TY  - CONF
AU  - Bozorgnia, Nassim
AU  - Calore, Francesca
AU  - Schaller, Matthieu
AU  - Lovell, Mark
AU  - Bertone, Gianfranco
AU  - Frenk, Carlos S.
AU  - Crain, Robert A.
AU  - Navarro, Julio F.
AU  - Schaye, Joop
AU  - Theuns, Tom
TI  - The Local Dark Matter Distribution from Hydrodynamic Simulations
IS  - DESY-PROC-2016-03
CY  - Hamburg
PB  - Verlag Deutsches Elektronen-Synchrotron
M1  - PUBDB-2017-12135
M1  - DESY-PROC-2016-03
SN  - 978-3-945931-06-6
T2  - DESY-PROC
SP  - 14-17
PY  - 2017
AB  - We investigate the predictions of the  and  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<sup>3</sup>, and their dark matter velocity distributions fit well a Maxwellian distribution with peak speed in the range of 223 − 289 km/s.
T2  - 12th Patras Workshop on Axions, WIMPs and WISPs
CY  - 20 Jun 2016 - 24 Jun 2016, Jeju Island (South Korea)
Y2  - 20 Jun 2016 - 24 Jun 2016
M2  - Jeju Island, South Korea
LB  - PUB:(DE-HGF)29 ; PUB:(DE-HGF)8 ; PUB:(DE-HGF)7
DO  - DOI:10.3204/DESY-PROC-2009-03/Bozorgnia_Nassim
UR  - https://bib-pubdb1.desy.de/record/395470
ER  -