Black Holes, Cosmological Solutions, Future Singularities, and Their Thermodynamical Properties in Modified Gravity Theorie
Data(s) |
08/02/2014
08/02/2014
18/09/2012
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Resumo |
54 p. 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–Lemaˆıtre–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. |
Identificador |
Entropy 14(9) : 1717-1770 (2012) 1099-4300 http://hdl.handle.net/10810/11391 10.3390/e14091717 |
Idioma(s) |
eng |
Publicador |
MDPI |
Relação |
http://www.mdpi.com/1099-4300/14/9/1717 |
Direitos |
© 2012 by the authors; licensee MDPI, Basel, Switzerland. This article is an open access article distributed under the terms and conditions of the Creative Commons Attribution license (http://creativecommons.org/licenses/by/3.0/). info:eu-repo/semantics/openAccess |
Palavras-Chave | #98.80.-k #04.50.+h |
Tipo |
info:eu-repo/semantics/article |