The Search for High-Energy Neutrinos from Gamma-Ray Bursts with AMANDA

Details The Search for High-Energy Neutrinos from Gamma-Ray Bursts with AMANDA The Search for High-Energy Neutrinos from Gamma-Ray Bursts with AMANDA

May 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aps..apr.s7003k&link_type=abstract

American Physical Society, April Meeting, 2004, May 1-4, 2004, Denver, Colorado April 2004, MEETING ID: APR04, abstract #S7.003

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Scientific paper

The second stage of the Antarctic Muon and Neutrino Detector Array (AMANDA-II), has been searching for signals from atmospheric and astrophysical neutrinos since February of 2000. High energy phenomena such as gamma-ray bursts (GRBs) are the most promising potential sources of such astrophysical neutrinos; by correlating observations with other ground- and satellite-based detectors, AMANDA is able to engage in nearly background-free searches for several dozen GRBs every year. We present here the final results from the 2000 GRB search, along with a comparison to prominent theories of GRB neutrino emission. The current status of GRB searches beyond the year 2000 are also briefly described.

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