Non-linear sigma model in de Sitter space
Hiroyuki Kitamoto, Yoshihisa Kitazawa

TL;DR
This paper studies the infra-red behavior of the non-linear sigma model in de Sitter space, revealing time-dependent couplings and a non-perturbative stability of the cosmological constant.
Contribution
It demonstrates the time dependence of the coupling constant and cosmological constant, and establishes a non-perturbative non-renormalization in the large N limit.
Findings
Infra-red logarithms cancel up to two loops.
Coupling constant becomes time dependent.
Cosmological constant remains stable non-perturbatively.
Abstract
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 limit of the non-linear sigma model.
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