Thus far we have concentrated on perfect gases.
It is important to appreciate that no gas actually is perfect
- they all deviate from ideal behaviour to some degree:
| One of our assumptions
about ideal gases was that the molecules didn't interact
except when they collided with each other. However,
in real gases there is a potential energy between two
molecules; |
 |
The attractions at medium distances are the result
of coulombic forces. These arise due to uneven distribution
of the electrons in the molecules, which may induce dipoles
in neighbouring molecules resulting in an attraction. The repulsions
are due to the two molecules being compressed together (the
mutual short-range repulsion between the negatively charged
electrons of the two molecules).
These attractions and repulsions make the gas
more compressible at low pressures and less compressible at
high pressures than a perfect gas would be.
Note that at large separations, the potential
energy tends to zero, ie at large separations the interactions
between particles in a gas are effectively zero. Hence low pressure
gases (in which the average separation of particles is large)
behave more like perfect gases than do high pressure gas samples.
The perfect gas equation pVm/RT
= 1 predicts that the ratio pVm/RT
is constant at 1. However, we find that in fact it is a function
of pressure.
 |
We say that pVm/RT
= Z. Z is the compressibility
factor. For a perfect gas it equals 1 always. However,
due to the molecular interactions in real gases, Z changes
with pressure. |
These deviations suggest that in fact pVm/RT
= 1 is just the first term of a series of powers
Z = pVm/RT
= 1 + B'p + C'p2
+ ......
The temperature at which
Z ® 1 is called the Boyle
Temperature. We could also consider that dZ/dp
® 0. In either case, B' ® 0.
At the Boyle Temperature real gases behave ideally over
a slightly larger pressure range than at other temperatures.
See graph opposite |
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