N. Itoh et al., NEUTRINO ENERGY-LOSS IN STELLAR INTERIORS .8. BRAATEN-SEGEL APPROXIMATION FOR THE PLASMA NEUTRINO PROCESS, The Astrophysical journal, 470(2), 1996, pp. 1015-1017
The accuracy of the Braaten-Segel approximation for the plasma neutrin
o calculation is quantitatively assessed by comparison with the result
obtained by using the Jancovici formula for the dielectric function f
or degenerate electrons. It is found that the Braaten-Segel approximat
ion is a reasonably good one when the plasma neutrino process is the m
ost dominant process; the error is within similar to 5% in this case.
When the plasma neutrino process is not the most dominant, the accurac
y of the Braaten-Segel approximation becomes much poorer.