Dark matter and the deformed Poincaré group

dc.creatorFernández, Julián Martín
dc.date1996
dc.date2021-08-23T14:50:20Z
dc.date.accessioned2023-07-15T02:43:46Z
dc.date.available2023-07-15T02:43:46Z
dc.identifierhttp://sedici.unlp.edu.ar/handle/10915/123144
dc.identifierissn:0370-2693
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/7463054
dc.descriptionIt has been recently suggested that models of deformed special relativity, based on a deformed Poincare group, could account for the missing mass problem, due to the nonadditivity of energy for large systems predicted by these models. We show that this is not correct and that, in fact, these models predict just the opposite effect.
dc.descriptionFacultad de Ciencias Exactas
dc.formatapplication/pdf
dc.format53-54
dc.languageen
dc.rightshttp://creativecommons.org/licenses/by/4.0/
dc.rightsCreative Commons Attribution 4.0 International (CC BY 4.0)
dc.subjectFísica
dc.subjectPoincaré group
dc.subjectPhysics
dc.subjectDoubly special relativity
dc.subjectDark matter
dc.subjectTheoretical physics
dc.subjectClassical mechanics
dc.titleDark matter and the deformed Poincaré group
dc.typeArticulo
dc.typeArticulo


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