Conveners
General Talk 1
- There are no conveners in this block
General Talk 1
- Chair: Kasia Krajewska
General Talk 1
- Chair: Arseny Mironov
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Kasia Krajewska27/08/2024, 14:30
We present a newly developed method for describing dynamical Sauter-Schwinger process using the S-matrix approach and reduction formulas [1]. The method is based on solving the Dirac equation with Feynmann or anti-Feynmann boundary conditions [2]. It leads to spin-resolved (helicity-resolved) probability amplitudes of produced electrons and positrons. With this approach, after summing up over...
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Dr Christian Kohlfürst (Helmholtz-Zentrum Dresden-Rossendorf)27/08/2024, 15:15
Strong-field quantum electrodynamics is the epitome of what happens when a quantum many-body system is pushed to the extreme. It tests our understanding of non-equilibrium physics, fundamental particle physics and everything we think we know about emergent phenomena and collective dynamics [1]. In particular, identifying the formation time of an electron-positron pair within a background field...
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Selym Villalba Chavez (Heinrich Heine U., Dusseldorf)27/08/2024, 15:40
Production of electron-positron pairs by a high-energy γ photon and a bichromatic laser wave is considered where the latter is composed of a strong low-frequency and a weak high-frequency component, both with circular polarization. An expression for the production rate is derived that accounts for the strong laser mode to all orders and for the weak laser mode to first order. The structure of...
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Stepan Bulanov27/08/2024, 16:25
It is widely accepted that the next lepton collider beyond a Higgs factory would require
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center-of-mass energy of the order of up to 15 TeV. Since, given reasonable space and cost restrictions,
conventional accelerator technology reaches its limits near this energy, high-gradient advanced
acceleration concepts are attractive. Advanced and novel accelerators (ANAs) are leading candidates
due to... -
Naser Ahmadiniaz27/08/2024, 16:50
Neutrino–antineutrino pair production is a key process contributing to energy loss in stars. While previous studies have examined pair creation via the collision of two (γγ→ννˉ) or three (γγγ→ννˉ) real photons, as well as photon collisions in the presence of nuclear Coulomb fields or external magnetic fields, this talk explores a new scenario.
We investigate the pair production of...
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