Brownian motion approach to anomalous rotation of galaxies
  It has been shown that the weak-interacting limit of the
metric-skew-tensor-gravity (MSTG) can explain the anomalous rotation of
galaxies without non-baryonic dark matter. We show that MSTG is related to the
equilibrium-state of ordinary Brownian motion. We also explore if other
stochastic processes can model anomalous rotation. Furthermore, we analyze
phase-diagrams that elucidate the condensation of a gravitating cloud towards a
Kepler-Newton system and illustrate regions of existence of rotating objects.
