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Symmetry non-restoration at high temperature and supersymmetry

We analyse the high temperature behaviour of softly broken supersymmetric theories taking into account the role played by effective non-renormalizable terms generated by the decoupling of superheavy degrees of freedom or the Planck scale physics. It turns out that discrete or continuous symmetries,...

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Detalles Bibliográficos
Autores principales: Dvali, G.R., Tamvakis, K.
Lenguaje:eng
Publicado: 1996
Materias:
Acceso en línea:https://dx.doi.org/10.1016/0370-2693(96)00437-6
http://cds.cern.ch/record/296685
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author Dvali, G.R.
Tamvakis, K.
author_facet Dvali, G.R.
Tamvakis, K.
author_sort Dvali, G.R.
collection CERN
description We analyse the high temperature behaviour of softly broken supersymmetric theories taking into account the role played by effective non-renormalizable terms generated by the decoupling of superheavy degrees of freedom or the Planck scale physics. It turns out that discrete or continuous symmetries, spontaneously broken at intermediate scales, may never be restored, at least up to temperatures of the cutoff scale. There are a few interesting differences from the usual non-restoration in non-supersymmetric theories case where one needs at least two Higgs fields and non-restoration takes place for a range of parameters only. We show that with non-renormalizable interactions taken into account the non-restoration can occur for any nonzero range of parameters even for a single Higgs field. We show that such theories in general solve the cosmological domain wall problem, since the thermal production of the dangerous domain walls is enormously suppressed.
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institution Organización Europea para la Investigación Nuclear
language eng
publishDate 1996
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spelling cern-2966852023-03-14T19:29:36Zdoi:10.1016/0370-2693(96)00437-6http://cds.cern.ch/record/296685engDvali, G.R.Tamvakis, K.Symmetry non-restoration at high temperature and supersymmetryParticle Physics - PhenomenologyWe analyse the high temperature behaviour of softly broken supersymmetric theories taking into account the role played by effective non-renormalizable terms generated by the decoupling of superheavy degrees of freedom or the Planck scale physics. It turns out that discrete or continuous symmetries, spontaneously broken at intermediate scales, may never be restored, at least up to temperatures of the cutoff scale. There are a few interesting differences from the usual non-restoration in non-supersymmetric theories case where one needs at least two Higgs fields and non-restoration takes place for a range of parameters only. We show that with non-renormalizable interactions taken into account the non-restoration can occur for any nonzero range of parameters even for a single Higgs field. We show that such theories in general solve the cosmological domain wall problem, since the thermal production of the dangerous domain walls is enormously suppressed.We analyse the high temperature behaviour of softly broken supersymmetric theories taking into account the role played by effective non-renormalizable terms generated by the decoupling of superheavy degrees of freedom or the Planck scale physics. It turns out that discrete or continuous symmetries, spontaneously broken at intermediate scales, may never be restored, at least up to temperatures of the cutoff scale. There are a few interesting differences from the usual non-restoration in non-supersymmetric theories case where one needs at least two Higgs fields and non-restoration takes place for a range of parameters only. We show that with non-renormalizable interactions taken into account the non-restoration can occur for any nonzero range of parameters even for a single Higgs field. We show that such theories in general solve the cosmological domain wall problem, since the thermal production of the dangerous domain walls is enormously suppressed.We analyse the high-temperature behaviour of softly broken supersymmetric theories, taking into account the role played by effective non-renormalizable terms generated by the decoupling of superheavy degrees of freedom or the Planck scale physics. It turns out that discrete or continuous symmetries, spontaneously broken at intermediate scales, may never be restored, at least up to temperatures of the cutoff scale. There are a few interesting differences from the usual non-restoration in the non-supersymmetric theories case where one needs at least two Higgs fields and non-restoration takes place for a range of parameters only. We show that with non-renormalizable interactions taken into account the non-restoration can occur for any nonzero range of parameters, even for a single Higgs field. We show that such theories in general solve the cosmological domain wall problem, since the thermal production of the dangerous domain walls is enormously suppressed.hep-ph/9602336CERN-TH-96-45CERN-TH-96-045oai:cds.cern.ch:2966851996-02-17
spellingShingle Particle Physics - Phenomenology
Dvali, G.R.
Tamvakis, K.
Symmetry non-restoration at high temperature and supersymmetry
title Symmetry non-restoration at high temperature and supersymmetry
title_full Symmetry non-restoration at high temperature and supersymmetry
title_fullStr Symmetry non-restoration at high temperature and supersymmetry
title_full_unstemmed Symmetry non-restoration at high temperature and supersymmetry
title_short Symmetry non-restoration at high temperature and supersymmetry
title_sort symmetry non-restoration at high temperature and supersymmetry
topic Particle Physics - Phenomenology
url https://dx.doi.org/10.1016/0370-2693(96)00437-6
http://cds.cern.ch/record/296685
work_keys_str_mv AT dvaligr symmetrynonrestorationathightemperatureandsupersymmetry
AT tamvakisk symmetrynonrestorationathightemperatureandsupersymmetry