Primordial non-Gaussianity from the covariance of galaxy cluster counts

Abstract

It has recently been proposed that the large-scale bias of dark matter halos depends sensitively on primordial non-Gaussianity of the local form. In this paper we point out that the strong scale dependence of the non-Gaussian halo bias imprints a distinct signature on the covariance of cluster counts. We find that using the full covariance of cluster counts results in improvements on constraints on the non-Gaussian parameter ${f}_{\mathrm{NL}}$ of 3 (1) orders of magnitude relative to cluster counts ($\mathrm{\text{counts}}+\mathrm{\text{clustering variance}}$) constraints alone. We forecast ${f}_{\mathrm{NL}}$ constraints for the upcoming Dark Energy Survey in the presence of uncertainties in the mass-observable relation, halo bias, and photometric redshifts. We find that the Dark Energy Survey can yield constraints on non-Gaussianity of $\ensuremath{\sigma}({f}_{\mathrm{NL}})\ensuremath{\sim}1--5$ even for relatively conservative assumptions regarding systematics. Excess of correlations of cluster counts on scales of hundreds of megaparsecs would represent a smoking-gun signature of primordial non-Gaussianity of the local type.