We have considered the motion of these
molecules to be in three directions, in other words we say that the molecule has three
degrees of freedom. It is therefore sensible to suppose that one-third of the total energy is
associated with each degree of freedom, and this is known as Boltzmann's law of
equipartition of energy. Thus each degree of freedom has an amount of energy ½ RT
associated with it.
If a gas has its temperature raised at constant volume the energy
input is the increase in kinetic energy of the gas molecules. So for a unit mass and for a rise
in temperature dT we have:
CVdT = kinetic energy increase = 3/2 RdT
Where CV
is the specific heat capacity of the gas at constant volume.
But CP - CV = R, so for a
monatomic gas:
The energy associated with axis X is very small however, and so we
say that the molecule has five degrees of freedom.
If we assume that the energy
associated with each rotational degree of freedom is the same as that for each translational
degree of freedom then the total energy of the molecule will be 5 x ½ RT = 5/2 RT. (The
vibrational energy of the molecule is insignificant except at very high temperatures.)
Using the same argument as for the monatomic gas, we have for the two
principal molar specific heats of a diatomic gas:
Gas | Value of γ |
Air | 1.41 |
Ammonia | 1.31 |
Argon | 1.66 |
Carbon dioxide | 1.30 |
Carbon monoxide | 1.40 |
Helium | 1.66 |
Hydrogen | 1.41 |
Oxygen | 1.40 |
These results show very good
agreement with theory.
The preceding section has dealt with one mole of a
gas. If we now consider a sample of gas containing n moles we have:
2/3 N (½
mc2) = nRT and this gives ½ mc2 = 3/2[R/L]T
where L
is the Avogadro constant.
The quantity R/L is known as the Boltzmann constant (k) and
its value can be shown to be: 1.38x10-23 J K-
1