Black Holes in Scalar-Tensor Gravity

被引：295
|
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.
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页数：4
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