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000408347 1001_ $$0P:(DE-HGF)0$$aAn, H.$$b0
000408347 1112_ $$0C13-06-24.5$$2inspire$$a9th Patras Workshop on Axions, WIMPs and WISPs$$cMainz$$d2013-06-24 - 2013-06-28$$gAXION-WIMP 2013$$wGermany
000408347 245__ $$aNew Light on Dark Photons
000408347 260__ $$aHamburg$$bVerlag Deutsches Elektronen-Synchrotron$$c2013
000408347 29510 $$aAn, H. "New Light on Dark Photons" in Proceedings, 9th Patras Workshop on Axions, WIMPs and WISPs (AXION-WIMP 2013) / Oberlack, Uwe, Sissol, Pierre (eds.), 2013 ; AXION-WIMP 2013 : 9th Patras Workshop on Axions, WIMPs and WISPs , 2013-06-23 - 2013-06-28, Mainz
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000408347 520__ $$a“Dark  Photons”,  light  new  vector  particles $V_μ$ kinetically   mixed with the photon, are a frequently considered extension of the Standard Model. For masses below 10 keV they are emitted from the solar interior. In the limit of small mass mV the dark pho-ton flux is strongly peaked at low energies and we demonstrate that the constraint on the atomic ionization rate imposed by the results of the XENON10 Dark Matter experiment sets the to-date most stringent limit on the kinetic mixing parameter of this model: $κ × mV < 3 × 10 ^{−12}$ eV. The result significantly improves previous experimental bounds and surpasses even the most stringent astrophysical and cosmological limits in a seven-decade-wide interval of mV .
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000408347 7001_ $$0P:(DE-HGF)0$$aPospelov, M.$$b1
000408347 7001_ $$0P:(DE-HGF)0$$aPradler, J.$$b2$$eCorresponding author
000408347 7870_ $$0PUBDB-2015-05816$$aOberlack, Uwe et. al.$$iisPartOf$$rDESY-PROC-2013-04$$tProceedings, 9th Patras Workshop on Axions, WIMPs and WISPs (AXION-WIMP 2013)
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