Abstract
The existence of the Hawking radiation of theblack hole surely affects spacetime. Here, using athermodynamic approach, to avoid the difficulty offinding the energy-momentum tensor, we obtainexpressions for the energy and entropy of theReissner–Nordstrom black hole (RNBH), and providea better way of solving the backreaction of more complexblack holes.
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Lichun, Z., Ren, Z. & Liao, L. Back Reaction of Charged Black Hole. International Journal of Theoretical Physics 37, 2273–2280 (1998). https://doi.org/10.1023/A:1026610607316
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DOI: https://doi.org/10.1023/A:1026610607316