Normal Modes of the Stretched Horizon: A Bulk Mechanism for Black Hole Microstate Level Spacing
Chethan Krishnan, Pradipta S. Pathak

TL;DR
This paper explicitly computes black hole normal modes to derive entropy and temperature, revealing a hierarchy in angular quantum numbers that explains area scaling and may relate to string theory.
Contribution
It provides a direct normal mode analysis that reproduces black hole thermodynamics, offering a more conventional statistical mechanics approach compared to previous indirect methods.
Findings
Normal modes reproduce Hawking temperature and entropy.
Angular quantum number degeneracy explains area scaling.
Hierarchy in quantum numbers suggests string theory connection.
Abstract
In 1984, 't Hooft famously used a brickwall (aka stretched horizon) to compute black hole entropy up to a numerical pre-factor. This calculation is sometimes interpreted as due to the entanglement of the modes across the horizon, but more operationally, it is simply an indirect count of the semi-classical modes trapped between the stretched horizon and the angular momentum barrier. Because the calculation was indirect, it needed both the mass and the temperature of the black hole as inputs, to reproduce the area. A more conventional statistical mechanics calculation should be able to get the entropy, once the ensemble is specified (say via the energy, in a microcanonical setting). In this paper, we explicitly compute black hole normal modes in various examples, numerically as well as (in various regimes) analytically. The explicit knowledge of normal modes allows us to reproduce …
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Astrophysical Phenomena and Observations · Cosmology and Gravitation Theories
