NEUTRON-STARS - GRAVEYARD OF CHARGED DARK MATTER

被引：140

作者：

GOULD, A ^{[1
]}

DRAINE, BT ^{[1
]}

ROMANI, RW ^{[1
]}

NUSSINOV, S ^{[1
]}

机构：

[1] TEL AVIV UNIV,IL-69978 TEL AVIV,ISRAEL

来源：

PHYSICS LETTERS B | 1990年 / 238卷 / 2-4期

基金：

美国国家科学基金会;

关键词：

D O I：

10.1016/0370-2693(90)91745-W

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

If charged massive particles (102 GeV {less-than or approximate} mx {less-than or approximate} 1016 GeV) made up the dark halo of the Galaxy, they would be present in large numbers in disk stars. In neutron stars theses particles would form a black hole and destroy the star on time scales {less-than or approximate} 10 yr. Charged massive particles therefore cannot make up even a tiny fraction ({less-than or approximate}10-5) of the dark halo. © 1990.

引用

页码：337 / 343

页数：7

共 11 条

[1]

BASDEVANT JL, 1989, DPHPE8919 PREPR

[2]

CHIVUKULA S, 1989, BUHEP89031 BOST U PR

[3] LOW ENERGY STOPPING POWER OF ATOMIC HYDROGEN [J].

DALGARNO, A .

PROCEEDINGS OF THE PHYSICAL SOCIETY OF LONDON, 1960, 75 (483) :374-377

[4] CHARGED DARK MATTER [J].

DERUJULA, A ;

GLASHOW, SL ;

SARID, U .

NUCLEAR PHYSICS B, 1990, 333 (01) :173-194

[5]

DIMOPOLOUS S, 1989, UNPUB PHYS REV D

[6]

GOLDMAN N, 1989, IN PRESS PHYS REV D

[7] PARTICLE CREATION BY BLACK-HOLES [J].

HAWKING, SW .

COMMUNICATIONS IN MATHEMATICAL PHYSICS, 1975, 43 (03) :199-220

[8]

KULKARNI SR, 1988, PHYSICS COMPACT OBJE, P343

[9] STAR FORMATION IN MOLECULAR CLOUDS - OBSERVATION AND THEORY [J].

SHU, FH ;

ADAMS, FC ;

LIZANO, S .

ANNUAL REVIEW OF ASTRONOMY AND ASTROPHYSICS, 1987, 25 :23-81

[10]

Teukolsky S. A., 1983, BLACK HOLES WHITE DW, DOI [DOI 10.1002/9783527617661, 10.1002/9783527617661]

← 1 2 →