Baryogenesis and Polyakov line condensate during inflation

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dc.creatorAbada, As.
dc.creatorGavela, M. B.
dc.creatorPène, O.
dc.date1996-02-24
dc.date.accessioned2026-07-07T03:58:55Z
dc.date.available2026-07-07T03:58:55Z
dc.descriptionThe thermal average of the Polyakov line is non-zero at high temperature. It has been suggested that its phase could be relevant for baryogenesis within the standard model, providing a source of spontaneously broken CP violation. This scenario suffers from a causal domain problem which cannot be cured by inflation: quantum fluctuations in de Sitter space overwhelm the periodicity of the potential.
dc.description20 pages, Latex2e
dc.identifierhttps://arxiv.org/abs/hep-ph/9602388
dc.identifierhttp://arxiv.org/abs/hep-ph/9602388
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/46011
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.titleBaryogenesis and Polyakov line condensate during inflation
dc.typetext

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