Neutrino signatures of the supernova - gamma ray burst relationship
We calculate the TeV-PeV neutrino fluxes of gamma-ray bursts associated with supernovae, based on the observed association between GRB 030329 and supernova SN 2003dh. The neutrino spectral flux distributions can test for possible delays between the supernova and the gamma-ray burst events down to mu...
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ftciteseerx:oai:CiteSeerX.psu:10.1.1.255.202 2023-05-15T18:22:15+02:00 Neutrino signatures of the supernova - gamma ray burst relationship Soebur Razzaque Peter Mészáros Eli Waxman The Pennsylvania State University CiteSeerX Archives 2004 application/pdf http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.255.202 http://arxiv.org/pdf/astro-ph/0308239v3.pdf en eng http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.255.202 http://arxiv.org/pdf/astro-ph/0308239v3.pdf Metadata may be used without restrictions as long as the oai identifier remains attached to it. http://arxiv.org/pdf/astro-ph/0308239v3.pdf text 2004 ftciteseerx 2016-01-07T19:54:13Z We calculate the TeV-PeV neutrino fluxes of gamma-ray bursts associated with supernovae, based on the observed association between GRB 030329 and supernova SN 2003dh. The neutrino spectral flux distributions can test for possible delays between the supernova and the gamma-ray burst events down to much shorter timescales than what can be resolved with photons. As an illustrative example, we calculate the probability of neutrino induced muon and electron cascade events in a km scale under-ice detector at the South Pole, from the GRB 030329. Our calculations demonstrate that km scale neutrino telescopes are expected to detect signals that will allow to constrain supernova-GRB models. PACS numbers: 95.85.Ry,96.40.Tv,98.70.Rz,98.70.Sa I. Text South pole Unknown South Pole |
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We calculate the TeV-PeV neutrino fluxes of gamma-ray bursts associated with supernovae, based on the observed association between GRB 030329 and supernova SN 2003dh. The neutrino spectral flux distributions can test for possible delays between the supernova and the gamma-ray burst events down to much shorter timescales than what can be resolved with photons. As an illustrative example, we calculate the probability of neutrino induced muon and electron cascade events in a km scale under-ice detector at the South Pole, from the GRB 030329. Our calculations demonstrate that km scale neutrino telescopes are expected to detect signals that will allow to constrain supernova-GRB models. PACS numbers: 95.85.Ry,96.40.Tv,98.70.Rz,98.70.Sa I. |
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The Pennsylvania State University CiteSeerX Archives |
format |
Text |
author |
Soebur Razzaque Peter Mészáros Eli Waxman |
spellingShingle |
Soebur Razzaque Peter Mészáros Eli Waxman Neutrino signatures of the supernova - gamma ray burst relationship |
author_facet |
Soebur Razzaque Peter Mészáros Eli Waxman |
author_sort |
Soebur Razzaque |
title |
Neutrino signatures of the supernova - gamma ray burst relationship |
title_short |
Neutrino signatures of the supernova - gamma ray burst relationship |
title_full |
Neutrino signatures of the supernova - gamma ray burst relationship |
title_fullStr |
Neutrino signatures of the supernova - gamma ray burst relationship |
title_full_unstemmed |
Neutrino signatures of the supernova - gamma ray burst relationship |
title_sort |
neutrino signatures of the supernova - gamma ray burst relationship |
publishDate |
2004 |
url |
http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.255.202 http://arxiv.org/pdf/astro-ph/0308239v3.pdf |
geographic |
South Pole |
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South Pole |
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South pole |
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South pole |
op_source |
http://arxiv.org/pdf/astro-ph/0308239v3.pdf |
op_relation |
http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.255.202 http://arxiv.org/pdf/astro-ph/0308239v3.pdf |
op_rights |
Metadata may be used without restrictions as long as the oai identifier remains attached to it. |
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1766201630518149120 |