on arXiv:2112.14765, arXiv:2204.08393, arXiv:2202.13498, arXiv:2106.16248, arXiv:2012.15860, and references therein.
Ethan Torres, University of Pennsylvania
Title: Getting High on Gluing Orbifolds,
Abstract: Quantum field theories (QFTs) engineered from M-theory on singular non-compact manifolds often enjoy a rich dictionary between physical data and geometric quantities. For instance, when real codimension-4 ADE orbifold singularities extend out to the asymptotic boundary, the local operators of the QFT form representations of the flavor group whose Lie algebra is specified by the ADE-types. We present a novel geometric procedure to calculate the global structure of this flavor group. Additionally, taking into account line operators of the QFT, this structure may generalize to a 2-group and we give a geometric picture for this as well. I will showcase this procedure in some examples of 5d SCFTs engineered from M-theory on quotients of C^3. Based on work with M. Cvetic, J.J. Heckman, and M. Hubner (2203.10102)
Mudasar Sabir, Hua-Zhong U. Sci.
Title: The Supersymmetry Breaking Soft Terms, and Fermion Masses and Mixings in the Supersymmetric Pati-Salam Model from Intersecting D6-branes
Abstract: A supersymmetric Pati-Salam model with wrapping number equal to 5 has been constructed in Type IIA orientifolds on T6/(ℤ2×ℤ2) with intersecting D6-branes recently. In particular, the string-scale gauge coupling unification can be achieved due to the intermediate-scale vector-like particles from N=2 sector. We calculate the supersymmetry breaking soft terms, and study the Standard Model (SM) fermion masses and mixings. There are nine pairs of Higgs doublets from N=2 sector. Interestingly, we can explain the SM quark masses and mixings, as well as the charged leptons masses from three point and four-point Yukawa interactions. Moreover, we calculate the supersymmetry breaking soft terms in a previous model with gauge coupling unification since we find a typo in the previous study.
Tuesday, June 7, 2022
11:00, Asymptotic Safety and the Swampland, Alessia Platania, Perimeter (Video)
Alessia Platania, Perimeter
Title: Asymptotic Safety and the Swampland,
Abstract: We investigate the consequences of combining swampland conjectures with the requirement of asymptotic safety. To this end, we explore the infrared regime of asymptotically safe gravity in the quadratic one-loop approximation, and we identify the hypersurface spanned by the endpoints of asymptotically safe renormalization group trajectories. These comprise the allowed values of higher-derivative couplings as well as standard logarithmic form factors. We determine the intersection of this hypersurface with the regions of parameter space allowed by the weak-gravity conjecture, the swampland de Sitter conjecture, and the trans-Planckian censorship conjecture. The latter two depend on some order-one constants, for generic values of which we show that the overlap region is a proper subspace of the asymptotically safe hypersurface. Moreover, the latter lies inside the region allowed by the weak gravity conjecture assuming electromagnetic duality. Our results suggest a non-trivial interplay between the consistency conditions stemming from ultraviolet completeness of the renormalization group flow, black hole physics, and cosmology.
Tuesday, May 31, 2022
11:00, Membranes in AdS4 orientifold vacua and their Weak Gravity Conjecture, David Prieto, IFT.(Video)
David Prieto, IFT
Title: Membranes in AdS4 orientifold vacua and their Weak Gravity Conjecture,
Abstract: We study type IIA orientifold compactifications with fluxes that give rise to perturbatively stable, non-supersymmetric AdS4 vacua with D6-brane gauge sectors. Non-perturbative instabilities can be mediated by D8-branes wrapped on the six internal dimensions X6, if they reduce to 4d membranes with a charge Q larger than its tension T. The mismatch between Q and T arises due to i) curvature corrections and ii) the BIon backreaction of D6-branes wrapping 3-cycles of X6. We give a simple expression for the second effect in toroidal orientifolds, and find that only pairs of 3-cycles at SU(2) angles contribute to it. They either contribute towards Q>T or Q<T depending on the 3-cycles separation, allowing to engineer 4d N=0 vacua in tension with the Weak Gravity Conjecture for membranes.
Tuesday, May 24, 2022
11:00, Making Wormholes Stable Again, Gregory J. Loges, University of Wisconsin-Madison. (Video)
Gregory J. Loges, University of Wisconsin-Madison
Title: Making Wormholes Stable Again,
Abstract: Giddings-Strominger wormholes have had a long history as smooth solutions of axion-gravity, but their interpretation and role in the Euclidean path integral has been unclear. I will discuss the perturbative stability of these axion wormholes using the dual, 3-form description where many of the difficulties faced in the axion frame are absent. Based on [2203.01956] with Gary Shiu and Nidhi Sudhir.
Max Wiesner, Harvard & CMSA
Title: Holography and the KKLT scenario,
Abstract: The KKLT scenario, one of the few ideas to realize dS vacua in string theory, consists of two steps: the first involves the construction of a supersymmetric AdS vacuum with a small negative cosmological constant, whereas the second involves breaking supersymmetry and uplifting the energy to achieve dS. In this talk I use conventional holography to argue why it is not possible to complete the first step, i.e. to obtain supersymmetric AdS vacua with small cosmological constant in type IIB/F-theory flux compactifications. Holography identifies the radius of the AdS flux vacuum with the IR central charge of the worldvolume theory on 5-branes wrapping special Lagrangian cycles in CY fourfolds dual to the flux. I will show that, as a consequence of tadpole cancellation, the central charge of this worldvolume theory is bounded by the Euler characteristic of the fourfold. Since the species scale is also set by the Euler characteristic of the fourfold, the AdS scale is at best of the order of the species scale such that one can only obtain highly curved AdS vacua beyond the validity of the EFT.
Álvaro Herráez, IPhT
Title: The Tadpole Conjecture in the Strict Asymptotic Limits,
Abstract: The Tadpole Conjecture puts severe constraints on the stabilization of a large number of moduli by claiming that in such settings the flux contribution to the tadpole grows at least linearly with the number of stabilized fields. In this talk we study the complex structure sector of F-theory compactifications on Calabi-Yau four-folds. We present the first conceptual argument that explains this linear scaling of the tadpole and clarifies why it sets in only for a large number of stabilized moduli. This is done in the strict asymptotic limits of moduli space, by using the tools of asymptotic Hodge theory, which make possible an explicit discussion of moduli stabilization close to any boundary of moduli space and allow us to establish the relevant scaling constraints for the tadpole.
Niccolò Cribiori, Max Planck Inst.
Title: Weak Gravity versus Scale Separation
Abstract: The existence of a separation of scales between the four observed spacetime dimensions and the yet unobserved additional ones is a minimal requirement for (string) phenomenology. Explaining its origin at the theoretical level is an open problem. I will present a general argument excluding scale separation in supersymmetric anti-de Sitter vacua of four-dimensional N=2,8 supergravity as a consequence of the weak gravity conjecture. This suggests that N=0,1 supersymmetry at the lagrangian level could be the most promising chances to obtain a truly four-dimensional effective description of quantum gravity.
Anthony Ashmore, Chicago
Title: Deformed N=1 SCFTs and their Supergravity Duals
Abstract: We consider the space of supersymmetric AdS5 solutions of type IIB supergravity corresponding to the conformal manifold of the dual 4d N = 1 conformal field theories. We describe how the background geometry naturally encodes a generalised holomorphic structure, dual to the superpotential of the field theory. Using this perspective, we address the long-standing problem of finding the gravity dual of the generic N = 1 deformations of N = 4 super Yang-Mills: though we are not able to give it in a fully explicit form, we provide a proof-of-existence of the supergravity solutions. Using this formalism, we analyse the moduli of the supergravity backgrounds and derive a new result for the Hilbert series of the deformed field theories.
Bruno Bento, Liverpool
Title: Gravity at the Tip of the Throat
Abstract: Warped throats have been used in countless works in the context of string theory compactifications, in particular for their ability to suppress high energy scales. The Klebanov-Strassler solution gives us an explicit description of the geometry of a warped throat which we can use to perform computations - my focus will be on the gravitational sector of the resulting 4d EFT, with its tower of Kaluza-Klein (KK) gravitons. By assuming that we live on a (3+1)-dimensional brane somewhere along the throat, we can study how the warping influences the effects of the tower on the brane.
In particular, I will show how the tower corrects the Newtonian potential and discuss how gravitational experiments and observations may be used to test the possibility that our Universe corresponds to a brane living in a warped throat.
Andres Rios Tascon, Cornell
Title: Computational Mirror Symmetry
Abstract: Abstract: In this talk, I will show that compactifications of the Heterotic String on a circle exhibit at the boundary of moduli space (R->0, or equivalently the decompactification limit R->infinity) a tower of winding or momentum modes that enhance the
E_8 x E_8 or SO(32) gauge algebras to the affine algebras (E_9+ E_9)/~ (the identification means that the two copies of E9 share the same central extension) and \hat{D}_16, respectively. I will also argue that these towers of modes satisfy the Lattice Weak Gravity and Repulsive Force Conjectures.
Tom Rudelius, Berkeley
Title: Higher-Group Symmetries, Axion Strings, and Weak Gravity Conjecture Mixing
Abstract: I will present some results on the infinite-distance properties of families of unstable flux vacua in string theory with broken supersymmetry. In the absence of a conformal manifold, I will employ the more general quantum information metric on theory space. The relevant trajectory undertaken along the tunneling cascade is described by a holographic renormalization group flow. In one limit an exponentially light tower of Kaluza-Klein states appears, while in the opposite limit a tower of higher-spin excitations of D1-branes becomes light, realizing the emergent string proposal. Moreover, the anomalous dimensions of scalar vertex operators and single-trace higher-spin currents decay exponentially in the distance. The holographic description of the latter includes a free sector, whose emergent superconformal symmetry resonates with supersymmetric stability, the CFT distance conjecture and S-duality.
Veronica Collazuol, IPHT
Title: E9 symmetry in the Heterotic Theory on S1 and the Weak Gravity Conjecture
Abstract: In this talk, I will show that compactifications of the Heterotic String on a circle exhibit at the boundary of moduli space (R->0, or equivalently the decompactification limit R->infinity) a tower of winding or momentum modes that enhance the
E_8 x E_8 or SO(32) gauge algebras to the affine algebras (E_9+ E_9)/~ (the identification means that the two copies of E9 share the same central extension) and \hat{D}_16, respectively. I will also argue that these towers of modes satisfy the Lattice Weak Gravity and Repulsive Force Conjectures.
Ivano Basile, Mons
Title: Emergent strings at infinite distance with broken supersymmetry
Abstract: I will present some results on the infinite-distance properties of families of unstable flux vacua in string theory with broken supersymmetry. In the absence of a conformal manifold, I will employ the more general quantum information metric on theory space. The relevant trajectory undertaken along the tunneling cascade is described by a holographic renormalization group flow. In one limit an exponentially light tower of Kaluza-Klein states appears, while in the opposite limit a tower of higher-spin excitations of D1-branes becomes light, realizing the emergent string proposal. Moreover, the anomalous dimensions of scalar vertex operators and single-trace higher-spin currents decay exponentially in the distance. The holographic description of the latter includes a free sector, whose emergent superconformal symmetry resonates with supersymmetric stability, the CFT distance conjecture and S-duality.
Manki Kim, MIT
Title: D(-1)-instanton superpotential in string theory
Abstract: In this talk, I will discuss the non-perturbative superpotential generated by D(-1)-branes in type IIB compactifications on orientifolds of Calabi-Yau threefold hypersurfaces. As a first step towards understanding D(-1)-instanton superpotential, I will consider orientifold compactifications in which all the D7-brane stacks carry SO(8) gauge groups and show that in such models the D(-1)-instanton superpotential vanishes.
Atakan Firat, MIT
Title: D-instanton superpotential in type II string theory on Calabi-Yau orientifolds
Abstract: In this talk, I will explain how one can fix the normalization of the D-instanton contribution to the superpotential in type II string theory on Calabi-Yau orientifolds using string field theory and show such normalization is holomorphic function of the moduli. Along the way I will sketch the proof for a folk theorem relating D-instantons to space-filling D-branes on Calabi-Yau's.
Pramod Shukla, ICTP Trieste
Title: Insights of (Global) String Model Building: Presumptions, Expectations and Reality
Abstract: The aim of this talk is to motivate the need for explicit global constructions on the way of string (inspired) model building. In this regard I will discuss several (sub-)leading contributions to the type IIB effective scalar potentials induced from various sources, and the subsequent underlying assumptions one usually makes in order to engineer attractive models of e.g. moduli stabilization or inflation. Taking a phenomenologist friendly approach, I will discuss the feasibility and challenges of fulfilling those naive and apparently simple assumptions in "some models" while aiming to find concrete Calabi Yau orientifolds. For illustration purposes, using the Kreuzer-Skarke CY dataset as well as the projective Complete Intersection Calabi Yau (pCICY) dataset, I will also present the scanning results for "suitable" divisor topologies of the CY threefolds, and their relevance for moduli stabilization, say in particular for scanning/classifying the perturbatively flat vacua, and inflation.
Alessandra Gnecchi, MPI Munich
Title: Large and Small Non-extremal Black Holes, Thermodynamics Dualities and the Swampland
Abstract: I will consider charged black holes at finite temperature and investigate infinite distance limits of these configurations in the temperature (T) vs entropy (S) parameter space. Due to the coupling of the geometry to scalar fields, I will show how the large/small T limit, as well as the small/large S limit, are often associated to the appearance of a tower of massless states, pushing these solutions outside of the quantum gravity landscape and into the swampland. I will discuss how this can be associated to a temperature distance conjecture. I will consider general couplings of charged, dilatonic black holes, and show that the same considerations apply to multi-charge solutions of N=2 supergravity.
Alberto Castellano, IFT Madrid
Title: IR/UV Mixing and The Swampland
Abstract: By applying the Bousso Bound to an EFT in a box one obtains that the UV and IR cut-offs of the EFT are necessarily correlated. We argue that in a theory of Quantum Gravity one should identify the UV cutoff with the `species scale', and give a general algorithm to calculate it in the case of multiple towers becoming light. One then obtains an upper bound on the characteristic mass scale of the tower in terms of the IR cut-off. Identifying such IR cut-off with a (non-vanishing) curvature in AdS one reproduces the statement of the AdS Distance Conjecture, also giving an explicit lower bound for the its relevant exponent. The UV/IR constraints found apply to both AdS and dS vacua. We comment on possible applications of these ideas to the dS Swampland conjecture as well as to the observed dS phase of the universe.
David Cyncynates, Stanford
Title: Friendship in the Axiverse
Abstract: The Axiverse is a scenario in which axion-like particles are distributed over many orders of magnitude in mass and interact with one another through a joint potential. In this talk, I will show how non-linearities in this potential lead to a new type of resonant energy transfer between "friendly" axions with nearby masses. This resonance generically transfers energy from axions with larger decay constants to those with smaller decay constants, leading to a multitude of signatures. These include enhanced direct detection prospects for a resonant pair comprising even a small subcomponent of dark matter, and boosted small-scale structure if the pair is the majority of DM. Near-future iterations of experiments such as ADMX and DM Radio will be sensitive to this scenario, as will astrophysical probes of DM substructure.
Gerben Venken, Heidelberg
Title: The LVS Parametric Tadpole Constraint
Abstract: The large volume scenario (LVS) for de Sitter compactifications of the type IIB string is in principle protected from various unknown corrections as the Calabi-Yau volume is exponentially large. However, as recently emphasised, the most explicit models are in practice on the border of parametric control. In this talk I identify what we believe to be the main issue behind this difficulty: A large volume implies a shallow AdS minimum and hence a small uplift. The latter, if it relies on an anti-D3 in a throat, requires a large negative tadpole. I provide a simple and explicit constraint for what this tadpole has to be in order to control the most dangerous corrections. The fundamental ingredients are parameters specifying the desired quality of control. I discuss directions for future work which could lead to LVS constructions satisfying our constraint with better control and the interplay between our constraint and the tadpole conjecture. Our constraint then represents a very concrete challenge for future searches for and the understanding of relevant geometries. Based on 2202.04087 .
Alberto Castellano, IFT Madrid
Title: IR/UV Mixing and The Swampland
Abstract: By applying the Bousso Bound to an EFT in a box one obtains that the UV and IR cut-offs of the EFT are necessarily correlated. We argue that in a theory of Quantum Gravity one should identify the UV cutoff with the `species scale', and give a general algorithm to calculate it in the case of multiple towers becoming light. One then obtains an upper bound on the characteristic mass scale of the tower in terms of the IR cut-off. Identifying such IR cut-off with a (non-vanishing) curvature in AdS one reproduces the statement of the AdS Distance Conjecture, also giving an explicit lower bound for the its relevant exponent. The UV/IR constraints found apply to both AdS and dS vacua. We comment on possible applications of these ideas to the dS Swampland conjecture as well as to the observed dS phase of the universe.
David Cyncynates, Stanford
Title: Friendship in the Axiverse
Abstract: The Axiverse is a scenario in which axion-like particles are distributed over many orders of magnitude in mass and interact with one another through a joint potential. In this talk, I will show how non-linearities in this potential lead to a new type of resonant energy transfer between "friendly" axions with nearby masses. This resonance generically transfers energy from axions with larger decay constants to those with smaller decay constants, leading to a multitude of signatures. These include enhanced direct detection prospects for a resonant pair comprising even a small subcomponent of dark matter, and boosted small-scale structure if the pair is the majority of DM. Near-future iterations of experiments such as ADMX and DM Radio will be sensitive to this scenario, as will astrophysical probes of DM substructure.
Irene Valenzuela, UAM
Title: The Desert and the Swampland
Abstract: The most natural expectation away from asymptotic limits in moduli space of supergravity theories is the desert scenario, where there are few states between massless fields and the quantum gravity cutoff. We initiate a systematic study of these regions deep in the moduli space, and compute the maximum value of the cutoff given by BPS states in large classes of supersymmetric vacua. We show that even though heuristically the species scale is compatible with expectations, the BPS states of the actual string vacua lead to a stronger dependence of the cutoff scale on the number of massless modes. We propose that this discrepancy can be resolved by placing a bound on the number of massless modes that is consistent with quantum gravity.
Luigi Tizzano, ULB
Title: Anomaly Matching Across Dimensions and Supersymmetric Cardy Formulae
Abstract: 't Hooft anomalies are known to induce specific contributions to the effective action at finite temperature. We present a general method to directly calculate such contributions from the anomaly polynomial of a given theory, including a term which involves a U(1) connection for the thermal circle isometry. Based on this observation, we show that the asymptotic behavior of the superconformal index of 4d N=1 theories can be calculated by integrating the anomaly polynomial on a particular background. Finally, we discuss how such asymptotic behavior captures the Bekenstein-Hawking entropy and phases of supersymmetric black holes in AdS.
Federico Carta, Durham
Title: Small flux superpotential and divisor topologies
Abstract: In this talk we discuss aspects of complex structure moduli stabilization in type IIB Calabi-Yau orientifolds. We will start reviewing the importance of obtaining an exponentially small flux superpotential W_0 in the context of KKLT, and a nice algorithm by the Cornell group which allows to obtain such result. We then proceed to study Calabi-Yaus in the Kreuzer-Skarke database, as well as the mirrors of the pCICYs (up to h11=2). Among them, we systematically identify which ones can be used to engineer models with small flux superpotentials, and list the resulting vacua. We briefly comment about the existence of vacua which remain flat even after the leading Gopakumar-Vafa corrections are included. Finally, we discuss the topology of divisors of pCICYs, and remark on their relevance for global model building.
Flavio Tonioni, Liverpool
Title: Misaligned Supersymmetry in String Theory
Abstract: Misaligned supersymmetry characterises a variety of non-supersymmetric string models: even if the particle spectrum lacks a one-by-one matching between fermionic and bosonic degrees of freedom, there exist theories in which an infinite oscillation between fermionic and bosonic surpluses results in cancellations leading to a finite one-loop cosmological constant. Misaligned supersymmetry has been often discussed with regard to closed-string theories and at leading order in the expansion of the net state degeneracies. After a general overview, for both open and closed strings, I will describe how to extend this beyond leading order and elucidate the mathematics underlying the heuristic interpretation of misaligned supersymmetry as a key to the one-loop cosmological constant finiteness. This can help in shedding further light on the relationship between supersymmetry and string theory.
Craig Lawrie, DESY
Title: Infinitely-many 4d SCFTs with a=c
Abstract: I will explore a special subset of the 4d SCFT landscape, with N=1 and N=2 supersymmetry and identical central charges: a = c, without any large N limit. Such SCFTs are obtained via N=1 or N=2 diagonal gauging of collections of non-Lagrangian Argyres--Douglas and conformal matter theories and I will discuss the classification problem for consistent gaugings with interacting infrared SCFTs in both cases. For N=2, the classification is in terms of an ADE Dynkin diagram Γ. Moreover, we find that the Schur indices for such theories can be written in terms of that of N=4 super-Yang-Mills theory upon rescaling fugacities. For generic choices of Γ and G, it can be regarded as a generalization of the affine quiver gauge theory obtained from D3-branes probing singularity of type Γ. For N=1, there exists a vast collection of gaugings, including with additional chiral multiplets on the gauge node, that flow in the infrared to interacting SCFTs with a=c, and I highlight some of their features.
Kajal Singh, HCRI
Title: Exploring Aspects of the String Landscape
Abstract: In type IIB flux compactifications, the magnitude of the vev of the Gukov-Vafa-Witten superpotential W_0 plays an important role. Recently exponentially small values of W_0 were achieved by constructing perturbatively flat vacua. In this talk, we will explore these vacua in a statistical context. I will discuss our findings using the 2-moduli case as an example and will generalize it to higher moduli. I will also present a statistical study of low energy physics after taking Kähler moduli stabilization into consideration, which is crucial to get reliable vacua.
Enrico Pajer, Cambridge
Title: From locality and unitarity to cosmological correlators
Abstract: In this talk, I will report on recent progress in developing a new "bootstrap" approach to perturbative QFT in de Sitter. The bootstrap approach builds directly upon the fundamental pillars of physics. In particular, I will discuss the recent breakthroughs in understanding the consequence of unitarity for cosmological correlators to all orders in perturbation theory, as well as the footprint of (bulk) locality. These principles can be used to derive many classical and new inflationary predictions associated with primordial non-Gaussianity in a way that is both computationally simpler and conceptually more transparent. Extending these results beyond perturbation theory might give us a tool to exclude theories without a consistent UV completion in de Sitter, and a useful framework to develop de Sitter holography.
Andreas Schachner, Cambridge
Title: The Large Scale Structure of α' Effects in String Theory
Abstract: In this talk, I discuss three approaches to understanding and completing the 10-dimensional effective actions of type II superstring theory. I provide concrete evidence at the level of 5-point superstring amplitudes that higher derivative terms in the maximally U(1)-violating (MUV) sector are obtained from standard superspace integrals over sixteen fermionic coordinates. This is in agreement with 11D superparticle amplitudes in M-theory where modular forms required for SL(2,Z) invariance of type IIB arise explicitly from integrating out winding modes on a 2-torus. Lastly, I argue that these observations can be generalised to the complete MUV sector of the type IIB effective action for the complex 3-form and the metric.
Lars Aalsma, Madison
Title: Extremal Black Hole Corrections from Iyer-Wald
Abstract: Extremal black holes play a key role in our understanding of various swampland conjectures and in particular the WGC. The mild form of the WGC states that higher-derivative corrections should decrease the mass of extremal black holes at fixed charge. Whether or not this conjecture is satisfied depends on the sign of the combination of Wilson coefficients that control corrections to extremality. Typically, corrections to extremality need to be computed on a case-by-case basis, but in this talk I will present a universal derivation of extremal black hole corrections using the Iyer-Wald formalism. This leads to a formula that expresses general corrections to the extremality bound in terms of the stress tensor of the perturbations under consideration, clarifying the relation between the WGC and energy conditions. This shows that a necessary condition for the mild form of the WGC to be satisfied is a violation of the Dominant Energy Condition. This talk is based on 2111.04201.
Nava Gaddam, Utrecht
Title: Page curve and emergent soft theorems from black hole scattering
Abstract: I hope to convey the following three messages in this talk:
1. There is a new interesting phase of quantum gravity where black hole scattering matrix elements can be computed in effective field theory.
2. These scattering amplitudes reveal the dynamics leading to information retrieval after Page time.
3. Remarkably, new emergent soft-graviton theorems arise near the black hole horizon in this phase.
Max Wiesner, Harvard
Title: Light Strings and Strong Coupling
Abstract: In this talk I will discuss a relation between light perturbative strings and strong coupling singularities in the Kähler moduli space of 4d N=1 compactifications of F-theory. In limits of the Kähler moduli space where a critical string becomes light, the F-theory moduli space reduces to the stringy moduli space of this light string. In certain cases, this allows to extract the non-perturbative singularity structure of the local F-theory moduli space. I will show that for simple setups with a heterotic dual description, a strong coupling singularity for a D7-brane gauge theory occurs in the region of moduli space where the critical string is classically expected to be light. In the vicinity of this non-perturbative singularity, the string can be shown to leave the spectrum of light strings thereby providing a non-perturbative explanation for the censoring of certain classical weak coupling limits in F-theory which were previously argued for at the purely perturbative level. On the other hand for the weakly-coupled critical string to remain part of the light string spectrum, the moduli space needs to factorise in a certain way. The strong coupling singularity occur whenever this factorisation is not protected by the string and broken at the quantum level.
Jakob Moritz, Cornell
Title: Modular Superpotentials from Singular Divisors
Abstract: We study Euclidean D3-branes wrapping holomorphic divisors D with normal crossing singularities along rational curves, in compactifications of type IIB string theory on orientifolds of Calabi-Yau threefolds. Witten's counting of fermion zero modes on smooth divisors D in terms of the cohomology of the structure sheaf O_D is not directly applicable in this setting. We argue that fermion zero modes are instead captured by the line bundle cohomology of the log resolution of D. We show this by detailing compactifications in which the normal crossing singularities can be unwound by passing through suitable flop transitions, giving a physical incarnation of the log resolution process. Analytically continuing the superpotential through the flops, we find non-vanishing results even in geometric phases where normal crossing singularities are present. Furthermore, these compactifications feature infinitely many isomorphic geometric phases, and thus give rise to infinite order monodromy groups Gamma, whose action on effective divisors can be used to determine exact effective cones, with infinitely many generators related to each other by the action of Gamma. As a consequence, the non-perturbative superpotentials can be resummed into Jacobi theta functions, whose modular symmetries suggest the existence of strong/weak coupling dualities involving inversion of divisor volumes.
Junsei Tokuda, Kobe
Title: Swampland conditions on scalar potentials from positivity bounds
Abstract: Various swampland conditions have been conjectured with various rigors and motivations. It is interesting if these swampland conjectures can be derived. We study positivity bounds on scalar field theories coupled to gravity under several clear assumptions on scattering amplitudes. We find that positivity bounds imply that scalar potentials cannot be arbitrarily flat unless some new physics enters well below the Planck scale. Our result provides a swampland condition for scalar potentials.
Paul Oehlmann, Uppsala
Title: Gauged 2-form symmetries in 6D SUGRAs
Abstract: 6D N=(2,0) and (1,0) SCFTs admit a wide range of global symmetries that are expected to be either broken or gauged when coupled to gravity. One particular symmetry is that of a discrete self-dual 2 form symmetry that couples the tensionless BPS strings to Wilson surface operators. Such SUGRA theories can be geometrically engineered in IIB and F-theory. We show that global symmetries are generically absent and derive a geometric condition on the BPS string embedding into the compact geometry such that a gauged 2-form symmetry survives. We check our proposal via various dualities, where the 2-form symmetry reduces to a 1-form symmetry in 5D.
Nicole Righi, DESY
Title: Fuzzy Dark Matter Candidates from String Theory
Abstract: We provide a string theoretical explanation of fuzzy dark matter as composed by ultralight axions coming from the compactification of type IIB string theory on Calabi-yau manifolds. In particular, we consider C2 and C4 axions stabilased in a Large Volume Scenario, and thraxions, axionic modes living in warped throats of the internal manifold. Based on the latest bounds, we study how likely it is for dark matter to be composed of such particles and in which abundance. We provide predictions on the preferred ranges of masses and decay constants when string axions behave as FDM. Moreover, requiring those axions to lie in the FDM range imposes constraints on the features of the internal manifold. We also comment on implications for the Weak Gravity Conjecture.
Joe Conlon, Oxford
Title: Exploring the Holographic Swampland
Abstract: I describe our work looking at `traditional' scenarios of moduli stabilisation from a holographic perspective. This reveals some interesting structure that is not apparent from the top-down perspective. For vacua in the extreme regions of moduli space, such as LVS in type IIB or the DGKT flux vacua in type IIA, the dual moduli conformal dimensions reduce to fixed values - in a certain sense, the low-conformal dimension part of the CFT is unique and independent of the large number of flux choices. For the DGKT flux vacua these conformal dimensions are also integer, for reasons we do not understand.
Gregory Loges, Madison
Title: Breeding Branes
Abstract: Machine learning has proven to be a useful tool in understanding the landscape of string vacua. One rich corner to explore is that of intersecting D6-branes on toroidal orbifolds, where the consistency conditions are simply phrased in terms of integer winding numbers. I will discuss ongoing work using genetic algorithms to search for consistent, MSSM-like models in this setting.
John Stout, Harvard
Title: Axion Masses from Monopoles
Abstract: I will describe a novel contribution to an axion's effective potential: loops of virtual magnetic monopoles. Gauge kinematics demand that monopoles must acquire an electric charge in the presence of a theta angle. Since the electric field sourced by this induced charge forces the monopole mass to depend on the theta angle, integrating out these states will generate a theta-dependent contribution to the vacuum energy, i.e. an axion effective potential, even in a gauge theories with no instantons.
Damian van de Heisteeg, Utrecht
Title: Title: Moduli Stabilization in Asymptotic String Compactifications
Abstract: In this talk we discuss novel approaches to moduli stabilization in Type IIB flux compactifications. Our strategies rely on recent insights about Calabi-Yau moduli spaces based on asymptotic Hodge theory. In the first approach we engineer flux vacua with small superpotentials by using certain essential exponential corrections. In the second approach we set up a systematic three-step approximation scheme by using asymptotic sl(2)-structures.
Mateo Galdeano, Oxford
Title: Superconformal Algebras for (Generalized) Connected Sums
Abstract: When string theory is compactified on special holonomy manifolds, a fascinating correspondence arises: covariantly constant forms are associated to currents in the worldsheet chiral algebra. I will discuss this relation in the context of Generalized Connected Sum Spin(7) manifolds, which are constructed by gluing together two open manifolds along isomorphic asymptotic ends. The geometric structure is reproduced in the worldsheet algebra, and this can be exploited to shed some light on Spin(7) mirror symmetry. This talk is based on joint work with M.-A. Fiset, [2104.05716].
Matilda Delgado, IFT Madrid
Title: Dynamical Cobordism and Swampland Distance Conjectures
Abstract: We consider spacetime-dependent solutions to string theory models with tadpoles for dynamical fields, arising from non-trivial scalar potentials. The solutions have necessarily finite extent in spacetime, and are capped off by boundaries at a finite distance, in a dynamical realization of the Cobordism Conjecture. We show that as the configuration approaches these cobordism walls of nothing, the scalar fields run off to infinite distance in moduli space, allowing one to explore the implications of the Swampland Distance Conjecture. We uncover new interesting scaling relations linking the moduli space distance and the SDC tower scale to spacetime geometric quantities, such as the distance to the wall and the scalar curvature. We show that walls at which scalars remain at finite distance in moduli space correspond to domain walls separating different (but cobordant) theories/vacua; this still applies even if the scalars reach finite distance singularities in moduli space, such as conifold points. We illustrate our ideas with explicit examples in massive IIA theory and M-theory on CY threefolds. In 4d N=1 theories, our framework reproduces a recent proposal to explore the SDC using 4d string-like solutions.
Xingyang Yu, NYU
Title: 2d N=(0,1) gauge theories, Spin(7) orientifolds and triality
Abstract: I will introduce a new brane engineering for 2d minimally supersymmetric, i.e. N=(0,1), gauge theories. Starting with 2d N=(0,2) gauge theories on D1-branes probing Calabi-Yau 4-folds, a brand new orientifold configuration named ’Spin(7) orientifold’ is constructed and the resultant 2d N=(0,1) theories on D1-branes are derived. Using this method, one can build an infinite family of 2d N=(0,1) gauge theories explicitly. Furthermore, the N=(0,1) triality, proposed by Gukov, Pei and Putrov, enjoys a geometric interpretation as the non-uniqueness of the map between gauge theories and Spin(7) orientifolds. The (0,1) triality can then be regarded as inherited from the N=(0,2) triality of gauge theories associated with Calabi-Yau 4-folds.
Title: BIonic membranes and AdS instabilities
Abstract: We study 4d membranes in type IIA flux compactifications of the form AdS4 x X_6, where X_6 admits a Calabi--Yau metric. These models feature scale separation and D6-branes/O6-planes on three-cycles of X_6. When the latter are treated as localised sources, explicit solutions to the 10d equations of motion and Bianchi identities are known in 4d N=1 settings, valid at first order in an expansion parameter related to the AdS4 cosmological constant. We extend such solutions to a family of perturbatively stable N=0 vacua, and analyse their non-perturbative stability by looking at 4d membranes. We find that either D4-branes or anti-D4-branes on holomorphic curves feel no force in both N =1 and N=0 AdS4. Differently, D8-branes wrapping X_6 and with D6-branes ending on them can be attracted towards the boundary of N=0 AdS4. The source of imbalance is the curvature of X_6 and the D8/D6-system BIon profile. The latter dominates when X_6 is a (blown-up) toroidal orbifold, rendering such 4d membranes superextremal. We argue that N=0 vacua of this sort with space-time filling D6-branes are unstable against bubble nucleation, and decay to N=0 vacua with less D6-branes and larger Romans mass.
Robert Rosati, UT Austin
Title: Rapid-turn inflation in supergravity is rare and tachyonic
Abstract: Strongly non-geodesic, or rapidly turning, trajectories in multifield inflation have attracted much interest recently from both theoretical and phenomenological perspectives. For example, such trajectories can evade the eta-problem in fat inflation, in which all inflatons are heavier than the Hubble scale. Most models with large turning rates in the literature are formulated as effective field theories. In this talk I'll discuss some investigations into rapid-turn inflation in supergravity as a first step toward understanding them in string theory. We find that large turning rates can be generated in a wide class of models, at the cost of high field space curvature. However, in these models one field is always tachyonic along the inflationary trajectory, implying that fat inflation may not be viable in supergravity. The high curvatures underscore the difficulty of obtaining rapid-turn inflation in realistic string-theoretical models.
Saghar Sophie Hosseini, Durham
Title: Higher form symmetries of geometrically engineered field theories
Abstract: I will discuss the geometric origin of higher form symmetries of quantum field theories. These symmetries may be found systematically in terms of the defect groups from geometric engineering in string theories, M-theory and F-theory. The flux non-commutativity in string theory constrains the corresponding global structures of the associated quantum fields.
Pietro Ferrero, Oxford
Title: Gluon scattering in AdS from CFT
Abstract: I will present a class of recently computed holographic correlators between half-BPS operators in a vast array of SCFTs with non-maximal superconformal symmetry in dimensions d=3,4,5,6. Via AdS/CFT, these four-point functions are dual to gluon scattering amplitudes in AdS. I will show that, at tree level, all such correlators are completely fixed by symmetries and consistency conditions. Our results encode a wealth of CFT data and exhibit various emergent structures, including Parisi-Sourlas supersymmetry, hidden conformal symmetry and color-kinematics duality.
Naomi Gendler, Cornell
Title: PQ Axiverse
Abstract: We show that the strong CP problem is solved in a large class of compactifications of string theory. The Peccei-Quinn mechanism solves the strong CP problem if the quality of the QCD axion is high, meaning that the breaking of the axion shift symmetry by the ultraviolet completion of gravity and of QCD is small compared to the CP-preserving axion potential generated by low-energy QCD instantons. We consider type IIB flux compactifications on Calabi-Yau hypersurfaces, taking a simple model of QCD on D7-branes. We compute an upper bound on the shift symmetry breaking from D-brane instanton couplings to hidden-sector axions, and from high-energy instantons in QCD. We find that in theories with a sufficiently large number of axions, the instantons that could perturb the vev of the QCD axion away from zero typically have large actions, and thus do not spoil Peccei-Quinn quality. Furthermore, we find that for the majority of geometries in a certain range of h^{1,1}, the axion masses and decay constants are compatible with standard cosmological and astrophysical constraints.
Vincent Van Hemelryck, Leuven
Title: Scale-separated AdS4 vacua of IIA orientifolds and M-theory
Abstract: Obtaining string compactifications where the KK scale is much higher than the cosmological constant scale is quite challenging. Such a separation of scales is however necessary for the theory to be genuinely lower-dimensional. In massive type IIA string theory there are such scale-separated vacua, e.g. the DGKT AdS4 solutions. It has been shown recently that the classical orientifold backreaction in these vacua can be tuned small. In this talk I show that massless IIA on the other hand allows both weakly and strongly coupled AdS4 vacua that exhibit scale separation and for which the backreaction can be tuned small as well. I will give evidence that the strongly coupled solutions can be lifted to scale separated and sourceless (but classically singular) geometries in 11D supergravity.
Thomas Vandermeulen, SUNY Albany
Title: A Constructive Approach to Orbifolds
Abstract: I will discuss an approach to constructing orbifold partition functions that puts modular invariance at the forefront, preserving it even for e.g. asymmetric actions. We will see how this approach always produces a consistent theory, which can be seen to decompose into a direct sum of orbifolds by non-anomalous subgroups of the orbifold group. This construction relates to a general method of resolving anomalies by group extensions, which we will examine in the context of orbifolds.
Robin Schneider, Uppsala
Title: Deep learning of Calabi-Yau metrics
Abstract: In this talk I will present a new open source package for approximating Calabi-Yau metrics. The metric tensor can be modeled by different neural networks, which take the complex and Kähler moduli as user specified input. Experimental results are compared against previous studies on the Fermat Quintic from the literature. Furthermore, I demonstrate that the learned metric tensor on the Bicubic manifold obeys the slope equation for line bundles.
Marieke van Beest, Oxford
Title: Holography, 1-Form Symmetries, and Confinement
Abstract: I will discuss confinement in 4d N = 1 SU(N) Super-Yang Mills from a holographic point of view, focusing on the 1-form symmetry and its mixed 0-/1-form symmetry anomaly, which is closely related to chiral symmetry breaking. From the dual gravity description we also identify the IR 4d topological field theory, which realises chiral symmetry breaking and matches the mixed anomaly. The talk is based on [2104.12764].
Martin Bies, UPenn
Title: Root Bundles and Towards Exact Matter Spectra of F-theory MSSMs
Abstract: Root bundles recently entered the quest for F-theory MSSM as their cohomologies count the vector-like spectra, which includes the number of Higgs pairs. I will elaborate on these developments by present the work done in 2102.10115 and 2104.08297.
Ethan Torres, UPenn
Title: On Reflection Anomalies and Matter Content of M-theory on Local Spin(7) Spaces
Abstract: M-theory compactified on local Spin(7) spaces fibered by ALE singularities engineer 3d N=1 gauge theories coupled to matter which are often strongly coupled in the infrared. Despite the lack of holomorphic tools, some mileage can be gained when the field theory is symmetric under spatial reflections. One can measure a mod-16 't Hooft anomaly that captures the obstruction to placing the theory on a non-orientable manifold (i.e. a mixed reflection-gravity anomaly) and restricts the possible low energy phases. I will discuss some recent work on how to compute this anomaly for various compactification geometries built using Higgs bundle constructions. Along the way we will see how CPT-like symmetries descend from M-theory to 7d SYM to the 3d field theory, and find (perhaps surprisingly) that natural choices for how to define these symmetries in each setting are quite different from one another. (Based on work with M.Cvetic, J.Heckman, and G.Zoccarato. hep-th/2107.00025)
Lorenz Schlechter, Utrecht
Title: Generalized Clausen identities and the swampland distance conjecture
Abstract: Clausen's hypergeometric identity relates the periods of certain K3 manifolds to the periods of elliptic curves. We show that generalizations of this identity together with period relations are sufficient to obtain global closed forms for the periods of all 1-parameter K3 manifolds valid in all phases. This mechanism can be further generalized to include all K3-manifolds as well as Fano 3-folds. The closed forms are used to compute distances in the moduli space of Calabi-Yau 3-folds analytically.
Sebastian Dumitru, UPenn
Title: Line Bundle Hidden Sectors for Strongly Coupled Heterotic Standard Models
Abstract: We present a formalism for constructing hidden-sector bundles induced from single line bundles, within the context of strongly coupled heterotic M-theory. We review the compactification from the eleven-dimensional Hořava-Witten orbifold to five-dimensional heterotic M-theory on a Schoen Calabi-Yau threefold, as well as the specific SU(4) vector bundle on the observable sector, which leads to the B−L MSSM low energy spectrum. In addition, we discuss a set of theoretical and phenomenological constraints and propose a viable vacuum configuration to satisfy them, which includes a specific hidden sector line bundle. For instance, one of the conditions that we demand is that N=1 supersymmetry is preserved at the compactification scale. This requirement allows us to attach a possible mechanism to break supersymmetry at low energy scales: gaugino condensation in the hidden sector. The condensation scale is computed and found to be low enough to be compatible with the energy scales available at the LHC.
First Talk
Title: Bounce of Nothing
Abstract: Theories with compact extra dimensions are sometimes unstable to decay into a bubble of nothing – an instability resulting in the destruction of spacetime. In this talk, I will discuss the existence of these bubbles in theories where the moduli fields that set the size of the extra dimensions are stabilized at a positive vacuum energy – a necessary ingredient of any theory that aspires to describe the real world. Using bottom-up methods, and focusing on a five-dimensional toy model, I will argue that four-dimensional de Sitter vacua admit bubbles of nothing for a wide class of stabilizing potentials. I will show that, unlike ordinary Coleman-De Luccia tunneling, the corresponding decay rate remains non-zero in the limit of vanishing vacuum energy. Potential implications include a lower bound on the size of compactified dimensions.
Second Talk
Title: The FL bound and its phenomenological implications
Abstract: The Festina Lente (FL) bound is a generalization of the Weak Gravity Conjecture to models of positive vacuum energy, which arises from demanding that extremal, large black holes must decay in a nonsingular way. It states that the mass of every charged state is lower-bounded by the vacuum energy scale. In this talk I will review the derivation of the bound, discuss some tentative evidence in string compactifications, and discuss a number of pheno implications ranging from neutrino and Higgs physics to antibrane uplifting scenarios.
First Talk
Title: Cyclic Free Quotients of Favorable CICY-3 Folds
Abstract: Free quotients of CICY-3 folds are important for string theory model building. In this talk we will report some progress on classifying all the cyclic free quotients of CICY-3 folds associated to their newly found favorable configurations presented in https://arxiv.org/abs/1708.07907. In the first part of the talk, I will discuss some basics of CICY free quotients. After this I will discuss a method introduced by Braun to judge fixed points freeness of a quotient manifold by using character valued indices of invariant line bundles. After this we will talk about the scanning process using the above method and finally we will discuss the new symmetries we obtained.
Second Talk
Title: Yukawa textures from spectral data
Abstract: Consider a Heterotic model (X,V) with X being an elliptically fibered Calabi-Yau threefold and V a stable holomorphic degree zero bundle. We compute the Yukawa textures of the effective theory in terms of the spectral data (i.e. the Fourier transform) of V. In addition, we will be able to find vanishing theorems in some cases. This approach has several advantages relative to the usual techniques: first, the Yukawa textures can be related to “simpler” cohomology groups, second, it can be easily related to the Higgs bundle spectral data over 7-branes, and the Yukawa textures of the local F-theory models. Since most of the Calabi-Yau threefolds are elliptically fibered this approach can be used in many cases.
First Talk
Title: Constraints on SM from AdS conjectures
Abstract: We consider constraints on D-dimensional EFTs in Minkowski, dS and AdS backgrounds in the light of AdS swampland conjectures as applied to their compactification in a circle. In particular we consider the non-SUSY AdS instability conjecture and the AdS distance conjecture. For Minkowski and dS vacua the results may be summarized by a Light Fermion Conjecture which states that if (-1)^(k+1) times the first non-vanishing supertrace is positive then a surplus of light fermions with masses smaller (or equal) than the cosmological constant must be present. We then focus on extensions of the SM with sterile neutrinos and find constraints on the mass of the lightest neutrino and rule out the standard See-Saw mechanism. Finally, we consider an extension of the SM including a quintessence field and show how the generalization of the dS conjecture to AdS vacua leads to similar results.
Second Talk
Title: Z5 Symmetries in F-theory, Homological Projective Duality and Modular Forms
Abstract: Genus-one fibered Calabi-Yau manifolds with 5-sections lead to F-theory vacua with Z_5 gauge symmetry. Geometrically, the N-section case with N>4 is interesting because the normal form of the fibers is not a complete intersection in a toric ambient space. This turns out to have striking implications for the modular structure of the topological string partition functions. One of the tools in our analysis are elliptic complete intersections in toric ambient spaces that lead to vacua with charge 5 matter in F-theory. Using Higgs transitions, which geometrically correspond to extremal transitions to genus-one fibrations with 5-sections, we discover a beautiful interplay between the modular structures on different genus-one fibrations, the associated physics in M-/F-theory and non-Abelian GLSMs, as well as the arithmetic and algebraic geometry.
First Talk
Title: Modelling General asymptotic Calabi-Yau Periods
Abstract: I will discuss an approach to the general study of period vectors of Calabi-Yau threefolds in asymptotic regions of complex structure moduli space. These period vectors play an important role in string compacitifcations, making a better understanding of their general structure desirable. The strategy is to exploit constraints imposed by completeness, symmetry, and positivity, which are formalised in asymptotic Hodge theory. Together with the classification of all possible boundaries in moduli space, these principles allow for a systematic construction of models for the asymptotic period vectors. One also gains insight about the necessity of exponentially suppressed corrections to the polynomial part of the period vector when away from the well-studied large complex structure point.
Second Talk
Title: F-theory flux vacua at large complex structure
Abstract: We compute the flux-induced F-term potential in 4d F-theory compactifications at large complex structure. In this regime, each complex structure field splits as an axionic field plus its saxionic partner, and the classical F-term potential takes the form V = Z^{AB}ρ_Aρ_B with ρ depending on the fluxes and axions and Z on the saxions. We provide explicit, general expressions for Z and ρ, and from there analyse the set of flux vacua, for an arbitrary number of fields. We identify two families of vacua with all complex structure fields fixed and a flux contribution to the tadpole Nflux which is bounded. In the first and most generic one, the saxion vevs are bounded from above by a power of Nflux. In the second, their vevs may be unbounded and Nflux is a product of two arbitrary integers, unlike what is claimed by the Tadpole Conjecture. We specialise to type IIB orientifolds, where both families of vacua are present, and link our analysis with several results in the literature. We finally illustrate our findings with several examples.
First Talk
Title: Open string methods and Gopakumar-Vafa invariants
Abstract: Topological invariants of singular Calabi-Yau threefolds, besides being of intrinsic interest for mathematicians, are objects that have great consequences in physics, as their properties are believed to capture instantonic effects in effective field theories arising from string compactifications. We are interested in finding new efficient ways of computing a specific class of topological invariants, known as Gopakumar-Vafa invariants, using string theory methods, thus also providing physical intuition about their origin. With this objective in mind, we focus on a class of non-toric Calabi-Yau threefolds in M-theory, exploiting the duality with type IIA to describe them in terms of D6-branes and O6-planes. In such setting, the tachyon condensation mechanism shows that computing Gopakumar-Vafa invariants is nothing but counting the states of strings stretching between the D6-branes. We show this technique in action for a variety of concrete examples, highlighting connections to the T-brane formalism and other physical implications.
Second Talk
Title:8d Supergravity, Reconstruction of Internal Geometry and the Swampland
Abstract: We sharpen Swampland constraints on 8d supergravity theories by studying consistency conditions on worldvolume theory of 3-brane probes. Combined with a stronger form of the cobordism conjecture, this leads to the reconstruction of the compact internal geometry and implies strong restrictions on the gauge algebra and on the level of the current algebra on the 1-brane probe. In particular, we argue that 8d supergravity theories with g2 gauge symmetry are in the Swampland. These results provide further evidence for the string lamppost principle in 8d with 16 supercharges.
First Talk
Title: On string vacua without supersymmetry
Abstract: We discuss the existence and stability of vacua in string theories where supersymmetry is either absent or broken at the string scale. In particular we present no-go results regarding de Sitter compactifications, connecting them to some Swampland conjectures, thereby focusing on anti-de Sitter (AdS) flux vacua arising from the USp(32) and U(32) orientifold models and from the SO(16) x SO(16) heterotic model. We investigate perturbative and non-perturbative instabilities and frame the vacua in terms of brane stacks, analyzing their back-reacted geometry and reproducing AdS in the near-horizon limit. Then we describe the instabilities in terms of brane interactions, connecting this scenario to some Swampland conjectures and to braneworld cosmology.
Second Talk
Title:Holography, 1-Form Symmetries and Confinement
Abstract: I will discuss confinement in 4d N = 1 SU(N) Super-Yang Mills (SYM) from holography, focusing on the 1-form symmetry and the holographic realization in terms of the Klebanov-Strassler solution. I will show how from the 5d consistent truncation it is possible to identify the topological couplings that determine the 1-form symmetry (and thus global forms of the gauge group) and its ’t Hooft anomalies. One of the topological couplings corresponds to a mixed 0-1-form symmetry anomaly, which is related to chiral symmetry breaking in the infrared (IR) vacuum. I will then discuss how other couplings in the 5d supergravity description of the IR Klebanov-Strassler solution lead to a 4d Topological Field Theory (TQFT) in the boundary, which saturates the mixed anomaly.
First Talk
Title: On the Finiteness of Supergravity Landscape in d=6
Abstract: In the past years, it has been well established that UV quantum gravity theory puts strict constraints on the set of quantum field theory that can appear in the low- energy. Such consistency conditions are said to divide the consistent quantum field theories to those in the Landscape (consistent when coupled to gravity) and those not consistent which are said to belong to the Swampland. I will start by reviewing such conditions in the context of supersymmetric theories and evaluate where we stand on the validity of the String Lamppost Principle, i.e. the idea that all consistent quantum gravitational theories are part of the string theory landscape. I will particularly focus on our recent work with Cumrun Vafa where we argue that there is an upper bound on the number of massless modes in d=6, consistent with the String Lamppost Principle.
Second Talk
Title: The Standard Model Quiver from Singular de Sitter String Compactifications
Abstract: With the advent of the string landscape, the realisation of the Standard Model in general string theory compactifications to 4D has become a primary focus. This talk concerns novel constructions of the Standard Model in global set-ups of type IIB Calabi-Yau compactifications. We argue that the Standard Model quiver can be embedded into Calabi-Yau threefolds through orientifolded D3 branes at del Pezzo singularities dPn with n ≥ 5. To illustrate our approach, we construct several distinct local dP5 models via a combination of Higgsing and orientifolding. This procedure reduces the original dP5 quiver gauge theory to the Left-Right symmetric model with three families of quarks and leptons and a Higgs sector to further break the symmetries to the Standard Model gauge group. Subsequently, we discuss explicit embeddings of the local model in a global Calabi-Yau compactification. We show that moduli can be stabilised in 4-dimensional de Sitter vacua with uplifting provided by T-branes.
First Talk
Title: Probing inflation with the stochastic gravitational wave background and an opportunity for string pheno
Abstract: Primordial scalar fluctuations sourced during inflation, if sufficiently enhanced, induce a contribution to the stochastic gravitational wave background that is potentially detectable with the upcoming generation of gravitational wave observatories. This enhancement requires a departure of inflation from the vanilla single-field slow-roll paradigm and e.g. occurs in models with features in the inflaton potential or due to multi-field dynamics. These properties necessary for an enhancement are generically present in string theory compactifications. String theory constructions can thus help in constraining such more complicated inflation models from the theory side, which is a task with interesting connections to the swampland program.
Second Talk
Title: Branes, fermions and superspace
Abstract: We provide an approach to obtain the fermionic expansion of brane actions and specialise in four-fermion terms. For doing so, we use the interpretation of branes being hypersurfaces in superspace, and obtain the fermion expansion in the most simple case: the M2-brane. Next, we use a superspace generalization of dimensional reduction and of T-duality to obtain fermion terms on all Dp-branes.
First Talk
Title: Vanishing Yukawa couplings in heterotic compactifications
Abstract: We consider the perturbative Yukawa couplings of effective field theories obtained from compactifications of the heterotic string on Calabi-Yau three-folds. Although the physical Yukawa coupling explicitly depends on the Calabi-Yau metric, it has been known since the 80s that there is a factor that is independent of this metric. This so-called holomorphic Yukawa coupling only depends on the cohomology classes of the moduli and the (perturbative) physical coupling must vanish whenever the holomorphic coupling does. While considerably simpler, the holomorphic coupling is still subtle to compute because it depends on a multiplicative structure on cohomology. Fortunately, in certain compactifications, geometric structures of the manifold impose constraints on the allowed non-vanishing holomorphic couplings, and this has led to vanishing theorems in the past. In this talk, recent work will be presented in which vanishing theorems with a much wider range of applicability than their precursors are derived. This is based on results from homological algebra and sheaf cohomology, which will be briefly reviewed before we present the arguments that lead to the new results. As far as time allows, examples will be presented demonstrating that the new theorems do indeed predict new vanishings, relative to older results.
Second Talk
Title: Dynamical tadpoles, stringy cobordism and the SM from spontaneous compactification
Abstract: We consider string theory configurations with tadpoles for dynamical fields and discuss properties of the resulting spacetime-dependent solutions. We argue that these solutions can extend only a finite distance away in the spacetime dimensions over which the fields vary, with a scaling controlled by the strength of the tadpole. We also show that naive singularities arising at this distance scale are replaced by ends of spacetime, related to the cobordism defects of the swampland cobordism conjecture. We illustrate these phenomena in several examples, including susy and non-susy 10 string theories and a 6d string model whose tadpole triggers spontaneous compactification to a semirealistic 3-family MSSM-like particle physics model.
First Talk
Title: The Gravitino and the Swampland
Abstract: We conjecture that the limit of vanishing gravitino mass belongs to the swampland, since it corresponds to the massless limit of an infinite tower of states and thus to the breakdown of the effective field theory. We test our proposal in large classes of models coming from compactification of string theory to four dimensions, where we identify the Kaluza-Klein nature of the tower of states becoming light. We point out a general relation between the gravitino mass and gauge coupling in models with extended supersymmetry, which can survive also in examples with minimal supersymmetry. This allows us to connect our conjecture to other well established swampland conjectures, such as the weak gravity conjecture or the absence of global symmetries in quantum gravity. We discuss phenomenological implications of our conjecture in (quasi-)de Sitter backgrounds and extract a lower bound for the gravitino mass in terms of the Hubble parameter.
First Talk
Title: Eternal Inflation and (Anti) de Sitter Bounds from Dimensional Reduction
Abstract: In recent years, much work has gone into understanding the implications of a set of interesting but more speculative Swampland conjectures, among which are the de Sitter conjectures and the (Anti) de Sitter distance conjecture. In order to place these statements on firmer ground and understand their domains of validity, it is crucial to understand the physical underpinning of these statements, and (relatedly) to fix presently unknown O(1) coefficients appearing in them. In this talk, we will see how dimensional reduction may play a useful role in this process, in that it distinguishes particular, physically-meaningful values of O(1) coefficients. We will also work out the conditions for slow-roll eternal inflation, and will we compare these bounds to the de Sitter conjecture bounds.
Second Talk
Title: The Gravitino Swampland Conjecture
Abstract: We extend the swampland from effective field theories (EFTs) inconsistent with quantum gravity to EFTs inconsistent with quantum supergravity. This enlarges the swampland to include EFTs that become inconsistent when the gravitino is quantized. We propose the Gravitino Swampland Conjecture (GSC): the gravitino sound speed must be non-vanishing in all EFTs that are low energy limits of quantum supergravity. This seemingly simple statement has important consequences for both theories and observations. Talk based on arXiv:2102.10113 and arXiv:2103.10437.
First Talk
Title: Non-flat elliptic fourfolds, three-form cohomology and strongly coupled theories in four dimensions
Abstract: In this talk we consider elliptic fourfolds with non-minimal singularities in codimension two in the base. These sectors admit an F-theory interpretation as compactifications of 6D superconformal matter on a Riemann surface. We consider resolutions of those non-minimal singularities which sacrifice flatness of the fibration and naturally leads to threeform cohomology in terms of the 6D SCFT data. Finally we consider a Higgs and Coulomb branch type of conifold transition. The former one pushes the non-flat fiber one codimension lower and leaves non-perturbative four-point matter coupling as a remnant. The second transition removes those fibers via a birational base blow-up which keeps the Euler number invariant.
Second Talk
Title: String defects, supersymmetry and the swampland
Abstract: In order to fully connect the swampland program and low-energy phenomenology, it appears necessary to consider the conjectures in string models with broken supersymmetry. In this talk, I will consider an approach pioneered by Kim, Shiu and Vafa, who ruled out anomaly-free supergravity theories based on the fact that they cannot be consistently coupled to a complete spectrum of string defects. To possibly extend their conditions, expressed in a pure effective theory language, to non-SUSY setups, I will discuss their origin in a microscopic string picture, namely perturbative 6d orientifold constructions, and study how they are modified in SUSY breaking setups of the brane supersymmetry breaking type. In the latter case, the supersymmetric conditions still hold if the string defect does not overlap with the SUSY breaking source. The general discussion also suggests a “null string conjecture”, that allows to exclude some 6d supergravity theories that have no known string or F-theory realization.
First Talk
Title: The Price of Curiosity: Information Recovery in de Sitter Space
Abstract: Recent works have revealed that the fine-grained entropy of a non-gravitating subsystem, when entangled with a gravitating region, can receive contributions from so-called quantum extremal islands. Applied to black holes, this reproduces the unitary Page curve for Hawking radiation. In this talk, I will show how these results can be applied to the thermal radiation measured by a static observer in de Sitter space. Focusing on JT gravity, I will emphasize the necessity of going beyond the thermal equilibrium of the Bunch-Davies state. We will see that a quantum extremal island can contribute to the fine-grained entropy, suggesting unitarity of the radiation, but this comes at a price: when the island appears a singularity forms that a static observer will eventually hit.
Second Talk
Title: Anomalies of (0,4) SCFTs from wrapped D3 branes in F-theory
Abstract: In this talk we will consider macroscopically, a class of 2d (0,4) SCFTs living on black strings. The black strings are constructed by wrapping D3-branes on a curve inside the base of a (singular) elliptically fibered Calabi—Yau three-fold. The asymptotic geometry in which the branes live in includes an ALE or ALF space which probes the D3 branes. Using macroscopic computations we will compute the various anomaly coefficients of the theory by reducing 6d N=(1,0) supergravity on the horizon of the black strings and extracting the coefficients of Chern—Simons terms. As we will, see the inclusion of one-loop corrections from integrating out massive modes is essential. Given time we will make some comments on the microscopic computation.
First Talk
Title: Algorithmically solving the Tadpole Problem
Abstract: I demonstrate how to use differential evolutionary algorithms to find flux compactifications of M-theory on K3xK3. The assumption that a large numbers of moduli can be stabilized with fluxes within the tadpole bound is one of the corner stones of the String Landscape and was recently challenged by the Tadpole Conjecture. Explicitly showing moduli stabilization for manifolds with many moduli is highly challenging. On K3xK3 moduli stabilization is well understood and can be formulated exclusively in terms of integer matrices and their eigenvalues and -vectors. In particular, there is no knowledge of complicated period integrals or the corresponding Picard-Fuchs equations required. This makes this example predestined for a computer aided search. Using differential evolution we show that there are no smooth compactifications on K3xK3 with arbitrarily small flux M2-charge, in tension with the tadpole bound.
Second Talk
Title: Tackling the SDC in AdS with CFTs
Abstract: Using the AdS/CFT correspondence, questions related to the Swampland Distance Conjecture (SDC) in AdS can be reformulated in the language of conformal manifolds. For AdS_5 backgrounds with eight or more supercharges, we find that for a large class of (and possibly all) infinite-distance points, there must exist a tower of massless higher-spin fields. On the conformal side, those points are those for which a sector of the CFT becomes free, and the tower follows from the presence of higher-spin conserved currents. We illustrate these results for type IIB compactifications on S^5 and its orbifolds.
First Talk
Title: New databases for model building: CICY orientifolds and GV invariants
Abstract: We present two recently computed explicit databases which could be relevant for model building in String Phenomenology. The first contains two million orientifolds supporting O3 and O7 planes that can be constructed for the list of Complete Intersection Calabi-Yau manifolds (CICYs). The second is an explicit computation of all the genus zero Gopakumar-Vafa (GV) invariants for such class of CYs, up to total degree 10. In both instances, we find interesting phenomena arising. In the orientifold scan, we discover a plethora of new cases with non-vanishing h11-odd, which can support C2 and B2 axions, as well as thraxions. We also observe the existence of conifold singularities that lie on-top of orientifold planes and thus cannot be deformed, but can still be resolved. We argue that on the resolution side we find a vast set of (possibly previously unknown) CY manifolds. In the GV scan, we find interesting hierarchies between the rate of growth of the invariants along different directions inside the Picard lattice. Such hierarchies have an application in complex structure moduli stabilization aiming at achieving a very small W0 superpotential, as well as winding inflation models. Furthermore, we eliminate redundancies in the list of CICYs, by a systematic implementation of Wall’s theorem.
Second Talk
Title: The Convex Hull Swampland Distance Conjecture and Bounds on Non-geodesics
Abstract: The Swampland Distance Conjecture (SDC) restricts the geodesic distances that scalars can traverse in effective field theories as they approach points at infinite distance in moduli space. We propose that, when applied to the subset of light fields in effective theories with scalar potentials, the SDC restricts the amount of non-geodesicity allowed for trajectories along valleys of the potential. This is necessary to ensure consistency of the SDC as a valid swampland criterium at any energy scale across the RG flow. We provide a simple description of this effect in moduli space of hyperbolic space type, and products thereof, and obtain critical trajectories which lead to maximum non-geodesicity compatible with the SDC. We recover and generalize these results by expressing the SDC as a new Convex Hull constraint on trajectories, characterizing towers by their scalar charge to mass ratio in analogy to the Scalar Weak Gravity Conjecture. We show that recent results on the asymptotic scalar potential of flux compatifications near infinity in moduli space precisely realize these critical amounts of non-geodesicity. Our results suggest that string theory flux compactifications lead to the most generic potentials allowing for maximum non-geodesicity of the potential valleys while respecting the SDC along them. Based on arXiv:2012.00034 with Angel M. Uranga and Irene Valenzuela.
First Talk
Title: Neural Network Approximations for Calabi-Yau metrics
Abstract: Ricci flat metrics for Calabi-Yau threefolds are not known analytically. In this work, we employ techniques from machine learning to deduce numerical approximations to flat metrics for the Fermat quintic, for the Dwork quintic, and for the Tian-Yau manifold. This investigation employs a single neural network architecture that is capable of approximating Ricci flat Kaehler metrics for several Calabi-Yau manifolds of dimensions two and three. We show that measures that assess the Ricci flatness of the geometry decrease after training by three orders of magnitude. This is corroborated on the validation set, where the improvement is more modest. Finally, we demonstrate that discrete symmetries of manifolds can be learned in the process of learning the metric.
Second Talk
Title: de Sitter Quantum Breaking, Swampland Conjectures and Thermal Strings
Abstract: We argue that the quantum breaking approach and the trans-Planckian censorship conjecture can both lead to bounds of the same functional form for the scalar potential. The proposal that dS quantum breaking is induced by tracing over states beyond the dS horizon gives rise to a thermal matter component, which can be straightforwardly generalized to string theory. Imposing a censorship of quantum breaking, we recover in the low temperature regime the no eternal inflation bound. The stronger dS swampland conjecture bound arises, under certain assumptions, in the mysterious high temperature regime of string theory.
First Talk
Title: A New Spin on the Weak Gravity Conjecture
Abstract: The mild form of the Weak Gravity Conjecture states that quantum or higher-derivative corrections should decrease the mass of large extremal charged black holes at fixed charge. This allows extremal black holes to decay, unless protected by a symmetry (such as supersymmetry). We reformulate this conjecture as an integrated condition on the effective stress tensor capturing the effect of quantum or higher-derivative corrections. In addition to charged black holes, we also consider rotating BTZ black holes and show that this condition is satisfied as a consequence of the c-theorem, proving a spinning version of the Weak Gravity Conjecture. We also apply our results to a five-dimensional boosted black string with higher-derivative corrections. The boosted black string has a BTZ×S2 near-horizon geometry and, after Kaluza-Klein reduction, describes a four-dimensional charged black hole. Combining the spinning and charged Weak Gravity Conjecture we obtain positivity bounds on the five-dimensional Wilson coefficients that are stronger than those obtained from charged black holes alone. This talk is based on work with L. Aalsma, G. Loges, and G. Shiu.
Second Talk
Title: Topological gravity as the early phase of our universe
Abstract: I will present a scenario for the early universe that is motivated by dualities in string theory. Dualities, as well as puzzles of cosmology, naturally lead to considering a topological theory of gravity. Using Witten’s 4d topological gravity as one realization, one can estimate phenomenological properties of the CMB fluctuations whose power spectrum is controlled by the conformal anomaly coefficients a and c. In particular, the strength of the fluctuations is controlled by 1/a and the tilt by cg^2 where g is the coupling constant of topological gravity. The positivity of c, a consequence of unitarity, leads automatically to an IR tilt for the power spectrum. In addition, the topological nature of gravity implies the absence of primordial tensor modes. Finally, I will discuss some analogies with particle physics that provide further clarification of this picture.
First Talk
Title: Numerical Calabi-Yau metrics from holomorphic networks
Abstract: Calabi-Yau metrics have many important applications in string compactification. However, it is generally believed that no closed-form expression exists. In this talk, I will introduce machine learning inspired methods for computing numerical Calabi-Yau metrics and the implementation using Tensorflow/Keras. I will compare them with previous work and show some results for manifolds with little or no symmetry.
Second Talk
Title: Infinite Distance, Emergent Strings and Quantum Corrections in 4D N=1
Abstract: Infinite distance limits in the Kähler moduli space of F-theory compactifications on elliptic Calabi-Yau fourfolds can feature tensionless heterotic or type II strings that emerge from wrapping D3-branes on shrinking curves. If a gauge coupling vanishes in the limit, the Weak Gravity and Distance Conjectures predict an infinite tower of light, (super-)extremal states. Such a tower is provided by the excitations of an emergent heterotic string. In this talk, I will first review the geometry of these limits at the classical level and argue that the resulting tensionless string is unique. We will then discuss how quantum corrections to the 4D $N=1$ effective action influence the classical limits and the tower of WGC states. We will see that the inclusion of \alpha’-corrections is crucial for the consistency of the theory.
First Talk
Title: Elliptic Calabi-Yau manifolds with the largest h11
Abstract: In this talk, I’m going to discuss the construction of elliptic Calabi-Yau manifolds with the largest known Hodge number h11 in the framework of F-theory. I’ll first review the cases of elliptic threefolds and fourfolds, and then present the new results on elliptic fivefolds.
Second Talk
Title: Supersymmetric Flux Vacua and Calabi-Yau Modularity
Abstract: Most familiar constructions in string theory are rooted in the complex geometry of the compact dimensions. On the other hand, much of modern mathematics focuses on arithmetic geometry, where we consider the properties of varieties over smaller fields such as Q. In this talk, following recent work (arXiv:2001.06022, arXiv:2010.07285) with S. Kachru and W. Yang, I will explain how string theory can be related to arithmetic. In particular, I will argue that supersymmetric flux vacua admit arithmetic structures closely related to those of elliptic curves, and moreover that these arithmetic structures are related to the geometry of the F-theory description of the flux compactification.
First Talk
Title: Elliptic Calabi-Yau manifolds with the largest h11
Abstract: We observe that in many 6D F-theory models, tuning a specific gauge group G and matter content M leads to an automatic enhancement to a larger gauge group G’ ⊃ G and matter content M’ ⊃ M. We propose that this is true for any theory G, M for which there exists a containing theory G’, M’ that cannot be Higgsed down to G, M. I will discuss a number of examples, including non-Higgsable gauge factors, nonabelian gauge factors, abelian gauge factors, and exotic matter. In each of the discussed cases, tuning an F-theory model with the desired features produces either an enhancement or an inconsistency, often when the associated anomaly coefficient becomes too large. This principle applies to a variety of models in the apparent 6D supergravity swampland, including some of the simplest cases with U(1) and SU(N) gauge groups and generic matter, as well as infinite families of U(1) models with higher charges presented in the prior literature, potentially ruling out all these apparent swampland theories.
Second Talk
Title: Resolving spacetime singularities in flux compactifications and KKLT
Abstract: In flux compactifications of type IIB string theory with D3 and seven-branes, the negative induced D3 charge localized on seven-branes leads to an apparently pathological profile of the metric sufficiently close to the source. With the volume modulus stabilized in a KKLT de Sitter vacuum this pathological region takes over a significant part of the entire compactification, threatening to spoil the KKLT effective field theory. I will argue that wrapped seven-branes can be thought of as bound states of more microscopic exotic branes. The low-energy worldvolume dynamics of a stack of $n$ such exotic branes is given by the $(A_1,A_{n-1})$ Argyres-Douglas theory. Moreover, the splitting of the perturbative (in $\alpha'$) seven-brane into its constituent branes at the non-perturbative level resolves the apparently pathological region close to the seven-brane and replaces it with a region of $\mathcal{O}(1)$ Einstein frame volume. While this region generically takes up an $\mathcal{O}(1)$ fraction of the compactification in a KKLT de Sitter vacuum we argue that small classical flux superpotentials dynamically ensure that KKLT de Sitter vacua are generically safe from dangerous corrections.
First Talk
Title: Towards realistic matter spectra in F-theory
Abstract: In this project I analyze in detail the exact massless vector-like spectrum of MSSM in F-theory compactified on elliptic Calabi-Yau fourfold. The massless zero modes are determined by line bundles over matter curves under the presence of gauge background. In realistic F-theory geometry, those line bundles we concerned turn into so-called root bundles, which are not computationally feasible on generic curves. We noticed that there exists so-called limit root construction for the matter curve to realize the global section counting on it under special complex structure choice. I will present an explicit example of indicating exactly three generations of quarks on a particular curve at the end and anticipate this method would further allows us to find complete matter spectra of MSSM in the future.
Second Talk
Title: The Holographic Swampland
Abstract: We investigate whether Swampland constraints on the low-energy dynamics of weakly coupled string vacua in AdS can be related to inconsistencies of their putative holographic duals or, more generally, recast in terms of CFT data. In the first part of the talk, we shall illustrate how various swampland consistency constraints are equivalent to a negativity condition on the sign of certain mixed anomalous dimensions. This condition is similar to well-established CFT positivity bounds arising from causality and unitarity, but not known to hold in general. Our analysis will include LVS, KKLT, perturbative and racetrack stabilisation, and we shall also point out an intriguing connection to the Distance Conjecture. In the second part, we show how a different, recently derived inequality on mixed anomalous dimensions maps to novel constraints on four-derivative interactions on AdS. As an application, we use this to constrain the interactions of scalars with a non standard kinetic term, finding in particular that the DBI action for multiple scalar fields is at the boundary of the allowed region. Based on 2006.01021 with Joseph Conlon and forthcoming works.
First Talk
Title: Probing Higgs Bundles for Local G2-Manifolds
Abstract: M-theory on local G2-manifolds engineers 4d minimally supersymmetric gauge theories. This class of geometries admits a description in terms of a Higgs bundle over a 3d base and engineers a partially twisted 7d supersymmetric Yang-Mills theory from which the 4d physics is derived. This talk will explain how Euclidean M2-brane instanton effects can be understood and calculated in the effective 7d SYM description using probe particles for the Higgs bundle.
Second Talk
Title: Pheno constraints from Charged Black Hole Evaporation in de Sitter
Abstract: I will discuss the decay of charged black holes in de Sitter space. We establish how the black hole mass and charge change over time due to both Hawking radiation and Schwinger pair production as a function of the masses and charges of the elementary particles in the theory. We find a lower bound on the mass of charged particles by demanding that large charged black holes evaporate back to empty de Sitter space, in accordance with the thermal picture of the de Sitter static patch. This constrains the allowed spectrum of charged particles in supergravity and string theory de Sitter constructions in an interesting way. This bound is satisfied by the charged spectrum of the Standard Model. This bound has phenomenological implications for the cosmological hierarchy problem and inflation.
First Talk
Title: Probing Higgs Bundles for Local G2-Manifolds
Abstract: A flop is one of the simplest topological transitions that a Calabi-Yau (CY) threefold can undergo, and flops frequently connect multiple CYs into a web having a single moduli space. Typically, the existence of flops for a given CY has been detected from flops of a toric ambient space. However, for one of the most useful collections of CYs, namely complete intersection Calabi-Yaus (CICYs), the ambient space does not admit flops. But in his talk two weeks ago, Andrei deduced from line bundle cohomologies the existence of flops for CICYs. These hence require a different description. In my talk I will explain how to explicitly perform these flops, which will provide in particular a description of the CY after the transition as a complete intersection in a toric ambient space. Additionally, I will show how one can easily deduce from only the configuration matrix the presence and properties of these flops, and I will illustrate that essentially all CICYs admit (many) flops. Finally, I will use these ideas in a slightly different direction to show that one can often immediately write down all zeroth cohomologies from only the configuration matrix.
Second Talk
Title: Pheno constraints from Charged Black Hole Evaporation in de Sitter
Abstract: Dark gauge sectors are ubiquitous in string theory. At some time in the early universe, gluons in these sectors confine into dark glueballs or hadrons, the phase transition known to be first-order for many choices of gauge groups and numbers of fermions. Such a transition produces a stochastic gravitational wave signal that might be measured in future searches. In this talk, we use a phenomenological matrix model to describe confinement in a dark gauge sector in order to estimate the gravitational wave signal produced in a dark confining transition. We focus on the case of pure Yang-Mills, as it shows up consistently in F-theory.
First Talk
Title: Control issues of KKLT
Abstract: We analyze to which extent the KKLT proposal for the construction of de Sitter vacua in string theory is quantitatively controlled. Our focus is on the quality of the 10d supergravity approximation. As our main finding, we uncover and quantify an issue which one may want to call the “singular-bulk problem”. In particular, we show that, requiring the curvature to be small in the conifold region, one is generically forced into a regime where the warp factor becomes negative in a significant part of the Calabi-Yau orientifold. This implies true singularities, independent of the familiar, string-theoretically controlled singularities of this type in the vicinity of O-planes.
Second Talk
Title: Non-Supersymmetric Branes
Abstract: D-branes are an important part in many string phenomenology models and can act as sources of spontaneous supersymmetry breaking. They are employed in many setups, including the famous KKLT scenario. The linear supersymmetry of the background will be realized non-linearly after it is broken by a D-brane. Fundamentally, this leads to non-linear, so-called de Sitter, supergravity. In this talk I will show how the correct description of such theories in 4d non-linear supergravity looks like and how it is possible to include any supersymmetry breaking Dp-brane via a modification of the Kähler- and Superpotential into an initially N=1 supersymmetric model.
First Talk
Title: New aspects of line bundle cohomology and applications to string phenomenology
Abstract: The calculation of vector bundle cohomology represents a key ingredient in string phenomenology, being associated to the massless modes of both heterotic and Type II string compactifications. In this talk I report some recent progress in deriving closed-form expressions for line bundle cohomology on spaces of interest in string theory, which include complex surfaces such as compact toric surfaces, generalised del Pezzo surfaces and K3 surfaces, as well as Calabi-Yau threefolds. I will concentrate on the case of three-folds, where it turns out that line bundle cohomology encodes a wealth of information about flops and Gromov-Witten invariants. Finally, I will briefly discuss two phenomenology applications: the prospect of implementing a bottom-up approach to model building and flop transitions in heterotic string theory.
Second Talk
Title: Dynamical Tadpoles and Weak Gravity Constraints
Abstract: Non-supersymmetric string models are plagued with tadpoles for dynamical fields, which signal uncanceled forces sourced by the vacuum. We argue that in certain cases, uncanceled dynamical tadpoles can lead to inconsistencies with quantum gravity, via violation of swampland constraints. We describe an explicit realization in a supersymmetric toroidal Z_2xZ_2 orientifold with D7-branes, where the dynamical tadpole generated by displacement of the D7-branes off its minimum leads to violation of the axion Weak Gravity Conjecture. In these examples, cancellation of dynamical tadpoles provides consistency conditions for the configuration, of dynamical nature (as opposed to the topological conditions of topological tadpoles, such as RR tadpole cancellation in compact spaces). We show that this approach provides a re-derivation of the Z-minimization criterion for AdS vacua giving the gravitational dual of a-maximization in 4d N=1 toric quiver SCFTs.
First Talk
Title: Scouting the Heights of the Kreuzer-Skarke Landscape
Abstract: The Kreuzer-Skarke (KS) database has been an important wellspring of Calabi-Yau manifolds for string compactifications in the past two decades. Until recently, its formidable size and complexity have only allowed the base of this large Everest to be explored. Our computational advancements have now turned it into a playground that we can easily scout throughout. I will explain our developments, and present a live demo of our upcoming open-source package CYTools, which we hope will open the doors of the KS playground to everyone.
Second Talk
Title: Non-SUSY String Phenomenology from Z2 x Z2 Heterotic Orbifolds
Abstract: We explore the space of non-SUSY string models via two distinct routes: the tachyon-free O(16) x O(16) heterotic string in 10D and a tachyonic 10D heterotic string. We classify 4D Z_2 x Z_2 orbifolds descending from these two starting points in the free fermionic construction. Having found a potentially stable Standard-like model descending from the tachyonic 10D vacuum in arXiv:1912.00061, the approach of taking these models on equal footing with the non-tachyonic 10D models is justified provided that the tachyonic states are projected out in the four dimensional models. In both classes of models we find examples of Type 0 and Type 0bar models, i.e. models free of fermionic massless states and models free of twisted massless bosons, respectively. Moving beyond these extreme configurations we seek to classify tachyon-free vacua according to standard phenomenological criteria in both classes of model, where an SO(10) GUT is broken to the Pati-Salam subgroup. An analysis of the cosmological constant and misaligned supersymmetry in the two classes of models finds notable vacua in both cases in which N_b=N_f at the massless level.
First Talk
Title: Eclectic flavor symmetries from orbifolds
Abstract: Flavor symmetry might play a crucial role in the standard model of particle physics, but its origin is still unknown. We consider a string theory-based scenario, in which the flavor symmetry arises from the compactification of extra dimensions. We observe that compactifications on toroidal orbifolds yield naturally discrete flavor symmetries that consist of traditional flavor symmetries as well as modular symmetries, combined in a so-called “eclectic flavor group”. More concretely, we will discuss the eclectic flavor groups of the two dimensional Z2 and Z3 Narain orbifolds.
Second Talk
Title: On supersymmetric AdS4 orientifold vacua
Abstract: In this talk I will study ten-dimensional solutions to type IIA string theory of the form AdS4 x X6 which contain orientifold planes and preserve N = 1 supersymmetry. In particular, I will consider solutions which exhibit some key features of the four-dimensional DGKT proposal for compactifications on Calabi-Yau manifolds with fluxes, and in this sense may be considered their ten-dimensional uplifts. I will show that it is possible to find solutions that are valid at the two-derivative level and at first order in an expansion parameter related to the AdS CC. This family of solutions exhibits a SU(3) × SU(3)-structure, and dilaton gradients and warp factors are induced.
First Talk
Title: On Scale Separation and a Membrane/Potential correspondence
Abstract: In the first part of the talk, we will explore the issue of Scale Separation and the ADC in a particular class of type II compactifications on twisted tori. After presenting different examples in which the naive 4d EFT appears to violate the relevant conjectures, we will show how taking into account the full 10d picture modifies the naive lower-dimensional EFT results in precisely the right way for the conjectures to be satisfied. In the second part, if time permits, we will we present a correspondence between the 4d F-term N=1 scalar potential and a system of parallel BPS membranes. More concretely, we will show how each of the different terms in the formula for the potential is in one-to-one correspondence with the exchange of 3-forms, scalars and gravitons between the membranes.
Second Talk
Title: The NN-QFT Correspondence
Abstract: All Neural Networks, backbones of deep learning, are Gaussian Processes in infinite width limit and at initialization. Euclidean scalar field theory without interactions is shown to be a natural description of NNGP (Neural Network Gaussian Process), indicating an interesting correspondence between EFT and NNs. Finite width NN correlation functions can be computed using Feynman diagrams, by turning on interactions in the field theory. Overparameterization problem of NNs can be solved using Wilsonian renormalization group flow, as it describes the minimal non-Gaussian Process (NGP) using most relevant non-Gaussian (interaction) terms. Experiments support that one single parameter can correct GP correlation functions to NGP correlation functions. Output space dimensions and symmetries in NN architectures have interesting effects on the interaction strengths describing the NGP.
First Talk
Title: Swampland Conjectures at the Boundary of Field Space
Abstract: The vicinity of boundaries in Calabi-Yau moduli spaces have been a fruitful setting to test swampland conjectures in recent years. In the first part of this talk we discuss the charge-to-mass spectrum of BPS states in CY threefold compactifications of Type IIB string theory. We obtain bounds for the weak gravity conjecture, and comment on how these relate to their counterparts for the Swampland Distance and de Sitter Conjectures. In the second part of this talk we consider a novel approach to constrain three-form periods. We use these techniques to obtain generic models for two-moduli CY compactifications.
Second Talk
Title: Do classical de Sitter string backgrounds exist?
Abstract: A classical solution of string theory with a 4d de Sitter space-time could be a simple and well-controlled setting, where to connect to cosmological models. So far however, no such solution has been found. As will be reviewed, attempts in this direction are plagued by many no-go theorems, or by the difficulty for concrete 10d supergravity solutions to fit in the classical string regime. This situation agrees with recent de Sitter swampland conjectures. As will be shown, the latter can actually be verified quantitatively, with a surprisingly good agreement. This may hint at a deeper reason against classical de Sitter background, even though not all possibilities have for now been excluded.
First Talk
Title: Analytic conifold periods for small superpotentials
Abstract: Many properties of string vacua depend on the underlying Calabi-Yau(CY) geometry. In this talk we give an analytic method to compute the CY periods close to conifold loci. After a short review of the existing methods we present the computation for the case of a curve shrinking to zero size. We then comment on the necessary number theoretical tools to extend the method to shrinking divisors as well as CYs.
Second Talk
Title: Small W0 near the conifold
Abstract: Much effort has recently been directed towards understanding and questioning KKLT as the prime example of dS constructions in string theory. The starting point of KKLT is to assume one has stabilized the complex structure moduli to a small superpotential W0. The final uplift to dS requires everything to happen in a strongly warped region, i.e. near a conifold. I present a mechanism to construct explicit models with CS moduli stabilized to small W0 near the conifold, showing that such solutions are fairly abundant. I will end with some remarks about the strained relationship between the AdS Distance Conjecture and the KKLT AdS vacuum.
First Talk
Title: String Universality and Non-Simply-Connected Gauge Groups in 8d
Abstract: Utilizing the interplay between Z 1-form center symmetries and gauge transformation of higher-form fields, we present a consistency condition for 8d N=1 supergravity theories with non-trivial global structure G/Z for the non-Abelian gauge group. This identifies the majority of combinations (G, Z), which have no string theory realization, as inconsistent quantum theories when coupled to gravity. This condition is shown to be equivalent to known constraints for Mordell-Weil torsion on K3 surfaces, providing a physical explanation for gauge groups observed in F-theory compactifications.
Second Talk
Title: Proving the WGC in tree level string theory
Abstract: It has recently emerged that the Weak Gravity Conjecture (WGC) can be formulated in (at least) two different forms when massless scalars (moduli) are present. Rather than imposing constraints on the charge-to-mass ratio of states in the spectrum, the second formulation, dubbed the Repulsive Force Conjecture (RFC), relies instead on determining bounds by analyzing the long range forces between them. Nonetheless, it is clear that these conjectures are related. In the talk, I will present a derivation in the context of tree level string theory, where we show how these fit together, and determine a series of states, present in the spectrum of a generic theory, that satisfy the RFC and the WGC, thus providing further evidence that these conjectures should hold in a theory of quantum gravity.
First Talk
Title: The Calabi-Yau Landscape: Beyond the Lampposts
Abstract: I will describe recent advances in constructing Calabi-Yau (CY) hypersurfaces in toric varieties, including methods for computing key topological data such as intersection numbers, Chern classes and Gopakumar-Vafa invariants. I will introduce CYTools: a software package for constructing and analyzing CY hypersurfaces. These advances enable many applications to string compactifications. I will discuss two examples. First, studying large ensembles of CY threefolds with large Hodge numbers reveals that the Kahler cone of a generic CY hypersurface is extremely narrow. Consequently, control of the alpha prime expansion is strongly correlated with the existence of ultralight axions. Next, I will show how one can use these tools to obtain exponentially small flux superpotentials in the presence of strongly warped throats in compactifications of type IIB string theory, as required by the KKLT mechanism.
Second Talk
Title: Cosmological Constraints on the KS Axiverse
Abstract: We study multi-ALP spectra in compactifications of type IIB string theory on O3/O7 orientifolds of CY3s in an attempt to understand their cosmological consequences. Using bounds from black hole superradiance, we are able to place limits on model-building with particular string geometries.
First Talk
Title: 6d N=(1,0) anomalies on S^1 and F-theory implications
Abstract: In this talk we show that the pure gauge anomalies of 6d N = (1, 0) theories compactified on a circle are captured by field-dependent Chern-Simons terms appearing at one-loop in the 5d effective theories. These terms vanish if and only if anomalies are canceled. In order to obtain this result, it is crucial to integrate out the massive Kaluza-Klein modes in a way that preserves 6d Lorentz invariance; the often-used zeta-function regularization is not sufficient. Since such field-dependent Chern-Simons terms do not arise in the reduction of M-theory on a threefold, six-dimensional F-theory compactifications are automatically anomaly free, whenever the M/F-duality can be used. A perfect match is then found between the 5d N = 1 prepotentials of the classical M-theory reduction and one-loop circle compactification of an anomaly free theory. Finally, from this potential, we read off the quantum corrections to the gauge coupling functions.ng theory, as required by the KKLT mechanism.
Second Talk
Title: Moduli Stabilisation and the Statistics of SUSY Breaking in the Landscape
Abstract: The statistics of the supersymmetry breaking scale in the string landscape has been extensively studied in the past finding either a power-law behaviour induced by uniform distributions of F-terms or a logarithmic distribution motivated by dynamical supersymmetry breaking. We point out that the inclusion of the Kähler moduli is crucial to understand the distribution of the supersymmetry breaking scale in the landscape since in general one obtains unstable vacua when the F-terms of the dilaton and the complex structure moduli are larger than the F-terms of the Kähler moduli. After taking Kähler moduli stabilisation into account, we find that the distribution of the gravitino mass and the soft terms is power-law only in KKLT and perturbatively stabilised vacua which therefore favour high scale supersymmetry. On the other hand, LVS vacua feature a logarithmic distribution of soft terms and thus a preference for lower scales of supersymmetry breaking.
First Talk
Title: 6D SCFTs and Integrable Spin Chains
Abstract: 6D SCFTs associated to long generalized quivers have a large R-charge sector; we find evidence that operator mixing in this sector is governed by a 1D spin chain Hamiltonian with operator scaling dimensions controlled by a perturbation series in inverse powers of the R-charge. When the 6D SCFT is rank R (G, G) conformal matter we study a class of operators where the mixing is controlled by the integrable open Heisenberg XXX_s spin chain, with the spin s depending on the particular ADE-type of G. I will review the construction of such 6D SCFTs and how to build the large R-charge operators from the individual conformal matter building blocks, derive the integrable Hamiltonian capturing the operator mixing, and determine the anomalous dimensions of one class of operators.
Second Talk
Title: Conifold Vacua with Small Flux Superpotential
Abstract: We introduce a method for finding flux vacua of type IIB string theory in which the flux superpotential is exponentially small and, at the same time, one or more complex structure moduli are stabilized exponentially near to conifold points.
First Talk
Title: Weak Gravity and Dualities
Abstract: The mild form of the Weak Gravity Conjecture requires that the charge-to-mass ratio of extremal black holes is shifted to be larger than one. In 4D Einstein-Maxwell theory, much mileage is gained in understanding the effect of higher derivative terms in the effective action along with principles such as unitarity of scattering amplitudes. I will discuss this form of the WGC in the presence of a dilaton, where the usual assumptions are insufficient to demonstrate the conjecture. Adding the assumption that the four-derivative action (approximately) respects a symmetry of the two-derivative action closes this gap.
Second Talk
Title: Swampland Conjectures for Strings and Membranes
Abstract: Swampland criteria like the Weak Gravity Conjecture should not only apply to particles, but also to objects with low codimension, such as strings and membranes in 4D. However, the latter introduce large backreaction effects, making their effective descriptions highly nontrivial. In this talk, focusing on 4D N=1 theories, I will illustrate how to include fundamental strings and membranes within EFTs, showing that the induced backreaction can be regarded as a classical RG flow of their couplings. In turn, this allows for a proper definition of the WGC for strings and membranes. I will further argue that strings and membranes may be helpful tools to thread new links among the conjectures. In particular, I will discuss how the WGC for strings implies the distance conjecture and how WGC-saturating membranes generate a potential satisfying the de Sitter Conjecture.
First Talk
Title: Orders of Vanishing and U(1) Charges in F-theory
Abstract: There are many interesting questions about the landscape and swampland of F-theory models that involve massless matter charged under U(1) gauge symmetries. As such, it is important to better understand the geometric properties of F-theory models realizing various U(1) charges. We present evidence that, for F-theory models in Weierstrass form, the U(1) charge of massless matter is encoded in the orders of vanishing of the section components supporting the U(1) gauge symmetry. We propose specific equations relating the U(1) charges to the orders vanishing that seem to hold for both U(1)-charged singlets and for matter additionally charged under a simply-laced nonabelian gauge algebra. Such formulas would provide a method of determining U(1) charges without resolution. Additionally, they give geometric information about F-theory models with general U(1) charges, which may be useful for exploring the F-theory landscape and swampland. Based on upcoming work with Andrew Turner.
Second Talk
Title: Duality and axionic weak gravity
Abstract: The axionic weak gravity conjecture predicts the existence of instantons whose actions are less than their charges in appropriate units. We show that the conjecture is satisfied for the axion-dilaton-gravity system if we assume duality constraints on the higher derivative corrections in addition to positivity bounds which follow from unitarity, analyticity, and locality of UV scattering amplitudes. On the other hand, the conjecture does not follow if we assume the positivity bounds only. This presents an example where derivation of the weak gravity conjecture requires more detailed UV information than the consistency of scattering amplitudes.
First Talk
Title: Geometric Unification of Higgs Bundle Vacua - Part II
Abstract: In this talk, I will discuss an approach to relate M-theory and F-theory on Spin(7)-manifolds via Higgs bundles. We develop solution building techniques for specific bulk BPS equations of motion for local M- and F-theory models. Furthermore, the 3D system unifying the Higgs bundle data associated with 4D N=1 M- and F-theory vacua appears as an interface between different 4D vacua. Similarly, the Pantev-Wijnholt system can be viewed as defining an interpolating profile between 5D N=1 vacua, as captured by the Hitchin system. Thus, I will discuss the resulting interfaces between those supersymmetric vacua. Finally, I will give explicit examples of interpolations between BHV and Pantev-Wijnholt solutions.
Second Talk
Title: Cobordisms, anomalies, and Swampland in nine dimensions
Abstract: The oldest and arguably best established Swampland conjecture is that there are no global symmetries in gravity. It is hard to use this to rule out EFTs, since one can often say that a would-be global symmetry is just broken by some obscure UV effect. However, sometimes this breaking forces the introduction of new objects, which can have a gauge anomaly, thus forcing the theory into the Swampland. We will illustrate this in the case of 9d, 8d and 7d supersymmetric theories, where breaking of an unoriented cobordism global symmetry leads to a modulo 8 constraint on the ranks of the gauge group, which matches known string theory constructions. This establishes Coulomb branch string universality in nine and eight dimensions. We also discuss constraints on the possible non-abelian enhancements of the gauge group.
First Talk
Title: Geometric Unification of Higgs Bundle Vacua - Part I
Abstract: In this talk I will consider the 3D N=1 effective field theory obtained by taking M-theory on a local Spin(7) manifold. I will discuss in detail the system of BPS equation governing supersymmetric vacua in Spin(7) compactification. The Spin(7) system provides a unification of other BPS systems appearing in M-theory and F-theory 4D N=1 vacua and I will show how it is related to the system of 1/2-BPS equations for domain walls in such 4D N=1 theories. Using effective field theory I will argue that these configurations are better interpreted as interfaces of 4D N=1 theories.
Second Talk
Title: Pair Production and Gravity as the Weakest Force
Abstract: In this talk we will argue for an alternative formulation of the Weak Gravity Conjecture in terms of particle pair production at threshold. Imposing that the production rate by any force mediator (photon or scalar) of pairs of charged particles be larger or equal to graviton production, we recover known conditions for the U(1) WGC and its extensions. Unlike other formulations though, threshold pair production is sensitive to short range couplings present in scalar interactions and gives rise to a Scalar WGC. Application to moduli scalars gives rise to specific conditions on the trilinear and quartic couplings which involve first and second derivatives of the WGC particle mass with respect to the moduli. Some extremal solutions to these equations correspond to massive states behaving like BPS, KK and winding states which feature duality invariance and are in agreement with the Swampland distance conjecture. Conditions for N=2 BPS states saturate our bounds and we discuss specific examples of BPS states which become massless at large Kahler moduli in Type IIA N=2, D=4 CY and orbifold compactifications. We study possible implications for potentials depending on moduli only through WGC massive states.
First Talk
Title: BPS States and Extremal Black Holes at Infinite Distance
Abstract: In this talk I will consider the 3D N=1 effective field theory obtained by taking M-theory on a local Spin(7) manifold. I will discuss in detail the system of BPS equation governing supersymmetric vacua in Spin(7) compactification. The Spin(7) system provides a unification of other BPS systems appearing in M-theory and F-theory 4D N=1 vacua and I will show how it is related to the system of 1/2-BPS equations for domain walls in such 4D N=1 theories. Using effective field theory I will argue that these configurations are better interpreted as interfaces of 4D N=1 theories.
Second Talk
Title: Pair Production and Gravity as the Weakest Force
Abstract: In this talk I will present part of the results of 2005.05983 on how to use geometric tools in order to analyze 3d interfaces in 4d systems. One key role in this analysis is played by time-reversal invariance and electric-magnetic dualities for generalized Maxwell theories. These further suggest the importance of the real components of the modular curves of SL(2,Z) and its congruence subgroups and allow interesting predictions which can be tested in N = 2 supersymmetric theories.
First Talk
Title: The web of swampland conjectures and the TCC bound
Abstract: The swampland program provides criteria to identify low energy effective theories consistent with quantum gravity. However, at present most of these criteria are conjectures and depend on unspecified order one parameters. In this talk, I will test some of these conjectures in specific examples and propose lower bounds for the corresponding parameters. As a byproduct of the analysis, possible relations among conjectures are suggested.
Second Talk
Title: Non-Simply-Connected Symmetries in SUGRA & 6D SCFTs
Abstract: Using F-theory, I discuss the construction of non-simply connected gauge and flavor groups in SUGRA and 6D SCFTs using the geometry of elliptic Calabi-Yau’s. First I discuss how non-simply-connected symmetries are encoded in globally reduced SL(2,Z) monodromies of the elliptic fiber to a congruence subgroup. By using their modular curves we are able to proof strict bounds on the fundamental group of the gauge group whenever whenever the base is compact and thus coupled to gravity. Second I discuss how the same structures can be used to construct 6D SCFTs with non-simply connected Flavor groups when gravity is absent. Here we discuss the difference in the non-Higgsable clusters as well as SCFTs with the same flavor algebra but different group structures.
First Talk
Title: On stratification diagrams, algorithmic spectrum estimates and vector-like pairs in F-theory
Abstract: I will discuss recent progress in constructing global 4d F-theory models with realistic vector-like spectra. We stratify the matter curve geometries with respect to the number of vector-like pairs and discuss how we can estimate the vector-like spectra from simple topological considerations.
Second Talk
Title: New Resolutions for F-theory and Chiral Matter in Standard Model-like Constructions
Abstract: Standard Model-like F-theory compactifications on singular elliptically fibered Calabi-Yau 4-folds with flux have received a great deal of attention in the literature for their potential phenomenological applications. Motivated by these constructions, I describe a procedure combining various known computational techniques to determine physical properties of 4D F-theory vacua associated to singular hypersurface Calabi-Yau 4-folds. This procedure can be used to compute flux backgrounds of locally universal models in full generality and can be applied to resolutions at finite Kaluza-Klein radius. I present selected examples and discuss forthcoming results about the tuned [SU(3) x SU(2) x U(1)] / Z_6 constructions recently proposed by Raghuram-Taylor-Turner in 1912.10991.