Keplerian prediction vs observed flat rotation · NFW halo · baryonic decomposition
Galaxy rotation curves measure stellar/gas orbital velocities v(r) = √(GM(r)/r).
For a centrally-concentrated baryonic disk alone, v should fall as ∝ 1/√r (Keplerian) at large radii.
Instead, observations show flat rotation curves extending to 10× the optical radius,
demanding an extended dark matter halo. The NFW profile ρ(r) = ρ_s/[(r/r_s)(1+r/r_s)²]
(Navarro-Frenk-White 1996) from N-body simulations provides an excellent fit.
Dark matter constitutes ~85% of total matter in the universe.