Properties and signatures of supersymmetric Q-balls

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dc.creatorKusenko, Alexander
dc.date2006-12-13
dc.date.accessioned2026-07-07T07:34:30Z
dc.date.available2026-07-07T07:34:30Z
dc.descriptionSupersymmetric extensions of the Standard Model predict the existence of Q-balls with baryon and lepton numbers. Stable Q-balls can form at the end of inflation from the fragmentation of the Affleck-Dine condensate and can exist as dark matter. The best current limits come from Super-Kamiokande and MACRO. The search beyond these limits can be conducted using the future water Cherenkov detectors.
dc.description7 pages; invited talk at the workshop on Exotic Physics with Neutrino Telescopes, Uppsala, Sweden, September 20-22, 2006
dc.identifierhttps://arxiv.org/abs/hep-ph/0612159
dc.identifierhttp://arxiv.org/abs/hep-ph/0612159
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/119787
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.titleProperties and signatures of supersymmetric Q-balls
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