Published November 1987
| Version v1
Journal article
Strange stars and the neutrino burst from supernova 1987a
Description
Possibility of strange star formation in the recently discovered LMC supernova is examined. If the proto-neutron star first formed is converted into a strange star about 1 sec after the core bounce, a large energy release with E/sub tot/ -- 10/sup 53/ erg having QCD origin occurs. The high energy ν-bar-events of long duration observed by Kamiokande II and IMB detectors can be naturally understood by the formation of the hot strange star
Additional details
Publishing Information
- Journal Title
- Mod. Phys. Lett. A
- Journal Volume
- 2
- Journal Issue
- 11
- Series
- Mod. Phys. Lett. A.
- Journal Page Range
- 805-810
- ISSN
- 0217-7323
- CODEN
- MPLAE
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 19080798
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ANTINEUTRINOS; COSMIC NEUTRINOS; NEUTRON STARS; QUANTUM CHROMODYNAMICS; STAR EVOLUTION; SUPERNOVAE
- Descriptors DEC
- ANTILEPTONS; ANTIMATTER; ANTIPARTICLES; BINARY STARS; COSMIC RADIATION; ELEMENTARY PARTICLES; ERUPTIVE VARIABLE STARS; FERMIONS; FIELD THEORIES; IONIZING RADIATIONS; LEPTONS; MASSLESS PARTICLES; MATTER; NEUTRINOS; QUANTUM FIELD THEORY; RADIATIONS; STARS; VARIABLE STARS