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Barenboim Szuchman, Gabriela Alejandra; Mena Requejo, Olga; Quigg, Chris | |||
Aquest document és un/a article, creat/da en: 2006 | |||
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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. | |||
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