Neutrino burst from SN1987A and the solar-neutrino puzzle

J. Arafune, M. Fukugita, T. Yanagida, and M. Yoshimura
Phys. Rev. Lett. 59, 1864 – Published 19 October 1987
PDFExport Citation

Abstract

The prompt νe signal from the supernova explosion in the Large Magellanic Cloud presumably detected by Kamiokande II does not necessarily mean that the Mikheyev-Smirnov-Wolfenstein effect on the solar-neutrino flux is not operative. The electron neutrino, once rotated to a different-flavor neutrino in the progenitor star, can come back via the matter-oscillation effect in the Earth, or a residual νe flux from the progenitor can directly hit the detector, saving the Mikheyev-Smirnov-Wolfenstein explanation of the solar-neutrino problem for a range of mixing parameters.

  • Received 14 August 1987

DOI:https://doi.org/10.1103/PhysRevLett.59.1864

©1987 American Physical Society

Authors & Affiliations

J. Arafune, M. Fukugita, T. Yanagida, and M. Yoshimura

  • Physics Department, Tokyo Institute of Technology, Tokyo 152, Japan
  • Research Institute for Fundamental Physics, Kyoto University, Kyoto 606, Japan
  • Physics Department, Tohoku University, Sendai 980, Japan
  • National Laboratory for High Energy Physics (KEK), Tsukuba, Ibaraki 305, Japan

References (Subscription Required)

Click to Expand
Issue

Vol. 59, Iss. 16 — 19 October 1987

Reuse & Permissions
Access Options
Author publication services for translation and copyediting assistance advertisement

Authorization Required


×
×

Images

×

Sign up to receive regular email alerts from Physical Review Letters

Log In

Cancel
×

Search


Article Lookup

Paste a citation or DOI

Enter a citation
×