Approaches to photon absorption in a Lorentz invariance violation scenario

Fuente: arXiv
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Main Authors: Carmona, J. M., Cortés, J. L., Rescic, F., Reyes, M. A., Terzić, T., Vrban, F. I.
Format: Preprint
Published: 2024
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author Carmona, J. M.
Cortés, J. L.
Rescic, F.
Reyes, M. A.
Terzić, T.
Vrban, F. I.
author_facet Carmona, J. M.
Cortés, J. L.
Rescic, F.
Reyes, M. A.
Terzić, T.
Vrban, F. I.
contents Very high-energy astrophysical gamma rays suffer a suppression of their flux along their propagation due to their interaction, through the $γγ\to e^+e^-$ pair-production process, with the soft photon backgrounds present in the Universe. We examine the Universe's transparency to gamma rays within a Lorentz Invariance Violation (LIV) framework, focusing on photon subluminal quadratic corrections driven by a high-energy scale. Based on an explicit calculation, we provide a new expression for the cross section that overcomes the limitations of previous approaches and refines existing constraints for the LIV scale, while we introduce a new approximation that may be useful in LIV scenarios beyond effective field theory. These improvements appear essential for setting constraints on LIV effects with future observations at ultra-high energies, where previous approximations may fall short.
format Preprint
id arxiv_https___arxiv_org_abs_2404_07842
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Approaches to photon absorption in a Lorentz invariance violation scenario
Carmona, J. M.
Cortés, J. L.
Rescic, F.
Reyes, M. A.
Terzić, T.
Vrban, F. I.
High Energy Physics - Phenomenology
High Energy Astrophysical Phenomena
General Relativity and Quantum Cosmology
Very high-energy astrophysical gamma rays suffer a suppression of their flux along their propagation due to their interaction, through the $γγ\to e^+e^-$ pair-production process, with the soft photon backgrounds present in the Universe. We examine the Universe's transparency to gamma rays within a Lorentz Invariance Violation (LIV) framework, focusing on photon subluminal quadratic corrections driven by a high-energy scale. Based on an explicit calculation, we provide a new expression for the cross section that overcomes the limitations of previous approaches and refines existing constraints for the LIV scale, while we introduce a new approximation that may be useful in LIV scenarios beyond effective field theory. These improvements appear essential for setting constraints on LIV effects with future observations at ultra-high energies, where previous approximations may fall short.
title Approaches to photon absorption in a Lorentz invariance violation scenario
topic High Energy Physics - Phenomenology
High Energy Astrophysical Phenomena
General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2404.07842