Dark Matter Halo: Modeling Rotational Effect on Galaxy V(r)

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Discussion Overview

The discussion revolves around the modeling of the rotational effects (V(r)) of galaxies in relation to the potential existence of dark matter halos. Participants explore the implications of dark matter density profiles, particularly in the context of the Milky Way Galaxy, and address questions regarding the physical interpretation of divergent integrals in mass density functions.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • One participant questions how to handle the divergence of the mass density function at zero radius and seeks clarification on its physical significance.
  • Another participant notes that while the density diverges at zero radius, the integral of the density does not diverge and approaches zero, suggesting a resolution to the divergence issue.
  • There is a discussion regarding whether the Milky Way Galaxy is dark matter-dominant, with one participant asserting that dark matter has more than five times the mass of baryonic matter when considering the entire galaxy.
  • Another participant agrees that the Milky Way is baryon-dominated in its inner regions but challenges the claim that the half-light radius is around 100 kpc, suggesting it is actually a few kpc.
  • A later reply confirms the correction regarding the half-light radius, agreeing that it is indeed on the order of a few kpc.

Areas of Agreement / Disagreement

Participants generally agree that the Milky Way is baryon-dominated in its inner regions, but there is disagreement regarding the specific value of the half-light radius and the implications of dark matter dominance overall.

Contextual Notes

There are unresolved assumptions regarding the models used to interpret dark matter density and its effects on galaxy rotation, particularly in relation to angular momentum exchange between normal matter and dark matter.

Creebe
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Hello,

I'm a third year engineering physics student, and my team and I are trying to model how the rotation (V(r)) of a galaxy is affected by the possible existence of the dark matter halo. Here are my questions:

Regarding the dark matter halo:

The integral of the mass density function is divergent at 0, how do we deal with it? How does it make any physical sense.
Here's the formula:
http://en.wikipedia.org/wiki/Navarro-Frenk-White_profile

Is the Milky Way Galaxy dark matter-dominant?
 
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Creebe said:
The integral of the mass density function is divergent at 0, how do we deal with it? How does it make any physical sense.
While the density diverges at 0 radius, the integral of the density (which gives the mass within a given radius) does not (it goes to zero as one might expect).
Creebe said:
Is the Milky Way Galaxy dark matter-dominant?
The wikipedia page you listed links to a http://iopscience.iop.org/0004-637X/573/2/597/pdf/0004-637X_573_2_597.pdf" that indicates (pg. 604, tables 1 and 2) that the ratio of the mass of dark matter to the mass of the disk and bulge of the galaxy within 3 kpc of the center is 0.95 according to the "favored" model without exchange of angular momentum (between normal matter and dark matter) and 0.24 according to the "favored" model with angular momentum exchange. So, while a significant percentage of the matter within that radius is dark matter, normal matter constitutes the majority of the matter (especially in the latter model, which I would think would be more realistic).
 
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Creebe said:
Is the Milky Way Galaxy dark matter-dominant?
Overall: yes. If you look at the entire milky-way galaxy, DM has >5 times as much mass. Baryonic matter, however, is dominant within about the half-light radius (something like 100 kpc)
 
Allthough I agree that in the inner parts the Milky Way is baryon dominated. Nevertheless, the half light radius of the Milky Way is not even close to 100 kpc (that is almost the virial radius of ots host dark matter halo), but rather of the order of a few kpc.
 
harcel said:
Allthough I agree that in the inner parts the Milky Way is baryon dominated. Nevertheless, the half light radius of the Milky Way is not even close to 100 kpc (that is almost the virial radius of ots host dark matter halo), but rather of the order of a few kpc.
Sorry, yes---more like a few kpc---for sure!
 

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