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Cited by 205

The DOI matches its Crossref record; 7 of the 7 references it cites were found in a registry or an index.

Inflation as a transient attractor inR2cosmology

Maeda, Kei-ichi·1988·Physical Review D
DOI 10.1103/physrevd.37.858
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Abstract

Using the equivalence between the curvature-squared gravity theory and the Einstein theory with a scalar field, we show that the potential in the latter system has a very flat plateau. It turns out that inflation is quite natural but transient in the ${R}^{2}$ cosmology. All anisotropic Bianchi types of space-time except IX approach the de Sitter solution as an attractor, followed by the Friedmann universe after sufficient inflation. We find a similar behavior in higher- (4<D<10) dimensional theories, in which inflation is not exponential-type but power-law-type. The dilaton coupling to the ${R}^{2}$ term is also investigated. The coupling destroys the inflationary solution.

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Metadata

Authors
Maeda, K.-I.
Venue
Physical Review D
Publisher
American Physical Society (APS)
Published
1988-02-15
Volume
37
Issue
4
Pages
858-862
ISSN
0556-2821 (ISSN-L)
DOI
10.1103/physrevd.37.858
OpenAlex
W2101882034
Cited by
205
References
7
FWCI
22.81
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: Inflation as a transient attractor inR2cosmology. https://app.cochat.ai/papers/10.1103/physrevd.37.858
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Maeda, K.-I. (1988). Inflation as a transient attractor inR2cosmology. Physical Review D. https://doi.org/10.1103/physrevd.37.858

Data sources

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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.