The Statistical Mechanics of Hawking Radiation
Noah M. MacKay

TL;DR
This paper proposes a heuristic statistical mechanics model for Hawking radiation, treating particles as timelike entities and linking microstates to the black hole's surface area, offering new insights into black hole evaporation.
Contribution
It introduces a novel statistical model using a worldline Lagrangian formalism to describe Hawking radiation and microstates, bridging quantum and thermodynamic perspectives.
Findings
Recovered Hawking particle mass from the model
Derived the black hole's thermal energy expression
Quantified microstates based on horizon surface area
Abstract
Hawking radiation and black hole thermodynamics are well understood in the frameworks of quantum field theory and general relativity, with contemporary extensions in string theory, AdS/CFT, and loop quantum gravity. However, an open question remains: Can Hawking radiation be consistently described using statistical mechanics? This challenge arises due to the ambiguous quantum nature of Hawking particles and constraints imposed by information conservation. This study develops a heuristic statistical model using a worldine Lagrangian formalism, treating Hawking particles as timelike with an effective mass and following an arbitrary statistical distribution. The flow of information is modeled as a transfer of microstates from the event horizon to the radiation background within a closed ensemble. From this framework, the Hawking particle mass is recovered, and the…
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Taxonomy
TopicsQuantum Electrodynamics and Casimir Effect · Spaceflight effects on biology · Cosmology and Gravitation Theories
