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@INPROCEEDINGS{Balzs:408349,
      author       = {Balázs, C. and Gupta, S. K.},
      title        = {{A}xion, axino and neutralino dark matter in minimal
                      supergravity},
      address      = {Hamburg},
      publisher    = {Verlag Deutsches Elektronen-Synchrotron},
      reportid     = {PUBDB-2018-02802, DESY-PROC-2013-04},
      isbn         = {978-3-935702-83-6},
      series       = {DESY-PROC},
      pages        = {141-144},
      year         = {2013},
      comment      = {Balázs, C. "Axion, axino and neutralino dark matter in
                      minimal supergravity" 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     = {Balázs, C. "Axion, axino and
                       neutralino dark matter in minimal
                       supergravity" 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 matter can be a mixture of axions, axinos and
                      neutralinos in a Peccei-Quinn extension of supergravity. To
                      find out which dark matter candidate is preferred by data we
                      perform a Bayesian statistical analysis on four such
                      scenarios. The main experimental constraints on these models
                      come from the Planck satellite and from the Large Hadron
                      Collider. Weaker constrains arise from other astrophysical,
                      collider and low energy measurements. Our study reveals that
                      the Peccei-Quinn scenario featuring axino dark matter is
                      clearly preferred over the minimal supegravity model with
                      neutralino dark matter.},
      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/balazs_csaba},
      url          = {https://bib-pubdb1.desy.de/record/408349},
}