Implications of the CBI Polarization Spectrum

Details Implications of the CBI Polarization Spectrum Implications of the CBI Polarization Spectrum

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aas...205.7307s&link_type=abstract

American Astronomical Society Meeting 205, #73.07; Bulletin of the American Astronomical Society, Vol. 36, p.1470

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The Cosmic Background Imager (CBI), a radio interferometer located in the Chilean Andes, has recently published a spectrum of the polarized power spectrum of the CMB in a range of ℓ ˜ 400-2000. The CBI's polarization spectrum has sufficient sensitivity that it can begin to place limits on allowed cosmological models, independent of the total-intensity spectrum. I discuss some of these limits, including the angular scale of the polarized spectrum and the phase of the polarized spectrum relative to that predicted by the total-intensity.

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