Maxwellian Distribution of Velocities

In summary: The mean speed is equal to the square root of 8 divided by pi multiplied by the sum of the squares of the individual speeds. So it would be 8/pi multiplied by (v_x^2+v_y^2+v_z^2)^{1/2} which is 3/2 Sigma squared.
  • #1
cahill8
31
0

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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  • #2
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?
 
  • #3
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?
 
  • #4
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.
 
  • #5
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]
 

FAQ: Maxwellian Distribution of Velocities

What is the Maxwellian Distribution of Velocities?

The Maxwellian Distribution of Velocities is a probability distribution that describes the distribution of speeds of particles in a gas at a given temperature. It is named after physicist James Clerk Maxwell, who developed the theory in the 19th century.

What does the shape of the Maxwellian Distribution of Velocities look like?

The shape of the Maxwellian Distribution of Velocities is a bell-shaped curve, similar to a normal distribution. The peak of the curve represents the most probable speed of the particles, while the width of the curve represents the range of speeds that the particles can have.

What factors affect the Maxwellian Distribution of Velocities?

The Maxwellian Distribution of Velocities is affected by temperature, mass of the particles, and the type of gas. As temperature increases, the curve becomes wider and the peak shifts to higher speeds. Heavier particles have a lower peak and a wider curve compared to lighter particles. Different gases have different peak speeds and curve shapes.

What is the significance of the Maxwellian Distribution of Velocities?

The Maxwellian Distribution of Velocities is an important concept in thermodynamics and statistical mechanics. It helps explain the behavior of gases and is used in many applications, such as in the design of engines and turbines. It also provides a basis for understanding diffusion, viscosity, and thermal conductivity.

Can the Maxwellian Distribution of Velocities be applied to all gases?

While the Maxwellian Distribution of Velocities is commonly used to describe the behavior of ideal gases, it can also be applied to real gases with some modifications. In some cases, more complex distributions may be used to accurately describe the behavior of specific gases. However, the Maxwellian Distribution is a good approximation for many gases and is widely used in scientific research and engineering applications.

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