Flaw in alternative approach to determine ideal gas speed distribution

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SUMMARY

The discussion centers on the flaw in an alternative approach to determining the ideal gas speed distribution, specifically regarding the relationship between kinetic energy and speed in an ideal gas. It is established that while there is a one-to-one relationship between speed and kinetic energy, the velocity distribution must account for the vector nature of velocity, which leads to the Maxwell-Boltzmann distribution. The derivation of the Maxwell-Boltzmann speed distribution involves integrating the phase-space distribution function and transforming from momentum to velocity, ultimately revealing the necessity of considering the solid angle in the distribution.

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  • Understanding of Boltzmann distribution and its implications in statistical mechanics.
  • Familiarity with Maxwell-Boltzmann speed distribution and its derivation.
  • Knowledge of phase-space distribution functions in statistical physics.
  • Basic concepts of kinetic energy and its relationship to particle velocity.
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  • Study the derivation of the Maxwell-Boltzmann speed distribution in detail.
  • Explore the implications of phase-space distribution functions in thermodynamics.
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If we assume the energy of particles in an ideal gas follows a Boltzmann distribution, then the energy distribution function can be defined as below:

1581235438328.png
, where k_B is the Boltzmann constant

Since the energy of particles in an ideal gas are assumed to only consist of translational kinetic energy (as they don't interact),

1581235483586.png
, where v is the speed of the particle

However, for a certain level of kinetic energy, there is only one speed that can be associated with it, as speeds take positive value and hence there is a one-to-one relationship between the speed of a particle and its kinetic energy.

By this reasoning, the distribution function of energy should be proportional to the distribution function of velocity. In other words, the velocity distribution function is also proportional to a Boltzmann factor, with a constant factor of proportionality.

However, the Maxwell-Boltzmann speed distribution shows the velocity distribution having the following form:

1581235505918.png


Although I can follow the derivation of the Maxwell-Boltzmann distribution, I fail to see why the line of reasoning I described in previous paragraphs is wrong. Any help would be much appreciated. Thank you!
 
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Indeed, there is just one speed for any energy, but the quantity of interest is given by the number of available states at a certain energy, which is not given by the speed, but by the velocity - a particle moving along the x-axis is certainly in a different state than a particle moving along the y-axis with the same speed.

Velocity is a vector and if you do a quick drawing of a 3D plot, where the three axes are given by the x-, y- and z-components of the velocity, you will find that all vectors that add up to the same speed form the surface of a sphere. If you take a moment to consider how the number of possible vector component combinations that sum up to the same speed scales with the total speed, you should be able to identify the additional factor in the Maxwell-Boltzmann distribution.
 
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Thank you!
 
The flow is that you don't take the word "distribution" seriously. The Maxwell distribution can be given in various forms. You have to start with the fundamental definition as a phase-space distribution function
$$f(\vec{x},\vec{p})=\frac{1}{(2 \pi \hbar)^3} \exp \left (-\frac{\vec{p}^2}{2m k_{\text{B}} T} \right).$$
Which denotes the number of particles at place ##(\vec{x},\vec{p})## per unit of phase space. If you want to transform this to a velocity distribution you have to integrate over space (which gives simply a factor ##V##) and to transform from momenta to ##\vec{v}=\vec{p}/m##. Now ##\mathrm{d}^3 v=\mathrm{d}^3 p/m^3## and thus
$$f_2(\vec{v})=\frac{m^3 V}{(2 \pi \hbar)^3} \exp \left (-\frac{m \vec{v}^2}{2 k_{\text{B}} T} \right).$$
Now you want the energy distribution. Using
$$E=\frac{m}{2} \vec{v}^2\; \Rightarrow \; \mathrm{d}E=m v \mathrm{d} v = \sqrt{2mE} \mathrm{d} v$$
you get
$$\mathrm{d}^3 v = v^2 \mathrm{d} v \mathrm{d} \Omega=\sqrt{\frac{2 E}{m}}\frac{1}{m} \mathrm{d} E.$$
Integrating over the solid angle leads finally to
$$f_3(E)=\frac{V\sqrt{2Em^3}}{2 \pi^2 \hbar^3} \exp \left (-\frac{E}{k_{\text{B}}} \right).$$
 
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