Black hole thermodynamics from an ensemble-averaged theory
Peng Cheng, Yu-Xiao Liu, and Shao-Wen Wei

TL;DR
This paper proposes an ensemble-averaged approach to quantum gravity path integrals, incorporating geometries with conical singularities, leading to natural emergence of phase transitions and insights into subleading quantum effects in black hole thermodynamics.
Contribution
It introduces an ensemble-averaged framework for black hole thermodynamics that includes geometries with conical singularities, revealing new subleading quantum effects.
Findings
Hawking-Page and black hole phase transitions emerge naturally
Subleading corrections relate to Newton constant contributions
Deviations from classical black hole thermodynamics are identified
Abstract
The path integral approach to a quantum theory of gravity is widely regarded as an indispensable strategy. However, determining what additional elements, beyond black hole or AdS spacetime, should be incorporated into the path integral remains crucial yet perplexing. We argue that the spacetime with a conical singularity in its Euclidean counterpart should be the most important ingredient to append to the path integral. Therefore, physical quantities should be ensemble-averaged over all geometries since they are described by the same Lorentzian metric. When the ensemble average is introduced, the Hawking-Page transition for the Schwarzschild-AdS black hole and the small-large black hole transition for the Reissner-Nordstr\"{o}m-AdS black hole naturally arise as semi-classical approximations, when the size of the black hole system is much larger than the Planck length. Away from the…
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Taxonomy
TopicsCosmology and Gravitation Theories · Black Holes and Theoretical Physics · Relativity and Gravitational Theory
