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dc.contributor.authorSantos Corchero, Emilio
dc.contributor.otherUniversidad de Cantabriaes_ES
dc.date.accessioned2025-07-11T16:33:54Z
dc.date.available2025-07-11T16:33:54Z
dc.date.issued2024
dc.identifier.issn1099-4300
dc.identifier.urihttps://hdl.handle.net/10902/36678
dc.description.abstractThe Einstein equation in a semiclassical approximation is applied to a spherical region of the universe, with the stress-energy tensor consisting of the mass density and pressure of the LCDM cosmological model plus an additional contribution due to the quantum vacuum. Expanding the equation in powers of Newton constant G, the vacuum contributes to second order. The result is that at least a part of the acceleration in the expansion of the universe may be due to the quantum vacuum fluctuations.es_ES
dc.format.extent14 p.es_ES
dc.language.isoenges_ES
dc.publisherMDPIes_ES
dc.rights© 2024 by the authors. Licensee MDPI, Basel, Switzerland. This article is an open access article distributed under the terms and conditions of the Creative Commons Attribution (CC BY) license.es_ES
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/*
dc.sourceEntropy, 2024, 26(12), 1042es_ES
dc.subject.otherDark energyes_ES
dc.subject.otherQuantum vacuumes_ES
dc.subject.otherQuantized Einstein equationes_ES
dc.titleEffects of the quantum vacuum at a cosmic scale and of dark energyes_ES
dc.typeinfo:eu-repo/semantics/articlees_ES
dc.rights.accessRightsopenAccesses_ES
dc.identifier.DOI10.3390/e26121042
dc.type.versionpublishedVersiones_ES


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Mostrar el registro sencillo

© 2024 by the authors. Licensee MDPI, Basel, Switzerland. This article is an open access article distributed under the terms and conditions of the Creative Commons Attribution (CC BY) license.Excepto si se señala otra cosa, la licencia del ítem se describe como © 2024 by the authors. Licensee MDPI, Basel, Switzerland. This article is an open access article distributed under the terms and conditions of the Creative Commons Attribution (CC BY) license.