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Cosmological inflation inF(R,G)gravity
Open accessAbstract
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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Metadata
- Authors
- De Laurentis, M., Paolella, M., & Capozziello, S.
- Venue
- Physical Review D
- Publisher
- American Physical Society (APS)
- 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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