Symmetry non restoration in hot scalar field theories for cosmology and condensed matter

Details Symmetry non restoration in hot scalar field theories for cosmology and condensed matter Symmetry non restoration in hot scalar field theories for cosmology and condensed matter

Jun 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003nuphs.121..226p&link_type=abstract

Nuclear Physics B Proceedings Supplements, Volume 121, p. 226-229.

Physics

Nuclear Physics

Scientific paper

We discuss how symmetry non restoration arises in multi scalar field theories at finite temperatures and present its consequences for a relativistic Higgs multi sector as well as for a non-relativistic model of hard core spheres. For the former, it is known that temperature effects on the couplings do not alter, qualitatively, the phase transition pattern. For the second model we show that symmetry non restoration cannot take place, at high temperatures, when the important temperature dependence of the couplings is considered.

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