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@INPROCEEDINGS{Jeong:408351,
      author       = {Jeong, K. S. and Takahashi, F.},
      title        = {{S}tronger {QCD} in the early {U}niverse to suppress axion
                      isocurvature perturbations},
      address      = {Hamburg},
      publisher    = {Verlag Deutsches Elektronen-Synchrotron},
      reportid     = {PUBDB-2018-02804, DESY-PROC-2013-04},
      isbn         = {978-3-935702-83-6},
      series       = {DESY-PROC},
      pages        = {153-158},
      year         = {2013},
      comment      = {Jeong, K.S. "Stronger QCD in the early Universe to suppress
                      axion isocurvature perturbations" 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     = {Jeong, K.S. "Stronger QCD in the early
                       Universe to suppress axion isocurvature
                       perturbations" 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     = {A stronger QCD in the early Universe renders the axion
                      heavy, and thus can suppress the isocurvature perturbations
                      of axion dark matter, relaxing the constraint on the
                      inflation scale. Supersymmetry provides a natural framework
                      for this because there is a flat direction involving Higgs
                      fields. Stabilized at a large value during inflation, the
                      Higgs flat direction leads to that the QCD interaction
                      becomes strong at a high energy scale, making high scale
                      inflation scenarios compatible with axion 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/jeong_kwang_sik},
      url          = {https://bib-pubdb1.desy.de/record/408351},
}