NFW Dark Matter Halos and Virial Radius

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Discussion Overview

The discussion revolves around the NFW Dark Matter Halos, specifically focusing on the definition of the virial radius, denoted as r_{200}, and the rationale behind using a density threshold of 200 times the critical density of the universe. Participants explore the historical and arbitrary nature of this definition and seek references for its origin.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • One participant explains the NFW density model and the significance of the virial radius r_{200} as the radius where the mass density equals 200 times the critical density.
  • Another participant suggests that the choice of 200 as a threshold is largely historical and arbitrary, noting that other thresholds like R500, R100, and R150 exist in the literature.
  • A request for references regarding the origin of the 200 threshold is made, indicating a desire for deeper understanding.
  • A suggestion to refer to the original NFW paper is provided as a potential starting point for further investigation.

Areas of Agreement / Disagreement

Participants generally agree that the choice of the density threshold is not universal and can vary, but there is no consensus on the specific historical context or the original paper that established the 200 threshold.

Contextual Notes

The discussion does not resolve the question of the historical rationale behind the choice of 200 as the density threshold, and the implications of using different thresholds are not fully explored.

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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