A new pressure-parametrization unified dark fluid model

We propose a new pressure-parametrization model to explain the accelerated expansion of the late-time Universe by considering the baryon matter and dark contents (dark matter and dark energy) as a unified dark fluid. To realize this model more physically, we reconstruct it with the quintessence and...

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Bibliographic Details
Published inThe European physical journal. C, Particles and fields Vol. 77; no. 4; pp. 1 - 9
Main Authors Wang, Deng, Yan, Yang-Jie, Meng, Xin-He
Format Journal Article
LanguageEnglish
Published Berlin/Heidelberg Springer Berlin Heidelberg 01.04.2017
Springer
Springer Nature B.V
SpringerOpen
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Summary:We propose a new pressure-parametrization model to explain the accelerated expansion of the late-time Universe by considering the baryon matter and dark contents (dark matter and dark energy) as a unified dark fluid. To realize this model more physically, we reconstruct it with the quintessence and phantom scalar fields, respectively. We use the recent cosmological data to constrain this model, distinguish it from the standard cosmological model and find that the value of the Hubble constant H 0 = 68 . 34 - 0.92 + 0.53 supports the global measurement by the Planck satellite at the 1 σ confidence level.
ISSN:1434-6044
1434-6052
DOI:10.1140/epjc/s10052-017-4827-4