Primordial fluctuations of the metric in the warm inflation scenario

Simple item page
dc.creatorBellini, Mauricio
dc.date2000-05-16
dc.date.accessioned2026-07-07T03:24:57Z
dc.date.available2026-07-07T03:24:57Z
dc.descriptionI consider a semiclassical expansion of the scalar field in the warm inflation scenario. I study the evolution for the fluctuations of the metric around the Friedmann-Robertson-Walker one. The formalism predicts that, in the power-law expansion universe, the fluctuations of the metric decreases with time.
dc.descriptionAccepted for publication in Il Nuovo Cimento B, 5 pages, no figures
dc.identifierhttps://arxiv.org/abs/gr-qc/0005072
dc.identifierhttp://arxiv.org/abs/gr-qc/0005072
dc.identifierNuovo Cim. B115 (2000) 369-374
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/33539
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titlePrimordial fluctuations of the metric in the warm inflation scenario
dc.typetext

Files

Collections

arXiv