Looking for a heavy wino LSP in collider and dark matter experiments

dc.creatorChattopadhyay, Utpal
dc.creatorDas, Debottam
dc.creatorKonar, Partha
dc.creatorRoy, D. P.
dc.date2006-10-06
dc.date2007-04-02
dc.date.accessioned2026-07-07T11:27:10Z
dc.date.available2026-07-07T11:27:10Z
dc.descriptionWe investigate the phenomenology of a wino LSP as obtained in AMSB and some string models. The WMAP constraint on the DM relic density implies a wino LSP mass of 2.0-2.3 TeV. We find a viable signature for such a heavy wino at CLIC, operating at its highest CM energy of 5 TeV. One also expects a viable monochromatic $γ$-ray signal from its pair-annihilation at the galactic centre at least for cuspy DM halo profiles.
dc.descriptionA discussion on non-perturbative effects on annihilation cross section of TeV scale wino LSP added. Version to appear in Phys. Rev. D.
dc.identifierhttps://arxiv.org/abs/hep-ph/0610077
dc.identifierhttp://arxiv.org/abs/hep-ph/0610077
dc.identifierPhys.Rev.D75:073014,2007
dc.identifierdoi:10.1103/PhysRevD.75.073014
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/196063
dc.subjectHigh Energy Physics - Phenomenology
dc.titleLooking for a heavy wino LSP in collider and dark matter experiments
dc.typetext

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