Using bright ellipticals as dark energy cosmic clocks

The age of the Universe has been increasingly constrained by different techniques such as the observations of type Ia supernovae at high redshift or dating the stellar populations of globular clusters. In this paper we present a complementary approach using the colours of the brightest elliptical galaxies in clusters over a wide redshift range (z<1). We put new and independent bounds on the dark energy equation of state parameterised by a constant pressure-to-density ratio as well as by a parameter which determines the scaling between the matter and dark energy densities. We find that accurate estimates of the metallicities of the stellar populations in moderate and high redshift cluster galaxies can pose stringent constraints on the parameters which describe the dark energy equation of state. Our results are in good agreement with the analysis of dark energy models using SNIa data as constraint. Accurate estimates of the metallicities of stellar populations in cluster galaxies at z<2 will make this approach a powerful complement to studies of cosmological parameters using high redshift SNIa.