Homework - Interparticle distance between galaxies

Click For Summary
SUMMARY

The discussion revolves around the calculation of interparticle distance between galaxies, focusing on the total number density of galaxies and its practical implications. Participants seek formal expressions for galaxy density, luminosity, and neighbor counts, while addressing the challenges of applying theoretical models to observational data. Key equations involve the number density of galaxies as a function of luminosity and mass, as well as power-law correlation functions for estimating neighbor counts.

PREREQUISITES
  • Understanding of galaxy luminosity and mass functions
  • Familiarity with power-law correlation functions in cosmology
  • Knowledge of density contrast in astrophysics
  • Basic principles of observational astronomy and data interpretation
NEXT STEPS
  • Research the formal expression for total galaxy number density as a function of luminosity and mass
  • Study the application of power-law correlation functions in estimating galaxy neighbor counts
  • Learn how to calculate density contrast from neighbor counts in a given volume
  • Explore observational techniques for measuring galaxy luminosity and density
USEFUL FOR

Astronomy students, astrophysicists, and researchers interested in galactic structures and intergalactic distances will benefit from this discussion.

fab13
Messages
300
Reaction score
7

Homework Statement


[/B]
I have the following questions as homeworks and I would like to get help.

Question 1) Give the formal expression of the total number density of galaxies. Why is this expressoin problematic in practice?

Question 2) In practice one uses a numerical value for the number density of galaxies and for their typical luminosity. Explain why and how.

Question 3) Using the above typical values, infer an estimation of ##l_{g}## ,
the inter galaxy distance.

Question 4) Using a powerlaw correlation function, give the formal expression of the total number neighbours of a galaxy.

Question 5) Infer the distance of the inter galaxy distance

Question 6) From the number of neigbours infer the density contrast it represents

Homework Equations

: equations concerned are not provided into this homework[/B]

The Attempt at a Solution



Question 1) I saw from my research different expressions for the total density of galaxies (as a function of Luminosity or Mass), but which one could correspond to this question 1 ? What is this formal expression ?

Then, why this total density is problematic ?

Question 2) It seems to be related to the problematic above.

Can I use, for a sample of galaxies ##S##, with ##L## luminosity :

##\Phi_{s}(L) = \dfrac{n_{s}(L)}{V_{s}(L)}## which is the number of galaxies in S per unit luminosity ?

? If yes, why have I got to use ##\Phi_{s}(L)## compared to formula in question 1 ?

Question 3): How can I infer an estimation of inter galaxy distance from expressions into question 1 and question 2 above ?

Question 4): I didn't see the expression of the total number neighbours of a galaxy : anyone could give me help about the expression to apply in this case ?

Question 5): If I knew the formula of question 4, I could compute the average distance between two galaxies

Question 5): I must estimate the number of neighbours of main galaxy up to a distance ##r##and so estimate the density contrast that represents.
I don't see how to estimate this density contrast since I have not the expression asked on question 5.
Sorry if the answers are simple but I am a beginner in galactic and extra-galactic matters.

Even short answers or suggestions could help me to solve these different questions.

Thanks
 
Physics news on Phys.org
fab13 said:
Question 1) I saw from my research different expressions for the total density of galaxies (as a function of Luminosity or Mass), but which one could correspond to this question 1 ? What is this formal expression ?
I am only guessing here, but what you find online will mostly be concerned with estimating the value from observations, whereas "formal expression" sounds like they are asking for a definition.
How would you define the term?
 
@haruspex

I wonder if the expression of this "total density of galaxies" has to imply luminosity distribution or mass distribution. But the clue is that expression has to be problematic from a physical point of view (from what is said in homework).

So if someone could give me indications to find the appropriate relation of "total density of galaxies". Regards
 

Similar threads

  • · Replies 8 ·
Replies
8
Views
1K
  • · Replies 1 ·
Replies
1
Views
3K
  • · Replies 4 ·
Replies
4
Views
2K
  • · Replies 9 ·
Replies
9
Views
2K
  • · Replies 5 ·
Replies
5
Views
3K
  • · Replies 6 ·
Replies
6
Views
4K
  • · Replies 15 ·
Replies
15
Views
3K
  • · Replies 8 ·
Replies
8
Views
2K
  • · Replies 10 ·
Replies
10
Views
2K
  • · Replies 0 ·
Replies
0
Views
2K