Abstract
This paper proposes a generalization of the dependence for the entropy of ‘‘ordinary’’ massive bodies with a relatively small entropy of the event horizon of the covering surface to the case of black holes (BH). By doing this, the nature of the famous Bekenstein bound, that is, the universal limit for entropy, is immediately explained and corrections to the values of the ‘‘gravitational’’ surface temperature are determined for the entire spectrum of astrophysical objects.
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Translated by L. Trubitsyna
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Belinsky, A.V., Shulman, M.H. The Entropy of a Gravitating Body. Moscow Univ. Phys. 75, 496–500 (2020). https://doi.org/10.3103/S0027134920050070
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DOI: https://doi.org/10.3103/S0027134920050070