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This document proposes using precision measurements of stellar accelerations to directly probe the local dark matter density and distribution in the Milky Way galaxy. The document discusses using radial velocity measurements of stars over time to measure their differential accelerations, which are directly related to the gravitational potential and thus the dark matter density. Numerical simulations suggest detecting accelerations at the level of 10^-8 cm/s^2 for over 100 stars could constrain both the loca

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afdsiomfsdiodfsio

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EN