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In Einstein's gravity, the entropy of horizons is proportional to their area.
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T. Padmanabhan, Apoorva Patel [gr-qc/0309053], T. Padmanabhan, Phys. Reports, 406, 49, (2005) [gr-qc/0311036]. The arguments were given for the case of Einstein’s theory in these references but they continue to be valid for any gravitational action
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This result only depends on spherical symmetry and the first law of black hole thermodynamics, and can be easily extended to black holes in Gauss-Bonnet gravity, leading to the same result for minimum increase of entropy
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Maggiore, Michele, Phys. Rev. Lett. 100, 141301, (2008)
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