The reach of a future Linear Collider after the g-2 result

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dc.creatorRichard, Francois
dc.date2001-04-11
dc.date.accessioned2026-07-07T03:44:19Z
dc.date.available2026-07-07T03:44:19Z
dc.descriptionCombining the cosmological requirement on dark matter with the recent BNL g-2 measurement it is argued that, within the mSUGRA framework, the preferred region for SUSY mass parameters falls well inside the area covered by the future linear colliders under consideration for right handed sleptons and of the 2 lightest neutralinos. The coverage for the lightest chargino and left handed sleptons is also favoured but with smaller confidence.
dc.description8 pages, 2 figures
dc.identifierhttps://arxiv.org/abs/hep-ph/0104106
dc.identifierhttp://arxiv.org/abs/hep-ph/0104106
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/40515
dc.subjectHigh Energy Physics - Phenomenology
dc.titleThe reach of a future Linear Collider after the g-2 result
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