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INTRODUCTION TO MODIFIED GRAVITY AND GRAVITATIONAL ALTERNATIVE FOR DARK ENERGY

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NOJIRI, SHIN'ICHI, ODINTSOV, SERGEI D.·2007·International Journal of Geometric Methods in Modern Physics

Abstract

We review various modified gravities considered as gravitational alternative for dark energy. Specifically, we consider the versions of f(R), f(G) or f(R, G) gravity, model with non-linear gravitational coupling or string-inspired model with Gauss-Bonnet-dilaton coupling in the late universe where they lead to cosmic speed-up. It is shown that some of such theories may pass the Solar System tests. On the same time, it is demonstrated that they have quite rich cosmological structure: they may naturally describe the effective (cosmological constant, quintessence or phantom) late-time era with a possible transition from decceleration to acceleration thanks to gravitational terms which increase with scalar curvature decrease. The possibility to explain the coincidence problem as the manifestation of the universe expansion in such models is mentioned. The late (phantom or quintessence) universe filled with dark fluid with inhomogeneous equation of state (where inhomogeneous terms are originated from the modified gravity) is also described.

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Metadata

Authors
NOJIRI, S., & ODINTSOV, S. D.
Venue
International Journal of Geometric Methods in Modern Physics
Published
2007-02
Volume
04
Issue
01
Pages
115-145
ISSN
  • 0219-8878 (ISSN-L)
  • 1793-6977
OpenAlex
W2949588884
Cited by
2,828
References
1
FWCI
75.69
Type
journal article
Language
en
Open access
green

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NOJIRI, S., & ODINTSOV, S. D. (2007). INTRODUCTION TO MODIFIED GRAVITY AND GRAVITATIONAL ALTERNATIVE FOR DARK ENERGY. International Journal of Geometric Methods in Modern Physics. https://doi.org/10.1142/s0219887807001928

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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

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