STELLAR ENERGY-LOSS RATES IN A CONVERGENT THEORY OF WEAK AND ELECTROMAGNETIC INTERACTIONS.
STELLAR ENERGY-LOSS RATES IN A CONVERGENT THEORY OF WEAK AND ELECTROMAGNETIC INTERACTIONS.
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弱电磁相互作用收敛理论中的恒星能量损失率。
DOI：
10.1103/physrevd.6.941
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发表时间：
1972
影响因子：
5
通讯作者：
D. Dicus
中科院分区：
文献类型：
--
作者：
D. Dicus
由于中微子对的产生而导致的恒星能量损失率是根据温伯格的电磁和弱相互作用理论计算的。这里计算的总速率+p g3 与普通弱相互作用理论中计算的速率之比为10，其中不确定性完全来自于缺乏对5'-介子质量的了解。实验速率与普通理论计算速率之比为10′。因此，温伯格的理论给出的数字完全在 8 英寸质量的所有值的实验限制内。
The stellar energy-loss rates due to the production of neutrino pairs are calculated in Weinberg's theory of electromagnetic and weak interactions. The ratio of the total rate +p g3 calculated here to the rate calculated in the ordinary theory of weak interactions is 10 where the uncertainty comes entirely from the lack of knowledge of the 5'-meson mass. The ratio of the experimental rate to the rate calculated in the ordinary theory is 10 ' . Thus Weinberg's theory gives numbers well within the experimental limits for all values of the 8"mass.