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Next: The Chapman-Enskog Method Up: The Boltzmann Equation Previous: The Collision Function

Boltzmann's H-Theorem

Boltzmann's equation describes the evolution of molecules in a rare gas. If no external forces are present ( tex2html_wrap_inline13171 ) then, after a long time, the gas should reach an equilibrium state. This can be seen [14, 11] by considering the function

  equation473

Differentiating equation (2.19) with respect to time we get

equation479

Substituting tex2html_wrap_inline13177 from equation (2.3), with tex2html_wrap_inline13171 , and using equation (2.16) we get

  equation486

Now, following [14], consider the first term on the right hand side of equation (2.21). Since tex2html_wrap_inline12921 and tex2html_wrap_inline12911 are independent variables we can write tex2html_wrap_inline13191 as tex2html_wrap_inline13193 and using Gauss's theorem we can write

equation505

where tex2html_wrap_inline13201 is the surface enclosing the volume tex2html_wrap_inline13071 . Now tex2html_wrap_inline13205 so the first term on the right-hand side of equation (2.21) vanishes. This leaves

  equation523

Now consider the reverse of the collision: particles with velocity tex2html_wrap_inline12921 and tex2html_wrap_inline13143 colliding and moving off with velocities tex2html_wrap_inline13137 and tex2html_wrap_inline13139 . For this collision we have

  equation536

since tex2html_wrap_inline13223 . Summing equations (2.23) and (2.24) and dividing by two gives

  equation554

Changing the dummy variables tex2html_wrap_inline13229 and tex2html_wrap_inline13231 we get

  equation568

Finally summing equations (2.25) and (2.26) and dividing by two gives

  equation580

Now tex2html_wrap_inline13241 and all the other terms in the integrand of equation (2.27) are positive so

  equation593

This means that H can never increase and is known as Boltzmann's H-theorem. It can also be shown that H is bounded below [11]. We know that tex2html_wrap_inline13249 converges because the total energy of the molecules must converge. Thus either H converges or tex2html_wrap_inline13253 more rapidly than tex2html_wrap_inline13255 as tex2html_wrap_inline13257 . In the later case tex2html_wrap_inline13259 more rapidly than tex2html_wrap_inline13261 which implies that H converges. Since H can never increase but tends to a finite limit the finite limit must correspond to tex2html_wrap_inline13267 . This is only possible, see equation (2.27), if

equation601

This condition is known as detailed balance [11] and can be expressed equivalently as

equation604

Thus if tex2html_wrap_inline13269 is the equilibrium distribution then tex2html_wrap_inline13271 is a collision invariant and so must be of the form

equation608

where tex2html_wrap_inline13049 are the collision invariants defined below equation (2.7) and tex2html_wrap_inline13275 are constants. This can be re-written [11]

equation613

where tex2html_wrap_inline13277 and tex2html_wrap_inline13279 . With tex2html_wrap_inline13281 where tex2html_wrap_inline13283 we can write

  equation628

This is the Maxwell distribution function for a gas [11, 12, 14] and it describes the equilibrium state of the distribution function f. The form of the constants can be found by substituting equation (2.33) into equation (2.5) to give the more common form of the Maxwell distribution function [11, 12]

  equation638

The H-theorem states that the distribution function f must tend towards its equilibrium state tex2html_wrap_inline13269 . The entropy S(t) of the system (which is a non-decreasing function of time) is given by [11, 14]

equation652


next up previous contents
Next: The Chapman-Enskog Method Up: The Boltzmann Equation Previous: The Collision Function

James Buick
Tue Mar 17 17:29:36 GMT 1998