Interior volume of the charged BTZ black holes

In Schwarzschild spacetime, Reinhart (1973) has shown the hypersurface rss=3M/2 (the subscript stands for “steady-state”) to be the maximal hypersurface. This steady-state radius rss plays a crucial role in defining and evaluating the interior volume of a black hole. In this article, we investigate...

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Bibliographic Details
Main Authors: Suraj Maurya, Sashideep Gutti, Rahul Nigam
Format: Article
Language:English
Published: Elsevier 2024-10-01
Series:Nuclear Physics B
Subjects:
Online Access:http://www.sciencedirect.com/science/article/pii/S0550321324002426
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