Black hole mass decreasing due to phantom energy accretion

被引：395

作者：

Babichev, E ^{[1
]}

Dokuchaev, V ^{[1
]}

Eroshenko, Y ^{[1
]}

机构：

[1] Russian Acad Sci, Inst Nucl Res, Moscow 117312, Russia

来源：

PHYSICAL REVIEW LETTERS | 2004年 / 93卷 / 02期

基金：

俄罗斯基础研究基金会;

关键词：

D O I：

10.1103/PhysRevLett.93.021102

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

Solution for a stationary spherically symmetric accretion of the relativistic perfect fluid with an equation of state p(rho) onto the Schwarzschild black hole is presented. This solution is a generalization of Michel solution and applicable to the problem of dark energy accretion. It is shown that accretion of phantom energy is accompanied by the gradual decrease of the black hole mass. Masses of all black holes tend to zero in the phantom energy Universe approaching the Big Rip.

引用

页码：021102 / 1

页数：4

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