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Modified Gravity with ln R Terms and Cosmic Acceleration

Open access
Nojiri, Shin'ichi, Odintsov, Sergei D.·2004·General Relativity and Gravitation

Abstract

The modified gravity with ln R or R−n (ln R)m terms which grow at small curvature is discussed. It is shown that such a model which has a well-defined Newtonian limit may eliminate the need for dark energy and may provide the current cosmic acceleration. It is demonstrated that R2 terms are important not only for early time inflation but also to avoid the instabilities and the linear growth of the gravitational force. It is very interesting that the condition of no linear growth for gravitational force coincides with the one for scalar mass in the equivalent scalar-tensor theory to be very large. Thus, modified gravity with R2 term seems to be a viable classical theory.

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Metadata

Authors
Nojiri, S., & Odintsov, S. D.
Venue
General Relativity and Gravitation
Published
2004-08
Volume
36
Issue
8
Pages
1765-1780
ISSN
  • 0001-7701 (ISSN-L)
  • 1572-9532
OpenAlex
W2050092510
Cited by
440
References
0
FWCI
18.12
Type
journal article
Language
en
Open access
green

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CoChat. (2026). Citation check: Modified Gravity with ln R Terms and Cosmic Acceleration. https://app.cochat.ai/papers/10.1023/b:gerg.0000035950.40718.48
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Nojiri, S., & Odintsov, S. D. (2004). Modified Gravity with ln R Terms and Cosmic Acceleration. General Relativity and Gravitation. https://doi.org/10.1023/b%3Agerg.0000035950.40718.48

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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.