STRANGE-PULSAR MODEL

被引：30

作者：

BENVENUTO, OG ^{[1
]}

HORVATH, JE ^{[1
]}

VUCETICH, H ^{[1
]}

机构：

[1] NATL UNIV LA PLATA,FAC CIENCIAS EXACTAS,DEPT FIS,RA-1900 LA PLATA,ARGENTINA

来源：

PHYSICAL REVIEW LETTERS | 1990年 / 64卷 / 07期

关键词：

D O I：

10.1103/PhysRevLett.64.713

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

Deep modifications to the current strange-star structure can occur if strange matter is not stable all the way down to zero pressure. This would be the case, for example, if some stable particle is formed at relatively low pressure and/or temperature. We show that the inclusion of a likely specific candidate particle (quark ) in the strange-matter picture leads to stellar models that present more realistic behavior in the light of current pulsar understanding. © 1990 The American Physical Society.

引用

页码：713 / 716

页数：4

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