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Higher Order Corrections to Black Hole Entropy
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A scheme for calculating corrections to all orders to the entropy of any thermodynamic system due to statistical fluctuations around equilibrium has been developed. It is then applied to the BTZ black hole, AdS-Schwarzschild black Hole and Schwarzschild black Hole in a cavity. The scheme that we present is a model-independent scheme and hence universally applicable to all classical black holes with positive specific heat. It has been seen earlier that the microcanonical entropy of a system can be more accurately reproduced by considering a logarithmic correction to the canonical entropy function. The higher order corrections will be a step further in calculating the microcanonical entropy of a black hole.
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Cited by 1 Pith paper
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Thermodynamics of deformed AdS-Schwarzschild black holes in the presence of Thermal fluctuations
For a deformed AdS-Schwarzschild black hole, increasing the deformation parameter raises the Hawking-Page temperature, while thermal corrections mainly alter small-horizon thermodynamics and leave second-order phase t...
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