Observing Dark Matter via the Gyromagnetic Faraday Effect

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dc.creatorGardner, S.
dc.date2006-11-21
dc.date2007-09-11
dc.date.accessioned2026-07-07T11:42:40Z
dc.date.available2026-07-07T11:42:40Z
dc.descriptionIf dark matter consists of cold, neutral particles with a non-zero magnetic moment, then, in the presence of an external magnetic field, a measurable gyromagnetic Faraday effect becomes possible. This enables direct constraints on the nature and distribution of such dark matter through detailed measurements of the polarization and temperature of the cosmic microwave background radiation.
dc.description4 pages, RevTeX; numerical error fixed, some conclusions modified
dc.identifierhttps://arxiv.org/abs/astro-ph/0611684
dc.identifierhttp://arxiv.org/abs/astro-ph/0611684
dc.identifierPhys.Rev.Lett.100:041303,2008
dc.identifierdoi:10.1103/PhysRevLett.100.041303
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/200963
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Phenomenology
dc.titleObserving Dark Matter via the Gyromagnetic Faraday Effect
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