Limits on the local dark matter density

Physics

Scientific paper

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Scientific paper

We study the systematic problems in determining the local dark matter density ρdm(R&sun;) from kinematics of stars in the Solar Neighbourhood, using a simulated Milky Way-like galaxy. We introduce a new unbiased method for recovering ρdm(R&sun;) based on the moments of the Jeans equations, combined with a Monte Carlo Markov Chain (MCMC) technique and apply it to real data [1].

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