TeV neutrinos from SN1987A (Shelton).

Details TeV neutrinos from SN1987A (Shelton). TeV neutrinos from SN1987A (Shelton).

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ncimb.102..583a&link_type=abstract

Nuovo Cimento B, Vol. 102, No. 6, p. 583 - 592

Physics

3

Supernovae: Neutrinos, Supernova 1987A In Lmc

Scientific paper

Cosmic rays injected into a supernova remnant can produce neutrinos by interactions on the gas. The authors give a simple analytic approximation for the neutrino flux, from which the rate of muons produced in the rock surrounding a plane detector can be estimated. If the power in accelerated protons is near the maximum that might be expected from a rapidly rotating neutron star, the signal could be detectable with underground detectors with projected area of order 100 m2, but only within the first few years.

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