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Centro de Astrofísica da Universidade do Porto
22-26 August 2011, Porto, Portugal

 

First season results from QUIET
Næss, Sigurd (Intitute of theoretical astrophysics, University of Oslo)

Inflationary cosmology predicts the excitation of gravitational waves during inflation, and these will leave a unique signature in the divergence-free part of the CMB polarization (B-modes). The Q/U Imaging ExperimenT (QUIET) is a coherent polarimeter experiment observing the CMB polarization at 43 GHz and 90 GHz in four 250 square degree low-foreground patches on the sky, with overlaps with POLARBEAR and ABS. The analysis of the 43 GHz data was recently completed, measuring the E- and B-mode power spectra in the multipole moment range l = 25-475. We confirm BICEP\'s detection of the first E-mode acoustic peak, while the B-mode spectrum is consistent with zero, giving a tensor-to-scalar ratio of r = 0.35 (+1.06 -0.87), with the lowest level of systematic contamination in the B-mode power so far reported. The 90 GHz data analysis is currently under way, and will significantly improve on the 43 GHz limits.