arXiv Analytics

Sign in

arXiv:0709.3684 [hep-th]AbstractReferencesReviewsResources

Hawking Radiation of Black p-Branes from Gravitational Anomaly

Zheng Ze Ma

Published 2007-09-24, updated 2008-08-01Version 2

We investigate the Hawking radiation of black $p$-branes of superstring theories using the method of anomaly cancelation, specially, we use the method of [S. Iso, H. Umetsu and F. Wilczek, {\sl Phys. Rev. Lett.} {\bf 96}, 151302 (2006); {\sl Phys. Rev. D} {\bf 74}, 044017 (2006)]. The metrics of black $p$-branes are spherically symmetric, but not the Schwarzschild type. In order to simplify the calculation, we first make a coordinate transformation to transform the metric to the Schwarzschild type. Then we calculate its energy-momentum flux from the method of anomaly cancelation of the above mentioned references. The obtained energy-momentum flux is equal to a black body radiation, the thermodynamic temperature of the radiation is equal to its Hawking temperature. And we find that the results are not changed for the original non-Schwarzschild type spherically symmetric metric.

Comments: 19 pages Latex, some mistakes corrected
Journal: Int.J.Mod.Phys.A23:2783-2800,2008
Categories: hep-th
Related articles: Most relevant | Search more
arXiv:0710.4766 [hep-th] (Published 2007-10-25, updated 2007-12-15)
Gravitational Anomaly and Hawking Radiation of Brane World Black Holes
arXiv:hep-th/0701048 (Published 2007-01-06, updated 2007-06-07)
Hawking radiation from (2+1)-dimensional BTZ black holes
arXiv:0707.2449 [hep-th] (Published 2007-07-17, updated 2008-01-18)
Hawking Radiation and Covariant Anomalies