Pair neutrino energy loss for nuclei 56^Fe at the late stages of stellar evolution
t Based on the Weinberg-Salam theory, the pair neutrino energy loss rates for nuclei 56^Fe are canvassed for the wide range of density and temperature. The results of ours （QLJ） are compared with those ofBeaudet G, Petrosian V and Salpeter E. E＇s （QBPs）, and it shows that the pair neutrino energy lo...
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| Published in | Chinese physics C Vol. 32; no. 8; pp. 617 - 619 |
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| Main Author | |
| Format | Journal Article |
| Language | English |
| Published |
01.08.2008
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| Subjects | |
| Online Access | Get full text |
| ISSN | 1674-1137 0254-3052 |
| DOI | 10.1088/1674-1137/32/8/005 |
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| Summary: | t Based on the Weinberg-Salam theory, the pair neutrino energy loss rates for nuclei 56^Fe are canvassed for the wide range of density and temperature. The results of ours （QLJ） are compared with those ofBeaudet 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. |
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| Bibliography: | Weinberg-Salam theory, pair neutrino energy loss, stellar evolution 11-5641/O4 P152 |
| ISSN: | 1674-1137 0254-3052 |
| DOI: | 10.1088/1674-1137/32/8/005 |