Heat Kernel Expansion and Extremal Kerr-Newmann Black Hole Entropy in
Einstein-Maxwell Theory [PDF]
Sayantani Bhattacharyya, Binata Panda, Ashoke SenWe compute the second Seely-DeWitt coefficient of the kinetic operator of the metric and gauge fields in Einstein-Maxwell theory in an arbitrary background field configuration. We then use this result to compute the logarithmic correction to the entropy of an extremal Kerr-Newmann black hole.View original: http://arxiv.org/abs/1204.4061
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