Dark Matter with (very) heavy SUSY scalars at ILC

Simple item page
dc.creatorBerggren, M.
dc.creatorRichard, F.
dc.creatorZhang, Z.
dc.date2005-10-07
dc.date.accessioned2026-07-07T06:46:37Z
dc.date.available2026-07-07T06:46:37Z
dc.descriptionIn this paper, six SUSY scenarios with heavy sfermions, mainly based on theoretical arguments and on experimental indications for new physics, are defined. These scenarios, consistent with the amount of dark matter (DM) measured by WMAP, are then analysed in detail providing pertinent examples of the potential of ILC. It is shown that in most cases ILC, with its high precision based on the chargino analysis and in spite of an incomplete coverage of the gaugino and slepton mass spectrum, can predict the amount of DM in our universe with an accuracy which matches the WMAP results.
dc.descriptionWork presented at the International Collider Physics and Detector Workshop Snowmass, Colorado, August 14-27, 2005
dc.identifierhttps://arxiv.org/abs/hep-ph/0510088
dc.identifierhttp://arxiv.org/abs/hep-ph/0510088
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/103392
dc.subjectHigh Energy Physics - Phenomenology
dc.titleDark Matter with (very) heavy SUSY scalars at ILC
dc.typetext

Files

Collections

arXiv