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P from the kinetic theory of gases

The kinetic theory of the ideal gas envisions the ideal gas as a cloud of non-interacting point particles. The methods and arguments of kinetic theory are fundamentally unlike those of Gibbs' ensemble treatment of classical statistical mechanics. In each element of a Gibbsian ensemble, atoms have fixed positions and momenta; mechanical variables are evaluated based on atomic coordinates at a single instant in time. In contrast, kinetic theory relies on model calculations in which the motions of atoms are computed over some short time interval tex2html_wrap_inline571 .

Suppose one traces the trajectories of the atoms of an ideal gas. During tex2html_wrap_inline571 , some atoms collide with a container wall, while other do not. The total momentum transferred into the wall by the atom-wall collisions during tex2html_wrap_inline571 is tex2html_wrap_inline769 . This momentum transfer corresponds to an average force tex2html_wrap_inline771 ; for a wall of area tex2html_wrap_inline773 the pressure is tex2html_wrap_inline775 .

Which atoms collide with a wall? Consider V to be an tex2html_wrap_inline609 cube, with the yz-plane at x = 0 as the wall, as shown in Figure 6-3. To collide with the wall between the times 0 and tex2html_wrap_inline571 , at t = 0 an atom with x-momentum tex2html_wrap_inline791 (and velocity tex2html_wrap_inline793 ) must be between x = 0 and tex2html_wrap_inline797 . Since atoms must have tex2html_wrap_inline799 , only atoms with tex2html_wrap_inline801 reach the wall. For an ideal gas, the atoms do not interact with each other, so interatomic collisions do not occur. In a real gas, collisions between atoms affect which atoms strike each wall.

 
Figure 6.3: Kinetic model of the ideal gas. Atoms 1, 2, 3 all have x-component of their velocity tex2html_wrap_inline569 . Atom 1 collides with the wall during tex2html_wrap_inline571 , but atoms 2 and 3 do not. Atom 2 is too far from the wall ( tex2html_wrap_inline573 ), while atom 3 is headed in the wrong direction. Atoms 4 and 5 both have tex2html_wrap_inline575 (with tex2html_wrap_inline577 ) for the x-component of their velocities. While atom 5 is at some tex2html_wrap_inline581 , tex2html_wrap_inline583 still satisfies tex2html_wrap_inline585 , so atom 5 will reach the wall during tex2html_wrap_inline571 .

During tex2html_wrap_inline571 , an atom that collides with the wall transfers to it an impulse tex2html_wrap_inline769 . The impulse's magnitude could be obtained by integrating tex2html_wrap_inline829 over the atom's trajectory x(t). The integration, besides being cumbersome, requires complete knowledge of U(x). Kinetic theory replaces the cumbersome integration with a conservation argument: Suppose tex2html_wrap_inline571 is much larger than the duration of any wall-atom collision. Each atom has an initial x-momentum tex2html_wrap_inline791 . Since an atom is brought to a stop when it hits the wall, all of tex2html_wrap_inline791 must be transferred into the wall. Furthermore, to maintain equilibrium, the atom cannot just stick to the wall. If the atoms all stayed on the wall, the supply of gas atoms within the container would eventually be depleted. A simple assumption, adequate to maintain equilibrium, is that atoms that strike the wall are elastically scattered. For collisions with the yz-plane, elastic scattering takes tex2html_wrap_inline845 onto tex2html_wrap_inline847 while leaving tex2html_wrap_inline849 and tex2html_wrap_inline851 unchanged. An elastically-scattered atom having initial momentum tex2html_wrap_inline791 therefore transfers to the wall an impulse tex2html_wrap_inline855 . [A detailed treatment of atom- wall collisions and adsorption is a hard problem.]

A fundamental assumption of the kinetic theory of gasses is that a gas atom's momentum is described by the Maxwell-Boltzmann distribution

  equation247

The kinetic theory ansatz[1] is that W(r, p) is taken to apply at a single time, the evolution of the system to other times being determined by applying the laws of mechanics. Combining all of the above arguments, the average force on a wall due to a single atom is

  equation259

whencefrom follows

  equation281

The gas atoms do not interact with each other, so the average force on a wall due to N atoms is just N times the average force from a single atom. The kinetic model thus yields the ideal gas law.

In the kinetic model, U(x) was constrained by several implicit assumptions, notably:

(i) Atoms move ballistically, (implied by the upper bound of tex2html_wrap_inline863 ) except during short collisions.

(ii) An atom that has collided with a wall then recedes off to infinity (so that it transfers exactly tex2html_wrap_inline865 of momentum into the wall, without experiencing multiple atom-wall collisions.)

(iii) A collision is an identifiable transient phenomenon.

These assumptions are consistent with a purely repulsive short-range U(x), but are not consistent, e. g. with potentials that allow formation of atom-wall bound states (see problem 6-4). These assumptions are completely wrong for atoms in liquids.

A careful reader will note that eq. 6.16 hides several effects. Suppose an atom strikes the x = 0 plane near tex2html_wrap_inline871 and (y,z) = (0,0), its y- and z- momenta both being large and positive. At t = 0, a simpleminded back-calculation puts such an atom someplace where y, z < 0, contrary to the requirement that atoms stay inside V. The dashed lines in Figure 6.5 indicate the notional original location of the atom, starting in a region which atoms cannot reach, and the atom's subsequent notional trajectory. If atom-wall collisions are elastic, a proper back-calculation shows that such an atom must have originated within V, been scattered by other container walls at some tex2html_wrap_inline885 , finally reaching the x = 0 plane via an indirect path. Figure 6.5 indicates how atom-wall reflections replace atoms coming from impossible locations (dashed lines) with atoms reflected from allowed locations(solid lines). Careful analysis shows that this replacement process has no effect on the pressure of the gas.

 
Figure 6.4: Atom-wall collisions


next up previous
Next: Remarks Up: Chapter 6 Previous: P from the partition function

Nicholas V Sushkin
Sun Jun 30 15:18:58 EDT 1996