Hawking radiation and Hawking flux from spherical reduction
W. Kummer, D.V. Vassilevich

TL;DR
This paper demonstrates how Hawking radiation and flux can be derived from spherically reduced actions using heat kernel methods, addressing a controversy about the D=2 anomaly and presenting a generalized Polyakov action with a dilaton.
Contribution
It shows the connection between Hawking radiation and spherically reduced actions, clarifies the D=2 anomaly controversy, and introduces a generalized Polyakov action with a dilaton.
Findings
Reproduces Hawking flux from spherically reduced action
Addresses the D=2 anomaly controversy
Presents a generalized Polyakov action with dilaton
Abstract
Using heat kernel techniques we show that the relation between Hawking temperature and radiation flux known from Einstein gravity in D dimensions can be reproduced from the spherically reduced action. A recent controversy regarding the D=2 anomaly for that case is discussed. The generalized effective Polyakov action in the presence of a dilaton field is presented.
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Taxonomy
TopicsCosmology and Gravitation Theories · Quantum Electrodynamics and Casimir Effect · Advanced Thermodynamics and Statistical Mechanics
