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@INPROCEEDINGS{Bozorgnia:395470,
      author       = {Bozorgnia, Nassim and Calore, Francesca and Schaller,
                      Matthieu and Lovell, Mark and Bertone, Gianfranco and Frenk,
                      Carlos S. and Crain, Robert A. and Navarro, Julio F. and
                      Schaye, Joop and Theuns, Tom},
      title        = {{T}he {L}ocal {D}ark {M}atter {D}istribution from
                      {H}ydrodynamic {S}imulations},
      address      = {Hamburg},
      publisher    = {Verlag Deutsches Elektronen-Synchrotron},
      reportid     = {PUBDB-2017-12135, DESY-PROC-2016-03},
      isbn         = {978-3-945931-06-6},
      series       = {DESY-PROC},
      pages        = {14-17},
      year         = {2017},
      comment      = {Bozorgnia, Nassim "The Local Dark Matter Distribution from
                      Hydrodynamic Simulations" 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     = {Bozorgnia, Nassim "The Local Dark
                       Matter Distribution from Hydrodynamic
                       Simulations" 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 investigate the predictions of the $\eagle$ and
                      $\apostle$ hydrodynamic simulations for dark matter direct
                      detection searches. We extract the dark matter density and
                      velocity distribution at the Solar position for a set of
                      simulated galaxies which satisfy Milky Way observational
                      constraints, and use them to analyze current direct
                      detection data. We find that the local dark matter density
                      of the Milky Way-like galaxies fall in the range of $0.41 -
                      0.73$ GeV$/$cm$^3$, and their dark matter velocity
                      distributions fit well a Maxwellian distribution with peak
                      speed in the range of $223 - 289$ km$/$s.},
      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/Bozorgnia_Nassim},
      url          = {https://bib-pubdb1.desy.de/record/395470},
}