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.

中文翻译：

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引力体的熵

摘要

本文提出了对“普通”质量体的熵的依赖性的一般化，其中覆盖表面的事件视界对黑洞（BH）情况的熵相对较小。通过这样做，立即说明了著名的贝肯斯坦界的性质，即熵的通用极限，并确定了整个天体物理物体的“引力”表面温度值的校正。