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

Ruth Lazkoz; Elisabetta Majerotto

doi:10.1088/1475-7516/2007/07/015

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arXiv · 0704.2606

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

Ruth Lazkoz·Elisabetta Majerotto

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Abstract

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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Ruth Lazkoz, Elisabetta Majerotto. 2007-07-27. Cosmological constraints combining H(z), CMB shift and SNIa observational data. https://doi.org/10.1088/1475-7516%2F2007%2F07%2F015

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