An Introduction to Modern Astrophysics · Problem 24.24
The Early Universe — Carroll & Ostlie
Physics — Astrophysics · nfw-profile-constants
Problem
Using data provided in the text for the mass of the dark matter halo interior to 50 kpc and interior to 230 kpc, estimate the values for the constants ρ0 and a in the NFW version of the dark matter halo density profile (Eq. 24.52).