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...
| Main Authors: | , |
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| Format: | Article |
| Published: |
American Physical Society
2014
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| Online Access: | https://eprints.nottingham.ac.uk/34504/ |