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arXiv · 1008.0946

Black Hole Entropy: From Shannon to Bekenstein

Subir Ghosh
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Abstract

In this note we have applied directly the Shannon formula for information theory entropy to derive the Black Hole (Bekenstein-Hawking) entropy. Our analysis is semi-classical in nature since we use the (recently proposed [8]) quantum mechanical near horizon mode functions to compute the tunneling probability that goes in to the Shannon formula, following the general idea of [5]. Our framework conforms to the information theoretic origin of Black Hole entropy, as originally proposed by Bekenstein.

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Subir Ghosh. 2010-08-05. Black Hole Entropy: From Shannon to Bekenstein. https://doi.org/10.1007/s10773-011-0859-y

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