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The DAMA/NaI and DAMA/LIBRA annual modulation data, which may be interpretedas a signal for the existence of weakly interacting dark matter (WIMPs) in ourgalactic halo, are re-examined in light of new measurements of the localvelocity relative to the galactic halo. In the vicinity of the Sun, thevelocity of the Galactic disk has been estimated to be 250 km/s rather than 220km/s. Our analysis is performed both with and without the channeling effectincluded. The best fit regions to the DAMA data are shown to move to slightlylower WIMP masses. Compatibility of DAMA data with null results from otherexperiments (CDMS, XENON10, and CRESST I) is investigated given these newvelocities. A small region of spin-independent (elastic) scattering for 7-8 GeVWIMP masses remains at 3$\sigma$. Spin-dependent scattering off of protons isviable for 5-15 GeV WIMP masses for direct detection experiments (but has beenargued by others to be further constrained by Super-Kamiokande due toannihilation in the Sun).

Compatibility of DAMA/LIBRA dark matter detection with other searches in light of new Galactic rotation velocity measurements