NEUTRINO-PAIR BREMSSTRAHLUNG FROM A DEGENERATE ELECTRON GAS

被引：91

作者：

FESTA, GG

RUDERMAN, MA

机构：

[1] City College, City University of New York, New York

[2] New York University, New York

来源：

PHYSICAL REVIEW | 1969年 / 180卷 / 05期

关键词：

D O I：

10.1103/PhysRev.180.1227

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

Neutrino-pair bremsstrahlung is calculated for a hot degenerate electron gas Coulomb scattering on imbedded nuclei in all regimes of possible astrophysical interest. Effects of possible lattice structure among nuclei are included. In the limit of infinite densities where the electrons are very relativistic, the power radiated per unit mass is about 0.8 (T×10-8)6Z2A erg/g sec, independent of density. Therefore, such bremsstrahlung is the dominant neutrino-pair emission process in the high-density limit. © 1969 The American Physical Society.

引用

页码：1227 / &

共 21 条

[1] NEUTRINO PAIR EMISSION BY A STELLAR PLASMA [J].