The seed of magnetic monopoles in the early inflationary universe from a 5D vacuum state

dc.creatorRomero, Jesus Martin
dc.creatorBellini, Mauricio
dc.date2008-12-03
dc.date2009-03-17
dc.date.accessioned2026-07-07T13:00:06Z
dc.date.available2026-07-07T13:00:06Z
dc.descriptionStarting from a 5D Riemann flat metric, we have induced an effective 4D Hermitian metric which has an antisymmetric part which is purely imaginary. We have worked an example in which both, non-metricity and contorsion are zero. We obtained that the production of monopoles should be insignificant at the end of inflation and the tensor metric should come asymptotically diagonal and describing a nearly 4D de Sitter expansion.
dc.descriptionVersion accepted in Physics Letters B
dc.identifierhttps://arxiv.org/abs/0812.0783
dc.identifierhttp://arxiv.org/abs/0812.0783
dc.identifierPhys.Lett.B674:143-145,2009
dc.identifierdoi:10.1016/j.physletb.2009.03.026
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/225762
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleThe seed of magnetic monopoles in the early inflationary universe from a 5D vacuum state
dc.typetext

Files

Collections