Black holes with a generalized gravitational action

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Abstract
Microscopic black holes are sensitive to higher-dimension operators in the gravitational action. We compute the influence of these operators on the Schwarzschild solution using perturbation theory. All (time-reversal-invariant) operators of dimension six are included (dimension-four operators do not alter the Schwarzschild solution). Corrections to the relation between the Hawking temperature and the black hole mass are found. The entropy is calculated using the Gibbons-Hawking prescription for the Euclidean path integral and using naive thermodynamic reasoning. These two methods agree; however, the entropy is not equal to ¼ the area of the horizon.

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