A serach for moderate- and high-energy neturino emission correlated with gamma-ray bursts

Details A serach for moderate- and high-energy neturino emission correlated with gamma-ray bursts A serach for moderate- and high-energy neturino emission correlated with gamma-ray bursts

May 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995apj...444..415b&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 444, no. 1, p. 415-418

Astronomy and Astrophysics

Astrophysics

11

Correlation, Gamma Ray Bursts, High Energy Interactions, Neutrinos, Interstellar Matter, Monte Carlo Method, Particle Flux Density, Statistical Distributions

Scientific paper

A temporal correlation analysis between moderate- (60 Mev less than or equal to Enugreater than or equal to 2500 MeV) and high-energy (Enu 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 numu 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.

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