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Constraints on perfect fluid and scalar field dark energy models from future redshift surveys

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We discuss the constraints that future photometric and spectroscopic redshift surveys can put on dark energy through the baryon oscillations of the power spectrum. We model the dark energy either with a perfect fluid or a scalar field and take into account the information contained in the linear gro...

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Main Authors: Amendola, Luca (Author) , Quercellini, Claudia (Author) , Giallongo, Emanuele (Author)
Format: Article (Journal)
Language:English
Published: 21 February 2005
In: Monthly notices of the Royal Astronomical Society
Year: 2005, Volume: 357, Issue: 2, Pages: 429-439
ISSN:1365-2966
DOI:10.1111/j.1365-2966.2004.08558.x
Online Access:Verlag, kostenfrei, Volltext: http://dx.doi.org/10.1111/j.1365-2966.2004.08558.x
Verlag, kostenfrei, Volltext: https://academic.oup.com/mnras/article/357/2/429/1369814
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Author Notes:L. Amendola, C. Quercellini, and E. Giallongo
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Constraints on perfect fluid and scalar field dark energy models from future redshift surveys by Amendola, Luca (Author) , Quercellini, Claudia (Author) , Giallongo, Emanuele (Author) ,


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