We study the systematic problems in determining the local dark matter density ρdm(R⊙) 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⊙) based on the moments of the Jeans equations, combined with a Monte Carlo Markov Chain technique and apply it to real data. ov
@article{arxiv.1111.5122,
title = {Limits on the local density of dark matter},
author = {Silvia Garbari and Justin I. Read and George Lake},
journal= {arXiv preprint arXiv:1111.5122},
year = {2012}
}
Comments
2 pages, 1 figure, to appear in the proceedings of "Assembling the Puzzle of the Milky Way", Le Grand Bornand (April 17-22, 2011), C. Reyle, A. Robin, M. Schultheis (eds.)