Neutrino Coannihilation on dark-matter relics?
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Neutrino Coannihilation on dark-matter relics?

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Neutrino Coannihilation on dark-matter relics?

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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.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.rights.uri info:eu-repo/semantics/openAccess
dc.source Barenboim Szuchman, Gabriela Mena Requejo, Olga 2006 Neutrino Coannihilation on dark-matter relics ? Physical Review D 74 023006
dc.title Neutrino Coannihilation on dark-matter relics?
dc.type info:eu-repo/semantics/article
dc.date.updated 2014-08-06T08:51:43Z
dc.identifier.doi http://dx.doi.org/10.1103/PhysRevD.74.023006
dc.identifier.idgrec 030690

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