Solving a Relativistic Ideal Gas Momentum Probability Distribution

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SUMMARY

The discussion focuses on deriving the normalization constant A for the momentum probability distribution of a relativistic ideal gas. The integral equation involves the modified Bessel function of the second kind, which arises during the integration process. The participants clarify that the momentum density distribution is not simply the absolute value of the momentum vector but rather the density of finding a particle with a specific momentum vector. The integration is simplified by converting to spherical coordinates, leading to a representation involving the modified Bessel function.

PREREQUISITES
  • Understanding of relativistic physics concepts, particularly momentum and energy relations.
  • Familiarity with integration techniques, including substitution and integration by parts.
  • Knowledge of Bessel functions, specifically modified Bessel functions of the second kind.
  • Proficiency in spherical coordinates and their application in multi-dimensional integrals.
NEXT STEPS
  • Study the properties and applications of modified Bessel functions of the second kind.
  • Learn about the derivation and significance of the momentum probability distribution in statistical mechanics.
  • Explore advanced integration techniques, particularly in the context of special functions.
  • Investigate the role of hyperbolic functions in mathematical physics and their relation to Bessel functions.
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Physicists, graduate students in theoretical physics, and anyone studying statistical mechanics and relativistic gas dynamics will benefit from this discussion.

Xerxes1986
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Homework Statement


For a relativistic ideal gas, the momentum probability distribution is given by

gif.latex?f(p)=Ae^{-\frac{\epsilon_p}{k_bT}}.gif


where [URL]http://latex.codecogs.com/gif.latex?\epsilon_p=\sqrt[]{m^2c^4+c^2p^2}.[/URL] Determine A

Homework Equations





The Attempt at a Solution



I know that:
[URL]http://latex.codecogs.com/gif.latex?\int_{-\infty}^{\infty}Ae^{-\frac{\epsilon_p}{k_bT}}dp=1[/URL]

Which boils down to:
[URL]http://latex.codecogs.com/gif.latex?A\int_{-\infty}^{\infty}e^{-\frac{\sqrt[]{m^2c^4+c^2p^2}}{k_bT}}dp=1[/URL]


I have no idea how to integrate this function. I have tried substitution, integration by parts...everything. After researching on line I know that the solution is:

[URL]http://upload.wikimedia.org/math/4/e/6/4e6b1c37ebe913700d63984beaa7a429.png[/URL]


But I need help understanding how a modified Bessel function pops into the solution...I don't even really understand what the Bessel function is.
 
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First of all the momentum density distribution you gave is not the distribution of the absolute value of the momentum vector. i.e. it is not the density of the probability of finding a particle between p and p+dp. Rather it is the density probability of finding a particle with momentum (p_x+dp_x,p_y+dp_y,p_z+dp_z) i.e. it is the distribution density of the momentum vector.

So to normalize we have to integrate over all three directions:

[tex]1=\int d^3p A\cdot \exp\left(\sqrt\left(m^2c^4+c^2(p_x^2+p_y^2+p_z^2\right)\right) = \int_{-\infty}^{\infty}dp_x\int_{-\infty}^{\infty}dp_y\int_{-\infty}^{\infty}dp_z A\exp\left(\sqrt\left(m^2c^4+c^2(p_x^2+p_y^2+p_z^2\right)\right)[/tex]

Now this integral looks quite tough, hence let's change to spherical coordinates in the momentum space. We see that the integrand doesn't depend on the angles hence In this case we know that the volume element is simply [tex]4\pi p^2 dp[/tex] where obviously [tex]p^2=p_x^2+p_y^2+p_z^2[/tex].

So the integral will look like:

[tex]1=4\pi A\int_0^{\infty}dp p^2e^{-\frac{mc^2}{kT}\sqrt{1+\frac{p^2}{m^2c^2}}}[/tex]

Now put [tex]\sinh u = \frac{p}{mc}[/tex]
Then perform the partial integration (which is a bit tricky, but i will let you think about it). And you will recognize one of the integral representations of the modified Bessel function of the second kind with order 2.
 
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The Bessel functions are basically solutions of the Bessel differential equation. The usually arise when writing the laplacian in cylindrical coordinates and separating the variables. The radial part will be the Bessel differential equation. The solutions to these are the Bessel functions.
In this case however we have modified Bessel functions. You can think of these just as of the usual Bessel functions, just with a purely imaginary argument.
They can be represented in many forms but not as a combination of elementary functions. Thats why they have a separate name and are called special functions. They have many power series representations, integral representations etc.
Usually as a rule of thumb when you see an integral which has an exponential term with an argument containing sines or cosines, hyperbolic functions , then it is most probably a representation of a Bessel function.
In our case as you will see the exponential term contains a hyperbolic cosine function, hence we can guess that it will be a modified Bessel function.
Here are some of the integral representations of the modified Bessel function we will obtain:

http://functions.wolfram.com/Bessel-TypeFunctions/BesselK/07/01/01/

Out of these number 3 will be the one you need.
 

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