Black holes in scalar-tensor gravity.
Black holes in scalar-tensor gravity.
复制标题
DOI：
10.1103/physrevlett.108.081103
复制
发表时间：
2011-09
影响因子：
8.6
通讯作者：
T. Sotiriou;V. Faraoni
中科院分区：
文献类型：
--
作者：
T. Sotiriou;V. Faraoni
霍金已经证明，在Brans-Dicke理论（没有势）中作为引力坍缩终点的黑洞与广义相对论中的黑洞没有什么不同。我们把这个证明推广到更一般的标量张量和f（R）引力理论，而不假设除平稳性以外的任何对称性。
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.