Higgs effect in Conformal Cosmology & Supernova Data

Simple item page
dc.creatorBarbashov, B. M.
dc.creatorGlinka, L. A.
dc.creatorPervushin, V. N.
dc.creatorZakharov, A. F.
dc.date2007-04-30
dc.date.accessioned2026-07-07T07:58:46Z
dc.date.available2026-07-07T07:58:46Z
dc.descriptionThe formulation of the Higgs effect is studied in the Glashow--Weinberg--Salam Standard Model, where the constant part of the Higgs potential is identified with the zeroth mode of the Higgs field. In this model, the Coleman--Weinberg effective potential obtained from the vacuum--vacuum transition amplitude is equal to unity at the extremum. This extremum immediately removes tremendous vacuum cosmological density and predicts mass of Higgs field. In this model, the kinetic energy density of the Higgs field and any scalar field can be treated as the rigid state origin that explains Supernova data in the conformal cosmology without the $Λ$ term.
dc.description8 pages, talk on Tenth European Meeting From the Planck Scale to the Electroweak Scale Warsaw, Poland, June 9 - 13, 2007 PLANCK'07
dc.identifierhttps://arxiv.org/abs/0704.3924
dc.identifierhttp://arxiv.org/abs/0704.3924
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/128126
dc.subjectHigh Energy Physics - Phenomenology
dc.titleHiggs effect in Conformal Cosmology & Supernova Data
dc.typetext

Files

Collections

arXiv