Previous Talks 

CHEP Seminar


Title: Universal features of 2 → N scattering in QCD and gravity from shockwave collisions


Speaker: Raju Venugopalan (Brookhaven National Lab)


Abstract: A remarkable double copy relation of Einstein gravity to QCD in Regge asymptotics is Γμν=(1/2)CμCν−(1/2)NμNν, where Γμν is the gravitational Lipatov vertex in the 2→3 graviton scattering amplitude, Cμ its Yang-Mills counterpart, and Nμ the QED bremssstrahlung vertex. In QCD, the Lipatov vertex is a fundamental building block of the BFKL equation describing 2→N scattering of gluons at high energies. Likewise, the gravitational Lipatov vertex is a key ingredient in a 2-D effective field theory framework describing trans-Planckian 2→N graviton scattering. We construct a quantitative correspondence between a semi-classical Yang-Mills framework for radiation in gluon shockwave collisions and its counterpart in general relativity. In particular, we demonstrate the Lipatov double copy in a dilute-dilute approximation corresponding to RS,L, RS,H ≪b, with RS,L, RS,H the respective emergent Schwarzchild radii generated in shockwave collisions and b is the impact parameter. We outline extensions of the correspondence developed here to the dilute-dense computation of gravitational wave radiation in close vicinity of one of the black holes, the construction of graviton propagators in the shockwave background, and a renormalization group approach to compute 2→N amplitudes that incorporates graviton reggeization and coherent graviton multiple scattering.


Date & time: 8th February 2024, 4 pm


Venue: LH3



CHEP Seminar

Speaker: Siddharth Prabhu, TIFR Mumbai


Title: Conformality of non-conformal correlators


Abstract: Recasting the flat space S-matrix as a boundary observable naturally leads us to a study of position space correlators. We describe the analytic structure of correlators of massless fields, and provide a description of the scattering submanifold i.e the space of all insertions that scatter in the bulk. Even though these correlators are not conformal, they can be recast as conformally invariant correlators, in other words, as functions of conformal cross ratios. This provides a new way to compute flat space massless correlators exactly. We apply this method to find exact answers for some Feynman diagrams involving massless fields, including several loop examples. We also show that flat space correlators of massive fields can be expressed as infinite sums of conformal correlators.


Time:  2:30 pm, 8th  February (Thursday) 2024

Venue: Lecture Hall 3, Physical Sciences Building


CHEP Seminar

Speaker: Vinayak Raj, IIT Kanpur


Title: Islands and dynamics at the interface


Abstract: We investigate a family of models described by two holographic CFT$_2$s coupled along a shared interface. The bulk dual geometry consists of two AdS$_3$ spacetimes truncated by a shared end-of-the-world (EOW) brane. A lower-dimensional effective model comprising of JT gravity coupled to two fat CFT$_2$ baths is subsequently realized by considering small fluctuations on the EOW brane and implementing a partial dimensional reduction where the transverse fluctuations of the EOW brane are identified as the dilaton field. We compute the generalized entanglement entropy for bipartite states through the island prescription in the effective lower-dimensional picture and obtain precise agreement in the limit of large brane tension with the corresponding doubly holographic computations in the bulk geometry. Furthermore, we obtain the corresponding Page curves for the Hawking radiation in this JT braneworld.


Time:  2 pm, 7th  February (Wednesday) 2024

Venue: Lecture Hall 3, Physical Sciences Building


CHEP Seminar

Speaker: Sridip Pal, Caltech

Title: Tauberian Theorems and High Energy Modular Bootstrap


based on arXiv:2307.02587 [hep-th] with Jiaxin Qiao and arXiv:2212.04893 [hep-th] with Jiaxin Qiao and Slava Rychkov


Time:  2:30 pm, 18th  January (Thursday)

Venue: Lecture Hall 3, Physical Sciences Building

CHEP Seminar

Speaker: Akshay Yelleshpur Srikant (Oxford)


Title: Two approaches to flat space holography 


Abstract: In this talk, I will outline the basic features of two approaches to flat space holography - Celestial and Carrollian - and how they are both related to the S-Matrix. I will then discuss correlation functions, their singularities and symmetries. 


Date: 5th January, 2024

Time: 2 pm

Venue: LH3


CHEP Seminar

Speaker: Jeevan Chandra Namburi, Cornell University


Title: On ETH and microstate averaging in quantum gravity


Abstract: In the talk, I shall describe the construction of black hole solutions in AdS$_{d+1}$ sourced by spherically symmetric thin shells of pressureless dust from which one can extract a universal function governing the statistics of microstate dynamics. This function determines the partition functions of the multi-boundary Euclidean wormhole geometries constructed by branching around the time-symmetric apparent horizon of these black holes, and in turn these wormholes help describe a replica formalism to coarse grain the black hole microstates. I shall then construct static star solutions in AdS$_{d+1}$ using thin shells with positive surface pressure and use these solutions to construct new single-boundary wormhole solutions which can estimate global charge violating amplitudes in quantum gravity. Finally, I shall show that the partition functions of multi-boundary wormholes constructed from stars are also consistent with the prediction from averaging black hole microstates. These results illustrate the universality of ETH-like statistics in quantum gravity.


Time:  11 am, 4th  January (Thursday) 2024.

Venue: Lecture Hall 3, Physical Sciences Building


CHEP SEMINAR

Speaker: Aditya Hebbar (Ecole Polytechnique, CPHT)  


Title: Constraining Glueball Couplings


Date and Time: at 3 pm on 3rd January, 2024


Abstract: We set up a numerical S-matrix bootstrap problem to rigorously constrain bound state couplings given by the residues of poles in elastic amplitudes. We extract upper bounds on these couplings that follow purely from unitarity, crossing symmetry, and the Roy equations within their proven domain of validity. First we consider amplitudes with a single spin 0 or spin 2 bound state, both with or without a self-coupling. Subsequently we investigate amplitudes with the spectrum of bound states corresponding to the estimated glueball masses of pure SU(3) Yang-Mills. In the latter case the 'glue-hedron', the space of allowed couplings, provides a first-principles constraint for future lattice estimates.


CHEP SEMINAR

Speaker: Shailesh Lal, Beijing Institute of Mathematical Sciences and Applications


Title: Neural Networks as Ansätze: Applications to Quantum Integrability


Abstract: We develop a novel neural network architecture, that learns solutions to the Yang Baxter equation for R matrices of difference form. This method already enables us to learn all solution classes of the 2d Yang Baxter equation. We propose and test paradigms for exploring the landscape of Yang Baxter equation solution space aided by these methods. Further, we shall also comment on the application of these methods to generating new solutions of the Yang Baxter equation. The talk is based on joint work with Suvajit Majumder and Evgeny Sobko available in part in arXiv:2304.07247.


Time: 3:30 pm, 19th  December (Tuesday) 2023

Venue: Lecture Hall 3, Physical Sciences Building

CHEP SEMINAR

Speaker: Manish Ram Chander, IMSc Chennai


Title: Theory dependence of black hole interior reconstruction


Abstract: An AdS eternal black hole in equilibrium with a finite temperature bath presents a Hawking-like information paradox due to a continuous exchange of radiation with the bath. The non-perturbative gravitational effect, the replica wormhole, cures this paradox by introducing a non-trivial entanglement wedge for the bath after Page time. In this talk, I will discuss the theory dependence of this non-perturbative effect by randomising the boundary conditions of some of the bulk matter fields in a model of JT gravity. Using the island formula and the extended strong subadditivity due to Carlen and Lieb, I will show that at late times the black hole interior is contained inside the entanglement wedge of a reference Hilbert space that encodes the information about the random boundary conditions. Consequently, the reconstruction of the black hole interior from the radiation, in particular the region near the singularity, requires a detailed knowledge of the theory.


Time: 4 pm, 14th  November (Tuesday) 2023

Venue: Lecture Hall 3, Physical Sciences Building


CHEP SEMINAR

Speaker: Nishant Gupta, IMSc, Chennai


Title: All chiral W-algebra extensions of so(2,3).

Date, time & venue:11th October (tomorrow) 2023 at 4pm in LH3.


Abstract: We show that there are four chiral W-algebra extensions of so(2,3) algebra and construct them explicitly. We do this by a simple identification of each of the inequivalent embeddings of a copy of sl(2,R) in the so(2,3) algebra. Then, using the standard 2D chiral CFT techniques we find the corresponding W-algebra extensions. Two of the four W-algebra are new, one of which may be thought of as the conformal bms3 algebra valid for finite values of its central charge, and the İnönü Wigner contraction of the other chiral W-algebra is a sector in celestial CFT that provides the holographic description of tree-level MHV graviton amplitudes. We then show how one obtains the latter chiral W-algebra as the asymptotic symmetry algebra of 3D conformal gravity and possibly of AdS4 gravity.


CHEP SEMINAR

Speaker: Narasimha Reddy, University of Lethbridge


Title: Non-Abelian Gauge Fields and Gravitational Waves 

Abstract: Gravitational waves (GWs) provide a new window to observe the universe. Detecting GWs requires an understanding of the interaction of GWs with the matter. In particular, we want to understand the role of primordial gravitational waves in the early universe cosmological processes like QCD Phase Transition. As a first step, we discuss the interaction of gravitational waves with SU(2) Yang-Mills waves in different backgrounds. We also discuss the interaction of GWs with the symmetry-broken phase of gauge fields. We also discuss the GW effect on condensates and quark-gluon plasma fluctuations. 


Date & time: 11th October, 2023 at 7pm


Venue: Online.

CHEP SEMINAR


Speaker: Pratik Nandy, Yukawa Institute for Theoretical Physics, Kyoto


Title: Recent progress on Krylov complexity


Abstract: The Hamiltonian evolution of a quantum system can cause a simple operator to become a complicated operator. This process reflects the scrambling of quantum information in the system. We probe such operator growth by Krylov complexity, quantifying the difficulty of simulating the operator evolution using a Krylov space method. We review the current progress and challenges of applying this approach to closed and open systems and illustrate some examples from the SYK model to quantum field theories.


Date and time: 10th October (tomorrow) 2023 at 3pm in LH3.


CHEP SEMINAR

Speaker: Pavan Dharanipragada, IMSc Chennai.


Title: Constructing a local AdS holographic dual from the ERG of a CFT


Date, Time & Venue: 3rd October 2023, at 4 pm in LH-3.


Abstract: The extra dimension in AdS/CFT, which is the radial direction in the bulk has the interpretation of the scale of the boundary theory. The programme of interpreting the bulk radial equations of motion as the boundary RG equations is called Holographic RG. I will present our work which does not assume the AdS/CFT correspondence, and begins with the boundary Wilsonian action, to obtain the bulk action from the exact RG of the boundary. I begin with the boundary theory, which is the free O(N) model in 3 dimensions, the AdS dual of which is the Vasilier higher spin theory in 4 dimensions. Deforming this theory with the scalar, vector current, and the energy momentum tensor, triggers an RG evolution. From the Polchinski ERG equation of this action, an evolution operator can be written and reintrepreted as a 4 dimensional functional integral. It becomes necessary to work a ``flipped" version of this ERG equation in order to make contact with AdS-CFT. I will describe the field redefinition that maps the action in the functional integral obtained to the AdS theory that is local at quadratic level. Then I will show how a local graviton scalar scalar interaction in the bulk can be obtained by suitable approximation.



CHEP Seminar

Speaker: Hemant Rathi, IIT-Roorkee


Title: $AdS_2/CFT_1$ holography at finite charge density


Date and Venue: 30th August 2023 at 3pm,  LH3.


Abstract:

I will briefly discuss $AdS_2/CFT_1$ holography, also known as JT/SYK duality, and explore various generalizations of JT gravity involving $U(1)$ gauge fields and $SU(2)$ Yang-Mills interactions. In particular, we will investigate the effects of non-trivial gauge couplings on the thermal properties of black holes/wormholes and examine the possibilities of the Hawking-Page transition and wormhole to black hole phase transition in two dimensions. Additionally, we will examine the transformation properties of the boundary stress-energy tensor under diffeomorphism and U(1) gauge transformation, thereby computing the central charge associated with the 1D boundary theory.




CHEP Seminar

Title : Marginal deformations of N = 2 SCFTs and Graviton spectrum

 

Speaker : Sourav Roychowdhury, Indian Association for the Cultivation of Science (IACS), Kolkata, India.


Date and Time: 24th August 2023 at 4pm 


Venue: LH3


Abstract : In this talk I will discuss the holographic dual of N = 2 SCFTs along with its marginal deformation. In particular I will show that due to the presence of the deformation factor, we yield a continuous graviton spectrum in deformed background. I will make comments on possible dual gauge theory operators corresponds to these modes.


The talk is based on the following paper:

S. Roychowdhury and D. Roychowdhury, “Spin 2 spectrum for marginal deformations of 4d N = 2 SCFTs,”

JHEP 03, 083 (2023), arXiv: 2301.12757 .

CHEP Seminar

Speaker: Jnanadeva Maharana, IOP Bhubaneshwar

 

Title: IS THE SCATTERING AMPLITUDE ANALYTIC IN A FIELD THEORY WITH A COMPACT SPATIAL COORDINATE?

 

Abstract: 

We consider a massive scalar field in five dimensional spacetime and then compactify one spatial dimension on a circle. In the context of potential scattering, Khuri considered a case when one spatial coordinate is compactified. He showed that, using Green function technique, the forward amplitude violates dispersion relation. If that will be true for QFT the consequences are serious. We show for above mentioned QFT that forward dispersion relation is safe. We also prove nonforward dispersion 

relation in compactified QFT.

 

Time: 3:30 pm, 10th  August (Thursday) 2023

Venue: Lecture Hall 3, New Physical Sciences Building


CHEP Seminar

Speaker: Ruchira Mishra, University of Chicago


Title: Applied nonrelativistic conformal field theory: scattering-length and effective-range corrections to nuclear physics


Abstract: In a range of energy, neutrons are described by the nonrelativistic conformal field theory of unitarity fermions, perturbed by one relevant and an infinite number of irrelevant operators.  We develop a formalism which provides a definition of local operators in that nonrelativistic conformal field theory.  We compute the scattering-length and effective-range corrections to the two-point functions of primary charge-3 operators.  These calculations allow us to find the first corrections to the scale-invariant behaviours of the rate of nuclear reactions with three neutrons in the final state in the regime when the neutrons have small relative momenta.


Time: 4 pm, 25th  July 2023 (Tuesday)

Venue: E1-14, New Meeting Room


CHEP Seminar

Speaker: Sayantani Bhattacharya, NISER Bhubaneswar.


Title: The zeroth law of black hole thermodynamics in arbitrary higher derivative theories of gravity


Date and Time: 16th June 2023 at 2:30 pm.


Venue: LH3



Abstract:  

We consider diffeomorphism invariant theories of gravity with arbitrary higher derivative terms in the Lagrangian as corrections to the leading two derivative theory of Einstein’s general relativity. We construct a proof of the zeroth law of black hole thermodynamics in such theories. We assume that a stationary black hole solution in an arbitrary higher derivative theory can be obtained by starting with the corresponding stationary solution in general relativity and correcting it order by order in a perturbative expansion in the coupling constants of the higher derivative Lagrangian. We prove that surface gravity remains constant on its horizon when computed for such stationary black holes, which is the zeroth law. We argue that the constancy of surface gravity on the horizon is related to specific components of the equations of motion in such theories. We further use a specific boost symmetry of the near horizon space-time of the stationary black hole to constrain the off-shell structure of the equations of motion. Our proof for the zeroth law is valid up to arbitrary order in the expansion in the higher derivative couplings.


CHEP Seminar

Speaker: Sachin Jain, IISER Pune


Title: Bulk Locality of Higher Spin theories, a CFT perspective


Abstract: It has been recently pointed out that HS theories are not local from bulk perspective. Our aim would be to explore possibility to make bulk theory local or find a subsector local by breaking HS symmetry weakly. In this discussion Momentum space CFT will play key role. I'll  briefy review recent progress made on 3d CFT in momentum space.


Time: 3 pm, 9th  May (Tuesday) 2023.

Venue: Lecture Hall 3, New Physical Sciences Building

CHEP Seminar 

Speaker: Abhiram Kidambi, Kavli IPMU, Tokyo University


Title: Gravitational Path Integrals in N = 4 string theory


Abstract: Using the microscopics (CFT) calculation of BPS BH entropy in N = 4 string theory, we improve on the localization techniques of the quantum entropy function. 

We find that the result involves a sum over Euclidean backgrounds including orbifolds of the Euclidean attractor geometry. We further show how a rewriting of the degeneracy formula is amenable, at a semi-classical level, to a gravitational interpretation involving 2D Euclidean wormholes.


Time: 2:30pm, 2nd May 2023. 

Venue: LH3.


CHEP Seminar

Speaker: Surbhi Khetrapal, University of Hyderabad.

Title: Quantum chaos in low dimensional quantum systems

Date and Time: 19th April 2023 at 2:30 pm.

Venue: LH-3.

Abstract: In this talk we will look at quantum chaos in two types of quantum systems: 1) A system of bosons in a Harmonic trap with weak contact interaction: in this case, the existence of quantum chaos is characterised by Wigner-Dyson distribution in the level-spacing statistics. 2) Conformal field theory (CFT) in two dimensions at large central charge, where quantum chaos is characterised by the out-of-time-ordered correlator (OTOC). (a) First, we will look at a computation of the OTOC in a CFT with unequal temperatures for left- and right- moving modes dual to a rotating black-hole. We find that the OTOC exhibits periodic oscillations about an average Lyapunov growth. We also study the OTOC in the extremal limit of the dual black-hole, and find that there are short periods of exponential growth in this largely integrable system. (b) Secondly, we compute the OTOC in a zero temperature 2d CFT under evolution by a certain combination of Virasoro generators (L_{+1}+L_{-1}), usually encountered in the study of inhomogeneous quenches. A bound was proposed on the growth of the OTOC set by the operator growth (i.e. rate at which an operator becomes more complex under evolution). In this theory, we find that the OTOC saturates this bound. We explain the bound saturation by expressing the Hamiltonian as the modular Hamiltonian of CFT with half-space traced out.

CHEP Seminar

Speaker: Onkar Parrikar, TIFR Mumbai. 


Title: Canonical Purification, Bulk reconstruction and the Quantum extremal shock


Date and Time​: 24th March,2023 at 2:30 pm.


Venue:​ LH3.


Abstract: We will discuss the canonical purification (with respect to one of the parties) of pure, bi-partite states obtained by turning on sources in the Euclidean path integral. In holographic conformal field theories, the Lorentzian bulk dual of the canonical purification consists of the corresponding entanglement wedge glued to its CPT image at the quantum extremal surface. However, the mismatch in the classical expansions at the QES due to quantum corrections needs to be supported by a shock in the bulk matter stress tensor in order for the bulk to satisfy Einstein's equations. Working perturbatively to first order in double-trace sources around the thermofield double state, we will demonstrate that the state of the bulk matter in the dual to the canonically purified boundary CFT state precisely has this quantum extremal shock in the bulk stress tensor. Along the way, we will discuss applications of these results to entanglement wedge reconstruction beyond HKLL. 


CHEP Seminar (Online)


Title: Quantum complexity and bulk timelike singularities


Speaker: Gaurav Katoch, IIT Hyderabad.


Date and Time: 13th March, Monday at 2.30 pm.


Abstract: In this talk, I will discuss the possibility of using holographic complexity as an alternative tool to the Gubser criterion in diagnosing bulk timelike singularities. Gubser criterion allows those naked timelike singularities which arise in the extremal limits of geometries containing cloaked singularities. I will present three examples we studied that hinted at the viability of action complexity as a reliable probe in the investigation of timelike singularities.  We propose that if the holographic (action) complexity of the quantum states dual to the bulk geometry containing naked timelike singularities is less than that of empty AdS, then that singularity cannot arise in the semiclassical limit of a UV-complete theory of quantum gravity.


YouTube Link: https://youtu.be/M6BaffgorUc

CHEP Seminar

Speaker: Pratik Rath, University of California, Santa Barbara.


Title: Multipartite entanglement in Holography and Tensor Networks


Date and Time: 9th March 2023, at 2.30 pm.


Venue: Lecture Hall 3, New Physical Sciences Building.


Abstract: In this talk, I will discuss various measures of multipartite entanglement such as the entanglement negativity and reflected entropy. I will use random tensor networks as a toy model for the replica trick, and apply lessons learnt from it to holographic systems. This will teach us about replica symmetry breaking and the failure of bit threads in capturing tripartite entanglement.

CHEP Seminar

Speaker: Tanay Milind Kibe, IIT Madras

Title: Encoding quantum information into black holes.

Date and Time:  17th February 2023, 4:00 pm

Venue: Online on Teams.

Abstract: Black holes past their Page time are extremely intriguing objects that display interesting information processing properties. Information thrown into such black holes after Page time is rapidly (after scrambling time) revealed into the Hawking radiation, whereas the information about the interior takes a long time to be revealed. Hayden and Harlow have argued that the time scale to decode the information about the interior from the radiation is extremely large compared to the evaporation time scale of the black hole, thus avoiding many paradoxes. Motivated to understand such features we study simple quantum systems coupled to an asymptotically AdS2 black hole and show how the initial state of the quantum system is encoded into the semi-classical black hole. These results can be applied to a class of black hole microstate models to understand some of the information processing properties of black holes such as information mirroring.

YouTube link: https://youtu.be/XyHkSCQnF9s

CHEP Seminar

SpeakerAradhita Chattopadhyaya ( Dublin Institute for Advanced Studies )


Title:  Numerical experiments on coefficients of instanton partition functions


Date and Time:  15th February 2023,  4:00 pm

 

Venue:  Lecture Hall 3, New Physical Sciences Building.


Abstract:   We analyze the coefficients of partition functions of Vafa-Witten theory for the complex projective plane ℂℙ2. We experimentally study the growth of the coefficients for gauge group SU(2) and SU(3), which are examples of mock modular forms of depth 1 and 2 respectively. We also introduce the notion of ``mock cusp form'' and study an example of weight 3 related to the SU(3) partition function.  Numerical experiments on the first 200 coefficients suggest that the coefficients of a mock modular form of weight k grow as the coefficients of a modular form of weight k, that is to say as 

nk−1. On the other hand, the coefficients of the mock cusp form appear to grow as n3/2, which exceeds the growth of classical cusp forms of weight 3. We provide bounds using saddle point analysis, which however largely exceed the experimental observation.

Faculty Seminar

Speaker: Prof. Chethan Krishnan,  CHEP,  IISc  Bangalore.

 

Title: Fuzzballs and Random Matrices 

 

Date and Time:  15th Feb 2023,  Wednesday 2:30 PM

 

Venue : LH-3

 

Abstract:

The fuzzball proposal is a controversial idea in string theory that claims that the true nature of black holes is that spacetime "stops" at the horizon. It has some encouraging features, but also some discouraging ones. One of the discouraging features is that (it is generally believed that) the fuzzball paradigm cannot realize the expectation that black holes are quantum chaotic systems, highly efficient at scrambling information. In order to satisfy this expectation, fuzzballs will have to have the spectral features of a random matrix, which is supposed to be challenging. In this talk, I will discuss an extremely simple calculation that suggests that this expectation is likely wrong, and that the fuzzball paradigm almost certainly can incorporate the key features of random matrix spectra. The calculation also suggests interesting new ideas about random matrices and the nature of their spectra.

CHEP Seminar

Speaker: Arnab Rudra, IISER Bhopal.


Title: On-shell Supersymmetry and higher-spin amplitudes


Date and Time: 13th February 2023 at 4 p.m.

 

Venue: Lecture Hall 3, New Physical Science Building. 


Abstract: We investigate the constraint from supersymmetry on the interaction of higher spin particles. We use on-shell Supersymmetry to constrain the three-point function of two massless particles and one massive particle in 3+1 dimensions. We use this framework to write down the tree-level four-point function of massless particles for theories with 4, 8 and 16 supercharges. In particular, we derive the expressions for four-photon/gluon amplitudes with a massive higher spin exchange in theories with N=4 Supersymmetry in 3+1 dimensions. If time permits, we will mention the extension of this story to higher dimensions.  

 

Reference: The talk is primarily based on 2209.06446 and the references mentioned in that preprint. 

CHEP Seminar

Speaker: Gautam Mandal, DTP, TIFR Mumbai.

1st Talk:


Title: Black hole evaporation, nonlinear noise and Thermalization in SYK


Date and Time: 9th February 2023 at 3.30 pm (Time changed)


Venue: Lecture Hall 3, New Physical Science Building.


Abstract: We describe a model of evolving pure states in an SYK model coupled to a bath, where the coupling is nonlinear. Once the bath is integrated out, the effective SYK model has non-Markovian evolution. The system shows some unconventional thermalization. The AdS dual provides an exact microscopic model of Black hole evaporation.  


2nd Talk:

Title: Target Space Entanglement


Date and Time: 10th February 2023 at 11.00 am (Please note the unusual timing).


Venue:  Lecture Hall 3, New Physical Science Building.


Abstract: Motivated by the Bekenstein Hawking formula and the area law behaviour of entanglement entropy, we propose that in any UV finite theory of quantum gravity with a smooth spacetime, the total entropy for a pure state in a co-dimension one spatial region, to leading order, is given by S = A/4G_N, where A is the area of the co-dimension two boundary.

CHEP Seminar

Title: Dispersion Relations:  From Classical Optics to String Theory


Speaker:  N.D. Hari Dass, Retd. Senior Professor, IMSc


Date and Time:  8th February 2023, 4:00 pm


Venue:  Lecture Hall 3, New Physical Sciences Building.


Abstract: I shall give a pedalogical narration of how a simple, but intriguing relation about colors impacted the most modern developments in physics, even to the point of anticipating String Theory. The strong thread that held these pearls of scientific creativity was the powerful mathematical idea of analyticity, which in this physical context turned out, rather surprisingly,  to be a consequence of the deeply cherished physical principle of Causality.


The talk will be at a level accessible to a wide audience.

Math-Physics Journal Club(CHEP) Talk

Title: Supersymmetric black holes and T\bar{T} deformation


Speaker: Swapnamay Mondal, Trinity College, Dublin


Date and Time: 3rd  February, 4:00 pm

 

Venue: Lecture Hall 3, New Physical Sciences Building.


Abstract:

The entropy of supersymmetric black holes in string theory compactifications can be related to that of a D- or M-brane system, which in many cases can be further reduced to a two-dimensional conformal field theory (2d CFT). For black holes in M-theory, this relation involves a decoupling limit where the black hole mass diverges. We suggest that moving away from this limit corresponds to a specific irrelevant perturbation of the 2d CFT, namely the supersymmetric completion of the T\bar{T} deformation. We demonstrate that the black hole mass matches precisely with the T \bar{T} deformed energy levels, upon identifying the T \bar{T} deformation parameter with the inverse of the leading term of the black hole mass. We discuss implications of this novel realization of the T \bar{T} deformation, including a Hagedorn temperature for wrapped M5-branes.


CHEP Seminar


Title:  ZZ instanton amplitudes in minimal string theory


Speaker:  Raghu Mahajan,  Stanford University.


Date and Time:   1st February 2023,  at 4 p.m.


Venue:   Lecture Hall 3,  New Physical Sciences Building.


Abstract: We use insights from string field theory to analyze and cure the divergences in the cylinder diagram in minimal string theory, with both boundaries lying on a ZZ brane. Minimal string theory refers to the theory of two-dimensional gravity coupled to a minimal model CFT that serves as the matter sector; it includes JT gravity as a limiting case. ZZ branes are akin to D-instantons, and give rise to features that reflect the underlying discreteness of the dual theory. The exponential of the cylinder diagram represents the one-loop determinant around the instanton saddle. The finite result for this one-loop constant computed using the string field theory procedure agrees precisely with independent calculations in the dual double-scaled matrix integrals performed by several authors many years ago.



Special Physics Colloquium 

Title: Optical Stochastic Cooling of Electrons: Maxwell's Demon Goes 

Speaker: Prof. Swapan Chattopadhyay(Infosys Chair Visiting Professor, IISc)

Date: 14th October 2022.

Time:  4.00 PM 

Venue: Physics Auditorium 

 

Abstract : ‘Stochastic Phase Cooling’’ of charged particles in particle colliders, historically by using Microwaves in the GHz frequency range, has led to ground-breaking discoveries in the past, such as the discovery of the W and Z Bosons at CERN in 1983 and the ‘top’ quark at Fermilab years later. Stochastic Cooling reduces the random motion of the beam particles through granular sampling and correction of the beam’s phase-space structure, thus resembling a ‘Maxwell’s demon’. The extension of Stochastic Cooling from the microwave regime to optical frequencies and bandwidths can increase the achievable cooling rates by three to four orders of magnitude. I will report on the recent first ever experimental observation and achievement of ‘‘Optical Stochastic Cooling’’ in the IOTA storage ring by a Fermilab team [Nature volume 608, pages 287–292 (August 11, 2022)]. The method has direct applications towards cooling of exotic unstable particles like Muons for a possible future muon collider and fundamental studies of “quantum entanglement” of “electric charge” and “virtual quanta" in an otherwise benign electron-photon Feynman vertex.




Title: Searches for supersymmetry, leptoquarks and muon high-level trigger at CMS

Speaker: Dr. Bibhuprasad Mahakud (CMS experiment, Purdue University, USA)

Time and Date: 2:30 p.m. on 29th Jan 2020 (Wednesday)

Venue: Multimedia Room, New Physical Sciences Building


Abstract:

Large Hadron Collider (LHC) at CERN is one of the finest human endeavour to understand the physics of the standard model (SM) and beyond. Despite being phenomenally successful, SM has several drawbacks: it does not explain dark matter, the stability of Higgs boson mass etc. In this context, the talk will summarize my work on  searches for supersymmetry in multijet final states,  leptoquarks in electron final states, some pileup mitigation techniques and muon high-level trigger (HLT). The muon HLT at Compact Muon Solenoid (CMS) experiment filters uninteresting  data from proton-proton collision using advanced algorithms implemented in software. Besides showing the results,  I will also discuss some general statistical techniques with reference to the above analyses. All the searches use the data collected by CMS experiment at a proton-proton centre of mass energy of 13 TeV.


Title: Feynman Integral: From Integration-By-Parts reduction to Intersection Theory

Speaker: Dr. Manoj Kumar Mandal (University of Padova) 

Date and Time:  2.00 p.m. (Thursday) January 23, 2020

Venue: D1-06, New Physical Sciences Building


Abstract: 

Scattering amplitudes encode crucial information about collision phenomena in our universe, from the smallest to the largest scales. Evaluation of multi-loop Feynman integrals are an integral part of the determination of these scattering amplitudes and related quantities. The Feynman integrals obey linear relations, which are exploited by employing the standard Integration-By-parts identities to simplify the evaluation of scattering amplitudes: they can be used both for decomposing the scattering amplitudes in terms of a basis of functions, referred to as master integrals (MIs), and for the evaluation of the latter using the differential equation. I will show that they are better understood using the Intersection Numbers, which act as scalar products between the vector spaces of the Feynman Integral. Application to few Feynman integrals at one- and two-loops will be shown, thereby sketching the first step towards potential applications to generic multi-loop integrals.



Title: Upgrade of the CMS Drift Tube muon detector system and associated activities

Speaker: Dr. Saranya Ghosh (CMS experiment, RWTH Aachen University, Germany)

Time and Date: 3.00 p.m. on 20th Jan 2020 (Monday)

Venue: Multimedia Room, New Physical Sciences Building


Abstract: 

Drift Tubes (DT) chambers make up the muon detector system in the central region of the Compact Muon Solenoid (CMS) experiment at the CERN Large Hadron Collider (LHC). The LHC is planned to be upgraded to the High Luminosity LHC (HL-LHC) after 2025, and the electronics for the DT system is to be upgraded to deal with the higher rates expected in the new environment of the HL-LHC. Prototypes of the upgraded electronics system are already being tested during the second long shutdown period of the LHC, between 2019 and 2020. The details of the CMS DT system and its upgrade will be discussed in this presentation, with a special focus on the calibration of the DT system.









​Title: Deriving the AdS_3/CFT_2 correspondence

     Speaker: Rajesh Gopakumar (ICTS)

Venue: LH 3 New physics building, 2.30pm, 19th December


    Abstract:

It was recently argued that string theory on AdS3 × S3 × T4 with one unit (k = 1) of NS-NS flux is exactly dual to the symmetric orbifold CFT Sym^N(T4). In this paper we show how to directly relate the n-point correlators of the two sides to one another. In particular, we argue that the correlators of the world-sheet theory are delta-function-localised in string moduli space to those configurations that allow for a holomorphic covering map of the S2 -boundary of AdS3 by the world-sheet. This striking feature can be seen both from a careful Ward identity analysis, as well as from semi-classically exact AdS3 solutions that are pinned to the boundary. The world-sheet correlators therefore have exactly the same structure as in the Lunin-Mathur construction of symmetric orbifold CFT correlators in terms of a covering surface — which now gets identified with the world-sheet. Together with earlier results this essentially demonstrates how the k = 1 AdS3 string theory becomes equivalent to the spacetime orbifold CFT in the genus expansion.

     

Speaker : Tathagata Ghosh

Date and time : 17/12/2019(Tuesday), 3:00pm

Venue: LH3, New Physical Sciences building

Title: Lepton Number Charged Scalar at the LHC


Abstract:

In this talk, I'll discuss the neutrino non-standard interaction induced by leptonic scalars, $\phi$, which are SM gauge-singlets, and carry two units of lepton-number-charge. These leptonic scalars are forbidden from interacting with the Standard Model (SM) fermions at the renormalizable level and if one allows for higher-dimensional operators, couple predominantly to SM neutrinos. For masses at or below the electroweak scale, $\phi$ decays exclusively into neutrinos. Its unique production signature at hadron collider experiments like the LHC would be via the vector boson fusion process and lead to same-sign dileptons, two forward jets in opposite hemispheres, and missing transverse energy. I'll show that the sensitivity of high-energy colliders is largely complementary to that of low-energy and precision measurements of the decays of charged leptons, charged mesons, W and Z bosons, neutrino beam experiments like MINOS, searches for light dark matter in NA64 and searches for neutrino self-interactions at IceCube and in cosmological observations. For $\phi$ mass larger than a few GeV, our projected LHC sensitivity would surpass all existing bounds.

Talk slides can be downloaded from here


Speaker: Shubham Maheshwari (Groningen)

Date and time: 17th December, 11 AM

Location: LH3, New Physical Sciences Building

Title -  Perturbations in higher derivative gravity beyond maximally symmetric spacetimes


Abstract -

I will introduce non-local gravity which avoid ghosts despite the presence of higher derivatives. Such theories may avoid the usual pathologies of gravity because they contain an infinite number of derivatives. But the question of well-behavedness of perturbations around specific backgrounds, needs to still be addressed. For maximally symmetric spacetimes, this was done before. We look into perturbations of such theories around certain non-maximally symmetric backgrounds, and show that indeed there exists theories of this type with no ghosts. 


Reference: arXiv:1905.03227


Speaker: Abhishek Mohapatra

Date and time: 16th December, 2019, Friday, 3 p.m.

Venue: LH3, New Physical Sciences building

Title:  Double Heavy baryons and Corrections to Heavy Quark- Diquark Symmetry


Abstract:

Doubly heavy baryons (QQq) and singly heavy antimesons $( \bar{Q} q)$ are related by the heavy quark-diquark (HQDQ) symmetry because in the heavy quark limit, the light degrees of freedom in both the hadrons are expected to be in identical configurations. Hyperfine splittings of the ground states in both systems are nonvanishing at ${\cal O}(1 / m_Q)$ in the heavy quark mass expansion and HQDQ symmetry relates the hyperfine splittings in the two sectors. In this talk, I will point out the existence of both perturbative and nonperturbative corrections to leading hyperfine splitting from HQDQ symmetry. The perturbative correction scales in powers of $\alpha_S$ and nonperturbative correction scales in powers of $\Lambda_QCD/m_Q$.   In the extreme heavy quark limit in which the potential between the quarks in the diquark is Coulombic, the perturbative correction to the hyperfine splittings is only a few percents or smaller for values of $\alpha_S$  relevant to doubly charm and doubly bottom systems.  We also argue that nonperturbative corrections to the prediction for the hyperfine splittings are suppressed by $(Λ_QCD/m_Q)^2$ which leads to hyperfine splitting corrections of order 10% in the charm sector and smaller in heavier systems. Eventually, I will compare my results to the lattice  calculations for hyperfine splittings.


Speaker: Shankha Banerjee.

Date and time: 13th December 2019, Friday, 2:30 p.m.

Venue: LH3, New Physical Sciences building.

Title: Constraining the Higgs-gauge couplings at the HL-LHC


Abstract:

In this talk, I will focus on the measurements of the Higgs couplings to the electroweak bosons, in the context of an effective field theory. I will also discuss the possibility of strongly constraining the couplings affecting the charged triple gauge boson vertices upon studying the Zh and Wh channels in the boosted Higgs regime. I will show the potential of the High-luminosity run of the LHC, to constrain such couplings to stronger degrees than LEP had constrained earlier. Finally, I will discuss the prospects of disentangling the various tensor structures in the hZZ/hWW vertices upon considering the full analytical structure of the Zh/Wh production and using the full angular information to resurrect the interference terms.

Talk slides can be downloaded from here


Pedagogical Lecture Series on Conformal Bootstrap


Kausik Ghosh, CHEP

Venue: LH-3, New Physical Sciences Building


3rd Dec    Tuesday (2:30-4.00 pm)

Basics of CFT and the bootstrap formulation in position space.


4th Dec    Wednesday (11:00 am-12.30 pm)

Mellin space approach to CFT bootstrap


5th Dec    Thursday (2:30-4.00 pm)

Mellin Bootstrap in 1d, comments on other modern developments and open problems.


Special CHEP Colloquium

==============================


Title:  NMR simulation of topological phases

Date: 20/11/2019, Wednesday 

Time: 4.00 pm

Venue: Auditorium, New Physical Science building

Speaker: Prof Ling-Yan Hung (Fudan University)


Abstract:

We will talk about recent progress in NMR technologies simulating topological phases. NMR simulators are the prototypes of quantum computers. Its high fidelity and long coherent times have allowed the class of simulators to be the first to demonstrate the implementation of quantum algorithms such as the Shor algorithm for factorization.  

 We will describe how states are prepared, how they are evolved in time and various tricks that we can play with it, including measurements of topological properties such as modular matrices, and thus potentially applied to identifying phases of matter in future simulations.


References: Z Luo, J Li, Z Li, LY Hung, Y Wan, X Peng, J Du

Nature Physics 14 (2), 160

K Li, Y Wan, LY Hung, T Lan, G Long, D Lu, B Zeng, R Laflamme

Physical review letters 118 (8), 080502



Title: psi(2S) enhancement at high pT: An indication of QGP formation in p-Pb collision at LHC.

Speaker:  S. Ganesh

Date and time: 11/11/2019, 3:00pm (Monday)

Venue: Lecture Hall 3


Abstract:

Quark-Gluon Plasma (QGP) is a state of matter speculated to exist after the Big Bang, and reproduced at the LHC and RHIC. While, Pb-Pb collisions at LHC does produce QGP, uncertainty exists over the production of QGP in p-Pb collisions. Psi(2S) enhancement at high pT is proposed as a novel signature, which if found can indicate that QGP is indeed formed in p-Pb collisions at the LHC.

Talk slides can be downloaded from here


Title : Discovery prospects with jets at LHC

Speaker: Dr. Debarati Roy (ATLAS experiment, University of the Witwatersrand, Johannesburg)

Time and Date:  3.00 p.m. on 6th November 2019 (Wednesday)

Venue: Lecture Hall 3, New Physical Sciences Building


Abstract: 

Jets are collimated bunches of hadrons, originating from quarks and gluons. They are produced in high energy proton-proton collisions at the Large Hadron Collider (LHC). It has direct manifestations to study different aspects of QCD and thus provide useful inputs to improve Monte Carlo model predictions in order to achieve precise measurements for Standard Model processes. LHC is a jet factory and thus either jets are the most dominating background in almost all new particle searches or it itself can act as a proxy of a new particle decaying hadronically. The higher is the energy of the LHC the more collimated is the hadronic decay products, resulting in the formation of a large radius jet. The internal structure of this jet is pretty much different from the structure of a QCD jet. Therefore this property is extensively utilized for signal background discrimination for a new particle search. Jet study is a wide ranging, a very rapidly developing field in LHC, widening the scope of its discovery potential at every new energy regime LHC runs. In this presentation, I will talk about some distinct features of jets, some recent jet measurements and jet related search where I have a significant contribution.

Talk slides can be downloaded from here


PHYSICS COLLOQUIUM

   ----------------------------------------------------------------

          Speaker: Prof. Jayant Murthy (Indian Institute of Astrophysics)

          Title:  New advances in the diffuse ultraviolet background

          Date: 18th  October 2019 (Friday)

         Time: 4:00 P.M.

          Venue: Physical Sciences Auditorium


Abstract:

Although an important part of our Galaxy, interstellar dust is difficult to characterize. Historically, most of our information about dust has come from observations of extinction curves against background stars but these are limited to those directions where there are suitable stars. Infrared observations of the thermal emission from dust heated by the interstellar radiation field fills the sky and has yielded considerable information about the properties and the distribution of the dust. Ultraviolet observations of the scattered light from the dust have been difficult and sparse until the launch of the GALEX mission. I will discuss my extraction of this diffuse light from the GALEX data and what it tells us about the properties of interstellar dust. My primary focus will be on the modeling I am now doing and on its successes and deficiencies. I will also present our latest results on the background at the Galactic poles where we have discovered a new component of the extragalactic radiation field, one for which we do not yet know the source.




Speaker: Prof Aswin Balasubramanian

Affiliation: Rutgers University

Title: Geometric tools for mass deformed 4d N=2 theories 

Date: 17th September, 2:30pm. 

Venue: LH3, New Physical Sciences Building


Abstract: 

4d N=2 SUSY theories have proved to be an attractive laboratory for gaining insight into non-perturbative behaviour of QFTs. They have also acted as a rich source of connections between physics and modern mathematics which includes topics like four manifold invariants, wall crossing formulae and more recently, the geometry Langlands program. I will survey some of these ideas and then proceed to talk about how the geometry of the Hitchin integrable system can be used to understand the infrared behaviour of a large class of mass deformed 4d "Class S" N=2 SCFTs and their 3d N=4 cousins. The last part is based on recent work with J. Distler ( arXiv:1810.10652 ).




Title: Recent Probes of the Physics Beyond the Standard Model

Speaker: Dr. Amit Chakraborty (IISc) 

Date and Time:  2.00 p.m. (Friday) September 6, 2019

Venue: Lecture Hall 3, New Physical Sciences Building 


Abstract:

The discovery of the Higgs boson at the Large Hadron Collider experiment was believed to be a precursor towards the realization of the physics beyond the Standard Model (BSM). However, no direct sign of new physics is observed to date. This situation poses unique challenges (and opportunities) from both theoretical and experimental perspectives. In this talk, I'll review a few recent developments in the area of particle physics phenomenology. In particular, the aim would be to highlight the application of traditional techniques as well as state-of-the-art Machine Learning methods to improve current understanding of the Standard Model physics and enhance the discovery potential of the BSM physics at the ongoing and future collider experiments.




Title: Parton Distribution Functions for Discovery Physics

Speaker: Prof. Amanda Cooper Sarkar (University of Oxford) 

Date and Time:  3.00 p.m. (Monday) August 26, 2019

Venue: Lecture Hall 3, New Physical Sciences Building 


Abstract:

The uncertainty on parton distribution functions has become the largest uncertainty on searches for physics Beyond the Standard Model, both for direct searches for exotic phenomena and for precision measurements of SM parameters which may deviate from SM values. The current state of the art and prospects for improvement will be reviewed.

Talk slides can be downloaded from here


PHYSICS COLLOQUIUM

-------------------------------------------


          Speaker: Prof. Subir Sarkar (University of Oxford) 

 Title:  Is the universe isotropic?

Date: 23rd  August 2019 (Friday)

Time: 4:00 P.M.

Venue: Physical Sciences Auditorium


Abstract: 

It is a foundational `principle’ of the standard cosmological model that the universe is (statistically) isotropic when averaged over large scales. Recent surveys of the distribution of galaxies and studies of the relic cosmic microwave background radiation now make it possible to test this - with some intriguing results. I will discuss the implications of these findings, in particular for the usual inference that the expansion rate is accelerating, as if driven by a dominant component of ‘dark energy’. 

Talk slides can be downloaded from here


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Title: LZ experiment for dark matter search

Speaker: Prof. Henning Flaecher

Affiliation: University of Bristol, UK

Venue: Multimedia Room, Physical Sciences Building

Time: 4:30 pm, Thursday, 8th August 2019

Host: Dr. Somnath Choudhury


Abstract:

LUX-ZEPLIN (LZ) is a xenon-based direct detection dark matter experiment, currently under construction one mile below ground at the Sandford Undeground Research Facility in the USA. The experiment's 5.6 tonnes of fiducial volume will be a 22-fold increase over its predecessor, LUX. This will allow the experiment to be sensitive to 40 GeV WIMPs with spin-independent cross-sections as low as 1.6x10^{-48} cm^2 at 90% C.L. following an exposure of 1000 live days, which will begin in 2020. LZ is designed around a two-phase xenon time projection chamber, contained in an ultra-low background titanium cryostat, and surrounded by several auxiliary veto systems including an outer liquid xenon layer and a gadolinium-doped liquid scintillator detector. This presentation gives an overview of the experiment, its current status and timeline, and the predicted sensitivity and backgrounds.



Title: Constraining Dark Matter Models with Experiment

Speaker: Prof. Henning Flaecher

Affiliation: University of Bristol, UK

Venue: Lecture Hall 3, Physical Sciences Building

Time: 3 pm, Wednesday, 7th August 2019

Host: Dr. Somnath Choudhury


Abstract:

The nature of Dark Matter is one of the great unresolved questions in particle physics and cosmology. The prevalent hypothesis is that it is a new, only weakly interacting fundamental particle. As such, we hope to be able to produce it in colliders or to detect its interactions with nuclei in direct detection experiments. In this seminar I will discuss in how far experimental measurements constrain the parameter space of two specific dark matter models.

The first concerns simplified dark matter models with leptophobic mediator of spin 1. By performing a global analysis combining results from the LHC, direct detection searches and the relic dark matter density limits are set on the parameter space of the model, i.e., the masses and couplings.

The second analysis focusses on a specific NMSSM model, where gluinos and squarks decay to the NLSP, which in turn decays to the LSP - the dark matter candidate - plus a higgs boson. This is of particular interest as for light LSPs, the experimental signature results in only small amounts of missing energy, which is difficult to detect at the LHC.

At the end of the seminar I will briefly touch on what’s next for the LHC.



SPECIAL CHEP SEMINAR

------------------------------------------


          Speaker: Prof. B. Ananthanarayan (CHEP)

          Title:  Prof. Murray Gell-Mann's work: contributions to Particle Physics 

          Date: 7th June 2019 (Friday)

          Time: 3:00 P.M.

          Venue: Physical Sciences Auditorium 

  

 Abstract: 


 Murray Gell-Mann was Caltech's Robert Andrews Millikan Professor of Theoretical Physics, Emeritus, and a winner of the 1969 Nobel Prize in Physics. In the 1960s Gell-Mann developed a method to categorize the huge number of particles that were being created at particle accelerators worldwide. Gell-Mann’s model also predicted the existence of another fundamental type of particle, named as "quark", that makes up particles including protons and neutrons. He is best known for developing the theory of "quarks" and classification of particles into a "eightfold way" scheme. 

Some of his contributions to the world of particle physics will be discussed in this seminar followed by a recollection of anecdotes about Prof. Murray Gell-Mann by Prof. Apoorva Patel (CHEP).

Talk slides can be downloaded from here 


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Informal CHEP Seminar

========================

Title: Does the EHT picture prove that at the center of M87 galaxy there is a black hole? 

And can we test string theory with this picture?


Speaker: Prof. Subhendra Mohanty (Physical Research Laboratory, Ahmedabad) 

Date and Time :  2.30 p.m. (Monday) May 13, 2019

Venue: Lecture Hall 3, New Physical Sciences Building 



Title: Production and decays of SM and MSSM Higgs bosons

Speaker: Prof. Michael Spira (Paul Scherrer Institute, Switzerland) 

Date and Time :  3.30 p.m. (Thursday) April 4, 2019

Venue: Lecture Hall 3, New Physical Sciences Building 


Abstract:


The recent discovery of the Higgs boson at the LHC marked the completion of the Standard Model (SM) of strong and electroweak interactions. I will summarize the theoretical ingredients involved in the production and decay processes at the LHC that allowed and will allow for a quite concise picture of the properties of the discovered resonance. These theoretical calculations are a crucial contribution to the discrimination of the SM from BSM scenarios at the LHC. I'll discuss the theoretical status of production cross sections and decay widths for MSSM Higgs bosons as an example of BSM Higgs bosons.

Talk slides can be downloaded from here 


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Title: Unravelling the mystery of dark matter in the light of experimental results

Speaker: Suchita Kulkarni (HEPHY, Austria)  

Date and Time :  3.00 p.m. (Tuesday) March 5, 2019

Venue: Lecture Hall 3, New Physical Sciences Building 


Abstract:


Hunt for dark matter is going on for more than 80 years. Despite intense searches, we have not identified the exact explanation behind almost 20% of energy density of the Universe. In this talk, I review the impact of experimental results on the landscape of particle dark matter. I will primarily focus on direct and indirect detection avenues.

Talk slides can be downloaded from here 


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Title: Confronting B anomalies with low energy parity violation experiments

Speaker: Abhishek Iyer (INFN Napoli, Italy)  

Date and Time :  3.00 p.m. (Wednesday) February 20, 2019

Venue: Lecture Hall 3, New Physical Sciences Building 


Abstract:


We consider a simple implementation of a minimal $Z^\prime$ model in the context of the anomalies in the $B$ decays. With the assumption of the primary contribution being due to the electron, implications from the recent measurements on the weak charge of proton $Q_W^p$ and the Caesium atom $Q_W^{Cs}$ are studied. The conclusion is characterized by different limiting behaviour depending on the chirality of the lepton current. The constraints are then compared with those coming from direct searches. This observation is crucial in determining the exact nature of the solution to the anomaly. The bounds on the simplified models from atomic physics are then compared with those from direct searches. We demonstrate that a minor improvement in the atomic physics measurements can be compared with the bounds from direct searches with possibly better sensitivities for the heavier masses ($ \gtrsim 3.5$ TeV). We finally comment on the collider prospect for observing states beyond the realm of resonant production at LHC.


(with  Giancarlo D'Ambrosio, Fulvio Piccinini and Antonio Polosa)

Talk slides can be downloaded from here 


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Title: Complementarity between Higgs searches at the LHC and Gravitational Waves signals 

Speaker: Tathagata Ghosh (University of Hawaii) 

Date and Time :  3.00 p.m. (Tuesday) February 12, 2019

Venue: Lecture Hall 3, New Physical Sciences Building 


Abstract:


The Higgs boson was postulated as a key component of the Standard Model (SM) of particle physics to explain the origin of mass. After 45 years of rigorous experimental searches, the Higgs boson was finally discovered on July 4th, 2012 at the CERN Large Hadron Collider (LHC). The discovery of the Higgs boson completes the SM and confirm one of its most mysterious predictions. The SM, although very effective, fails to address many important questions of nature. In this seminar, I will discuss how the newly discovered Higgs boson is connected with one of the most critical puzzles of the nature that is not explained by the SM - how the asymmetry between matter and antimatter was created in the early universe? A first order phase transition is an out-of-equilibrium process, and this is needed for the generation of the observed baryon asymmetry (as stated by the third Sakharov condition). However, the newly discovered 125 GeV Higgs boson by itself cannot bring about a first-order phase transition, but an additional real singlet scalar field added to the SM can. Such strongly first-order phase transition in the early universe can also generate gravitational waves signals observable at future space-based interferometers like LISA. On the other hand, the presence of the additional scalar particle in the model will lead to interesting signatures of physics beyond the SM at the LHC. In this talk, I will discuss the possibility for complementary searches for electroweak phase transition in collider and gravitational wave experiments within the SM augmented by a real singlet scalar. 

Talk slides can be downloaded from here 


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Title: High Luminosity LHC Physics and the CMS Detector Upgrade

Speaker: Prof. Maxwell Chertok  

Affiliation: University of California - Davis, USA.

 Date:  Friday, 8th February 2019   

Time: 2:30 p.m. – 3.45p.m.

Venue: LH3, New Physical Sciences Building 

 

Abstract: 

 

Almost from the start, the Large Hadron Collider at CERN has exceeded expectations in performance and integrated luminosity delivered, and the LHC experiments have followed suit with many important results that deepen our understanding of nature at the smallest scale.  The Higgs boson has evolved from the discovery of the millennium to a new laboratory for study with increasing precision as the data accumulate.  Simultaneously, plans are well underway for an ultimate High Luminosity LHC (HL-LHC) program, which will collect an order of magnitude more data to leave no stone unturned in the quest for new fundamental particles and interactions.  In this talk, I outline the history and status of the LHC, give an overview of HL-LHC including physics prospects, and present the CMS upgrade plans with a focus on the state-of-the-art outer tracker. 

Talk slides can be downloaded from here 


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Title: High-energy neutrinos and gravitational waves: search for Standard Model and beyond the Standard Model phenomena

Speaker: Ranjan Laha (U. Mainz)

Date and Time :  4.00 p.m. (Thursday) February 7, 2019

Venue: Lecture Hall 3, New Physical Sciences Building


Abstract: 


Studying physics with different messengers gives us a unique understanding of the workings of the Universe.  In this talk, I will discuss two newest messengers: high-energy neutrinos and gravitational waves.  I will show how these messengers can be used to study both Standard Model and beyond the Standard Model phenomena.  Studying high-energy extraterrestrial neutrinos, one can learn more about high-energy tau propagation and the charm content of the proton.  These are sensitive to photo-nuclear interactions and intrinsic charm, and can complement various collider studies.  I will also discuss gravitational waves from neutron star mergers and how these observations can constrain the presence of a long range force in the hidden sector.  Considering various constraints, I will present how gravitational wave observations can probe new parts of the parameter space.

Talk slides can be downloaded from here 


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Colloquium

----------------------------------------------------


Title: Search for dark matter in astroparticle physics

Speaker: Ranjan Laha (U. Mainz)

Date and Time :  3.00 p.m. (Wednesday) February 6, 2019

Venue: Lecture Hall 3, New Physical Sciences Building


Abstract: 


The astrophysical evidence for dark matter is overwhelming.  It is one of the main hints that suggest the presence of new physics.  Despite this evidence, we do not know the constituent(s) of dark matter. A comprehensive search program is required to solve this mystery. I will discuss new ways to search for dark matter candidate(s) in the entire mass range using different astroparticle physics methods. I will present techniques which can efficiently search for ultra-light dark matter, sterile neutrino dark matter, very heavy dark matter, and primordial black holes. I will show how these search strategies can complement each other to comprehensively search for dark matter candidate(s).

Talk slides can be downloaded from here 


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Title:  dS vacua and the swampland

Speaker: Timm Wrase

Affiliation: Technical University of Vienna

Date: 17th January 2:30 pm.

Venue: LH3, New Physical Sciences Building

 

Abstract: 

 After briefly reviewing dark energy, dS vacua and the standard model of cosmology, I will discuss recent conjectures that say that metastable dS vacua cannot arise in string theory. These conjectures lead to interesting observational predictions and are currently being tested experimentally. On the theoretical side I will discuss the support for these conjectures as well as the status of explicit counter examples like the KKLT and LVS scenario. Then I present recent progress on constructing dS vacua in type IIA string theory using anti-D6-branes.

Talk slides can be downloaded from here 


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Colloquium

----------------------------------------------------


Title: Various directions for physics beyond the Standard Model 

Speaker: Shankha Banerjee (IPPP, Durham)

Date and Time :  4.00 p.m. (Wednesday) January 16, 2019 

Venue: Lecture Hall 3, New Physical Sciences Building


Abstract: 

In this talk, I will address the necessity to look beyond the Standard Model of particle physics (BSM) in the purview of several experimental observations and theoretical requirements. Specifically, I will discuss several scenarios involving a dark matter candidate including pseudoscalar-mediated dark matter, mixed dark matter and sneutrino dark matter. I will discuss the importance of considering higher order corrections in the calculation of the relic abundance and direct-detection cross-section. Moreover, I will discuss several scenarios involving a long-lived particle (LLP), upon including strict constraints from Big Bang nucleosynthesis. I will address some exotic signatures of LLPs which are yet to be studied by the experiments. Finally, I will briefly discuss models with extended scalar and fermionic sectors, including models with heavy Higgs, heavy neutrinos, heavy quarks and leptons, and exotic decays of the top quark.

Talk slides can be downloaded from here 


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Title: Higgs coupling measurements at the HL-LHC and beyond

Speaker: Shankha Banerjee (IPPP, Durham)

Date and Time :  3.00 p.m. (Tuesday) January 15, 2019

Venue: Lecture Hall 3, New Physical Sciences Building


Abstract: 

In this talk, I will review the present status of the Higgs boson's properties since its discovery in 2012. I will focus on the measurements of several Higgs couplings at the LHC and at future lepton colliders, upon considering standard production and decay modes, in the context of an effective field theory. I will also discuss the possibility of strongly constraining the couplings affecting the triple gauge boson vertices upon studying the Zh channel in the boosted Higgs regime. I will show the potential of the High luminosity run of the LHC (HL-LHC) and the future 100 TeV FCC-hh machine, to constrain such couplings to stronger degrees than LEP had constrained earlier. Moreover, I will discuss studies pertaining to the non-resonant and resonant Higgs pair production at the HL-LHC and at a future 100 TeV collider. Finally, I will discuss the possibility of certain exotic decay modes of the Higgs, including it's possible decay to invisible particles and to a pair of differently-flavoured leptons.

Talk slides can be downloaded from here 


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Title: FIMPs and their signatures

Speaker: Prof. Genevieve Belanger (LAPTH, France)

Date and Time :  10.00 a.m. (Tuesday) January 15, 2019

Venue: Lecture Hall 3, New Physical Sciences Building


Abstract: 

Dark matter that is extremely weakly coupled to the standard model can be directly produced in the early universe  via the freeze-in mechanism. After describing this  mechanism, I will present some specific models where freeze-in can be realised and discuss the implications for dark matter searches in astrophysics and at the LHC. 

Talk slides can be downloaded from here 


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Series of lectures on positive geometries and scattering amplitudes for massless particle

--------------------------

First Talk

======

Date and time: 11th January (Friday) @ 4.30 pm

Speaker: Alok Laddha

Venue: Lecture Hall 3

Title: Amplituhedron for bi-adjoint scalar field theory.


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Second Talk

======

Date and time: 14th January (Monday) @ 3.30 pm

Speaker: Alok Laddha

Venue: Lecture Hall 3

Title: Amplituhedron for bi-adjoint scalar field theory (Lecture 2).

Introduction to Associahedron


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Third Talk

======

Date and time: 15th January (Tuesday) @ 4.15pm

Speaker: Alok Laddha

Venue: Lecture Hall 3

Title: Associahedron for cubic interaction and extension to quartic interaction.


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Title: Freeze-in Dark Matter

Speaker: Debtosh Chowdhury (Ecole Polytechnique)

Date and Time :  3.00 p.m. (Friday) January 11, 2019

Venue: Lecture Hall 3, New Physical Sciences Building


Abstract:

Despite indirect but clear pieces of evidence of the presence of a large amount of dark matter in our Universe, its nature still remains elusive. The absence of any signal in direct detection experiments like XENON, LUX, and PANDAX questions the weakly coupled dark matter paradigm. This uncomfortable situation justifies the need to look for different scenarios, allowing feeble couplings, or the possibility of dark matter production at the very early stages of reheating. In such scenarios, the observed dark matter abundance consists of Feebly Interacting Massive Particles (FIMPs), produced non-thermally by the so-called freeze-in mechanism. In contrast to the usual freeze-out scenario, frozen-in FIMP dark matter interacts very weakly with the particles in the visible sector and never attained thermal equilibrium with the baryon-photon fluid in the early Universe. In this talk, we introduce the freeze-in mechanism as well as will outline some of the key features of the reheating process. Realization of the freeze-in mechanism in a concrete model will also be discussed.

Talk slides can be downloaded from here 


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COLLOQUIUM

----------------------------------------------------


Title: The Quest for New Physics: Impact of Direct and Indirect Searches

Speaker: Debtosh Chowdhury (Ecole Polytechnique)

Date and Time :  3.45 p.m. (Wednesday) January 9, 2019

Venue: Lecture Hall 3, New Physical Sciences Building


Abstract: 

Our current understanding of the fundamental structure of the Universe is captured by the Standard Model (SM). Over the years the SM has been tested in numerous experiments and it has been one of the most successful theories constructed to date. The discovery of the Higgs boson at the Large Hadron Collider has provided us with evidence for the last missing piece of the SM. While the experimental results strengthen our understanding of the SM, they also point out some key questions which the SM fails to answer, including the following: (i) Why there is a hierarchy in mass scales in the SM?, (ii) What is dark matter made of? Where does it come from?, (iii) What are the origin of neutrino mass and its mixing?, (iv) What is the reason behind the fermion masses and mixings? etc. To address any of these above questions one would need to extend the SM. In this talk, I will primarily focus on those models which extend the SM to solve one or more of the above-mentioned questions. In particular, I will try to infer the nature of the New Physics both from the direct and indirect search experiments as well as from the interplay between them.

Talk slides can be downloaded from here 


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TECHNICAL TALK

----------------------------------------------------

Title:  Causality and energy conditions in CFT

Speaker:  Dr. Sandipan Kundu

Institute: Johns Hopkins University,

Dept. of Physics & Astronomy,

Bloomberg Centre for Physics & Astronomy,

Baltimore, MD 21218.

Time:  Thursday, 3rd January 2019 at 3 pm

Venue:  LH-3, Physical Sciences Building


Abstract:

Causality places nontrivial constraints on conformal field theory (CFT) in Lorentzian signature. I will show how causality is encoded in the analytic structure of Euclidean correlators and explain the connection between the causality constraints in the lightcone limit and the averaged null energy condition. In particular, causality implies that the averaged null energy must be positive in flat spacetime for any unitary quantum field theory with an interacting UV fixed point. Whereas, for CFTs with large central charge and a sparse spectrum, causality constraints in the Regge limit lead to a stronger energy condition which is a generalization of the averaged null energy condition. This new energy condition leads to nontrivial constraints on CFT 3-point couplings. In addition, I will also show that these constraints are consistent with the expectation that CFTs in this class, irrespective of their microscopic details, admit universal gravity-like holographic dual description. Furthermore, this new energy condition when applied to higher spin operators implies that any finite number of massive elementary particles with spin more than two cannot interact with gravitons  in anti-de Sitter spacetime in a way that preserves causality.


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Title:  Theories of gravity coupled to spin 2 fields

Speaker: Fawad Hasan

Affiliation: Department of Physics, Stockholm University

Venue: Lecture Hall 3, physical sciences building.

Time: 2nd January 3:30 PM.


Abstract:

 Theories of fields with spin s less than 2 are well established, while for fields of spin greater than 2 no theories with finite field content are known to exist. For spin s=2 the only established field theory is General Relativity which contains a single massless field. Spin 2 theories beyond this are generically plagued by pathologies, raising the question if GR is unique in this respect. This talk will describe the current status of theories of massive and multiple spin 2 fields that avoid the known ghost instabilities. These are commonly known as theories of massive gravity, bimetric gravity, and multimetric gravity.

Talk slides can be downloaded from here 


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COLLOQUIUM

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Title:  Causality in QFT

Speaker:  Dr. Sandipan Kundu

Institute:  Johns Hopkins University,

Dept. of Physics & Astronomy,

Bloomberg Centre for Physics & Astronomy,

Baltimore, MD 21218.

Time:  Wednesday, 2nd January 2019 at 2 pm

Venue:  LH-3, Physical Sciences Building


Abstract:

Causality is an essential feature of any unitary, Lorentz-invariant quantum field theory (QFT) in flat space time. In QFT, causality is an operator statement: commutators of local operators vanish at space like separation. Requiring a QFT to be causal in every state of the theory can impose non-trivial constraints on QFTs. In addition, I will show that QFTs that appear to be causal in flat space time can violate causality when coupled to gravity. These basic principles, as I will explain, can provide us a way to learn general lessons about QFTs. In particular, for any interacting QFT in more than two dimensions, causality implies that the averaged null energy must be positive. The same formalism also explains how gravity like behaviour emerges from certain class of QFTs. Finally, I will show that causality imposes strong restrictions on elementary particles with spin more than two.

Talk slides can be downloaded from here 


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Condensed Matter Physics Seminar

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    Title:  Residual entropy of spin-liquids

Speaker:  Prof. Rajiv Singh

      Institute:  University of California, Davis

    Time:  Friday, 21st December at 3 pm

   Venue:  Auditorium, Physical Sciences Building

                    

Abstract:

Residual ground state entropy is well known theoretically in two-dimensional highly frustrated Ising models and experimentally in rare-earth pyrochlore family of spin-ice materials. In quantum systems, the ground state entropy is typically zero, but there can be an entropy plateau over a range of temperatures, reflecting a degenerate low-energy manifold from which the ground state emerges. Computational studies of Kagome antiferromagnets and quantum spin-ice models give hints of such a plateau. More recent studies of honeycomb-lattice Kitaev models and their spin-S generalizations show evidence for entropy plateaus, where the magnitude of the entropy keeps increasing with S. We discuss numerical evidence and possible explanations.

Talk slides can be downloaded from here 


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Title: Relaxion Double Miracle

Speaker: Rick. S. Gupta (IPPP, Durham) 

Date and Time :  3.00 p.m. (Wednesday) November 28, 2018

Venue: Lecture Hall 3, New Physical Sciences Building


Abstract:  

We begin by an introduction to relaxion models, outlining some of the main issues that still need to be addressed and possible solutions.  We then describe some current work where we show that spontaneous baryogenesis occurs automatically in relaxion models if the reheating temperature is larger than the weak scale, provided the Standard Model fields are charged under  the relaxion shift symmetry. During the slow roll, the relaxion breaks CPT, biasing the thermal equilibrium in favour of baryons, with sphalerons providing the necessary baryon number violation. Successful baryogenesis can be achieved for a range of relaxion masses between 10^−5 and 10^−10 eV. The mechanism operates precisely in the region of parameter space where recent work has shown relaxion oscillations to be a dark matter candidate.

Talk slides can be downloaded from here 

 

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Title: Perspectives on the scale of new Physics

Speaker: Rick. S. Gupta (IPPP, Durham) 

Date and Time :  3.00 p.m. (Tuesday) November 27, 2018

Venue: Lecture Hall 3, New Physical Sciences Building


Abstract: 

Abstract: So far the Large Hadron Collider (LHC) has discovered the Higgs boson and nothing else, a possibility that had been previously dubbed as ‘the nightmare scenario’. We argue that such a negative attitude is unwarranted and in fact the absence of new physics at the LHC motivates two very concrete research directions depending on our perspective on the question: what is the scale of new physics ? First of all, new physics may be just beyond LHC reach, and then the Standard Model Effective Field Theory (SMEFT) becomes a powerful framework to study indirect deviations. We discuss how the higher accessible centre of mass energy at LHC can potentially compensate for the smaller intrinsic precision of LHC relative to LEP. In the second part of this talk we consider the possibility that there is no new physics close to the TeV scale and view the current situation as an opportunity for a fundamental questioning of the conventionally held rationale for TeV scale physics. More concretely we discuss the recently proposed relaxion models that can accommodate a light Higgs even with a high new physics scale. 

Talk slides can be downloaded from here 

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Title: Stronger 21cm absorption from charge sequestration

Speaker: Prof.  Adam Falkowski (Laboratoire de Physique Théorique, Paris)

Date and Time :  3.00 p.m. (Thursday) November 22, 2018

Venue: Lecture Hall 3, New Physical Sciences Building


Abstract:

The unexpectedly strong 21cm absorption signal detected by the EDGES experiment suggests that the baryonic gas at the end of the dark ages was colder than predicted within the standard cosmological scenario. I will introduce one novel mechanism to lower the baryon temperature after recombination. The model includes a stable, negatively-charged particle with a significant cosmological abundance, such that the universe remains charge-neutral but the electron and proton numbers are no longer equal. The deficit of electrons after recombination results in an earlier decoupling of the baryon and CMB temperatures, and thus in a colder gas at the cosmic dawn. I will discuss the phenomenological constraints and possible smoking guns of this scenario.

Talk slides can be downloaded from here 

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    CHEP PHYSICS COLLOQUIUM

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Title : Low-energy precision frontier

          Speaker : Prof.  Adam Falkowski (Laboratoire de Physique Théorique, Paris)       

          Date :  19th November 2018 (Monday)

          Time : 3:45 P.M.

         Venue : Physical Sciences Auditorium


Abstract:  Precision measurements are an integral part of modern particle physics. Apart from determining the free parameters of the Standard Model (SM) and testing its predictions, their role is to search for signals of new physics. The presence of new particles beyond the SM, even if they are very heavy, may affect scattering cross sections, masses, or decay widths of the known particles. Precision measurements of these observables may provide us with information about physics well beyond the direct reach of the existing particle colliders. In this talk I will review various sensitive precision observables, focusing on measurements at energy scale well below the weak scale, in particular on decays of light mesons and tau leptons, atomic parity violation, and neutrino scattering.   I will also discuss a model independent characterization of the information provided by these experiments in the language of effective field theory.

Talk slides can be downloaded from here 

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Title: Getting the gist of Next-to-Leading Order QCD calculation

Speaker:  Satyajit Seth (IPPP, Durham)

Date and Time :  3.00 p.m. (Wednesday) November 14, 2018

Venue: Lecture Hall 3, New Physical Sciences Building


Abstract: 

In this talk, I'll discuss the nitty-gritty of next-to-leading order (NLO) QCD correction. I'll first talk of fixed order NLO calculation and then come to its matching with parton shower. Such calculations are highly important to come up with precise theoretical results close to the experimental outcomes of a hadron collider. 

Talk slides can be downloaded from here

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Title: Next-to-Leading Order: Numerical vs. Analytical

Speaker:  Satyajit Seth (IPPP, Durham)

Date and Time :  3.00 p.m. (Tuesday) November 13, 2018

Venue: Lecture Hall 3, New Physical Sciences Building


Abstract: 

In this talk, I'll describe how to integrate out various subtraction terms that arise in NLO computation numerically. Such numerical technique is inevitable to handle complexity of the calculation when the number of external leg gets bigger. Besides, I'll present the first systematic analytical calculation of Higgs production associated with up to five gluons at one loop level when all gluons carry same helicities. This calculation is important to study higher order corrections on Higgs+jet(s) in the region where large top-mass approximation is not applicable and numerical outcome in the full theory shows instability.

Talk slides can be downloaded from here


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CHEP PHYSICS COLLOQUIUM

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Title : Down-To-Earth String Theory

Speaker : Prof. Rajesh Gopakumar,  (ICTS-TIFR)

Date : 9th November 2018 (Friday)

Time : 4:00 P.M.

Venue : Physical Sciences Auditorium


  Abstract

String theory has evolved into a powerful framework which is capable of providing fresh insights into well established frameworks like quantum field theory (QFT). One such set of new perspectives have been on conformal field theories (CFTs) which are central to our understanding of QFTs. This talk will be centred on some very "down-to-earth CFTs" such as the Wilson-Fisher fixed point (and its analogues and generalisations) that governs critical phenomena in statistical mechanics. We will aim to bring out the utility as well as beauty of the new angles that string theory methods bring to these well studied systems.

 Talk slides can be downloaded from here 


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Title: Electroweakinos in the era of LHC

Speaker: Nabanita Ganguly (Calcutta University)

Date and Time : 4.30 p.m. (Monday) September 24, 2018

Venue: Lecture Hall 3, New Physical Sciences Building

Abstract:

In this talk I will mainly consider the electroweak sector of the MSSM. I will discuss the need to go beyond the simplified model which is often opted by the LHC collaborations to interpret their results. This will bring the heavier electroweakinos in our discussion. Some interesting channels that may have discovery prospect will also be discussed.



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Title: The semi-classical fate of black hole horizons

Speaker: Debajyoti Sarkar(Institute for Theoretical Physics (ITP), Universität Bern)

Date: Monday 24th September, 14:30

Venue: Lecture Hall 3, New Physical Sciences Building.


Abstract: I will discuss the possibility that in the semiclassical gravitational theory, the black hole horizon is non-perturbatively replaced by a tiny throat, whose parameters make it a perfect mimicker of a classical black hole. Based on work with Clément Berthiere and Sergey Solodukhin (PLB; arXiv: 1712.09914 [hep-th]).


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Title: Dirac Neutrinos

Speaker:Rahul Srivastava  (IFIC, Spain)

Date and Time :  3.00 p.m. (Monday) September 17, 2018

Venue: Lecture Hall 3, New Physical Sciences Building

Abstract:

More than eighty years after they were first proposed, neutrinos still remain an enigma. Although they are an integral part of Standard Model , still we know very little about them. In particular, the Dirac or Majorana nature of neutrinos remains a mystery. For a long time, theoretical particle physicists believed that neutrinos must be Majorana in nature and several elegant mass generation mechanisms have been proposed for Majorana neutrinos. In this talk, I will discuss many ways in which naturally small Dirac neutrino masses can be generated. I will also discuss the various interesting and sometimes surprising connections between Dirac nature of neutrinos and Dark Matter stability, proton decay etc.