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• W2314606145 abstract "We investigate, in the case of a Reissner--Nordstrom black hole, the definitions of gravitational energy and gravitational pressure that naturally arise in the framework of the teleparallel equivalent of general relativity. In particular, we calculate the gravitational energy enclosed by the event horizon of the black hole, $E$, and the radial pressure over it, $p$. With these quantities, we then analyze the thermodynamic relation $dE+pdV$ (as $p$ turns out to be a density, and $dV$ is actually given by $dV=drdensuremath{theta}densuremath{phi}$, in spherical-type coordinates). We compare the latter with the standard first law of black hole dynamics. Also, by identifying $TdS=dE+pdV$, we comment on a possible modification of the standard, Bekenstein--Hawking entropy-area relation due to the gravitational energy and gravitational pressure of the black hole. The infinitesimal variations in question refer to the Penrose process for a Reissner--Nordstrom black hole." @default.
• W2314606145 created "2016-06-24" @default.
• W2314606145 creator A5056788453 @default.
• W2314606145 creator A5072695606 @default.
• W2314606145 date "2013-07-25" @default.
• W2314606145 modified "2023-10-06" @default.
• W2314606145 title "Gravitational energy, gravitational pressure, and the thermodynamics of a charged black hole in teleparallel gravity" @default.
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• W2314606145 doi "https://doi.org/10.1103/physrevd.88.024045" @default.
• W2314606145 hasPublicationYear "2013" @default.
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