Published October 19, 1987
| Version v1
Journal article
Neutrino burst from SN1987A and the solar-neutrino puzzle
- 1. Physics Department, Tokyo Institute of Technology, Tokyo 152, Japan
Description
The prompt ν/sub e/ 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 ν/sub e/ 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
Additional details
Publishing Information
- Journal Title
- Phys. Rev. Lett.
- Journal Volume
- 59
- Journal Issue
- 16
- Series
- Phys. Rev. Lett.
- Journal Page Range
- 1864-1867
- ISSN
- 0031-9007
- CODEN
- PRLTA
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 19015411
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Descriptors DEI
- COSMIC RAY FLUX; NEUTRINO DETECTION; NEUTRINO OSCILLATION; NEUTRINO-ELECTRON INTERACTIONS; NEUTRINOS; SOLAR NEUTRINOS; SUPERNOVAE
- Descriptors DEC
- BINARY STARS; DETECTION; ELEMENTARY PARTICLES; ERUPTIVE VARIABLE STARS; FERMIONS; INTERACTIONS; LEPTON-LEPTON INTERACTIONS; LEPTONS; MASSLESS PARTICLES; PARTICLE INTERACTIONS; RADIATION DETECTION; RADIATION FLUX; RADIATIONS; SOLAR PARTICLES; SOLAR RADIATION; STARS; STELLAR RADIATION; VARIABLE STARS