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@INPROCEEDINGS{An:408347,
      author       = {An, H. and Pospelov, M. and Pradler, J.},
      title        = {{N}ew {L}ight on {D}ark {P}hotons},
      address      = {Hamburg},
      publisher    = {Verlag Deutsches Elektronen-Synchrotron},
      reportid     = {PUBDB-2018-02800, DESY-PROC-2013-04},
      isbn         = {978-3-935702-83-6},
      series       = {DESY-PROC},
      pages        = {129-132},
      year         = {2013},
      comment      = {An, 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},
      booktitle     = {An, 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},
      abstract     = {“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 .},
      month         = {Jun},
      date          = {2013-06-24},
      organization  = {9th Patras Workshop on Axions, WIMPs
                       and WISPs, Mainz (Germany), 24 Jun 2013
                       - 28 Jun 2013},
      keywords     = {Hypothetisches Teilchen (gnd)},
      cin          = {L},
      cid          = {I:(DE-H253)L-20120731},
      pnm          = {899 - ohne Topic (POF3-899)},
      pid          = {G:(DE-HGF)POF3-899},
      experiment   = {EXP:(DE-MLZ)NOSPEC-20140101},
      typ          = {PUB:(DE-HGF)29 / PUB:(DE-HGF)8 / PUB:(DE-HGF)7},
      doi          = {10.3204/DESY-PROC-2013-04/pradler_josef},
      url          = {https://bib-pubdb1.desy.de/record/408347},
}