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      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-Lemaitre-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.

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          Operator content of two-dimensional conformally invariant theories

          John Cardy (1986)
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            Thermodynamics of Spacetime: The Einstein Equation of State

            The Einstein equation is derived from the proportionality of entropy and horizon area together with the fundamental relation \(\delta Q=TdS\) connecting heat, entropy, and temperature. The key idea is to demand that this relation hold for all the local Rindler causal horizons through each spacetime point, with \(\delta Q\) and \(T\) interpreted as the energy flux and Unruh temperature seen by an accelerated observer just inside the horizon. This requires that gravitational lensing by matter energy distorts the causal structure of spacetime in just such a way that the Einstein equation holds. Viewed in this way, the Einstein equation is an equation of state. This perspective suggests that it may be no more appropriate to canonically quantize the Einstein equation than it would be to quantize the wave equation for sound in air.
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              4D Gravity on a Brane in 5D Minkowski Space

              We suggest a mechanism by which four-dimensional Newtonian gravity emerges on a 3-brane in 5D Minkowski space with an infinite size extra dimension. The worldvolume theory gives rise to the correct 4D potential at short distances whereas at large distances the potential is that of a 5D theory. We discuss some phenomenological issues in this framework.
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                Author and article information

                Journal
                11 July 2012
                2012-09-18
                Article
                10.3390/e14091717
                1207.2663
                717b6c49-ded0-424e-a7f7-0fd606b1a2a0

                http://arxiv.org/licenses/nonexclusive-distrib/1.0/

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                Entropy 2012, 14, 1717-1770
                37 pages. arXiv admin note: substantial text overlap with arXiv:1002.1942, arXiv:1109.4519, arXiv:0907.3872. Version published in Entropy Journal
                gr-qc astro-ph.CO hep-th

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