Gravitational and electromagnetic Cherenkov radiation constraints in modified dispersion relations

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Main Authors: Artola, Mikel, Cembranos, José A. R., Martín-Moruno, Prado
Format: Preprint
Published: 2024
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author Artola, Mikel
Cembranos, José A. R.
Martín-Moruno, Prado
author_facet Artola, Mikel
Cembranos, José A. R.
Martín-Moruno, Prado
contents Motivated by different approaches to quantum gravity, one could consider that Lorentz invariance is not an exact symmetry of nature at all energy scales. Following this spirit, modified dispersion relations have been used to encapsulate quantum gravity phenomenology. In the present work, we propose a class of Lorentz invariance violating phenomenological dispersion relations, which could be different for each particle species, to study the generalized vacuum Cherenkov radiation process. We identify the kinematic regions where the process is allowed and then compute the energy loss rate due to the emission of vacuum electromagnetic and gravitational Cherenkov radiation. Furthermore, we estimate constraints for the Lorentz invariance breaking parameters of protons and gravitons taking into account the existence (or absence) of vacuum gravitational Cherenkov radiation using ultra high energy cosmic ray detections.
format Preprint
id arxiv_https___arxiv_org_abs_2410_18544
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Gravitational and electromagnetic Cherenkov radiation constraints in modified dispersion relations
Artola, Mikel
Cembranos, José A. R.
Martín-Moruno, Prado
General Relativity and Quantum Cosmology
Cosmology and Nongalactic Astrophysics
High Energy Astrophysical Phenomena
High Energy Physics - Phenomenology
Motivated by different approaches to quantum gravity, one could consider that Lorentz invariance is not an exact symmetry of nature at all energy scales. Following this spirit, modified dispersion relations have been used to encapsulate quantum gravity phenomenology. In the present work, we propose a class of Lorentz invariance violating phenomenological dispersion relations, which could be different for each particle species, to study the generalized vacuum Cherenkov radiation process. We identify the kinematic regions where the process is allowed and then compute the energy loss rate due to the emission of vacuum electromagnetic and gravitational Cherenkov radiation. Furthermore, we estimate constraints for the Lorentz invariance breaking parameters of protons and gravitons taking into account the existence (or absence) of vacuum gravitational Cherenkov radiation using ultra high energy cosmic ray detections.
title Gravitational and electromagnetic Cherenkov radiation constraints in modified dispersion relations
topic General Relativity and Quantum Cosmology
Cosmology and Nongalactic Astrophysics
High Energy Astrophysical Phenomena
High Energy Physics - Phenomenology
url https://arxiv.org/abs/2410.18544