Statistics of the Sunyaev-Zel'dovich Effect power spectrum

Abstract

Using large numbers of simulations of the microwave sky, incorporating the Cosmic Microwave Background (CMB) and the Sunyaev-Zel'dovich (SZ) effect due to clusters, we investigate the statistics of the power spectrum at microwave frequencies between spherical multipoles of 1000 and 10000. From these virtual sky maps, we find that the spectrum of the SZ effect has a larger standard deviation by a factor of 3 than would be expected from purely Gaussian realizations, and has a distribution that is significantly skewed towards higher values, especially when small map sizes are used. The standard deviation is also increased by around 10 percent compared to the trispectrum calculation due to the clustering of galaxy clusters. We also consider the effects of including residual point sources and uncertainties in the gas physics. This has implications for the excess power measured in the CMB power spectrum by the Cosmic Background Imager and BIMA experiments. Our results indicate that the observed excess could be explained using a lower value of ${\sigma }_8$ than previously suggested, however the effect is not enough to match ${\sigma }_8=0.825$. The uncertainties in the gas physics could also play a substantial role. We have made our maps of the SZ effect available online.

21 pages, 23 figures, 3 tables. Accepted by MNRAS. We have made our maps of the SZ effect available online

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• Simulations of the Microwave Sky
• An accurate tool for the fast generation of dark matter halo catalogs
• The Websky Extragalactic CMB Simulations
• Templates for the Sunyaev-Zel'dovich Angular Power Spectrum
• Modeling Extragalactic Foregrounds and Secondaries for Unbiased Estimation of Cosmological Parameters From Primary CMB Anisotropy
• 30 GHz observations of sources in the VSA fields