Dark energy from topology

dc.contributor.authorEspiro, J. Lorca
dc.contributor.authorDelliou, M. Le [UNESP]
dc.contributor.institutionUniversidad de la Frontera
dc.contributor.institutionLanzhou University
dc.contributor.institutionFaculdade de Ciências
dc.contributor.institutionUniversidade Estadual Paulista (Unesp)
dc.date.accessioned2020-12-12T02:04:44Z
dc.date.available2020-12-12T02:04:44Z
dc.date.issued2020-03-01
dc.description.abstractThe concordance model of cosmology suffers from the major theoretical problems surrounding the observed value and recent emergence of a cosmological constant. In this paper we present a novel approach, which explains more naturally its value than that based on quantum vacuum energy, in the form of topological invariants characteristic classes, included as Lagrange multipliers in the action. The approach draws from topological as well as dynamical system consideration, generating as a byproduct an effective cosmological constant. General Relativity is recovered by canceling the torsion in a region containing the observable Universe, which boundary constraints the invariants, thus yielding the effective cosmological constant's form. As that form's denominator contains the total volume of the average black hole, calculated from a geometrical mean on the estimated black hole mass distribution and directly associated to the ratio of the total volume boundary of the space-time manifold and the dominant term in its Euler characteristic. The constant's small estimated value compared to the Planck scale is therefore natural and our evaluation fits remarkably well with the observed value.en
dc.description.affiliationDepartamento de Ciencias Físicas Facultad de Ingenieriá Ciencias y Administración Universidad de la Frontera, Avda. Francisco Salazar 01145
dc.description.affiliationInstitute of Theoretical Physics School of Physical Science and Technology Lanzhou University, No. 222, South Tianshui Road
dc.description.affiliationInstituto de Astrofísica e Ciências Do Espaço Universidade de Lisboa Faculdade de Ciências, Ed. C8, Campo Grande
dc.description.affiliationInstituto de Física Teórica Universidade Estadual de Saõ Paulo (IFT-UNESP), Rua Dr. Bento Teobaldo Ferraz 271, Bloco 2, Barra Funda
dc.description.affiliationUnespInstituto de Física Teórica Universidade Estadual de Saõ Paulo (IFT-UNESP), Rua Dr. Bento Teobaldo Ferraz 271, Bloco 2, Barra Funda
dc.identifierhttp://dx.doi.org/10.1088/1475-7516/2020/03/020
dc.identifier.citationJournal of Cosmology and Astroparticle Physics, v. 2020, n. 3, 2020.
dc.identifier.doi10.1088/1475-7516/2020/03/020
dc.identifier.issn1475-7516
dc.identifier.scopus2-s2.0-85084211584
dc.identifier.urihttp://hdl.handle.net/11449/200368
dc.language.isoeng
dc.relation.ispartofJournal of Cosmology and Astroparticle Physics
dc.sourceScopus
dc.titleDark energy from topologyen
dc.typeArtigo
unesp.campusUniversidade Estadual Paulista (Unesp), Instituto de Física Teórica (IFT), São Paulopt

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