New entropy formula for Kerr black holes
arXiv:1709.09667 · doi:10.1051/epjconf/201816801009
Abstract
We introduce a new entropy formula for Kerr black holes inspired by recent results for 3-dimensional black holes and cosmologies with soft Heisenberg hair. We show that also Kerr-Taub-NUT black holes obey the same formula.
arXiv comment10 pp, talk presented at ICGAC XIII in Seoul
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Cited by in corpus (8)
- Black Hole Entropy and Soft Hair
- Warped Symmetries of the Kerr Black Hole
- Warped Black Holes in Lower-Spin Gravity
- The First Law for the Lorentzian Rotating Taub-NUT
- A class of Taub-NUT-scalar metrics via Ehlers transformations
- Near Horizon Symmetry and Entropy Formula for Kerr-Newman (A)dS Black Holes
- Entropy formula in Einstein-Maxwell-Dilaton theory and its validity for black strings
- A class of charged and charged-Taub-NUT metrics in the presence of a massless scalar field and some of their astrophysical aspects