Stars and halos of degenerate relativistic heavy-neutrino and neutralino matter

被引：40

作者：

Bilic, N ^{[1
]}

Munyaneza, F

Viollier, RD

机构：

[1] Univ Cape Town, Dept Phys, ZA-7700 Rondebosch, South Africa

[2] Rudjer Boskovic Inst, Zagreb 10000, Croatia

来源：

PHYSICAL REVIEW D | 1999年 / 59卷 / 02期

关键词：

D O I：

10.1103/PhysRevD.59.024003

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Heavy-neutrino (or neutralino) stars are studied using the general relativistic equations of hydrostatic equilibrium and the relativistic equation of state for degenerate fermionic matter. The Tolman-Oppenheimer-Volkoff equations are then generalized to include a system of degenerate neutrino and neutralino matter that is gravitationally coupled. The properties and implications of such an interacting astrophysical system are discussed in detail. [S0556-2821(98)05124-8].

引用

页数：10

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