Neutrino energy loss in stellar interiors. III. Pair, photo-, plasma, and bremsstrahlung processes
Neutrino energy loss in stellar interiors. III. Pair, photo-, plasma, and bremsstrahlung processes
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DOI：
10.1086/167301
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发表时间：
1989-04
期刊：
影响因子：
--
通讯作者：
N. Itoh;T. Adachi;M. Nakagawa;Y. Kohyama;H. Munakata
中科院分区：
文献类型：
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作者：
N. Itoh;T. Adachi;M. Nakagawa;Y. Kohyama;H. Munakata
本文给出了对应于密度-温度区（1-10 ^ 14 g/cu cm, 10 ^ 7 -10 ^ 11 K）对中微子能量损失率、光、等离子体和轫致辐射过程的详细计算结果。计算是基于温伯格-萨拉姆理论。目前的计算是迄今为止最精确的计算，涵盖了最广泛的密度-温度范围。仔细检查了与以前作品的差异。准备了大量的表格来显示光中微子能量损失率的详细结果。参26。
Detailed results of the calculation of the neutrino energy-loss rates due to pair, photo-, plasma, and bremsstrahlung processes corresponding to the density-temperature regime 1-10 to the 14th g/cu cm, 10 to the 7th - 10 to the 11th K are presented. The calculation is based on the Weinberg-Salam theory. The present calculation is the most accurate calculation to date covering the widest density-temperature regime. The discrepancies with the previous works are carefully examined. Extensive tables are prepared to show the detailed results of the photo-neutrino energy-loss rate. 26 refs.