Neutrino Energy Loss in Stellar Interiors. VIII. Braaten-Segel Approximation for the Plasma Neutrino Process

Details Neutrino Energy Loss in Stellar Interiors. VIII. Braaten-Segel Approximation for the Plasma Neutrino Process Neutrino Energy Loss in Stellar Interiors. VIII. Braaten-Segel Approximation for the Plasma Neutrino Process

Oct 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996apj...470.1015i&link_type=abstract

Astrophysical Journal v.470, p.1015

Astronomy and Astrophysics

Astronomy

17

Dense Matter, Elementary Particles, Radiation Mechanisms: Thermal, Stars: Interiors

Scientific paper

The accuracy of the Braaten-Segel approximation for the plasma neutrino calculation is quantitatively assessed by comparison with the result obtained by using the Jancovici formula for the dielectric for degenerate electrons. It is found that the Braaten-Segel approximation is a reasonably good one when the plasma neutrino process is the most dominant process; the error is within ˜5% in this case. When the plasma neutrino process is not the most dominant, the accuracy of the Braaten-Segel approximation becomes much poorer.

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