Black Holes, Cosmological Solutions, Future Singularities, and Their Thermodynamical Properties in Modified Gravity Theorie


Autoria(s): De la Cruz-Dombriz, Álvaro; Sáez Gómez, Diego
Data(s)

08/02/2014

08/02/2014

18/09/2012

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