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Cited by 415

The DOI matches its Crossref record; 8 of the 8 references it cites were found in a registry or an index.

Scalar-tensor gravity in an accelerating universe

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Esposito-Farèse, Gilles, Polarski, David·2001·Physical Review D

Abstract

We consider scalar-tensor theories of gravity in an accelerating universe. The equations for the background evolution and the perturbations are given in full generality for any parametrization of the Lagrangian, and we stress that apparent singularities are sometimes artifacts of a pathological choice of variables. Adopting a phenomenological viewpoint, i.e., from the observations back to the theory, we show that knowledge of the luminosity distance as a function of redshift up to $z\ensuremath{\sim}1\ensuremath{-}2,$ which is expected in the near future, severely constrains the viable subclasses of scalar-tensor theories. This is due to the requirement of positive energy for both the graviton and the scalar partner. Assuming a particular form for the Hubble diagram, consistent with present experimental data, we reconstruct the microscopic Lagrangian for various scalar-tensor models, and find that the most reasonable ones are obtained if the universe is (marginally) closed.

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Metadata

Authors
Esposito-Farèse, G., & Polarski, D.
Venue
Physical Review D
Published
2001-02-14
Volume
63
Issue
6
ISSN
  • 0556-2821 (ISSN-L)
  • 1089-4918
OpenAlex
W2165174996
Cited by
415
References
8
FWCI
8.15
Type
journal article
Language
en
Open access
green

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CoChat. (2026). Citation check: Scalar-tensor gravity in an accelerating universe. https://app.cochat.ai/papers/10.1103/physrevd.63.063504
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Esposito-Farèse, G., & Polarski, D. (2001). Scalar-tensor gravity in an accelerating universe. Physical Review D. https://doi.org/10.1103/physrevd.63.063504

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