Gravitationally Induced Scalar Field Fluctuations in the Radiation Dominated R-W Universe

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dc.creatorLalak, Zygmunt
dc.creatorMeissner, Krzysztof
dc.creatorPawełczyk, Jacek
dc.date1992-08-25
dc.date.accessioned2026-07-07T06:27:49Z
dc.date.available2026-07-07T06:27:49Z
dc.descriptionIt is shown that quantum fluctuations due to a nontrivial gravitational background in the flat radiation dominated universe can play an important cosmological role generating nonvanishing cosmological global charge, e.g. baryon number, asymmetry. The explicit form of the fluctuations at vacuum and at finite temperature is given. Implications for particle physics are discussed.
dc.description13, IFT-15/92
dc.identifierhttps://arxiv.org/abs/hep-ph/9208246
dc.identifierhttp://arxiv.org/abs/hep-ph/9208246
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/97523
dc.subjectHigh Energy Physics - Phenomenology
dc.titleGravitationally Induced Scalar Field Fluctuations in the Radiation Dominated R-W Universe
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