An Improved RF Cavity Search for Halo Axions

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dc.creatorAsztalos, S. J.
dc.creatorBradley, R. F.
dc.creatorDuffy, L.
dc.creatorHagmann, C.
dc.creatorKinion, D.
dc.creatorMoltz, D. M.
dc.creatorRosenberg, L. J
dc.creatorSikivie, P.
dc.creatorStoeffl, W.
dc.creatorSullivan, N. S.
dc.creatorTanner, D. B.
dc.creatorvan Bibber, K.
dc.creatorYu, D. B.
dc.date2003-10-01
dc.date.accessioned2026-07-07T10:27:04Z
dc.date.available2026-07-07T10:27:04Z
dc.descriptionThe axion is a hypothetical elementary particle and cold dark matter candidate. In this RF cavity experiment, halo axions entering a resonant cavity immersed in a static magnetic field convert into microwave photons, with the resulting photons detected by a low-noise receiver. The ADMX Collaboration presents new limits on the axion-to-photon coupling and local axion dark matter halo mass density from a RF cavity axion search in the axion mass range 1.9-2.3 microeV, broadening the search range to 1.9-3.3 microeV. In addition, we report first results from an improved analysis technique.
dc.description5 pages, submitted to Physical Review D rapid communications
dc.identifierhttps://arxiv.org/abs/astro-ph/0310042
dc.identifierhttp://arxiv.org/abs/astro-ph/0310042
dc.identifierPhys.Rev.D69:011101,2004
dc.identifierdoi:10.1103/PhysRevD.69.011101
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/177047
dc.subjectAstrophysics
dc.titleAn Improved RF Cavity Search for Halo Axions
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