Oscillons in Scalar Field Theories: Applications in Higher Dimensions and Inflation

dc.creatorGleiser, Marcelo
dc.date2006-02-19
dc.date.accessioned2026-07-07T10:45:59Z
dc.date.available2026-07-07T10:45:59Z
dc.descriptionThe basic properties of oscillons -- localized, long-lived, time-dependent scalar field configurations -- are briefly reviewed, including recent results demonstrating how their existence depends on the dimensionality of spacetime. Their role on the dynamics of phase transitions is discussed, and it is shown that oscillons may greatly accelerate the decay of metastable vacuum states. This mechanism for vacuum decay -- resonant nucleation -- is then applied to cosmological inflation. A new inflationary model is proposed which terminates with fast bubble nucleation.
dc.description11 pages, 4 figures, to appear in Int. J. Mod. Phys. D
dc.identifierhttps://arxiv.org/abs/hep-th/0602187
dc.identifierhttp://arxiv.org/abs/hep-th/0602187
dc.identifierInt.J.Mod.Phys.D16:219-229,2007
dc.identifierdoi:10.1142/S0218271807009954
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/183090
dc.subjectHigh Energy Physics - Theory
dc.subjectAstrophysics
dc.titleOscillons in Scalar Field Theories: Applications in Higher Dimensions and Inflation
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