Castro, P.G. and Ade, P. and Bock, J. and Bowden, M.L. and Brown, M.L. and Cahill, G. and Church, S. and Culverhouse, T. and Friedman, R.B. and Ganga, K. and Gear, W.K. and Gupta, S. and Hinderks, J. and Kovac, J. and Lange, A.E. and Leitch, E. and Melhuish, S.J. and Memari, Y. and Murphy, J.A. and Orlando, A. and Pryke, C. and Schwarz, R. and O'Sullivan, C. and Piccirillo, L. and Taylor, A.N. and Thompson, K.L. and Turner, A.H. and Wu, E.Y.S. and Zemcov, M.
Cosmological Parameters from the QUaD CMB Polarization Experiment.
Astrophysical Journal, 701 (2).
In this paper, we present a parameter estimation analysis of the polarization and temperature power spectra from the
second and third season of observations with the QUaD experiment. QUaD has for the first time detected multiple
acoustic peaks in the E-mode polarization spectrum with high significance. Although QUaD-only parameter
constraints are not competitive with previous results for the standard six-parameter ΛCDM cosmology, they do
allow meaningful polarization-only parameter analyses for the first time. In a standard six-parameter ΛCDM
analysis, we find the QUaD TT power spectrum to be in good agreement with previous results. However, the QUaD
polarization data show some tension with ΛCDM. The origin of this 1σ–2σ tension remains unclear, and may point
to new physics, residual systematics, or simple random chance. We also combine QUaD with the five-year WMAP
data set and the SDSS luminous red galaxies 4th data release power spectrum, and extend our analysis to constrain
individual isocurvature mode fractions, constraining cold dark matter density, αcdmi < 0.11 (95% confidence limit
(CL)), neutrino density, αndi < 0.26 (95% CL), and neutrino velocity, αnvi < 0.23 (95% CL), modes. Our analysis
sets a benchmark for future polarization experiments.
||cosmic microwave background; cosmological parameters; methods statistical; polarization;
||Science & Engineering > Experimental Physics
Dr. Anthony Murphy
||18 Aug 2010 16:03
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||American Astronomical Society
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