Published March 1988
| Version v1
Journal article
Axion bremsstrahlung in dense stars. II. Phonon contributions
Description
The energy-loss rate due to axion bremsstrahlung in dense stars such as white dwarfs or neutron stars is calculated by taking into account the phonon contributions in the crystalline lattice state accurately. It is found that the phonon contributions amount to 50-70 percent of the state lattice contributions near the melting temperature. Accurate analytic fitting formulas for the axion bremsstrahlung rate are given. 11 references
Additional details
Publishing Information
- Journal Title
- Astrophys. J.
- Journal Volume
- 326
- Series
- Astrophys. J.
- Journal Page Range
- 241-248
- ISSN
- 0004-637X
- CODEN
- ASJOA
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 19080737
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ANALYTICAL SOLUTION; BREMSSTRAHLUNG; CRYSTAL LATTICES; CRYSTAL STRUCTURE; ENERGY LOSSES; NEUTRON STARS; PHONONS; STELLAR RADIATION; WHITE DWARF STARS
- Descriptors DEC
- DWARF STARS; ELECTROMAGNETIC RADIATION; QUASI PARTICLES; RADIATIONS; STARS