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Cited by 527

The DOI matches its Crossref record; 11 of the 11 references it cites were found in a registry or an index.

Reconciling dark energy models withf(R)theories

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Capozziello, S., Cardone, V. F., Troisi, A.·2005·Physical Review D

Abstract

Higher-order theories of gravity have recently attracted a lot of interest as alternative candidates to explain the observed cosmic acceleration without the need of introducing any scalar field. A critical ingredient is the choice of the function $f(R)$ of the Ricci scalar curvature entering the gravity Lagrangian and determining the dynamics of the Universe. We describe an efficient procedure to reconstruct $f(R)$ from the Hubble parameter $H$ depending on the redshift $z$. Using the metric formulation of $f(R)$ theories, we derive a third order linear differential equation for $f[R(z)]$ which can be numerically solved after setting the boundary conditions on the basis of physical considerations. Since $H(z)$ can be reconstructed from the astrophysical data, the method we present makes it possible to determine, in principle, what is the $f(R)$ theory which best reproduces the observed cosmological dynamics. Moreover, the method allows to reconcile dark energy models with $f(R)$ theories finding out what is the expression of $f(R)$ which leads to the same $H(z)$ of the given quintessence model. As interesting examples, we consider ``quiessence'' (dark energy with constant equation of state) and the Chaplygin gas.

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Metadata

Authors
Capozziello, S., Cardone, V. F., & Troisi, A.
Venue
Physical Review D
Published
2005-02-15
Volume
71
Issue
4
ISSN
  • 0556-2821 (ISSN-L)
  • 1550-7998
  • 1550-2368
OpenAlex
W2142607228
Cited by
527
References
11
FWCI
24.40
Type
journal article
Language
en
Open access
green

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CoChat. (2026). Citation check: Reconciling dark energy models withf(R)theories. https://app.cochat.ai/papers/10.1103/physrevd.71.043503
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Capozziello, S., Cardone, V. F., & Troisi, A. (2005). Reconciling dark energy models withf(R)theories. Physical Review D. https://doi.org/10.1103/physrevd.71.043503

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