Ultrahigh Energy Cosmic Rays and Prompt TeV Gamma Rays from Gamma Ray Bursts
Gamma Ray Bursts (GRBs) have been proposed as one {\it possible} class of sources of the Ultrahigh Energy Cosmic Ray (UHECR) events observed up to energies $\gsim10^{20}\ev$. The synchrotron radiation of the highest energy protons accelerated within the GRB source should produce gamma rays up to TeV...
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ftdatacite:10.48550/arxiv.astro-ph/0305185 2023-05-15T18:22:24+02:00 Ultrahigh Energy Cosmic Rays and Prompt TeV Gamma Rays from Gamma Ray Bursts Bhattacharjee, Pijushpani Gupta, Nayantara 2003 https://dx.doi.org/10.48550/arxiv.astro-ph/0305185 https://arxiv.org/abs/astro-ph/0305185 unknown arXiv https://dx.doi.org/10.1007/bf02705371 Assumed arXiv.org perpetual, non-exclusive license to distribute this article for submissions made before January 2004 http://arxiv.org/licenses/assumed-1991-2003/ Astrophysics astro-ph High Energy Physics - Phenomenology hep-ph FOS Physical sciences article-journal Article ScholarlyArticle Text 2003 ftdatacite https://doi.org/10.48550/arxiv.astro-ph/0305185 https://doi.org/10.1007/bf02705371 2022-04-01T16:38:37Z Gamma Ray Bursts (GRBs) have been proposed as one {\it possible} class of sources of the Ultrahigh Energy Cosmic Ray (UHECR) events observed up to energies $\gsim10^{20}\ev$. The synchrotron radiation of the highest energy protons accelerated within the GRB source should produce gamma rays up to TeV energies. Here we briefly discuss the implications on the energetics of the GRB from the point of view of the detectability of the prompt TeV gamma rays of proton-synchrotron origin in GRBs in the up-coming ICECUBE muon detector in the south pole. : 3 pages Latex including 1 ps figure, invited parallel session talk given at the IXth International Symposium on Particles, Strings and Cosmology (PASCOS-03), TIFR, Mumbai, India, Jan 2003, to appear in the proceedings to be published as a special issue of Pramana -- Jour. of Physics, style files included Text South pole DataCite Metadata Store (German National Library of Science and Technology) South Pole |
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Astrophysics astro-ph High Energy Physics - Phenomenology hep-ph FOS Physical sciences |
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Astrophysics astro-ph High Energy Physics - Phenomenology hep-ph FOS Physical sciences Bhattacharjee, Pijushpani Gupta, Nayantara Ultrahigh Energy Cosmic Rays and Prompt TeV Gamma Rays from Gamma Ray Bursts |
topic_facet |
Astrophysics astro-ph High Energy Physics - Phenomenology hep-ph FOS Physical sciences |
description |
Gamma Ray Bursts (GRBs) have been proposed as one {\it possible} class of sources of the Ultrahigh Energy Cosmic Ray (UHECR) events observed up to energies $\gsim10^{20}\ev$. The synchrotron radiation of the highest energy protons accelerated within the GRB source should produce gamma rays up to TeV energies. Here we briefly discuss the implications on the energetics of the GRB from the point of view of the detectability of the prompt TeV gamma rays of proton-synchrotron origin in GRBs in the up-coming ICECUBE muon detector in the south pole. : 3 pages Latex including 1 ps figure, invited parallel session talk given at the IXth International Symposium on Particles, Strings and Cosmology (PASCOS-03), TIFR, Mumbai, India, Jan 2003, to appear in the proceedings to be published as a special issue of Pramana -- Jour. of Physics, style files included |
format |
Text |
author |
Bhattacharjee, Pijushpani Gupta, Nayantara |
author_facet |
Bhattacharjee, Pijushpani Gupta, Nayantara |
author_sort |
Bhattacharjee, Pijushpani |
title |
Ultrahigh Energy Cosmic Rays and Prompt TeV Gamma Rays from Gamma Ray Bursts |
title_short |
Ultrahigh Energy Cosmic Rays and Prompt TeV Gamma Rays from Gamma Ray Bursts |
title_full |
Ultrahigh Energy Cosmic Rays and Prompt TeV Gamma Rays from Gamma Ray Bursts |
title_fullStr |
Ultrahigh Energy Cosmic Rays and Prompt TeV Gamma Rays from Gamma Ray Bursts |
title_full_unstemmed |
Ultrahigh Energy Cosmic Rays and Prompt TeV Gamma Rays from Gamma Ray Bursts |
title_sort |
ultrahigh energy cosmic rays and prompt tev gamma rays from gamma ray bursts |
publisher |
arXiv |
publishDate |
2003 |
url |
https://dx.doi.org/10.48550/arxiv.astro-ph/0305185 https://arxiv.org/abs/astro-ph/0305185 |
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South Pole |
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South Pole |
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South pole |
genre_facet |
South pole |
op_relation |
https://dx.doi.org/10.1007/bf02705371 |
op_rights |
Assumed arXiv.org perpetual, non-exclusive license to distribute this article for submissions made before January 2004 http://arxiv.org/licenses/assumed-1991-2003/ |
op_doi |
https://doi.org/10.48550/arxiv.astro-ph/0305185 https://doi.org/10.1007/bf02705371 |
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1766201819986395136 |