Maxwellian Distribution of Velocities

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Homework Help Overview

The discussion revolves around the Maxwellian distribution of velocities in a one-dimensional context, specifically focusing on calculating the mean speed and mean square speed of a group of stars characterized by a velocity dispersion, \sigma. Participants are analyzing the integrals related to the distribution function and attempting to reconcile their results with known values.

Discussion Character

  • Exploratory, Mathematical reasoning, Assumption checking

Approaches and Questions Raised

  • Participants discuss the integration of the velocity distribution function to find mean values, questioning the correctness of their calculations and the assumptions regarding dimensionality. There is a focus on the integration methods used and the implications of one-dimensional versus three-dimensional distributions.

Discussion Status

Some participants have identified discrepancies in their calculations and are seeking clarification on integration techniques. There is an ongoing exploration of the relationship between the one-dimensional case and the expected results, with some suggesting that the provided answers may be incorrect. The discussion remains open, with various interpretations being considered.

Contextual Notes

Participants note that the problem is framed within a one-dimensional context, which may differ from standard results typically associated with three-dimensional distributions. There is also mention of potential errors in the integration process and the need for careful consideration of the setup and definitions used in the calculations.

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Homework Statement


A group of stars in a Maxwellian distribution have a one-dimensional velocity dispersion [itex]\sigma[/itex]. The number of objects within an element [itex]d^3v[/itex] is

[itex]dN=F(v) d^3 v=\beta\hspace{2pt}Exp[-v^2/2 \sigma^2]d^3v[/itex] where [itex]\beta[/itex] is a constant

Find that the mean speed [itex]\bar{v}=\sqrt{8/\pi} \text{ }\sigma[/itex] and [itex]\bar{v^2}=3\sigma^2[/itex]

Homework Equations



I think I need to use these:

[itex]\bar{v}=<v>=\int^\infty_0 v F(v) dv[/itex]
[itex]\bar{v^2}=<v^2>=\int^\infty_0 v^2 F(v) dv[/itex]


The Attempt at a Solution



I'm trying to find the right approach, neither of the above integrals yield the correct answer. Here's what I tried:

[itex]F(v)[/itex] can be found in the equation for [itex]dN[/itex]
[itex]F(v)=\beta Exp[-v^2/2\sigma^2][/itex]

[itex]\bar{v}=\beta \int^\infty_0 v Exp[-v^2/2\sigma^2] dv[/itex]
[itex]\bar{v}=\beta [4 \sigma^4][/itex]
which can equal [itex]\sqrt{8/\pi}[/itex] if [itex]\beta=\sqrt{2}/2\sigma^3[/itex]

However then [itex]\bar{v^2}=\beta \int^\infty_0 v^2 Exp[-v^2/2\sigma^2] dv[/itex]
[itex]\bar{v^2}=\beta [16 \sigma^6][/itex]

Putting in [itex]\beta=\sqrt{2}/2\sigma^3[/itex]:
[itex]\bar{v^2}=\sqrt{2}\hspace{3pt} 8 \sigma^3[/itex]

while the given answer above was [itex]\bar{v^2}=3\sigma^2[/itex]

Where have I gone wrong? Thanks
 
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cahill8 said:

Homework Statement


Find that the mean speed [itex]\bar{v}=\sqrt{8/\pi} \text{ }\sigma[/itex] and [itex]\bar{v^2}=3\sigma^2[/itex]

Are you sure that's the answer? It is for the 3-dimensional case, but we're only talking about a 1-dimensional distribution.

[itex]\bar{v}=\beta \int^\infty_0 v Exp[-v^2/2\sigma^2] dv[/itex]
[itex]\bar{v}=\beta [4 \sigma^4][/itex]

You made a mistake somewhere in the integration.

However then [itex]\bar{v^2}=\beta \int^\infty_0 v^2 Exp[-v^2/2\sigma^2] dv[/itex]
[itex]\bar{v^2}=\beta [16 \sigma^6][/itex]

This is also not correct. How did you integrate these functions?
 
Thanks for the reply. That is the answer given (from the textbook galaxy dynamics, problem 4.18)

Your right those answers were wrong, I calculated them using mathematica when writing this topic but inputted the equation wrong.

The first can be done by making a u substitution [itex]u=v^2/2\sigma^2[/itex] which leads to an answer of [itex]\bar{v}=\beta \sigma^2[/itex]. This can be correct if [itex]\beta=\dfrac{\sqrt{8/\pi}}{\sigma}[/itex]

In order to check this, I calculate [itex]\beta \int^\infty_0 v^2 exp[-v^2/2\sigma^2] dv[/itex] in mathematica, this gives [itex]\bar{v^2}=\beta \sqrt{\pi/2} \hspace{2pt}\sigma^3[/itex] and after substituting the above [itex]\beta[/itex]:

[itex]\bar{v^2}=\sqrt{\dfrac{8\pi}{2\pi}}\sigma^2=2 \sigma^2[/itex] While close, the correct answer is [itex]3\sigma^2[/itex].

Can you see where I went wrong?
 
I got the exact same answer, so as long as the question is one-dimensional, I think we're both right and the answer key is wrong.

The reason the answer is different for 3 dimensions is that dN has an extra factor of v^2, to account for the fact that the number of combinations of one-dimensional velocities that give a total speed of "v" increases as v^2. However, no such factor exists for the one-dimensional case.
 
Well another part of the question says the mean of one component of velocity, [itex]\bar{v_x^2} = \sigma^2[/itex]

could I simply continue and say [itex]\bar{v_x^2}=\beta\int^\infty_0 v_x^2\hspace{2pt} exp\left[-(\sqrt{v_x^2+v_y^2+v_z^2})^2/2\sigma^2\right] dv= \beta\int^\infty_0 v_x^2\hspace{2pt} exp\left[-(v_x^2+v_y^2+v_z^2)/2\sigma^2\right] dv[/itex]
Not so sure about [itex]dv[/itex] though, [itex]v=(v_x^2+v_y^2+v_z^2)^{1/2}[/itex] [itex]dv=?[/itex]
 

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