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A serach for moderate- and high-energy neturino emission correlated with gamma-ray burstsA temporal correlation analysis between moderate- (60 Mev less than or equal to E(sub nu)greater than or equal to 2500 MeV) and high-energy (E(sub nu) greater than or equal to 2000 MeV) neutrino interactions consist of two types: the moderate-energy interactions that are contained within the volume of IMB-3 and the upward-going muons produced by high-energy nu(sub mu) interactions in the rock around the detector. No evidence is found for moderate- or high-energy neutrino emission from GRBs nor for any neutrino/neutrino correlation. The nonobservation of nu/GRB correlations allows upper limits to be placed on the neutrino flux associated with GRBs.
Document ID
19950060171
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1086/175615
Authors
Becker-Szendy, R. (SLAC, Stanford, California United States)
Bratton, C. B. (Cleveland State University Cleveland, Ohio, United States)
Breault, J. (University of California, Irvine, California United States)
Casper, D. (CERN Geneva, Switzerland)
Dye, S. T. (Boston University Boston, Massachusetts, United States)
Gajewski, W. (University of California, Irvine, California United States)
Goldhaber, M. (Brookhaven National Laboratory, Upton, New York United States)
Haines, T. J. (University of Maryland, College Park, Maryland United States)
Halverson, P. G. (University of California, Irvine, California United States)
Kielczewska, D. (University of California, Irvine, California United States)
Date Acquired
August 16, 2013
Publication Date
May 1, 1995
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 444
Issue: 1
ISSN: 0004-637X
Subject Category
Astronomy
Accession Number
95A91770
Distribution Limits
Public
Copyright
Other

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