% IMPORTANT: The following is UTF-8 encoded. This means that in the presence
% of non-ASCII characters, it will not work with BibTeX 0.99 or older.
% Instead, you should use an up-to-date BibTeX implementation like “bibtex8” or
% “biber”.
@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},
}