Soonkeon Nam and Jong-Dae Park 2009 Class. Quantum Grav. 26 145015 doi:10.1088/0264-9381/26/14/145015
Soonkeon Nam1,2 and Jong-Dae Park3
Show affiliationsIn an insightful approach, Robinson and Wilczek proposed that Hawking radiation can be obtained as the compensation of a breakdown of general covariance and gauge invariance and the radiation is a black body radiation at Hawking temperature. We apply this method to two types of black holes in three-dimensional spacetime, both of which have the form of a metric such that the tt component of the metric is not inverse of the rr component of the metric. The first one is the warped AdS3 black hole in three-dimensional topologically massive gravity with the negative cosmological constant, and the second one is the charged rotating black hole in three dimensions.
04.70.Dy Quantum aspects of black holes, evaporation, thermodynamics
81T13 Yang-Mills and other gauge theories (See also 53C07, 58E15)
83C05 Einstein's equations (general structure, canonical formalism, Cauchy problems)
Issue 14 (21 July 2009)
Received 5 February 2009, in final form 3 June 2009
Published 2 July 2009
Soonkeon Nam and Jong-Dae Park 2009 Class. Quantum Grav. 26 145015
Q E Wang et al 2009 J. Phys.: Condens. Matter 21 485506
Sébastien Blaineau et al 2007 J. Phys.: Condens. Matter 19 455207
Duan Su Hua et al 2009 J. Phys.: Conf. Ser. 188 012018
Y Doi et al 2009 J. Phys.: Conf. Ser. 191 012017
A H AlOmari et al 2009 Physiol. Meas. 30 371
R Stadler et al 2007 Nanotechnology 18 165501
T M Adamo and E T Newman 2009 Class. Quantum Grav. 26 155003
Pedro Lacerda and David C. Jewitt 2007 The Astronomical Journal 133 1393
S Castelletto et al 2004 New J. Phys. 6 87