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Cited by 393

The DOI matches its Crossref record; 15 of the 15 references it cites were found in a registry or an index.

Cosmological consequences of a time-dependentΛterm

Carvalho, J. C., Lima, J. A. S., Waga, I.·1992·Physical Review D

Abstract

The phenomenological approach to investigate the decay of the effective cosmological constant, as recently proposed by Chen and Wu, is generalized to include a term proportional to ${H}^{2}$ on the time dependence of $\ensuremath{\Lambda}$, where $H$ is the Hubble parameter. This new term can modify some features of the standard Friedmann-Robertson-Walker model and its free parameter may be adjusted in accordance with nucleosynthesis constraints. The model also allows a deceleration parameter ${q}_{0}$ assuming negative values so that the density parameter ${\ensuremath{\Omega}}_{0}$ is smaller than ⅔ and the age of the Universe is always bigger than ${H}_{0}^{\ensuremath{-}1}$. In these cases, the usual matter creation rate appearing in models with a decaying vacuum energy is smaller than the one present in the steady-state model.

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Metadata

Authors
Carvalho, J. C., Lima, J. A. S., & Waga, I.
Venue
Physical Review D
Published
1992-09-15
Volume
46
Issue
6
Pages
2404-2407
ISSN
0556-2821 (ISSN-L)
OpenAlex
W2039536451
Cited by
393
References
15
FWCI
5.90
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: Cosmological consequences of a time-dependentΛterm. https://app.cochat.ai/papers/10.1103/physrevd.46.2404
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Carvalho, J. C., Lima, J. A. S., & Waga, I. (1992). Cosmological consequences of a time-dependentΛterm. Physical Review D. https://doi.org/10.1103/physrevd.46.2404

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