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dc.contributor.authorWagner, A.
dc.contributor.authorRybka, G.
dc.contributor.authorHotz, M.
dc.contributor.authorRosenberg, L.J.
dc.contributor.authorAsztalos, S.J.
dc.contributor.authorCarosi, G.
dc.contributor.authorHagmann, C.
dc.contributor.authorKinion, D.
dc.contributor.authorvan Bibber, K.
dc.contributor.authorHoskins, J.
dc.contributor.authorMartin, C.
dc.contributor.authorSikivie, P.
dc.contributor.authorTanner, D.B.
dc.contributor.authorBradley, R.
dc.contributor.authorClarke, J.
dc.date28 Oct 2010
dc.date.accessioned2013-08-28T22:27:01Z
dc.date.available2013-08-28T22:27:01Z
dc.date.issued2010
dc.identifier.urihttp://hdl.handle.net/10945/35437
dc.descriptionThe article of record as published may be located at http://dx.doi.org/10.1103/PhysRevLett.105.171801en_US
dc.description.abstractHidden U(1) gauge symmetries are common to many extensions of the Standard Model proposed to explain dark matter. The hidden gauge vector bosons of such extensions may mix kinetically with Standard Model photons, providing a means for electromagnetic power to pass through conducting barriers. The ADMX detector was used to search for hidden vector bosons originating in an emitter cavity driven with microwave power. We exclude hidden vector bosons with kinetic couplings {\chi} > 3.48x10-8 for masses less than 3 {\mu}eV. This limit represents an improvement of more than two orders of magnitude in sensitivity relative to previous cavity experiments.en_US
dc.rightsThis publication is a work of the U.S. Government as defined in Title 17, United States Code, Section 101. Copyright protection is not available for this work in the United States.en_US
dc.titleA Search for Hidden Sector Photons with ADMXen_US
dc.typeArticleen_US


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