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The European Physical Journal C

, Volume 66, Issue 1–2, pp 325–331 | Cite as

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

  • Jun-Jin Peng
  • Shuang-Qing WuEmail author
Regular Article - Theoretical Physics

Abstract

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.

Keywords

Black Hole High Energy Phys Energy Momentum Tensor Anomaly Cancelation Gravitational Anomaly 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© Springer-Verlag / Società Italiana di Fisica 2010

Authors and Affiliations

  1. 1.College of Physical Science and TechnologyCentral China Normal UniversityWuhanPeople’s Republic of China

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