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arxiv: 1109.4892 · v2 · pith:RVFCRUI2new · submitted 2011-09-22 · ✦ hep-th · astro-ph.CO

Infra-red effects of Non-linear sigma model in de Sitter space

classification ✦ hep-th astro-ph.CO
keywords infra-redlogarithmssittersymmetrybreakingcancellargeloop
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We extend our investigation on a possible de Sitter symmetry breaking mechanism in non-linear sigma models. The scale invariance of the quantum fluctuations could make the cosmological constant time dependent signaling the de Sitter symmetry breaking. To understand such a symmetry breaking mechanism, we investigate the energy-momentum tensor. We show that the leading infra-red logarithms cancel to all orders in perturbation theory in a generic non-linear sigma model. When the target space is an N sphere, the de Sitter symmetry is preserved in the large N limit. For a less symmetric target space, the infra-red logarithms appear at the three loop level. However there is a counter term to precisely cancel it. The leading infra-red logarithms do not cancel for higher derivative interactions. We investigate such a model in which the infra-red logarithms first appear at the three loop level. A nonperturbative investigation in the large N limit shows that they eventually grow as large as the one loop effect.

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