NFW Dark Matter Halos and Virial Radius

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SUMMARY

The discussion centers on NFW Dark Matter Halos, a density model formulated by Navarro, Frenk, and White. The model's density structure is defined by the equation ρ(r) = (δc ρc) / ((r/rs)(1 + r/rs)^2), where δc and rs are critical parameters related to the halo's virial radius, r200. The mass within this radius, M200, is calculated as M200 = (800π/3)ρc r200^3. The choice of the factor 200 in defining r200 as the radius where the density equals 200ρc is primarily historical and arbitrary, with variations like R500 and R100 used in different contexts.

PREREQUISITES
  • Understanding of NFW Dark Matter Halo models
  • Familiarity with cosmological density parameters
  • Knowledge of virial radius and its significance in astrophysics
  • Basic calculus for integrating density functions
NEXT STEPS
  • Research the original NFW paper for foundational concepts in dark matter halo modeling
  • Explore the implications of different density multipliers like R500 and R100 in cosmology
  • Study the critical density of the universe and its role in structure formation
  • Investigate the mathematical derivation of mass within dark matter halos
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Astronomers, astrophysicists, and researchers in cosmology who are studying dark matter structures and their implications for the universe's evolution.

zephyr5050
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I've been working with NFW Dark Matter Halos recently. This is a particular density model for the halo developed by Navarro, Frenk, & White (NFW). The density structure has the form
\rho (r) = \frac{\delta_c \rho_c}{(r/r_s)(1+r/r_s)^2}
where
\delta_c = \frac{200}{3} \frac{c^3}{ln(1+c)-c/(1+c)}
r_s = r_{200}/c
and \rho_c is the critical density of the universe (as a function of redshift). The parameter r_{200} is the virial radius which is defined as the radius at which the mass density of the halo is 200\rho_c.

Now we can't really talk about the mass of this halo because the integral from 0 to \infty diverges. Instead, we use the fiducial radius r_{200} and define the quantity M_{200} to be the mass inside the radius r_{200}. It can be shown that
M_{200} = \frac{800\pi}{3}\rho_c r_{200}^3
While all this makes sense to me, there's one thing that I don't understand here. Where does this 200 come from? Why say r_{200} \equiv 200 \rho_c? Is there any logic to this, is it historical, arbitrary? What's going on here?
 
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I think it's basically historical and arbitrary. You have to draw a line somewhere, and the accepted way to do it is when the average density of the cluster falls to 200X the critical density. It's not universal, however. You will find papers referring to R500, R100, R150, etc., all defined in the same way, but with different multipliers.
 
Do you happen to know the paper which proposed this commonly accepted line? If any?
 

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