Dark matter and the deformed Poincaré group

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dc.date.accessioned	2021-08-23T14:50:20Z
dc.date.available	2021-08-23T14:50:20Z
dc.date.issued	1996
dc.identifier.uri	http://sedici.unlp.edu.ar/handle/10915/123144
dc.description.abstract	It 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.	en
dc.format.extent	53-54	es
dc.language	en	es
dc.subject	Poincaré group	es
dc.subject	Physics	es
dc.subject	Doubly special relativity	es
dc.subject	Dark matter	es
dc.subject	Theoretical physics	es
dc.subject	Classical mechanics	es
dc.title	Dark matter and the deformed Poincaré group	en
dc.type	Articulo	es
sedici.identifier.other	doi:10.1016/0370-2693(95)01490-x	es
sedici.identifier.issn	0370-2693	es
sedici.creator.person	Fernández, Julián Martín	es
sedici.subject.materias	Física	es
sedici.description.fulltext	true	es
mods.originInfo.place	Facultad de Ciencias Exactas	es
sedici.subtype	Articulo	es
sedici.rights.license	Creative Commons Attribution 4.0 International (CC BY 4.0)
sedici.rights.uri	http://creativecommons.org/licenses/by/4.0/
sedici.description.peerReview	peer-review	es
sedici.relation.journalTitle	Physics Letters B	es
sedici.relation.journalVolumeAndIssue	vol. 368, no. 1-2	es

Excepto donde se diga explícitamente, este item se publica bajo la siguiente licencia Creative Commons Attribution 4.0 International (CC BY 4.0)