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Constraints from Observational Data for a Running Cosmological Constant and Warm Dark Matter with Curvature

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dc.contributor.authorAgudelo, Ruiz, J. A.
dc.contributor.authorVelasquez-Toribio, A. M.
dc.contributor.authorShapiro, I. L.
dc.contributor.authorFabris, J. C.
dc.date.accessioned2024-11-27T10:36:03Z
dc.date.available2024-11-27T10:36:03Z
dc.date.issued2020
dc.description.abstract© 2020, Pleiades Publishing, Inc.Abstract: It is known than the inclusion of spatial curvature can modify the evolution of matter perturbations and affect the Large Scale Structure (LSS) formation. We quantify the effects of the nonzero spatial curvature in terms of LSS formation for a cosmological model with a running vacuum energy density and a warm dark matter component. The evolution of density perturbations and the modified shape of their power spectrum are constructed and analyzed.
dc.format.extentС. 316-325
dc.identifier.citationConstraints from Observational Data for a Running Cosmological Constant and Warm Dark Matter with Curvature / Agudelo, Ruiz, J.A. [et al.] // Gravitation and Cosmology. - 2020. - 26. - № 4. - P. 316-325. - 10.1134/S0202289320040106
dc.identifier.doi10.1134/S0202289320040106
dc.identifier.urihttps://www.doi.org/10.1134/S0202289320040106
dc.identifier.urihttps://www.scopus.com/record/display.uri?eid=2-s2.0-85097287140&origin=resultslist
dc.identifier.urihttp://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=Alerting&SrcApp=Alerting&DestApp=WOS_CPL&DestLinkType=FullRecord&UT=WOS:000596545200003
dc.identifier.urihttps://openrepository.mephi.ru/handle/123456789/22675
dc.relation.ispartofGravitation and Cosmology
dc.titleConstraints from Observational Data for a Running Cosmological Constant and Warm Dark Matter with Curvature
dc.typeArticle
dspace.entity.typePublication
oaire.citation.issue4
oaire.citation.volume26
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relation.isOrgUnitOfPublication.latestForDiscoveryba0b4738-e6bd-4285-bda5-16ab2240dbd1
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