Pair neutrino energy loss for nuclei 56Fe at the late stages of stellar evolution

Details Pair neutrino energy loss for nuclei 56Fe at the late stages of stellar evolution Pair neutrino energy loss for nuclei 56Fe at the late stages of stellar evolution

Aug 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008chphc..32..617l&link_type=abstract

Chinese Physics C, Volume 32, Issue 8, pp. 617 (2008).

Physics

3

Scientific paper

Based on the Weinberg-Salam theory, the pair neutrino energy loss rates for nuclei 56Fe are canvassed for the wide range of density and temperature. The results of ours (QLJ) are compared with those of Beaudet G, Petrosian V and Salpeter E. E's (QBPS), and it shows that the pair neutrino energy loss rates of QBPS are always larger than QLJ. The QBPS is 12.57%, 12.86%, 14.99%, 19.80% times higher than QLJ corresponding to the temperature T9=0.385, 1.0, 5.0, 10, respectively.
Supported by National Natural Science Foundation of China (10347008) and Scientific Research and Fund of Sichuan Provincial Education Department (2006A079)

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