Kerr and Kerr-AdS black shells and black hole entropy
As an operational approach to the Bekenstein-Hawking formula S_{BH}=A/4l_{Pl}^{2} for the black hole entropy, we consider the reversible contraction of a spinning thin shell to its event horizon and find that its thermodynamic entropy approaches $S_{\mathrm{BH}}$. In this sense the shell, called a &...
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| Language: | English en |
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2007
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| Online Access: | http://hdl.handle.net/1828/241 |