Axion bremsstrahlung in dense stars. II - Phonon contributions

Details Axion bremsstrahlung in dense stars. II - Phonon contributions Axion bremsstrahlung in dense stars. II - Phonon contributions

Mar 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988apj...326..241n&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 326, March 1, 1988, p. 241-248.

Astronomy and Astrophysics

Astrophysics

13

Bremsstrahlung, Neutron Stars, Phonons, Stellar Composition, Stellar Radiation, White Dwarf Stars, Coulomb Collisions, Crystal Lattices, Crystal Structure

Scientific paper

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.

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