Constraints on neutrino mass from Sunyaev-Zeldovich cluster surveys

The presence of massive neutrinos has a characteristic impact on the growth of large scale structures such as galaxy clusters. We forecast on the capability of the number count and power spectrum measured from the ongoing and future Sunyaev-Zeldovich cluster surveys, combined with cosmic microwave background (CMB) observation to constrain the total neutrino mass M-nu in a flat Lambda CDM cosmology. We adopt self-calibration for the mass-observable scaling relation and evaluate constraints for the South Pole Telescope normally and with polarization, Planck, and Atacama Cosmology Telescope Polarization surveys. We find that a sample of approximate to 1000 clusters obtained from the Planck cluster survey plus extra information from CMB lensing extraction could tighten the current upper bound on the sum of neutrino masses to sigma(M nu) = 0.17 eV at 68% C. L. Our analysis shows that cluster number counts and the power spectrum provide complementary constraints, and as a result they help reducing the error bars on M-nu by a factor of 4-8 when both probes are combined. We also show that the main strength of cluster measurements in constraining M-nu is when good control of cluster systematics is available. When applying a weak prior on the mass-observable relations, which can be at reach in the upcoming cluster surveys, we obtain sigma M-nu = 0.48 eV using cluster only probes and, more interestingly, sigma(M nu) = 0.08 eV using cluster + CMB, which corresponds to a S/N approximate to 4 detection for M-nu >= 0.3 eV. We analyze and discuss the degeneracies of M-nu with other parameters and investigate the sensitivity of neutrino mass constraints with various surveys specifications.