The uniqueness of the Bekenstein black hole
The uniqueness of the Bekenstein black hole
复制标题
贝肯斯坦黑洞的独特性
DOI：
10.1063/1.529253
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发表时间：
1991
影响因子：
1.3
通讯作者：
T. Zannias
中科院分区：
文献类型：
--
作者：
B. Xanthopoulos;T. Zannias
一般静态的，球对称的，渐近平坦的爱因斯坦方程耦合到一个共形标量场的解决方案是确定的，它取决于三个自由参数。其中一个参数被要求解决方案允许一个光滑的视界和没有裸曲率奇点，导致黑洞的解决方案发现贝肯斯坦。虽然标量场在视界上是无界的，但这不应被视为一种物理病理。
The general static, spherically symmetric, asymptotically flat solution of the Einstein equations coupled to a conformal scalar field is determined; it depends on three free parameters. One of the parameters is eliminated by the requirement that the solution admits a smooth horizon and no naked curvature singularities, leading to the black hole solution discovered by Bekenstein. Although the scalar field is unbounded on the horizon, this should not be considered as a physical pathology.