Experimental upper limit to the galactic stellar-collapse rate

  • S. T. Dye
  • , J. Annis
  • , R. Becker-Szendy
  • , C. B. Bratton
  • , D. Casper
  • , R. Claus
  • , M. Crouch
  • , S. Errede
  • , W. Gajewski
  • , M. Goldhaber
  • , T. J. Haines
  • , T. W. Jones
  • , D. Kielczewska
  • , W. R. Kropp
  • , J. G. Learned
  • , J. M. Losecco
  • , C. McGrew
  • , J. Matthews
  • , M. S. Mudan
  • , L. R. Price
  • F. Reines, J. Schultz, S. Seidel, D. Sinclair, H. W. Sobel, J. L. Stone, L. R. Sulak, R. Svoboda, G. Thornton, J. C. Van Der Velde

Research output: Contribution to journalArticlepeer-review

Abstract

A search is made for bursts of low-energy (20-60 MeV) neutrino interactions, signaling stellar core collapse, in a large underground water-Cerenkov detector. Over a period of 5.6 years (2.1 live years) no bursts were observed. A 90%-confidence-level (C.L.) upper limit to the rate of stellar collapse in the Galaxy is set at <1.5 yr-1. A limit of <1.1 stellar collapses per year (90% C.L.) is set for a smaller volume of the Galaxy (10 kpc radius) which includes the Galactic center and >50% of the stars in the Milky Way.

Original languageEnglish (US)
Pages (from-to)2069-2072
Number of pages4
JournalPhysical review letters
Volume62
Issue number18
DOIs
StatePublished - 1989

ASJC Scopus subject areas

  • General Physics and Astronomy

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