Search for High Energy Neutrino Emission from Gamma-Ray Bursts with the A ntarctic Muon and Neutrino Detector Array (AMANDA)

The photo-meson production of pions by shock-accelerated protons could generate a burst of ~10^14 eV neutrinos from gamma-ray bursts (GRBs) observable in the Antarctic Muon and Neutrino Detector Array (AMANDA) or its larger successors. Measurement of this flux can test the hypothesis that GRBs are t...

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Bibliographic Details
Published inarXiv.org
Main Author Bay, Ryan C
Format Paper
LanguageEnglish
Published Ithaca Cornell University Library, arXiv.org 16.08.2000
Subjects
Cosmic rays
Equivalence principle
Fluence
Gamma ray bursts
Gamma rays
Limiting speed
Muons
Neutrinos
Northern Hemisphere
Particle production
Pions
Windows (intervals)
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Summary:The photo-meson production of pions by shock-accelerated protons could generate a burst of ~10^14 eV neutrinos from gamma-ray bursts (GRBs) observable in the Antarctic Muon and Neutrino Detector Array (AMANDA) or its larger successors. Measurement of this flux can test the hypothesis that GRBs are the sources of the highest-energy cosmic rays, and GRB neutrinos could permit high-precision experiments in neutrino limiting speed, neutrino oscillations, and the weak equivalence principle. Neutrino emission can be expected primarily during the prompt gamma-ray flash and satellite coincidence provides a well-defined window in position and time that can be searched for an excess of upgoing muon events in AMANDA from bursts in the Northern Hemisphere. Using an event quality analysis to further reduce background in a sample of 78 GRBs from the 1997 AMANDA-B10 data set, I find a fluence limit of (E_nu)^2 (dN_nu)/(dE_nu)<3.8*10^-4 min(1,E_nu/E_break) [TeV cm^-2] per average burst, which is orders of magnitude more stringent than in similar previous searches.
ISSN:2331-8422