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Quasilinear observables in dark energy cosmologies

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What are the fundamental limitations of reconstructing the properties of dark energy, given cosmological observations in the quasilinear regime in a range of redshifts, to be as precise as required? The aim of this paper is to address this question by constructing model-independent observables, whil...

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Main Authors: Rampf, Cornelius (Author) , Villa, Eleonora (Author) , Amendola, Luca (Author)
Format: Article (Journal)
Language:English
Published: 13 June 2017
In: Physical review
Year: 2017, Volume: 95, Issue: 12, Pages: 123516
ISSN:2470-0029
DOI:10.1103/PhysRevD.95.123516
Online Access:Verlag, Volltext: http://dx.doi.org/10.1103/PhysRevD.95.123516
Verlag, Volltext: https://link.aps.org/doi/10.1103/PhysRevD.95.123516
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Author Notes:Cornelius Rampf, Eleonora Villa, and Luca Amendola
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Quasilinear observables in dark energy cosmologies by Rampf, Cornelius (Author) , Villa, Eleonora (Author) , Amendola, Luca (Author) ,


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