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Accelerated Expansion of the Universe via Energy Conservation

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dc.creator Ortíz González, Carlos Alberto
dc.date.accessioned 2019-03-28T21:09:26Z
dc.date.available 2019-03-28T21:09:26Z
dc.date.issued 2019-03-28
dc.identifier info:eu-repo/semantics/submittedVersion es_ES
dc.identifier.uri http://localhost/xmlui/handle/20.500.11845/903
dc.description.abstract This 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.iso eng es_ES
dc.publisher Universidad Autónoma de Zacatecas es_ES
dc.relation.uri generalPublic es_ES
dc.rights Atribución-NoComercial-CompartirIgual 3.0 Estados Unidos de América es_ES
dc.rights.uri http://creativecommons.org/licenses/by-nc-sa/3.0/us/ *
dc.subject.classification CIENCIAS FISICO MATEMATICAS Y CIENCIAS DE LA TIERRA [1] es_ES
dc.subject.other General Relativity es_ES
dc.subject.other Cosmology es_ES
dc.subject.other Dark Energy es_ES
dc.title Accelerated Expansion of the Universe via Energy Conservation es_ES
dc.type info:eu-repo/semantics/preprint es_ES


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