GEOPHYSICS, ASTRONOMY, AND ASTROPHYSICS: Observational Constraints on Purely Kinetic k-Essence Dark Energy Models

Details GEOPHYSICS, ASTRONOMY, AND ASTROPHYSICS: Observational Constraints on Purely Kinetic k-Essence Dark Energy Models GEOPHYSICS, ASTRONOMY, AND ASTROPHYSICS: Observational Constraints on Purely Kinetic k-Essence Dark Energy Models

Aug 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009chphl..26h9501y&link_type=abstract

Chinese Physics Letters, Volume 26, Issue 8, pp. 089501 (2009).

Physics

8

Scientific paper

We consider constraints on purely kinetic k-essence models from the latest observational data (including 182 gold SNIa data, the shift parameter, and the acoustic scale). We find the best-fit values of the parameters are Ωm = 0.37 ± 0.01 and k0 = 0.064 ± 0.013 at 68.3% confidence level. The phase transition from deceleration to acceleration is found to occur at redshift zq = 0 ~ 0.48-0.52 in 68.3% confidence level limits. By applying model-comparison statistics (F-test, AICc, and BIC), we find that the purely kinetic k-essence scenario is favored over the ?CDM model by the combined data. These results are also confirmed by combined data 307 SNIa + R + la.

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