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2007

Black hole entropy in modified gravity models

Briscese, F., Elizalde, E.

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An analysis of some modified gravity models, based on the study of pure Schwarzschild and of Schwarzschild-de Sitter black holes, and involving the use of the Noether charge method, is carried out.

Corrections to the classical Einsteinian black hole entropy appear.
It is shown explicitly how the condition of positive entropy can be used in order to constrain the viability of modified gravity theories.

Black hole entropy in modified gravity models · Around

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S. Nojiri and S.D. Odintsov, arXiv:hep-th/0707.1941
Original
1941
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S. Nojiri, S.D. Odintsov. Phys. Rev. D68
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S. Capozziello, Int. J. Mod. Phys. D11
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S. Nojiri and S.D. Odintsov, Gen. Rel. Grav. 36
2004
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F. Faraoni, arXiv:gr-qc/0607116; arXiv:gr-qc/0511094; A. Cruz-Dombriz and A. Dobado, arXiv:gr-qc/0607118; N. Poplawski, gr-qc/0610133; A. Brookfield, C. van de Bruck and L. Hall, arXiv:hep-th/0608015; T. Sotiriou and S. Liberati, arXiv:gr-qc/0604006; A. Bustelo and D. Barraco, arXiv:gr-qc/0611149; G. Olmo, arXiv:gr-qc/0612047; F. Briscese, E. Elizalde, S. Nojiri and S.D. Odintsov, Phys. Lett. B646
Original
2005
Earlier work this paper cites.

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In order to be able to obtain the Schwarzschild solution in modified gravity, the function f ⁡ ( R ) f(R) must satisfy the condition f ⁡ ( 0 ) = 0 f(0)=0

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