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We study the implications of galaxy formation on dark matter direct detection using high resolution hydrodynamic simulations of Milky Way-like galaxies simulated within the EAGLE and APOSTLE projects.
1910
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1915
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2002
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C. W. Purcell, J. S. Bullock, and M. Kaplinghat, The Dark Disk of the Milky Way
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R. Schönrich, J. Binney, and W. Dehnen, Local kinematics and the local standard of rest
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R. Catena and P. Ullio, A novel determination of the local dark matter density
2010
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M. Weber and W. de Boer, Determination of the Local Dark Matter Density in our Galaxy
2010
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2010
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R. Schoenrich, J. Binney, and W. Dehnen, Local Kinematics and the Local Standard of Rest
2010
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2010
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C. McCabe, DAMA and CoGeNT without astrophysical uncertainties
2011
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P. J. McMillan, Mass models of the Milky Way
2011
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2011
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2011
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2014
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2014
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P. J. Fox, Y. Kahn, and M. McCullough, Taking Halo-Independent Dark Matter Methods Out of the Bin
2014
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2014
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2011
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2012
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P. Gondolo and G. B. Gelmini, Halo independent comparison of direct dark matter detection data
2012
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2012
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2012
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C. D. Vecchia and J. Schaye, Simulating galactic outflows with thermal supernova feedback
2012
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M. C. Smith, S. H. Whiteoak, and N. W. Evans, Slicing and dicing the Milky Way disk in SDSS
2012
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J. Bovy and S. Tremaine, On the local dark matter density
2012
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2014
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2014
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2014
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2014
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T. Piffl et al., The RAVE survey: the Galactic escape speed and the mass of the Milky Way
2014
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2014
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F. Iocco, M. Pato, and G. Bertone, Evidence for dark matter in the inner Milky Way
2015
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2015
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2015
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2015
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2015
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2015
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2015
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2015
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2015
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2015
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2015
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Y. Sofue, Dark halos of M?31 and the Milky Way
2015
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2015
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2015
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2016
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