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• W3103242986 abstract "We study the deformation caused by the influence of extrinsic curvature on a vacuum spherically symmetric metric embedded in a five-dimensional bulk. In this sense, we investigate the produced black-holes and derive general characteristics such as their masses, horizons, singularities and thermal properties. As a test, we also study the bending of light near such black-holes analyzing the movement of a test particle and the modification caused by extrinsic curvature on its movement. Accordingly, using the asymptotically conformal flat condition for the extrinsic curvature, an analytical expansion of a set of emph{n}-scalar fields can be defined and we show that the corresponding black holes must be large and constrained in the range of allowed values $-1/2 leq n leq 1.8$. As a result, they are locally thermodynamically stable, but not globally preferred." @default.
• W3103242986 created "2020-11-23" @default.
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• W3103242986 date "2017-05-01" @default.
• W3103242986 modified "2023-09-30" @default.
• W3103242986 title "On classical thermal stability of black holes with a dynamical extrinsic curvature" @default.
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• W3103242986 doi "https://doi.org/10.1016/j.aop.2017.03.006" @default.
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