Revised WMAP constraints on neutrino masses and other extensions of the minimalΛCDMmodel

Recently, two issues concerning the three-year Wilkinson Microwave Anisotropy Probe (WMAP) likelihood code were pointed out. On large angular scales (l30), a suboptimal likelihood approximation resulted in a small power excess. On small angular scales (l300), over-subtraction of unresolved point sources produced a small power deficit. For a minimal six-parameter cosmological model, these two effects conspired to decrease the value of nₛ by ~0.7σ. In this paper, we study the change in preferred parameter ranges for extended cosmological models, including running of nₛ, massive neutrinos, curvature, and the equation of state for dark energy. We also include large-scale structure and supernova data in our analysis. We find that the parameter ranges for αₛ, Ωₖ and w are not much altered by the modified analysis. For massive neutrinos the upper limit on the sum of the neutrino masses decreases from M_ν<1.90 eV to M_ν<1.57 eV when using the modified WMAP code and WMAP data only. We also find that the shift of nₛ to higher values is quite robust to these extensions of the minimal cosmological model.