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Modern Engineering Thermodynamics

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18.3 Kinetic Theory of Gases 729<br />

3. All the molecules behave like rigid elastic spheres.<br />

4. The molecules exert no forces on each other except when they collide (i.e., there are no long-range forces).<br />

5. All molecular collisions are perfectly elastic.<br />

6. The molecules are always distributed uniformly in their container.<br />

7. The molecular velocities range continuously between zero and infinity. 1<br />

8. The laws of classical mechanics govern the behavior of all molecules in the system.<br />

Each of the N molecules has its own unique velocity V i . Using this velocity, we can define the following<br />

concepts for the system of molecules.<br />

The average molecular velocity : V avg = ∑ N<br />

i=1<br />

V i<br />

N<br />

(18.2)<br />

The root mean square molecular velocity : V rms =<br />

∑ N<br />

V 2 !1/2<br />

i<br />

i=1<br />

N<br />

(18.3)<br />

and in the limit as N → ∞, we can extend the summations in Eqs. (18.2) and (18.3) into integrals as follows<br />

Z ∞ <br />

V<br />

V avg = dN V (18.4)<br />

N<br />

0<br />

Z ∞<br />

<br />

V rms =<br />

V 2 1/2<br />

dN V<br />

(18.5)<br />

N<br />

0<br />

where dN V is the number of molecules with velocities between V and V + dV. Wealsodefinethetranslational total<br />

internal energy U trans as the sum of the kinetic energies of all the molecules in the system, or 2<br />

U trans = ∑ N<br />

i=1<br />

m i V 2 i /2 (18.6)<br />

Since assumption 1 requires that all the molecules have identical mass, we can set m i = m, and Eq. (18.6) becomes<br />

!<br />

U trans = m 2<br />

∑N Vi<br />

2<br />

i=1<br />

= 1 2 Nm<br />

Consider now a spherical shell of radius R containing N ≫ 1 molecules. The radial force F r on the shell due to a<br />

single molecular collision is (see Figure 18.1)<br />

ðF r Þ per<br />

= ma r = m dV r<br />

≈ m ΔV r<br />

dt Δt<br />

molecule<br />

where a r and V r are the radial components of the acceleration and velocity. Using the geometry shown in<br />

Figure 18.1, this equation becomes<br />

ðF r Þ per<br />

≈ m V i cos θ − ð−V i cos θÞ<br />

= 2mV i cos θ<br />

Δt<br />

Δt<br />

molecule<br />

and the total radial force on the shell due to collisions by all N molecules is<br />

ðF r Þ total = ∑ N<br />

i=1<br />

ð<br />

F r<br />

Þ per<br />

= ∑ N<br />

2mV i cos θ<br />

molecule i=1<br />

Δt<br />

The internal pressure inside the shell can now be computed from<br />

p =<br />

ð F rÞ total<br />

= 1 2mV i cos θ<br />

Area 4πR 2 ∑N<br />

i=1<br />

Δt<br />

(18.7)<br />

1 Clearly, no molecule can have a velocity greater than the speed of light, but allowing the velocities to range to infinity is of<br />

tremendous mathematical value in the development of this theory. Though fundamentally wrong, we find that this assumption adds<br />

little error to the results.<br />

2 Since the formulae presented in this chapter were developed by physicists using the SI units system wherein g c = 1, I elected to set<br />

g c = 1 in all the relevant equations in this chapter to simplify them somewhat. Thus, we write mV 2 /2 instead of mV 2 /2g ð c Þ for kinetic<br />

energy and so forth.

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