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Cited by 302

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How to determine an effective potential for a variable cosmological term

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Starobinsky, A. A.·1998·Journal of Experimental and Theoretical Physics Letters

Abstract

It is shown that if a variable cosmological term in the present Universe is described by a scalar field with minimal coupling to gravity and with some phenomenological self-interaction potential V (ϕ), then this potential can be unambiguously determined from the following observational data: either from the behavior of density perturbations in dustlike matter component as a function of redshift (given the Hubble constant additionally), or from the luminosity distance as a function of redshift (given the present density of dustlike matter in terms of the critical value).

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Metadata

Authors
Starobinsky, A. A.
Venue
Journal of Experimental and Theoretical Physics Letters
Published
1998-11
Volume
68
Issue
10
Pages
757-763
ISSN
  • 0021-3640 (ISSN-L)
  • 1090-6487
OpenAlex
W2014738408
Cited by
302
References
1
FWCI
9.06
Type
journal article
Language
en
Open access
green

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CoChat. (2026). Citation check: How to determine an effective potential for a variable cosmological term. https://app.cochat.ai/papers/10.1134/1.567941
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Starobinsky, A. A. (1998). How to determine an effective potential for a variable cosmological term. Journal of Experimental and Theoretical Physics Letters. https://doi.org/10.1134/1.567941

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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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