Non-Baryonic Dark Matter

Simple item page
dc.creatorRoszkowski, Leszek
dc.date2001-02-27
dc.date.accessioned2026-07-07T03:44:00Z
dc.date.available2026-07-07T03:44:00Z
dc.descriptionThere exist several well-motivated candidates for non-baryonic cold dark matter, including neutralinos, axions, axinos, gravitinos, Wimpzillas. I review the dark matter properties of the neutralino and the current status of its detection. I also discuss the axino as a new interesting alternative.
dc.descriptionInvited plenary review talk given at 6th International Workshop on Topics in Astroparticle and Underground Physics (TAUP 99), 6-10 September, 1999, Paris, France
dc.identifierhttps://arxiv.org/abs/hep-ph/0102327
dc.identifierhttp://arxiv.org/abs/hep-ph/0102327
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/40440
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.titleNon-Baryonic Dark Matter
dc.typetext

Files

Collections

arXiv