Claims that inner-halo power-law profiles in core-collapsing globular clusters follow from Buckingham's Pi theorem and conservation laws, without assuming self-similarity.
Numerical integration of the fokker-planck equation and the evolution of star clusters
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Origin of the power-law profile in a core-collapsing galactic globular-cluster model
Claims that inner-halo power-law profiles in core-collapsing globular clusters follow from Buckingham's Pi theorem and conservation laws, without assuming self-similarity.