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dc.contributor.authorGonzález-Díaz, Pedro F.-
dc.date.accessioned2012-11-13T10:25:48Z-
dc.date.available2012-11-13T10:25:48Z-
dc.date.issued2004-
dc.identifierdoi: 10.1103/PhysRevD.69.103512-
dc.identifierissn: 0556-2821-
dc.identifier.citationPhysical Review D - Particles, Fields, Gravitation and Cosmology 69: 103512-1-103512-8 (2004)-
dc.identifier.urihttp://hdl.handle.net/10261/60073-
dc.description.abstractA procedure is considered that upgrades the Lagrangian description of quantum relativistic particles to the Lagrangian of a proper field theory in the case that the Klein-Gordon wave equation is classically interpreted in terms of a relativistic subquantum potential. We apply the resulting field theory to cosmology and show that the relativistic version of Bohm's subquantum potential which can be associated with a homogeneous and isotropic distribution of particles behaves as though it was a cosmological constant responsible for the current accelerating expansion of the Universe, at least in the limit where the field potential vanishes.-
dc.description.sponsorshipThe author thanks Carmen L. Sigu¨enza for useful discussions. This work was supported by DGICYT under Research Project BMF2002-03758.-
dc.language.isoeng-
dc.publisherAmerican Physical Society-
dc.rightsopenAccess-
dc.titleSubquantum dark energy-
dc.typeartículo-
dc.identifier.doi10.1103/PhysRevD.69.103512-
dc.date.updated2012-11-13T10:25:48Z-
dc.description.versionPeer Reviewed-
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