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• W2038077144 abstract "New techniques for the laboratory direct detection of dark matter weakly interacting massive particles (WIMPs) are sensitive to the recoil direction of the struck nuclei. We compute and compare the directional recoil rates $dR/dmathrm{cos}ensuremath{theta}$ (where $ensuremath{theta}$ is the angle measured from a reference direction in the sky) for several WIMP velocity distributions including the standard dark halo and anisotropic models such as Sikivie's late-infall halo model and logarithmic-ellipsoidal models. Since some detectors may be unable to distinguish the beginning of the recoil track from its end (lack of head-tail discrimination), we introduce a folded directional recoil rate $dR/d|mathrm{cos}ensuremath{theta}|$, where $|mathrm{cos}ensuremath{theta}|$ does not distinguish the head from the tail of the track. We compute the ${mathrm{CS}}_{2}$ and ${mathrm{CF}}_{4}$ exposures required to distinguish a signal from an isotropic background noise, and find that $dR/d|mathrm{cos}ensuremath{theta}|$ is effective for the standard dark halo and some but not all anisotropic models." @default.
• W2038077144 created "2016-06-24" @default.
• W2038077144 creator A5009682080 @default.
• W2038077144 creator A5074732736 @default.
• W2038077144 date "2008-02-29" @default.
• W2038077144 modified "2023-10-14" @default.
• W2038077144 title "Directional recoil rates for WIMP direct detection" @default.
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• W2038077144 doi "https://doi.org/10.1103/physrevd.77.043532" @default.
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