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We present an equilibrium statistical mechanical theory of collisionless self-gravitational systems with isotropic velocity distributions.
The conjecture that the ancient globular clusters (GCs) formed at the center of their own dark matter halos was first proposed by Peebles (1984), and has recently been revived to explain the puzzling ...
The apparent presence of large core radii in Low Surface Brightness galaxies has been claimed as evidence in favor of warm dark matter. Here we show that WDM halos do not have cores that are large fra...
We investigate the dynamical basis of the classic empirical models (specifically, Sersic-Einasto and generalized NFW) that are widely used to describe the distributions of collisionless matter in gala...
We present an equilibrium statistical mechanical theory of collisionless self-gravitational systems with isotropic velocity distributions.

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