Results of a Search for Cold Flows of Dark Matter Axions

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dc.creatorDuffy, L.
dc.creatorSikivie, P.
dc.creatorTanner, D. B.
dc.creatorAsztalos, S.
dc.creatorHagmann, C.
dc.creatorKinion, D.
dc.creatorRosenberg, L. J
dc.creatorvan Bibber, K.
dc.creatorYu, D.
dc.creatorBradley, R. F.
dc.date2005-05-11
dc.date.accessioned2026-07-07T12:24:55Z
dc.date.available2026-07-07T12:24:55Z
dc.descriptionTheoretical arguments predict that the distribution of cold dark matter in spiral galaxies has peaks in velocity space associated with non-thermalized flows of dark matter particles. We searched for the corresponding peaks in the spectrum of microwave photons from axion to photon conversion in the cavity detector of dark matter axions. We found none and place limits on the density of any local flow of axions as a function of the flow velocity dispersion over the axion mass range 1.98 to 2.17 $μ$eV.
dc.description5 pages, 3 figures
dc.identifierhttps://arxiv.org/abs/astro-ph/0505237
dc.identifierhttp://arxiv.org/abs/astro-ph/0505237
dc.identifierPhys.Rev.Lett.95:091304,2005
dc.identifierdoi:10.1103/PhysRevLett.95.091304
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/214473
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Experiment
dc.subjectHigh Energy Physics - Phenomenology
dc.titleResults of a Search for Cold Flows of Dark Matter Axions
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