Exploring Dark Matter: Distribution, Effects, and Resources

In summary, there are various models and proposals for dark matter distribution, but current research suggests that it is highly concentrated in the center of galaxies like the Milky Way and has a low density within our solar system. There are also resources available for learning more about dark matter, including articles and textbooks on observational cosmology.
  • #1
Lapidus
344
11
How is dark matter distributed (as far as we know)?

Let's stay with a single galaxy like the Milky Way. I heard that dark matter is even more concentrated in the center than in the halo, that it is falling off when moving outside, but since the halo is so huge (how huge, ten times larger?) most dark matter can be found there. Is that correct?

So there is dark matter also in our solar system. But by what density? If the density would be high, we would have noticed it by the motion of the planets or nearby stars. Can the effect of dark matter only be seen at larger distances where it accumulates despite its low density?

thanks!
 
Space news on Phys.org
  • #2
What you said is largely correct. There's lots of work to understand the Milky Way dark matter halo. One model (see this paper) is a density profile like:
[tex] \rho_{DM} = \rho_0 (r/r_s)^{-\gamma} (1+r/r_s)^{-3+\gamma}[/tex]

with gamma = 1.24, rs = 28.1 kpc, and rho0 = 3.5E-3 Msun/pc^3.

This profile never goes to zero, so it is hard to characterize how "big" it is, but one way that is often used is to ask at what radius does the density drop off to 200 times the average density of the universe. For this profile, this is atound 300 kpc, so about 10 times the size of the Milky Way galaxy. Within this radius, this profile has a total mass of about 2E12 Msun, so it dominates the mass of the galaxy. However, at smaller radii, the ordinary matter dominates. If we look at the radius of the sun (r = ~8 kpc), then the dark matter density is about .01 Msun/pc^3. We can then ask how much dark matter is, say, inside Saturn's orbit, and the result is about 1E-18 Msun or about 7E15 kg. This is the mass of a small asteroid, and is completely negligible compared to the mass of the sun and planets. Does this answer your questions?
 
  • Like
Likes exmarine and Lapidus
  • #3
Yes, that answers my question, thanks!
 
  • #4
Btw, does anybody know a great review/ overview article (or a book or sections of a book) about dark matter? One that is not complete layman but not complete specialist either.

thanks!
 
  • #5
Lapidus said:
Btw, does anybody know a great review/ overview article (or a book or sections of a book) about dark matter? One that is not complete layman but not complete specialist either.

thanks!
my signature contains numerous article that have sections covering dark matter. Most articles directly related to DM are related to distributions, properties etc of specific proposals and models. the misconceptions section on the http://cosmology101.wikidot.com/main signature link has one decent non technical article with a dark matter section. The articles on the site are primarily geared to helping teach modern cosmology. In particular the FLRW metrics etc. There are some textbook style articles on cosmology that include DM modelling.

http://arxiv.org/abs/1304.4446 :"What we have leaned from Observational Cosmology." -A handy write up on observational cosmology in accordance with the LambdaCDM model

you can also browse www.arxiv.com however keep in mind what I stated above, concerning the numerous alternate proposals.
 
  • Like
Likes 1 person

What is dark matter?

Dark matter is a type of matter that makes up a large portion of the universe, but does not interact with light or other forms of electromagnetic radiation. It is invisible and cannot be directly observed, but its presence can be detected through its gravitational effects on visible matter.

How is dark matter distributed in the universe?

The distribution of dark matter is not uniform, but rather it is clumped in certain areas of the universe. It is thought to be distributed in a web-like structure, with filaments connecting clusters of galaxies.

What evidence do we have for the existence of dark matter?

The existence of dark matter is supported by a variety of observations, including the rotation of galaxies, gravitational lensing, and the large-scale structure of the universe. These observations cannot be explained by the presence of only visible matter, leading scientists to propose the existence of dark matter.

How does dark matter interact with regular matter?

Dark matter does not interact with regular matter through electromagnetic forces, so it cannot be seen or felt. It only interacts with regular matter through its gravitational pull.

How does the distribution of dark matter affect the formation of galaxies?

The clumped distribution of dark matter plays a crucial role in the formation of galaxies. The gravitational pull of dark matter helps to draw in normal matter, which then forms into galaxies. Without the presence of dark matter, galaxies would not have formed in the way that they have.

Similar threads

  • Cosmology
Replies
14
Views
1K
Replies
4
Views
910
Replies
10
Views
1K
Replies
20
Views
2K
Replies
9
Views
949
Replies
4
Views
1K
Replies
2
Views
1K
Replies
14
Views
2K
Replies
17
Views
2K
Back
Top