Cosmological Constraints from Hubble parameter $H(z)$ and SN Ia observations

Abstract

In this paper, we use a set of observational $H(z)$ data (OHD) to constrain the $\hat{I}›$CDM cosmology. This data set can be derived from the differential ages of the passively evolving galaxies. Meanwhile, the $\mathcal{A}$-parameter, which describes the Baryonic Acoustic Oscillation (BAO) peak, and the newly measured value of the Cosmic Microwave Background (CMB) shift parameter $\mathcal{R}$ are used to present combinational constraints on the same cosmology. The combinational constraints favor an accelerating flat universe while the flat $\hat{I}›$CDM cosmology is also analyzed in the same way. We obtain a result compatible with that by many other independent cosmological observations. We find that the observational $H(z)$ data set is a complementarity to other cosmological probes.

8 pages, 4 figures and 3 tables. Accepted for pubication in Modern Physics Letters A. Any comment welcome