Neutrino Coannihilation on dark-matter relics?

Neutrino Coannihilation on dark-matter relics?

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Neutrino Coannihilation on dark-matter relics?

Show simple item record Barenboim Szuchman, Gabriela Alejandra Mena Requejo, Olga Quigg, Chris 2014-08-06T08:51:43Z 2014-08-06T08:51:43Z 2006
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 2014-08-06T08:51:43Z
dc.identifier.idgrec 030690

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