Cosmological constraints combining H(z), CMB shift and SNIa observational data

Details Cosmological constraints combining H(z), CMB shift and SNIa observational data Cosmological constraints combining H(z), CMB shift and SNIa observational data

2007-04-20

arxiv.org/abs/0704.2606v2

JCAP 0707:015,2007

Astronomy and Astrophysics

Astrophysics

17 pages, 11 figures; improved discussion, new figures, updated to match published version

Scientific paper

10.1088/1475-7516/2007/07/015

Recently H(z) data obtained from differential ages of galaxies have been proposed as a new geometrical probe of dark energy. In this paper we use those data, combined with other background tests (CMB shift and SNIa data), to constrain a set of general relativistic dark energy models together with some other models motivated by extra dimensions. Our analysis rests mostly on Bayesian statistics, and we conclude that LCDM is at least substantially favoured, and that braneworld models are less favoured than general relativistic ones.

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