Maximizing small-scale clustering in action space recovers the Milky Way dark matter halo parameters (f_h, alpha) = (0.391, 1.835) and (0.351, 1.687) in two radial bins from Gaia DR2.
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Gravitational Potential from small-scale clustering in action space: Application to Gaia DR2
Maximizing small-scale clustering in action space recovers the Milky Way dark matter halo parameters (f_h, alpha) = (0.391, 1.835) and (0.351, 1.687) in two radial bins from Gaia DR2.