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

  • We present quantitative and qualitative arguments in favor of the claim that, within the present cosmological epoch, the U(1)gamma factor in the Standard Model is an effective manifestation of SU(2) pure gauge dynamics of Yang-Mills scale Lambda ~ 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 temperature fluctuations and temperature-polarization cross correlations.

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Author:Ralf Hofmann
URN:urn:nbn:de:hebis:30-45271
DOI:https://doi.org/10.22323/1.022.0021
ISSN:1824-8039
ArXiv Id:http://arxiv.org/abs/hep-ph/0508176
Parent Title (English):Proceedings of Science
Publisher:SISSA
Place of publication:Trieste
Document Type:Article
Language:English
Year of Completion:2006
Year of first Publication:2005
Publishing Institution:Universit├Ątsbibliothek Johann Christian Senckenberg
Creating Corporation:29th Johns Hopkins Workshop on current problems in particle theory: strong matter in the heavens, 1-3 August, Budapest
Release Date:2007/06/13
Volume:2005
Page Number:13
First Page:1
Last Page:13
Note:
Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-ShareAlike Licence.
Note:
v3: consequences of a modification of the evolution equation for the coupling implemented
Source:Proceedings of Science (JHW2005)021 ; http://www.arxiv.org/abs/hep-ph/0508176. - 29th Johns Hopkins workshop on current problems in particle theory: strong matter in the heavens, 1-3 August, Budapest
HeBIS-PPN:188841873
Institutes:Physik / Physik
Dewey Decimal Classification:5 Naturwissenschaften und Mathematik / 53 Physik / 530 Physik
Licence (German):License LogoCreative Commons - Namensnennung-Keine kommerzielle Nutzung-Weitergabe unter gleichen Bedingungen