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Neutrino Coannihilation on dark-matter relics?

Repositori DSpace/Manakin

dc.contributor.author	Barenboim Szuchman, Gabriela Alejandra
dc.contributor.author	Mena Requejo, Olga
dc.contributor.author	Quigg, Chris
dc.date.accessioned	2014-08-06T08:51:43Z
dc.date.available	2014-08-06T08:51:43Z
dc.date.issued	2006
dc.identifier.citation	Barenboim Szuchman, Gabriela Mena Requejo, Olga 2006 Neutrino Coannihilation on dark-matter relics ? Physical Review D 74 023006
dc.identifier.uri	http://hdl.handle.net/10550/37366
dc.description.abstract	High-energy neutrinos may resonate with relic background neutralinos to form short-lived sneutrinos. In some circumstances, the decay chain that leads back to the lightest supersymmetric particle would yield few-GeV gamma rays or charged-particle signals. Although resonant coannihilation would occur at an appreciable rate in our galaxy, the signal in any foreseeable detector is unobservably small.
dc.language.iso	eng
dc.relation.ispartof	Physical Review D, 2006, vol. 74, p. 023006
dc.title	Neutrino Coannihilation on dark-matter relics?
dc.type	journal article	es_ES
dc.date.updated	2014-08-06T08:51:43Z
dc.identifier.doi	10.1103/PhysRevD.74.023006
dc.identifier.idgrec	030690
dc.rights.accessRights	open access	es_ES