Nassim Bozorgnia, Graciela B. Gelmini, Paolo Gondolo
We discuss a novel dark matter signature relevant for directional detection
of Weakly Interacting Massive Particles (WIMPs). For heavy enough WIMPs and low
enough recoil energies, the maximum of the recoil rate is not in the direction
of the average WIMP arrival direction but in a ring around it at an angular
aperture that increases with the WIMP mass and can approach 90 degrees at very
low energies. The ring is easier to detect at smaller WIMP velocity dispersions
and larger average WIMP velocities relative to the detector. The ring could be
used to infer the WIMP mass.
View original:
http://arxiv.org/abs/1111.6361
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