Ten Theses on Black Hole Entropy
Rafael D. Sorkin (Perimeter Institute, Syracuse University)

TL;DR
This paper offers a perspective on black hole thermodynamics, suggesting that entropy arises from horizon degrees of freedom, is finite due to spacetime discreteness, and obeys the second law because of non-unitary exterior dynamics.
Contribution
It introduces a novel viewpoint linking horizon structure, spacetime discreteness, and non-unitary evolution to black hole entropy and thermodynamics.
Findings
Entropy derives from horizon degrees of freedom
Spacetime discreteness makes entropy finite
Non-unitary dynamics ensure the second law holds
Abstract
I present a viewpoint on black hole thermodynamics according to which the entropy: derives from horizon "degrees of freedom"; is finite because the deep structure of spacetime is discrete; is "objective" thanks to the distinguished coarse graining provided by the horizon; and obeys the second law of thermodynamics precisely because the effective dynamics of the exterior region is not unitary.
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Cosmology and Gravitation Theories · Noncommutative and Quantum Gravity Theories
