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We present a method to calculate, without making assumptions about the local dark matter velocity distribution, the maximal and minimal number of signal events in a direct detection experiment given a set of constraints from other direct detection experiments and/or neutrino telescopes.
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C. W. Purcell, J. S. Bullock and M. Kaplinghat, The Dark Disk of the Milky Way , Astrophys.J. 703
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2009
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Cambridge U. Press, 2010
G. Bertone, ed., Particle Dark Matter: Observations, Models and Searches · 2010
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2010
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A. M. Green, Dependence of direct detection signals on the WIMP velocity distribution , JCAP 1010
2010
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T. Marrodán Undagoitia and L. Rauch, Dark matter direct-detection experiments , J. Phys. G43
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