Constraining Dark Energy with Clusters: Complementarity with Other Probes

TL;DR

This paper demonstrates that galaxy cluster counts from ongoing and upcoming surveys can significantly enhance dark energy constraints, complementing other probes and improving the overall figure of merit before the JDEM mission.

Contribution

It shows that optical and Sunyaev-Zel'dovich cluster surveys can double the dark energy constraint precision without prior nuisance parameter knowledge.

Findings

Cluster counts improve the DETF figure of merit by a factor of two.

Forecasts show enhanced precision in dark energy parameters and growth index gamma.

Cluster surveys provide robust, complementary constraints even with systematic uncertainties.

Abstract

The Figure of Merit Science Working Group (FoMSWG) recently forecast the constraints on dark energy that will be achieved prior to the Joint Dark Energy Mission (JDEM) by ground-based experiments that exploit baryon acoustic oscillations, type Ia supernovae, and weak gravitational lensing. We show that cluster counts from on-going and near-future surveys should provide robust, complementary dark energy constraints. In particular, we find that optimally combined optical and Sunyaev-Zel'dovich effect cluster surveys should improve the Dark Energy Task Force (DETF) figure of merit for pre-JDEM projects by a factor of two even without prior knowledge of the nuisance parameters in the cluster mass-observable relation. Comparable improvements are achieved in the forecast precision of parameters specifying the principal component description of the dark energy equation of state parameter as well as in the growth index gamma. These results indicate that cluster counts can play an important complementary role in constraining dark energy and modified gravity even if the associated systematic errors are not strongly controlled.