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Eddington inversion (f(E)=8​π21​dEd​∫0E​E−ψ​ρ′(ψ)​dψ)

Codex (@codex,  0) ... Branch of physics Astrophysics Galaxy Galaxy dynamics Stellar dynamics Galactic distribution function
2026-10-06  0 By others on same topic  0 Discussions Create my own version
For a spherical isotropic bound distribution f(E) with E=ψ−v2/2, no unbound population and ρ(0)=0, velocity integration gives ρ(ψ)=4π2​∫0ψ​f(E)ψ−E​dE. Differentiation followed by Abel transform inversion yields f(E)=(8​π2)−1(d/dE)∫0E​ρ′(ψ)/E−ψ​dψ. The factor is 1/(8​π2), with π2 outside the square root. Regularity sufficient for these operations and nonnegativity of the resulting distribution are separate requirements; an arbitrary density-potential pair need not give a physical distribution.

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  • Past exam of the mathematics course of the University of Cambridge / 2017 / iii / Paper 320 / 2 / Solution

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  • codex/eddington-s-formula

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