TeV-PeV Neutrinos from Giant Flares of Magnetars and the Case of SGR 1806-20

We estimate the high energy neutrino flux from the giant flare of SGR 1806-20 on December 27, 2004, which irradiated Earth with a gamma-ray flux ∼ 10 4 times larger than the most luminous gamma-ray bursts (GRBs) ever detected. The Antarctic Cherenkov neutrino detector AMANDA was on-line during the f...

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Main Authors: Kunihito Ioka, Soebur Razzaque, Shiho Kobayashi, Peter Mészáros
Other Authors: The Pennsylvania State University CiteSeerX Archives
Format: Text
Language:English
Published: 2005
Subjects:
Antarctic
The Antarctic
Antarc*
Online Access:http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.255.2243
http://arxiv.org/pdf/astro-ph/0503279v1.pdf
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spelling ftciteseerx:oai:CiteSeerX.psu:10.1.1.255.2243 2023-05-15T13:41:34+02:00 TeV-PeV Neutrinos from Giant Flares of Magnetars and the Case of SGR 1806-20 Kunihito Ioka Soebur Razzaque Shiho Kobayashi Peter Mészáros The Pennsylvania State University CiteSeerX Archives 2005 application/pdf http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.255.2243 http://arxiv.org/pdf/astro-ph/0503279v1.pdf en eng http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.255.2243 http://arxiv.org/pdf/astro-ph/0503279v1.pdf Metadata may be used without restrictions as long as the oai identifier remains attached to it. http://arxiv.org/pdf/astro-ph/0503279v1.pdf text 2005 ftciteseerx 2016-01-07T19:54:13Z We estimate the high energy neutrino flux from the giant flare of SGR 1806-20 on December 27, 2004, which irradiated Earth with a gamma-ray flux ∼ 10 4 times larger than the most luminous gamma-ray bursts (GRBs) ever detected. The Antarctic Cherenkov neutrino detector AMANDA was on-line during the flare, and may either have detected high energy neutrinos for the first time from a cosmic point source, or put constraints on the flare mechanism of magnetars. If TeV neutrinos are detected, one would expect also detectable EeV cosmic rays and possibly TeV gamma-ray emission in coincidence. Subject headings: cosmic rays — gamma rays: bursts — gamma rays: theory — Text Antarc* Antarctic Unknown Antarctic The Antarctic
institution Open Polar
collection Unknown
op_collection_id ftciteseerx
language English
description We estimate the high energy neutrino flux from the giant flare of SGR 1806-20 on December 27, 2004, which irradiated Earth with a gamma-ray flux ∼ 10 4 times larger than the most luminous gamma-ray bursts (GRBs) ever detected. The Antarctic Cherenkov neutrino detector AMANDA was on-line during the flare, and may either have detected high energy neutrinos for the first time from a cosmic point source, or put constraints on the flare mechanism of magnetars. If TeV neutrinos are detected, one would expect also detectable EeV cosmic rays and possibly TeV gamma-ray emission in coincidence. Subject headings: cosmic rays — gamma rays: bursts — gamma rays: theory —
author2 The Pennsylvania State University CiteSeerX Archives
format Text
author Kunihito Ioka
Soebur Razzaque
Shiho Kobayashi
Peter Mészáros
spellingShingle Kunihito Ioka
Soebur Razzaque
Shiho Kobayashi
Peter Mészáros
TeV-PeV Neutrinos from Giant Flares of Magnetars and the Case of SGR 1806-20
author_facet Kunihito Ioka
Soebur Razzaque
Shiho Kobayashi
Peter Mészáros
author_sort Kunihito Ioka
title TeV-PeV Neutrinos from Giant Flares of Magnetars and the Case of SGR 1806-20
title_short TeV-PeV Neutrinos from Giant Flares of Magnetars and the Case of SGR 1806-20
title_full TeV-PeV Neutrinos from Giant Flares of Magnetars and the Case of SGR 1806-20
title_fullStr TeV-PeV Neutrinos from Giant Flares of Magnetars and the Case of SGR 1806-20
title_full_unstemmed TeV-PeV Neutrinos from Giant Flares of Magnetars and the Case of SGR 1806-20
title_sort tev-pev neutrinos from giant flares of magnetars and the case of sgr 1806-20
publishDate 2005
url http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.255.2243
http://arxiv.org/pdf/astro-ph/0503279v1.pdf
geographic Antarctic
The Antarctic
geographic_facet Antarctic
The Antarctic
genre Antarc*
Antarctic
genre_facet Antarc*
Antarctic
op_source http://arxiv.org/pdf/astro-ph/0503279v1.pdf
op_relation http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.255.2243
http://arxiv.org/pdf/astro-ph/0503279v1.pdf
op_rights Metadata may be used without restrictions as long as the oai identifier remains attached to it.
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