Published April 1989
| Version v1
Journal article
Neutrino energy loss in stellar interiors. III. Pair, photo-, plasma, and bremsstrahlung processes
Creators
- 1. Tsurumi Univ., Yokohama (Japan)
- 2. Sophia Univ., Tokyo (Japan)
Description
Detailed results of the calculation of the neutrino energy-loss rates due to pair, photo-, plasma, and bremsstrahlung processes corresponding to the density-temperature regime 1-10 to the 14th g/cu cm, 10 to the 7th - 10 to the 11th K are presented. The calculation is based on the Weinberg-Salam theory. The present calculation is the most accurate calculation to date covering the widest density-temperature regime. The discrepancies with the previous works are carefully examined. Extensive tables are prepared to show the detailed results of the photo-neutrino energy-loss rate. 26 refs
Additional details
Publishing Information
- Journal Title
- Astrophysical Journal
- Journal Volume
- 339
- Series
- Astrophys. J.
- Journal Page Range
- 354-364
- ISSN
- 0004-637X
- CODEN
- ASJOA
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 21000708
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ASTROPHYSICS; BREMSSTRAHLUNG; ENERGY LOSSES; NEUTRINOS; PAIR PRODUCTION; PHOTONS; PLASMA; STAR EVOLUTION; STARS
- Descriptors DEC
- BOSONS; ELECTROMAGNETIC RADIATION; ELEMENTARY PARTICLES; FERMIONS; LEPTONS; MASSLESS PARTICLES; PARTICLE PRODUCTION; RADIATIONS