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Cited by 264

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ΛCDM epoch reconstruction from F ( R , G ) and modified Gauss–Bonnet gravities

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Elizalde, E, Myrzakulov, R, Obukhov, V V, Sáez-Gómez, D·2010·Classical and Quantum Gravity

Abstract

Dark energy cosmology is considered in a modified Gauss–Bonnet model of gravity with and without a scalar field. It is shown that these generalizations of general relativity endow it with a very rich cosmological structure: it may naturally lead to an effective cosmological constant, quintessence or phantom cosmic acceleration, with the possibility of describing the transition from a decelerating to an accelerating phase explicitly. It is demonstrated here that these modified GB and scalar-GB theories are perfectly viable as cosmological models. They can describe the ΛCDM cosmological era without any need for a cosmological constant. The specific properties of these theories of gravity in different particular cases, such as the de Sitter one, are studied.

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Metadata

Authors
Elizalde, E., Myrzakulov, R., Obukhov, V. V., & Sáez-Gómez, D.
Venue
Classical and Quantum Gravity
Published
2010-03-19
Volume
27
Issue
9
Pages
095007
ISSN
  • 0264-9381 (ISSN-L)
  • 1361-6382
OpenAlex
W2331076783
Cited by
264
References
1
FWCI
8.75
Type
journal article
Language
en
Open access
bronze

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Elizalde, E., Myrzakulov, R., Obukhov, V. V., & Sáez-Gómez, D. (2010). ΛCDM epoch reconstruction from F ( R , G ) and modified Gauss–Bonnet gravities. Classical and Quantum Gravity. https://doi.org/10.1088/0264-9381/27/9/095007

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