Heat Kernel Expansion and Extremal Kerr-Newmann Black Hole Entropy in Einstein-Maxwell Theory

Abstract

We 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.

12 pages

References in corpus (4)

• Logarithmic Corrections to Extremal Black Hole Entropy from Quantum Entropy Function
• The Kerr/CFT correspondence and its extensions: a comprehensive review
• Entanglement entropy of round spheres
• Generalized mirror symmetry and trace anomalies

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