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Diego Saviot
Diego Saviot
Title of the talk:
Strong-field regime within effective field theory
Abstract:
In this talk, I present an expansion of the effective action obtained when integrating out scalar QED in presence of a strong-field background. The computation is carried out in momentum space by adapting the framework of Covariant Derivative Expansion to capture non-perturbative effects. I will draw parallels with the worldline formalism both to guide the way and to compute Green functions.
I eventually specialise to the case of small inhomogeneities of a strong background and compute the first correction to the Heisenberg-Euler effective action in a derivative expansion.
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André Gontijo Campos
André Gontijo Campos
Title of the talk:
Strong-field regime within effective field theory Laboratory cosmology with free spinorial wave packets
Abstract:
The electron quantum dynamics at crossing the black hole horizon is investigated. Exploiting the equivalence principle, we show a way to emulate the electron’s dynamics via an appropriately chirped free electron wave packet, where the dynamical characteristics is encoded in the interference fringes of the wave packet. Apart from creating an analog of the gravitational effect, we deduce the electron’s explicit wavefunction at the horizon of a black hole and provide quantitative predictions on the quantum properties of the electron crossing the horizon.
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Mohammed Alkhateeb
Mohammed Alkhateeb
Title of the talk:
Computational Quantum Field Theory for Fermionic Pair Production in 1+1 Dimensions
Abstract:
Computational quantum field theory (CQFT) provides a real-time numerical framework for studying quantum field dynamics in strong, space- and time-dependent external backgrounds beyond perturbation theory. In this talk, I will first introduce the CQFT formalism in flat spacetime, demonstrating how the time evolution of first-quantized states can be used to evaluate QFT time-dependent observables such as charge densities and currents, as well as how CQFT might address the ambiguity problem of particle number at transient times.
I will then present an extension of this framework to quantum fields in curved spacetime, focusing on fermionic fields in 1+1-dimensional gravitational backgrounds. Using the vielbein formalism, I provide an effective Dirac Hamiltonian for a prescribed curved geometry and show how an appropriate field rescaling leads to a Hermitian Hamiltonian and unitary time evolution. This enables the direct numerical simulation of vacuum excitation and fermion–antifermion pair creation induced by spacetime curvature.
As an illustration, I will discuss results for a smooth, asymptotically flat spacetime generated by a localized Gaussian curvature deformation, introduced into the Minkowski vacuum as a quench. The evolution of particle number densities and total particle production is analyzed, highlighting the role of curvature strength and spatial extension and the Pauli blockade.
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worldliners2026.pdfDavide Rovere
Davide Rovere
Title of the talk:
Worldline Formulations of Covariant Fracton Theories
Abstract:
Fractons first appeared in spin lattice models as quasiparticle excitations characterised by reduced mobility, due to the conservation of the dipole moment. The so-called "covariant fracton gauge theories" are a family of Lorentz-covariant extensions of the gauge theory of fractons, which can be viewed as a generalisation of linearised Einstein gravity. In this talk, based on the paper arXiv:2508.14591 with F. Fecit, some worldline formulations of covariant fracton gauge theories will be presented, based on additional bosonic coordinates to the phase space. These models allow for the BV spectrum of covariant fracton gauge theories to be obtained, from the spacetime perspective, in a completely covariant way, through the BRST quantisation of the classical phase space. The possibility of deriving covariant fracton gauge theories from a worldline perspective is a further confirmation of the worldline/spacetime duality of gauge theories in BV formulation.
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Azadeh Maleknejad
Azadeh Maleknejad
Title of the talk:
The Stochastic Schwinger Effect
Abstract:
The Schwinger effect predicts nonperturbative particle–antiparticle pair production in a strong classical electric field. In realistic environments, however, gauge fields are rarely coherent or constant — they are transient, inhomogeneous, and often stochastic. In this talk, I introduce a new type of Schwinger effect, which we call the stochastic Schwinger effect. We formulate vacuum decay in statistically fluctuating gauge-field backgrounds and compute the decay rate and particle number density using the effective action formalism, obtaining closed analytical results for both scalars and fermions. Working in flat spacetime and at zero temperature to isolate the core physics, we demonstrate that stochastic fluctuations themselves can drive vacuum instability. This framework opens a new avenue for understanding particle production in early-Universe and high-energy astrophysical settings.
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Emil Akhmedov
Emil Akhmedov
Title of the talk:
Does Schwinger's value for the current of created pairs gets modified for long and strong enough pulse?
Abstract:
We determine the parametric conditions (pulse strength and duration) under which Schwinger's prediction for the pair-creation current - and therefore the probability - is significantly altered. Then we will discuss the possibility of an avalanche of particle creation in external fields and similar phenomena in background fields of other nature.
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