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Black Holes, Cosmological Solutions, Future Singularities, and Their Thermodynamical Properties in Modified Gravity Theories
Open accessAbstract
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.
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Cites
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Cited by
Modified gravity theories on a nutshell: Inflation, bounce and late-time evolution
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Cosmological inflation inF(R,G)gravity
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Metadata
- Authors
- De la Cruz-Dombriz, A., & Sáez-Gómez, D.
- Venue
- Entropy
- Publisher
- MDPI AG
- Published
- 2012-09-18
- Volume
- 14
- Issue
- 9
- Pages
- 1717-1770
- ISSN
- 1099-4300 (ISSN-L)
- OpenAlex
- W2005030502
- Cited by
- 334
- References
- 14
- FWCI
- 10.81
- Type
- journal article
- Language
- en
- Open access
- gold
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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.