A two-fluid conduction model of stars plus collisionless dark matter predicts that most globular clusters have undergone mass segregation and core collapse on a Hubble time, whereas most dwarf galaxies have not.
Note that the first and second terms on the right- hand sides of Eqs
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Dynamical Evolutions in Globular Clusters and Dwarf Galaxies: Conduction Fluid Simulations
A two-fluid conduction model of stars plus collisionless dark matter predicts that most globular clusters have undergone mass segregation and core collapse on a Hubble time, whereas most dwarf galaxies have not.