Black holes, cosmological solutions, future singularities, and their thermodynamical properties in modified gravity theories

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Abstract

Along this review, we focus on the study of several properties of modified gravity theories, in particular on black-hole solutions and its comparison with those solutions in General Relativity, and on Friedmann-Lemaître-Robertson-Walker metrics. The thermodynamical properties of fourth order gravity theories are also a subject of this investigation with special attention on local and global stability of paradigmatic f(R) models. In addition, we revise some attempts to extend the Cardy-Verlinde formula, including modified gravity, where a relation between entropy bounds is obtained. Moreover, a deep study on cosmological singularities, which appear as a real possibility for some kind of modified gravity theories, is performed, and the validity of the entropy bounds is studied. ©2012 by the authors.

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de la Cruz-Dombriz, A., & Sáez-Gómez, D. (2012). Black holes, cosmological solutions, future singularities, and their thermodynamical properties in modified gravity theories. Entropy, 14(9), 1717–1770. https://doi.org/10.3390/e14091717

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