Multi-messenger Astrophysics at Ultra-High Energy with the Pierre Auger Observatory

The study of correlations between observations of fundamentally different nature from extreme cosmic sources promises extraordinary physical insights into the Universe. With the Pierre Auger Observatory, we can significantly contribute to multi-messenger astrophysics by searching for ultra-high ener...

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Main Author: Alvarez-Muñiz Jaime
Format: Article
Language:English
Published: EDP Sciences 2019-01-01
Series:EPJ Web of Conferences
Online Access:https://www.epj-conferences.org/articles/epjconf/pdf/2019/15/epjconf_uhecr18_03002.pdf
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spelling doaj-dc5f2a8b8270495eaa2774fc81bf516b2021-08-02T10:35:28ZengEDP SciencesEPJ Web of Conferences2100-014X2019-01-012100300210.1051/epjconf/201921003002epjconf_uhecr18_03002Multi-messenger Astrophysics at Ultra-High Energy with the Pierre Auger ObservatoryAlvarez-Muñiz Jaime0Departamento de Física de Partículas & Instituto Galego de Física de Altas Enerxías, Universidade de Santiago de CompostelaThe study of correlations between observations of fundamentally different nature from extreme cosmic sources promises extraordinary physical insights into the Universe. With the Pierre Auger Observatory, we can significantly contribute to multi-messenger astrophysics by searching for ultra-high energy particles, particularly neutrinos and photons which, being electrically neutral, point back to their origin. Using Pierre Auger Observatory data, stringent limits at EeV energies have been established on the photon and neutrino fluxes from a large fraction of the sky, probing the production mechanisms of ultra-high energy cosmic rays. The good angular resolution and the neutrino identification capabilities of the Observatory at EeV energies allow the follow-up of events detected in gravitational waves, such as the binary mergers observed with the Advanced LIGO/Virgo detectors, or from other energetic sources of particles.https://www.epj-conferences.org/articles/epjconf/pdf/2019/15/epjconf_uhecr18_03002.pdf
collection DOAJ
language English
format Article
sources DOAJ
author Alvarez-Muñiz Jaime
spellingShingle Alvarez-Muñiz Jaime
Multi-messenger Astrophysics at Ultra-High Energy with the Pierre Auger Observatory
EPJ Web of Conferences
author_facet Alvarez-Muñiz Jaime
author_sort Alvarez-Muñiz Jaime
title Multi-messenger Astrophysics at Ultra-High Energy with the Pierre Auger Observatory
title_short Multi-messenger Astrophysics at Ultra-High Energy with the Pierre Auger Observatory
title_full Multi-messenger Astrophysics at Ultra-High Energy with the Pierre Auger Observatory
title_fullStr Multi-messenger Astrophysics at Ultra-High Energy with the Pierre Auger Observatory
title_full_unstemmed Multi-messenger Astrophysics at Ultra-High Energy with the Pierre Auger Observatory
title_sort multi-messenger astrophysics at ultra-high energy with the pierre auger observatory
publisher EDP Sciences
series EPJ Web of Conferences
issn 2100-014X
publishDate 2019-01-01
description The study of correlations between observations of fundamentally different nature from extreme cosmic sources promises extraordinary physical insights into the Universe. With the Pierre Auger Observatory, we can significantly contribute to multi-messenger astrophysics by searching for ultra-high energy particles, particularly neutrinos and photons which, being electrically neutral, point back to their origin. Using Pierre Auger Observatory data, stringent limits at EeV energies have been established on the photon and neutrino fluxes from a large fraction of the sky, probing the production mechanisms of ultra-high energy cosmic rays. The good angular resolution and the neutrino identification capabilities of the Observatory at EeV energies allow the follow-up of events detected in gravitational waves, such as the binary mergers observed with the Advanced LIGO/Virgo detectors, or from other energetic sources of particles.
url https://www.epj-conferences.org/articles/epjconf/pdf/2019/15/epjconf_uhecr18_03002.pdf
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