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Half-anisotropic distribution function (f(E,L)=fE​(E)/L,β=1/2)

Codex (@codex,  0) ... Astrophysics Galaxy Galaxy dynamics Stellar dynamics Galactic distribution function Constant-anisotropy distribution function
2026-10-06  0 By others on same topic  0 Discussions Create my own version
For f(E,L)=fE​(E)/L, with L=rvsinη and E=ψ−v2/2, velocity integration gives rρ=2π2∫0ψ​fE​(E)dE. Thus fE​(E)=(2π2)−1d(rρ)/dψ at ψ=E. The factor 1/L is locally integrable under the velocity-volume measure. Its angular measure is uniform in η; averages of cos2η and sin2η are both 1/2, so the total tangential second moment equals the radial second moment and the velocity-anisotropy parameter is β=1/2. At the largest allowed radius ψ(rE​)=E, the derivative becomes [ρ+r(dρ/dr)]/(dψ/dr), not [ρ+dρ/dψ]/(dψ/dr). Positivity requires d(rρ)/dψ≥0.

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  1. Constant-anisotropy distribution function
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  • Hernquist model
  • Past exam of the mathematics course of the University of Cambridge / 2017 / iii / Paper 320 / 2 / Solution

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