A First Principles Warm Inflation Model that Solves the Cosmological Horizon/Flatness Problems

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dc.creatorBerera, Arjun
dc.creatorGleiser, Marcelo
dc.creatorRamos, Rudnei O.
dc.date1998-09-29
dc.date1999-05-18
dc.date.accessioned2026-07-07T10:33:44Z
dc.date.available2026-07-07T10:33:44Z
dc.descriptionA quantum field theory warm inflation model is presented that solves the horizon/flatness problems. The model obtains, from the elementary dynamics of particle physics, cosmological scale factor trajectories that begin in a radiation dominated regime, enter an inflationary regime and then smoothly exit back into a radiation dominated regime, with nonnegligible radiation throughout the evolution.
dc.descriptionIn Press Physical Review Letters 1999, 5 pgs, 1 fig., latex
dc.identifierhttps://arxiv.org/abs/hep-ph/9809583
dc.identifierhttp://arxiv.org/abs/hep-ph/9809583
dc.identifierPhys.Rev.Lett.83:264-267,1999
dc.identifierdoi:10.1103/PhysRevLett.83.264
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/179225
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Theory
dc.titleA First Principles Warm Inflation Model that Solves the Cosmological Horizon/Flatness Problems
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