TeV-PeV neutrinos from giant flares of magnetars and the case of SGR 1806-20

Kunihito Ioka, Soebur Razzaque, Shiho Kobayashi, Peter Mészáros

Research output: Contribution to journalArticlepeer-review

47 Scopus citations

Abstract

We estimate the high-energy neutrino flux from the giant flare of SGR 1806-20 on 2004 December 27, which irradiated Earth with a gamma-ray flux ∼104 times larger than the most luminous gamma-ray bursts (GRBs) ever detected. The Antarctic Cerenkov neutrino detector AMANDA was online 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 also expect detectable EeV cosmic rays and possibly TeV gamma-ray emission in coincidence.

Original languageEnglish (US)
Pages (from-to)1013-1017
Number of pages5
JournalAstrophysical Journal
Volume633
Issue number2 I
DOIs
StatePublished - Nov 10 2005

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

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