ELECTRON-ELECTRON NEUTRINO BREMSSTRAHLUNG .I.

被引：5

作者：

CAZZOLA, P

SAGGION, A

机构：

[1] Istituto di Fisica Dell’Universita, Ferrara

[2] Istituto di Fisica Dell’Universita, Padova

来源：

NUOVO CIMENTO DELLA SOCIETA ITALIANA DI FISICA A-NUCLEI PARTICLES AND FIELDS | 1969年 / 63卷 / 01期

关键词：

D O I：

10.1007/BF02963175

中图分类号：

O412 [相对论、场论]; O572.2 [粒子物理学];

学科分类号：

摘要：

We compute the transition probability per unit time and volume relative to processes of the general type a1 + a2 → a3 + a4 + v + v, where a1, a3 are charged baryons or leptons and a2, a4 are leptons, in view of estimating the neutrino energy loss rate in stars due to these processes. A general expression is given for the neutrino energy loss rate in the case of a nondegenerate gas of fermions. © 1969, Società Italiana di Fisica. All rights reserved.

引用

页码：354 / +

页数：1