The AMANDA Search for High Energy Neutrinos From Gamma Ray Bursts

Details The AMANDA Search for High Energy Neutrinos From Gamma Ray Bursts The AMANDA Search for High Energy Neutrinos From Gamma Ray Bursts

Sep 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aipc..727..158h&link_type=abstract

GAMMA-RAY BURSTS: 30 YEARS OF DISCOVERY: Gamma-Ray Burst Symposium. AIP Conference Proceedings, Volume 727, pp. 158-161 (2004).

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Gamma-Ray Sources, Gamma-Ray Bursts, Neutrino, Muon, Pion, And Other Elementary Particle Detectors, Cosmic Ray Detectors

Scientific paper

We have searched three and a half years of AMANDA data for high energy muon neutrinos from gamma-ray bursts (GRBs). The data was recorded from 1997 through 1999 by the AMANDA-B10 detector and in 2000 by the AMANDA-II detector. AMANDA is a Čerenkov detector embedded 1.5 to 2 km deep in the transparent ice of the South Polar plateau. We searched for neutrino candidates from the direction of, and coincident with, GRBs detected by the Burst and Transient Source Experiment (BATSE). The current result is consistent with no signal. A preliminary event upper limit for GRB neutrino emission is presented as well as a description of AMANDA's cubic-kilometer successor, IceCube.

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