Experimental limit on the flux of relic antineutrinos from past supernovae

Details Experimental limit on the flux of relic antineutrinos from past supernovae Experimental limit on the flux of relic antineutrinos from past supernovae

Jul 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988phrvl..61..385z&link_type=abstract

Physical Review Letters (ISSN 0031-9007), vol. 61, July 25, 1988, p. 385-388. Research supported by the University of Pennsylvan

Physics

29

Antineutrinos, Cerenkov Counters, Electron Energy, Particle Flux Density, Stellar Radiation, Supernovae, Photomultiplier Tubes, Positrons, Red Shift

Scientific paper

The authors report the result of a search in the Kamiokande II detector for the interactions of electron-type antineutrinos in the energy level 19 to 35 MeV. They measure directly a 90%-C.L. upper limit of 226 cm-2sec-1 on the flux of electron antineutrinos with energies in that interval. An upper limit on the total flux of relic antineutrinos from past supernovae is obtained as a function of the effective equilibrium temperature of the relic antineutrino sea.

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