Hou, Z. and de Putter, R. and Padin, S. (2014) Constraints on Cosmology from the Cosmic Microwave Background Power Spectrum of the 2500 deg^2 SPTSZ Survey. Astrophysical Journal, 782 (2). Art. No. 74. ISSN 0004637X. doi:10.1088/0004637X/782/2/74. https://resolver.caltech.edu/CaltechAUTHORS:20140519094821926

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Abstract
We explore extensions to the ΛCDM cosmology using measurements of the cosmic microwave background (CMB) from the recent SPTSZ survey, along with data from WMAP7 and measurements of H_0 and baryon acoustic oscillation (BAO). We check for consistency within ΛCDM between these data sets, and find some tension. The CMB alone gives weak support to physics beyond ΛCDM, due to a slight trend relative to ΛCDM of decreasing power toward smaller angular scales. While it may be due to statistical fluctuation, this trend could also be explained by several extensions. We consider running of the primordial spectral index (dn_s /d ln k), as well as two extensions that modify the damping tail power (the primordial helium abundance Y_p and the effective number of neutrino species N_(eff)) and one that modifies the largescale power due to the integrated SachsWolfe effect (the sum of neutrino masses ∑m_ν). These extensions have similar observational consequences and are partially degenerate when considered simultaneously. Of the six oneparameter extensions considered, we find CMB to have the largest preference for dn_s/d ln k with –0.046 < dns/d ln k < –0.003 at 95% confidence, which strengthens to a 2.7σ indication of dn_s/d ln k < 0 from CMB+BAO+H_0. Detectable dn_s/d ln k ≠ 0 is difficult to explain in the context of singlefield, slowroll inflation models. We find N_(eff) = 3.62 ± 0.48 for the CMB, which tightens to N(eff) = 3.71 ± 0.35 from CMB+BAO+H_0. Larger values of N_(eff) relieve the mild tension between CMB, BAO, and H_0. When the SunyaevZel'dovich selected galaxy cluster abundances (SPT_(CL)) data are also included, we obtain N_(eff) = 3.29 ± 0.31. Allowing for ∑m_ν gives a 3.0σ detection of ∑m_ν > 0 from CMB+BAO+H_0 + SPT_(CL). The median value is (0.32 ± 0.11) eV, a factor of six above the lower bound set by neutrino oscillation observations. All data sets except H_0 show some preference for massive neutrinos; data combinations including H_0 favor nonzero masses only if BAO data are also included. We also constrain the twoparameter extensions N_(eff) + ∑m_ν and N_(eff) + Y_p to explore constraints on additional light species and big bang nucleosynthesis, respectively.
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Alternate Title:  Constraints on Cosmology from the Cosmic Microwave Background Power Spectrum of the 2500square degree SPTSZ Survey  
Additional Information:  © 2014 American Astronomical Society. Received 2012 December 26; accepted 2013 November 12; published 2014 January 29. The SPT is supported by the National Science Foundation through grant ANT0638937, with partial support provided by NSF grant PHY1125897, the Kavli Foundation, and the Gordon and Betty Moore Foundation. The McGill group acknowledges funding from the National Sciences and Engineering Research Council of Canada, Canada Research Chairs program, and the Canadian Institute for Advanced Research. R. Keisler acknowledges support from NASA Hubble Fellowship grant HF51275.01, B.A. Benson a KICP Fellowship, M. Dobbs an Alfred P. Sloan Research Fellowship, O. Zahn a BCCP fellowship. This research used resources of the National Energy Research Scientific Computing Center (NERSC), which is supported by the Office of Science of the U.S. Department of Energy under Contract No. DEAC0205CH11231, and the resources of the University of Chicago Computing Cooperative (UC3), supported in part by the Open Science Grid, NSF grant NSF PHY 1148698. We acknowledge the use of the Legacy Archive for Microwave Background Data Analysis (LAMBDA). Support for LAMBDA is provided by the NASA Office of Space Science.  
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Subject Keywords:  cosmic background radiation; cosmological parameters; early universe; inflation  
Issue or Number:  2  
DOI:  10.1088/0004637X/782/2/74  
Record Number:  CaltechAUTHORS:20140519094821926  
Persistent URL:  https://resolver.caltech.edu/CaltechAUTHORS:20140519094821926  
Official Citation:  Constraints on Cosmology from the Cosmic Microwave Background Power Spectrum of the 2500 deg2 SPTSZ Survey Z. Hou et al. 2014 ApJ 782 74  
Usage Policy:  No commercial reproduction, distribution, display or performance rights in this work are provided.  
ID Code:  45816  
Collection:  CaltechAUTHORS  
Deposited By:  Ruth Sustaita  
Deposited On:  19 May 2014 17:31  
Last Modified:  10 Nov 2021 17:16 
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