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dc.creatorCapozziello, Salvatore
dc.creatorJovanović, Predrag
dc.creatorBorka Jovanović, Vesna
dc.creatorBorka, Duško
dc.date.accessioned2018-03-01T17:48:04Z
dc.date.available2018-03-01T17:48:04Z
dc.date.issued2017
dc.identifier.issn1475-7516 (print)
dc.identifier.urihttp://vinar.vin.bg.ac.rs/handle/123456789/1696
dc.description.abstractWe demonstrate that the existence of a Noether symmetry in f theories of gravity gives rise to a further gravitational radius, besides tile standard Schwarzschild one, determining the dynamics at galactic scales. By this feature, it is possible to explain the baryonic Fully-Fisher relation and the rotation curve of gas-rich galaxies without the dark matter hypothesis.en
dc.relationinfo:eu-repo/grantAgreement/MESTD/Basic Research (BR or ON)/176003/RS//
dc.relationINFN (iniziative specifiche TEONGRAV), INFN (QGSKY), Bilateral Cooperation [451-03-01231/2015-09/1], COST Actions [MP1304, CA15117], COST (European Cooperation in Science and Technology)
dc.rightsrestrictedAccessen
dc.sourceJournal of Cosmology and Astroparticle Physicsen
dc.subjectmodified gravityen
dc.subjectrotation curves of galaxiesen
dc.titleAddressing the missing matter problem in galaxies through a new fundamental gravitational radiusen
dc.typearticleen
dcterms.abstractЦапоззиелло, С.; Јовановиц, П.; Борка-Јовановић Весна; Борка Душко;
dc.citation.issue6
dc.identifier.wos000408310600014
dc.identifier.doi10.1088/1475-7516/2017/06/044
dc.citation.otherArticle Number: 044
dc.identifier.scopus2-s2.0-85021652997


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