Black Holes in Scalar-Tensor Gravity

被引：312

作者：

Sotiriou, Thomas P. ^{[1
,2
]}

Faraoni, Valerio ^{[3
,4
]}

机构：

[1] SISSA ISAS, I-34136 Trieste, Italy

[2] Ist Nazl Fis Nucl, Sez Trieste, Trieste, Italy

[3] Bishops Univ, Dept Phys, Sherbrooke, PQ J1M 1Z7, Canada

[4] Bishops Univ, STAR Res Cluster, Sherbrooke, PQ J1M 1Z7, Canada

来源：

PHYSICAL REVIEW LETTERS | 2012年 / 108卷 / 08期

基金：

加拿大自然科学与工程研究理事会;

关键词：

GRAVITATIONAL COLLAPSE;

D O I：

10.1103/PhysRevLett.108.081103

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

Hawking has proven that black holes which are stationary as the end point of gravitational collapse in Brans-Dicke theory (without a potential) are no different than in general relativity. We extend this proof to the much more general class of scalar-tensor and f(R) gravity theories, without assuming any symmetries apart from stationarity.

引用

页数：4

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