Emissivity of a hot plasma from photon and plasmon decay

Details Emissivity of a hot plasma from photon and plasmon decay Emissivity of a hot plasma from photon and plasmon decay

Apr 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991phrvl..66.1655b&link_type=abstract

Physical Review Letters, Volume 66, Issue 13, April 1, 1991, pp.1655-1658

Physics

39

Elementary Particle Processes, Electromagnetic Radiation Interactions With Plasma, Neutron Stars

Scientific paper

Previous calculations of the emissivity of a plasma due to the decay of transverse photons and plasmons into neutrino pairs have used dispersion relations that are inaccurate at relativistic temperatures or densities. In the high-temperature limit, the use of the current ultrarelativistic dispersion relations increases the emissivity by a factor of 3.185. This may have a significant effect on the initial cooling rate for the core of a neutron star.

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