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Cited by 274

The DOI matches its Crossref record; 65 of the 65 references it cites were found in a registry or an index.

Cosmological inflation inF(R,G)gravity

Open access
De Laurentis, Mariafelicia, Paolella, Mariacristina, Capozziello, Salvatore·2015·Physical Review D

Abstract

Cosmological inflation is discussed in the framework of $F(R,\mathcal{G})$ gravity where $F$ is a generic function of the curvature scalar $R$ and the Gauss--Bonnet topological invariant $\mathcal{G}$. The main feature that emerges in this analysis is the fact that this kind of theory can exhaust all the curvature budget related to curvature invariants without considering derivatives of $R$, ${R}_{\ensuremath{\mu}\ensuremath{\nu}}$, ${R}_{\ensuremath{\sigma}\ensuremath{\mu}\ensuremath{\nu}}^{\ensuremath{\lambda}}$, etc., in the action. Cosmological dynamics results driven by two effective masses (lengths) are related to the $R$ scalaron and the $\mathcal{G}$ scalaron working respectively at early and very early epochs of cosmic evolution. In this sense, a double inflationary scenario naturally emerges.

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Crossref · 10.1103/physrevd.91.083531

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Metadata

Authors
De Laurentis, M., Paolella, M., & Capozziello, S.
Venue
Physical Review D
Published
2015-04-23
Volume
91
Issue
8
ISSN
  • 0556-2821 (ISSN-L)
  • 1550-7998
  • 1550-2368
OpenAlex
W1569511886
Cited by
274
References
65
FWCI
11.38
Type
journal article
Language
en
Open access
green

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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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