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@INPROCEEDINGS{Branca:395469,
      author       = {Branca, Antonio},
      collaboration = {{AURIGA Collaboration}},
      title        = {{L}ight {D}ark {M}atter {S}earch with {AURIGA}},
      address      = {Hamburg},
      publisher    = {Verlag Deutsches Elektronen-Synchrotron},
      reportid     = {PUBDB-2017-12134, DESY-PROC-2016-03},
      isbn         = {978-3-945931-06-6},
      series       = {DESY-PROC},
      pages        = {9-13},
      year         = {2017},
      comment      = {Branca, Antonio "Light Dark Matter Search with AURIGA" in
                      12th "Patras" Workshop on Axions, WIMPs and WISPs, PATRAS
                      2016 / Kim, Younglm, Lindner, Axel, Semertzidis, Yannis K.
                      (eds.), Verlag Deutsches Elektronen-Synchrotron : 2017 ;
                      PATRAS 2016 : 12th "Patras" Workshop on Axions, WIMPs and
                      WISPs, 2016-06-20 - 2016-06-24, Jeju Island},
      booktitle     = {Branca, Antonio "Light Dark Matter
                       Search with AURIGA" in 12th "Patras"
                       Workshop on Axions, WIMPs and WISPs,
                       PATRAS 2016 / Kim, Younglm, Lindner,
                       Axel, Semertzidis, Yannis K. (eds.),
                       Verlag Deutsches Elektronen-Synchrotron
                       : 2017 ; PATRAS 2016 : 12th "Patras"
                       Workshop on Axions, WIMPs and WISPs,
                       2016-06-20 - 2016-06-24, Jeju Island},
      abstract     = {We present a search for a new scalar particle, called
                      moduli, performed using the cryogenic resonant-mass
                      gravitational wave detector AURIGA. This particle may give a
                      significant contribution to the Dark Matter (DM) in our
                      Universe. DM clusters under the galaxies gravitational
                      effect, forming the so called galactic halo. The interaction
                      of ordinary matter with a DM halo composed by moduli causes
                      the oscillation of solids with a frequency equal to the mass
                      of the DM particle. In particular, the putative signal would
                      appear as a narrow peak ($\triangle f\sim1\,\mathrm{mHz}$)
                      in the sensitive band of AURIGA, some $100\,\mathrm{Hz}$ at
                      about $1\,\mathrm{kHz}$. We used high quality data, selected
                      out of an acquisition of years of continuous running. The
                      search sets upper limits at $95\\%\,C.L.$ on the moduli
                      coupling to matter $d_{i}\lesssim10^{-5}$ around moduli
                      masses $m_{\Phi}=3.6\cdot10^{-12}\,\mathrm{eV}$.},
      month         = {Jun},
      date          = {2016-06-20},
      organization  = {12th Patras Workshop on Axions, WIMPs
                       and WISPs, Jeju Island (South Korea),
                       20 Jun 2016 - 24 Jun 2016},
      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-2009-03/Branca_Antonio},
      url          = {https://bib-pubdb1.desy.de/record/395469},
}