The anomaly-induced effective action and natural inflation

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dc.creatorPelinson, A. M.
dc.creatorShapiro, I. L.
dc.creatorSola, J.
dc.creatorTakakura, F. I.
dc.date2003-11-27
dc.date.accessioned2026-07-07T03:51:25Z
dc.date.available2026-07-07T03:51:25Z
dc.descriptionThe anomaly-induced inflation (modified Starobinsky model) is based on the application of the effective quantum field theory approach to the Early Universe. We present a brief general review of the model and show that it does not require a fine-tuning for the parameters of the theory or initial data, gives a real chance to meet a graceful exit to the FRW phase and also has positive features with respect to the metric perturbations.
dc.descriptionInvited talk at the International Workshop on Astroparticle and High Energy Physics, October 14 - 18, 2003, Valencia, Spain
dc.identifierhttps://arxiv.org/abs/hep-ph/0311363
dc.identifierhttp://arxiv.org/abs/hep-ph/0311363
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/43086
dc.subjectHigh Energy Physics - Phenomenology
dc.titleThe anomaly-induced effective action and natural inflation
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