Hawking radiation of black holes in infrared modified Hořava–Lifshitz gravity

We study the Hawking radiation of spherically symmetric, asymptotically flat black holes in the infrared modified Hořava–Lifshitz gravity by applying the methods of covariant anomaly cancelation and effective action, as well as the approach of Damour–Ruffini–Sannan’s. These black holes behave as the...

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Bibliographic Details
Published in:The European physical journal. C, Particles and fields Particles and fields, 2010-03, Vol.66 (1-2), p.325-331
Main Authors: Peng, Jun-Jin, Wu, Shuang-Qing
Format: Article
Language:English
Subjects:
Analysis
Astronomy
Astrophysics and Cosmology
Asymptotic properties
Black holes
Elementary Particles
Exact sciences and technology
Gravitation
Hadrons
Hawking radiation
Heavy Ions
Measurement Science and Instrumentation
Nuclear Energy
Nuclear Physics
Nuclear radiation
Physics
Physics and Astronomy
Quantum Field Theories
Quantum Field Theory
Regular Article - Theoretical Physics
Relativity
String Theory
The physics of elementary particles and fields
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Summary:We study the Hawking radiation of spherically symmetric, asymptotically flat black holes in the infrared modified Hořava–Lifshitz gravity by applying the methods of covariant anomaly cancelation and effective action, as well as the approach of Damour–Ruffini–Sannan’s. These black holes behave as the usual Schwarzschild ones of general relativity when the radial distance is very large. We also extend the method of covariant anomaly cancelation to derive the Hawking temperature of the spherically symmetric, asymptotically AdS black holes that represent the analogues of the Schwarzschild AdS ones.
ISSN:1434-6044
1434-6052
DOI:10.1140/epjc/s10052-010-1241-6