Mirror matter-type dark matter

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dc.creatorFoot, R.
dc.date2004-07-30
dc.date.accessioned2026-07-07T11:29:25Z
dc.date.available2026-07-07T11:29:25Z
dc.descriptionThere are six main things which any non-baryonic dark matter theory should endeavour to explain: (1) The basic dark matter particle properties [mass, stability, darkness]; (2) The similarity in cosmic abundance between ordinary and non-baryonic dark matter, $Ω_B \sim Ω_{dark}$; (3) Large scale structure formation; (4) Microlensing (MACHO) events; (5) Asymptotically flat rotation curves in spiral galaxies; (6) The impressive DAMA/NaI annual modulation signal. Only mirror matter-type dark matter is capable of explaining all six of these desirable features. The purpose of this article is to provide an up-to-date and pedagogical review of this dark matter candidate.
dc.descriptionabout 30 pages
dc.identifierhttps://arxiv.org/abs/astro-ph/0407623
dc.identifierhttp://arxiv.org/abs/astro-ph/0407623
dc.identifierInt.J.Mod.Phys.D13:2161-2192,2004
dc.identifierdoi:10.1142/S0218271804006449
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/196707
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Phenomenology
dc.titleMirror matter-type dark matter
dc.typetext

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