arXiv Analytics

Sign in

arXiv:1012.5930 [hep-th]AbstractReferencesReviewsResources

Non-linear sigma model in de Sitter space

Hiroyuki Kitamoto, Yoshihisa Kitazawa

Published 2010-12-29, updated 2011-09-22Version 3

We investigate infra-red dynamics of the non-linear sigma model in de Sitter space. In the presence of minimally coupled massless scalar fields, the de Sitter symmetry is dynamically broken and physical constants become time dependent. We find that the coupling constant of the non-linear sigma model becomes time dependent. The power counting arguments of the infra-red logarithms indicate that the cosmological constant also acquires time dependence. We find that such infra-red logarithms cancel out in a perturbative investigation up to the two loop level. We further demonstrate a non-perturbative non-renormalization of the cosmological constant in the large $N$ limit of the non-linear sigma model.

Comments: 34pages
Journal: Phys.Rev.D83:104043,2011
Categories: hep-th, astro-ph.CO
Related articles: Most relevant | Search more
arXiv:1101.4888 [hep-th] (Published 2011-01-25)
The holographic principle and the cosmological constant
arXiv:hep-th/0310075 (Published 2003-10-08)
Vacuum Polarization in an Anti-de Sitter Space as an Origin for a Cosmological Constant in a Brane World
arXiv:1010.1106 [hep-th] (Published 2010-10-06)
The cosmological constant and the relaxed universe