SU(2,CMB), the nature of light and accelerated cosmological expansion

Details SU(2,CMB), the nature of light and accelerated cosmological expansion SU(2,CMB), the nature of light and accelerated cosmological expansion

Sep 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006jhw..confe..21h&link_type=abstract

Proceedings of the 29th Johns Hopkins Workshop on current problems in particle theory: strong matter in the heavens. 1-3 August,

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We present quantitative and qualitative arguments in favor of the claim that, within the present cosmological epoch, the U(1)Y factor in the Standard Model is an effective manifestation of SU(2) pure gauge dynamics of Yang-Mills scale Λ ˜ 10-4 eV. Results for the pressure and the energy density in the deconfining phase of this theory, obtained in a nonperturbative and analytical way, support this connection in view of large-angle features inherent in the map of the CMB tempera- ture fluctuations and temperature-polarization cross correlations. Dedicated to Pierre van Baal with best wishes for a soon recuperation.

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