Issue |
EAS Publications Series
Volume 30, 2008
Spanish Relativity Meeting - Encuentros Relativistas Españoles , ERE2007: Relativistic Astrophysics and Cosmology
|
|
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Page(s) | 157 - 160 | |
DOI | https://doi.org/10.1051/eas:0830018 | |
Published online | 30 September 2008 |
Spanish Relativity Meeting - Encuentros Relativistas Españoles
, ERE2007:
Relativistic Astrophysics and Cosmology
A. Oscoz, E. Mediavilla and M. Serra-Ricart (eds)
EAS Publications Series, 30 (2008) 157-160
A. Oscoz, E. Mediavilla and M. Serra-Ricart (eds)
EAS Publications Series, 30 (2008) 157-160
Constraining dark energy using H(z), CMB shift and SNIa observational data
1
F. Teorikoa, Euskal Herriko Unibertsitatea, 48080 Bilbao, Spain
2
Institute of Cosmology & Gravitation, University of Portsmouth, Portsmouth PO1 2EG, UK
We constrain a set of general relativistic dark energy models, together with some other models motivated by extra dimensions, using a combination of three background geometry tests: H(z) data, CMB shift and SNIa data. Resting mostly on Bayesian statistics, we conclude that LCDM is at least substantially favored, and that models with extra dimensional motivation are less favored than general relativistic ones.
© EAS, EDP Sciences, 2008