NEUTRINO EMISSIVITY FROM ELECTRON-POSITRON ANNIHILATION IN HOT MATTER IN A STRONG MAGNETIC-FIELD

被引：2

作者：

AMSTERDAMSKI, P

HAENSEL, P

机构：

[1] Nicolaus Copernicus Astronomical Center, Bartycka 18

来源：

PHYSICAL REVIEW D | 1990年 / 42卷 / 08期

关键词：

D O I：

10.1103/PhysRevD.42.2915

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The neutrino emissivity due to electron-positron annihilation in a strong magnetic field is computed. A strong magnetic field can significantly increase the neutrino emissivity at T109 K. © 1990 The American Physical Society.

引用

页码：2915 / 2918

页数：4

共 6 条

[1] NEUTRINO EMISSION FROM A SUPER-NOVA SHOCK [J].

BETHE, HA ;

APPLEGATE, JH ;

BROWN, GE .

ASTROPHYSICAL JOURNAL, 1980, 241 (01) :343-354

[2]

Canuto V, 1977, FUNDAM COSMIC PHYS, V2, P203

[3] SUPERNOVAE - HOT BUBBLES DRIVE EXPLOSIONS [J].

COLGATE, SA .

NATURE, 1989, 341 (6242) :489-490

[4] STELLAR ENERGY-LOSS RATES IN A CONVERGENT THEORY OF WEAK AND ELECTROMAGNETIC INTERACTIONS [J].

DICUS, DA .

PHYSICAL REVIEW D, 1972, 6 (04) :941-+

[5] NEUTRINO ENERGY-LOSS IN STELLAR INTERIORS [J].

MUNAKATA, H ;

KOHYAMA, Y ;

ITOH, N .

ASTROPHYSICAL JOURNAL, 1985, 296 (01) :197-203

[6]

Yakovlev D. G., 1981, Astronomische Nachrichten, V302, P167, DOI 10.1002/asna.19813020401

← 1 →