Science with Future Cosmic Microwave Background Observations

Details Science with Future Cosmic Microwave Background Observations Science with Future Cosmic Microwave Background Observations

Oct 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009nuphs.194..350d&link_type=abstract

Nuclear Physics B Proceedings Supplements, Volume 194, p. 350-356.

Physics

Nuclear Physics

1

Scientific paper

After the successful measurements of many ground based, balloon-borne and satellite experiments, which started the era of “Precision Cosmology”, Cosmic Microwave Background (CMB) observations are now focusing on two targets: the precision measurement of B-modes in the polarization field, and the measurement of the Sunyaev-Zeldovich effect in distant clusters of galaxies. Polarization measurements represent the best way to probe the very early universe, and the energy scale of inflation. Fine-scale anisotropy measurements, possibly with spectral capabilities, can provide important information on dark matter and dark energy. Here we describe original approaches to these measurements.

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