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Authordc.contributor.authorHojman Guiñerman, Sergio 
Authordc.contributor.authorNúñez, Darío 
Authordc.contributor.authorRyan, Michael P. 
Admission datedc.date.accessioned2018-12-20T14:06:50Z
Available datedc.date.available2018-12-20T14:06:50Z
Publication datedc.date.issued1992
Cita de ítemdc.identifier.citationPhysical Review D, Volumen 45, Issue 10, 2018, Pages 3523-3527
Identifierdc.identifier.issn05562821
Identifierdc.identifier.other10.1103/PhysRevD.45.3523
Identifierdc.identifier.urihttps://repositorio.uchile.cl/handle/2250/154022
Abstractdc.description.abstractWe present the construction of a Hamiltonian description for a (non-Lagrangian) Bianchi type-V cosmological model using the solutions of the equations of motion as a starting point. We study the quantization of the model and compare our results to those found using a more standard approach. © 1992 The American Physical Society.
Lenguagedc.language.isoen
Publisherdc.publisherAmerican Physical Society
Type of licensedc.rightsAttribution-NonCommercial-NoDerivs 3.0 Chile
Link to Licensedc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/
Sourcedc.sourcePhysical Review D
Keywordsdc.subjectNuclear and High Energy Physics
Títulodc.titleMinisuperspace example of non-Lagrangian quantization
Document typedc.typeArtículo de revista
Catalogueruchile.catalogadorSCOPUS
Indexationuchile.indexArtículo de publicación SCOPUS
Indexationuchile.indexArtículo de publicación ISI
uchile.cosechauchile.cosechaSI


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Except where otherwise noted, this item's license is described as Attribution-NonCommercial-NoDerivs 3.0 Chile