Please use this identifier to cite or link to this item: http://ricaxcan.uaz.edu.mx/jspui/handle/20.500.11845/903
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dc.creatorOrtíz González, Carlos Alberto-
dc.date.accessioned2019-03-28T21:09:26Z-
dc.date.available2019-03-28T21:09:26Z-
dc.date.issued2019-03-28-
dc.identifierinfo:eu-repo/semantics/submittedVersiones_ES
dc.identifier.urihttp://localhost/xmlui/handle/20.500.11845/903-
dc.description.abstractThis paper analyzes the boundary term of the Hilbert-Einstein action for an FRW metric, and uses it to set the conditions of the Einstein’s Field Equations. By means of the energy conservation equation, we identify a new non gravitational general relativistic effect that modifies the space-time fabric. This effect is due to the energy density that surrounds a given space-time region, and it gives a physical explanation to the accelerated expansion of the universe. It also explains why we have not found any particle or fluid responsible of the dark energy and it clarifies the coincidence problem. These explanations are achieved without assuming the existence of exotic matter of unphysical meaning or having to modify the Einstein’s Field Equations.es_ES
dc.language.isoenges_ES
dc.publisherUniversidad Autónoma de Zacatecases_ES
dc.relation.urigeneralPublices_ES
dc.rightsAtribución-NoComercial-CompartirIgual 3.0 Estados Unidos de Américaes_ES
dc.rights.urihttp://creativecommons.org/licenses/by-nc-sa/3.0/us/*
dc.subject.classificationCIENCIAS FISICO MATEMATICAS Y CIENCIAS DE LA TIERRA [1]es_ES
dc.subject.otherGeneral Relativityes_ES
dc.subject.otherCosmologyes_ES
dc.subject.otherDark Energyes_ES
dc.titleAccelerated Expansion of the Universe via Energy Conservationes_ES
dc.typeinfo:eu-repo/semantics/preprintes_ES
Appears in Collections:*Documentos Académicos*-- UA Física

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