A self-consistent phase-space distribution function for the anisotropic dark matter halo of the Milky Way

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A self-consistent phase-space distribution function for the anisotropic dark matter halo of the Milky Way

Dark Matter (DM) direct detection experiments usually assume the simplest possible ‘Standard Halo Model’ for the Milky Way (MW) halo in which the velocity distribution is Maxwellian. This model assumes that the MW halo is an isotropic, isothermal sphere, hypotheses that are unlikely to be valid in r...

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Bibliographic Details
Main Authors:	Fornasa, Mattia, Green, Anne M.
Format:	Article
Published:	American Physical Society 2014
Online Access:	https://eprints.nottingham.ac.uk/34504/

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