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Cited by 458

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The state of the dark energy equation of state

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Melchiorri, Alessandro, Mersini, Laura, Ödman, Carolina J., Trodden, Mark·2003·Physical Review D

Abstract

By combining data from seven cosmic microwave background experiments (including the latest WMAP results) with the Hubble parameter measurement from the Hubble space telescope and luminosity measurements of type Ia supernovae, we demonstrate the bounds on the dark energy equation of state ${w}_{Q}$ to be $\ensuremath{-}1.45<{w}_{Q}<\ensuremath{-}0.74$ at the 95% confidence level. Although our limit on ${w}_{Q}$ is improved with respect to previous analyses, cosmological data do not rule out the possibility that the equation of state parameter ${w}_{Q}$ of the dark energy Q is less than $\ensuremath{-}1.$ We present a tracking model that ensures ${w}_{Q}<~\ensuremath{-}1$ at recent times and discuss the observational consequences.

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Metadata

Authors
Melchiorri, A., Mersini, L., Ödman, C. J., & Trodden, M.
Venue
Physical Review D
Published
2003-08-12
Volume
68
Issue
4
ISSN
  • 0556-2821 (ISSN-L)
  • 1089-4918
OpenAlex
W2075588446
Cited by
458
References
6
FWCI
37.69
Type
journal article
Language
en
Open access
green

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CoChat. (2026). Citation check: The state of the dark energy equation of state. https://app.cochat.ai/papers/10.1103/physrevd.68.043509
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Melchiorri, A., Mersini, L., Ödman, C. J., & Trodden, M. (2003). The state of the dark energy equation of state. Physical Review D. https://doi.org/10.1103/physrevd.68.043509

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