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Logarithmic correction to the Bekenstein-Hawking entropy

Romesh K. Kaul·Parthasarathi Majumdar
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Abstract

The exact formula derived by us earlier for the entropy of a four dimensional non-rotating black hole within the quantum geometry formulation of the event horizon in terms of boundary states of a three dimensional Chern-Simons theory, is reexamined for large horizon areas. In addition to the {\it semiclassical} Bekenstein-Hawking contribution to the area obtained earlier, we find a contribution proportional to the logarithm of the area together with subleading corrections that constitute a series in inverse powers of the area.

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Romesh K. Kaul, Parthasarathi Majumdar. 2000-06-14. Logarithmic correction to the Bekenstein-Hawking entropy. https://doi.org/10.1103/physrevlett.84.5255

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