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Constraints on Cosmology from the Cosmic Microwave Background Power Spectrum of the 2500 deg2 SPT-SZ Survey

  • Authors: Z. Hou, C. L. Reichardt, K. T. Story, B. Follin, R. Keisler, K. A. Aird, B. A. Benson, L. E. Bleem, J. E. Carlstrom, C. L. Chang, H.-M. Cho, T. M. Crawford, A. T. Crites, T. de Haan, R. de Putter, M. A. Dobbs, S. Dodelson, J. Dudley, E. M. George, N. W. Halverson, G. P. Holder, W. L. Holzapfel, S. Hoover, J. D. Hrubes, M. Joy, L. Knox, A. T. Lee, E. M. Leitch, M. Lueker, D. Luong-Van, J. J. McMahon, J. Mehl, S. S. Meyer, M. Millea, J. J. Mohr, T. E. Montroy, S. Padin, T. Plagge, C. Pryke, J. E. Ruhl, J. T. Sayre, K. K. Schaffer, L. Shaw, E. Shirokoff, H. G. Spieler, Z. Staniszewski, A. A. Stark, A. van Engelen, K. Vanderlinde, J. D. Vieira, R. Williamson, and O. Zahn

Hou et al. 2014 The Astrophysical Journal 782 74.

  • Provider: AAS Journals

Caption: Figure 12.

Data prefer negative running; this preference remains when additional parameters are freed. We show the marginalized two-dimensional posteriors for n s (at k = 0.025 Mpc −1) and dn s / dln  k. Left panel: the n s dn s / dln  k joint distribution in the ΛCDM+ dn s / dln  k model for different combinations of the data sets. Right panel: the n s dn s / dln  k joint distribution obtained by marginalizing N eff (red) and Y p (blue) for WMAP 7 +SPT data. The purple filled contours show the case with Y p marginalized with the prior Y p < 0.294, the 2σ upper limit of the solar initial helium abundance by Serenelli & Basu (2010). We show the region where | dn s / dln  k| < (1 − n s ) 2 in gray. Inflation models with slow-roll expansion that can be terminated at second order make predictions in this region.

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