Neutrino-pair bremsstrahlung in dense stars. III - Low-temperature quantum corrections in the liquid metal phase

Details Neutrino-pair bremsstrahlung in dense stars. III - Low-temperature quantum corrections in the liquid metal phase Neutrino-pair bremsstrahlung in dense stars. III - Low-temperature quantum corrections in the liquid metal phase

May 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984apj...280..787i&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 280, May 15, 1984, p. 787-791. Sponsorship: Ministry of Education, Science,

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28

Bremsstrahlung, Liquid Metals, Neutrinos, Neutron Stars, Nuclear Reactions, Stellar Mass, Low Temperature, Quantum Mechanics, Thermodynamic Properties

Scientific paper

Low-temperature quantum corrections to the neutrino-pair bremsstrahlung rate are calculated for dense stellar matter in the liquid metal phase. The corrections arise from the quantum nature of semiclassical ions. The numerical results are parameterized in the form of analytic formulae in order to facilitate applications. The typical corrections are on the order of 5 % or less in the density-temperature region where the present method is valid.

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