Properties of Local Group galaxies in hydrodynamical simulations of sterile neutrino dark matter cosmologies

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Lovell , M R , Bose , S , Boyarsky , A , Crain , R A , Frenk , C S , Hellwing , W A , Ludlow , A D , Navarro , J F , Ruchayskiy , O , Sawala , T , Schaller , M , Schaye , J & Theuns , T 2017 , ' Properties of Local Group galaxies in hydrodynamical simulations of sterile neutrino dark matter cosmologies ' , Monthly Notices of the Royal Astronomical Society , vol. 468 , no. 4 , pp. 4285-4298 . https://doi.org/10.1093/mnras/stx654

Title: Properties of Local Group galaxies in hydrodynamical simulations of sterile neutrino dark matter cosmologies
Author: Lovell, Mark R.; Bose, Sownak; Boyarsky, Alexey; Crain, Robert A.; Frenk, Carlos S.; Hellwing, Wojciech A.; Ludlow, Aaron D.; Navarro, Julio F.; Ruchayskiy, Oleg; Sawala, Till; Schaller, Matthieu; Schaye, Joop; Theuns, Tom
Contributor: University of Helsinki, Department of Physics
Date: 2017-07
Language: eng
Number of pages: 14
Belongs to series: Monthly Notices of the Royal Astronomical Society
ISSN: 0035-8711
URI: http://hdl.handle.net/10138/209210
Abstract: We study galaxy formation in sterile neutrino dark matter models that differ significantly from both cold and from 'warm thermal relic' models. We use the EAGLE code to carry out hydrodynamic simulations of the evolution of pairs of galaxies chosen to resemble the Local Group, as part of the APOSTLE simulations project. We compare cold dark matter (CDM) with two sterile neutrino models with 7 keV mass: one, the warmest among all models of this mass (LA120) and the other, a relatively cold case (LA10). We show that the lower concentration of sterile neutrino subhaloes compared to their CDM counterparts makes the inferred inner dark matter content of galaxies like Fornax (or Magellanic Clouds) less of an outlier in the sterile neutrino cosmologies. In terms of the galaxy number counts, the LA10 simulations are indistinguishable from CDM when one takes into account halo-to-halo (or 'simulation-to-simulation') scatter. In order for the LA120 model to match the number of Local Group dwarf galaxies, a higher fraction of low-mass haloes is required to form galaxies than is predicted by the EAGLE simulations. As the census of the Local Group galaxies nears completion, this population may provide a strong discriminant between cold and warm dark matter models.
Subject: Local Group
dark matter
LARGE-MAGELLANIC-CLOUD
MILKY-WAY SATELLITES
3.5 KEV LINE
X-RAY-LINE
DWARF GALAXIES
EAGLE SIMULATIONS
CHARGE-EXCHANGE
GALACTIC-CENTER
MASS FUNCTION
ENERGY SURVEY
115 Astronomy, Space science
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