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000295130 0881_ $$aDESY-PROC-2011-04
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000295130 1001_ $$0P:(DE-HGF)0$$aPovey, Rhys G.$$b0
000295130 1112_ $$a7th Patras Workshop on Axions, WIMPs and WISPs$$cMykonos$$d2011-06-27 - 2011-07-01$$gAXION-WIMP 2011$$wGreece
000295130 245__ $$aMicrowave hidden sector photons at UWA
000295130 260__ $$aHamburg$$bDeutsches Elektronen-Synchrotron, DESY$$c2011
000295130 300__ $$a64-67
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000295130 520__ $$aIn these proceedings we present the latest progress on our microwave cavity light shining through a wall hidden sector photon experiment, as well as introduce a new method of hidden sector photon detection. Our new experiment uses a high Q superconducting Niobium emitter cavity and moderate Q room temperature copper detector cavity separated by ample shielding. The projected sensitivity of our setup to the kinetic mixing factor is $\chi \sim 1.8 \times 10^{-8}$ at a hidden sector photon mass of 52.1 $\mu$eV. A new technique for detecting hidden sector photons using a threshold crossing is also presented.
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000295130 7001_ $$0P:(DE-HGF)0$$aHartnett, John G.$$b1
000295130 7001_ $$0P:(DE-HGF)0$$aTobar, Michael E.$$b2
000295130 773__ $$a10.3204/DESY-PROC-2011-04/povey_rhys
000295130 7870_ $$0PUBDB-2016-01039$$aSchumann, Marc et.al.$$d2011$$iIsPartOf$$rDESY-PROC-2011-04$$tProceedings, 7th Patras Workshop on Axions, WIMPs and WISPs 
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