Testing effects of Lorentz invariance violation in the propagation of astroparticles with the Pierre Auger Observatory

Lorentz invariance violation (LIV) is often described by dispersion relations of the form E2 i = m2 i + p2 i + δi,nE2+n with delta different based on particle type i, with energy E, momentum p and rest mass m. Kinematics and energy thresholds of interactions are modified once the LIV terms become co...

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Autores principales: Binet, V., Micheletti, M. I., The Pierre Auger collaboration
Formato: article artículo publishedVersion
Lenguaje:Inglés
Publicado: IOP Publishing 2022
Materias:
Acceso en línea:http://hdl.handle.net/2133/23387
http://hdl.handle.net/2133/23387
Aporte de:
id I15-R121-2133-23387
record_format dspace
institution Universidad Nacional de Rosario
institution_str I-15
repository_str R-121
collection Repositorio Hipermedial de la Universidad Nacional de Rosario (UNR)
language Inglés
orig_language_str_mv eng
topic Cosmic ray experiments
Ultra high energy cosmic rays
Physics of the early universe
spellingShingle Cosmic ray experiments
Ultra high energy cosmic rays
Physics of the early universe
Binet, V.
Micheletti, M. I.
The Pierre Auger collaboration
Testing effects of Lorentz invariance violation in the propagation of astroparticles with the Pierre Auger Observatory
topic_facet Cosmic ray experiments
Ultra high energy cosmic rays
Physics of the early universe
description Lorentz invariance violation (LIV) is often described by dispersion relations of the form E2 i = m2 i + p2 i + δi,nE2+n with delta different based on particle type i, with energy E, momentum p and rest mass m. Kinematics and energy thresholds of interactions are modified once the LIV terms become comparable to the squared masses of the particles involved. Thus, the strongest constraints on the LIV coefficients δi,n tend to come from the highest energies. At sufficiently high energies, photons produced by cosmic ray interactions as they propagate through the Universe could be subluminal and unattenuated over cosmological distances. Cosmic ray interactions can also be modified and lead to detectable fingerprints in the energy spectrum and mass composition observed on Earth. The data collected at the Pierre Auger Observatory are therefore possibly sensitive to both the electromagnetic and hadronic sectors of LIV. In this article, we explore these two sectors by comparing the energy spectrum and the composition of cosmic rays and the upper limits on the photon flux from the Pierre Auger Observatory with simulations including LIV. Constraints on LIV parameters depend strongly on the mass composition of cosmic rays at the highest energies. For the electromagnetic sector, while no constraints can be obtained in the absence of protons beyond 1019 eV, we obtain δγ,0 > −10−21, δγ,1 > −10−40 eV−1 and δγ,2 > −10−58 eV−2 in the case of a subdominant proton component up to 1020 eV. For the hadronic sector, we study the best description of the data as a function of LIV coefficients and we derive constraints in the hadronic sector such as δhad,0 < 10−19, δhad,1 < 10−38 eV−1 and δhad,2 < 10−57 eV−2 at 5σ CL.
format article
artículo
publishedVersion
author Binet, V.
Micheletti, M. I.
The Pierre Auger collaboration
author_facet Binet, V.
Micheletti, M. I.
The Pierre Auger collaboration
author_sort Binet, V.
title Testing effects of Lorentz invariance violation in the propagation of astroparticles with the Pierre Auger Observatory
title_short Testing effects of Lorentz invariance violation in the propagation of astroparticles with the Pierre Auger Observatory
title_full Testing effects of Lorentz invariance violation in the propagation of astroparticles with the Pierre Auger Observatory
title_fullStr Testing effects of Lorentz invariance violation in the propagation of astroparticles with the Pierre Auger Observatory
title_full_unstemmed Testing effects of Lorentz invariance violation in the propagation of astroparticles with the Pierre Auger Observatory
title_sort testing effects of lorentz invariance violation in the propagation of astroparticles with the pierre auger observatory
publisher IOP Publishing
publishDate 2022
url http://hdl.handle.net/2133/23387
http://hdl.handle.net/2133/23387
work_keys_str_mv AT binetv testingeffectsoflorentzinvarianceviolationinthepropagationofastroparticleswiththepierreaugerobservatory
AT michelettimi testingeffectsoflorentzinvarianceviolationinthepropagationofastroparticleswiththepierreaugerobservatory
AT thepierreaugercollaboration testingeffectsoflorentzinvarianceviolationinthepropagationofastroparticleswiththepierreaugerobservatory
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