170
THE MASS-LUMINOSITY RELATION
average separation have a mutual potential energy nearly equal to the
average kinetic energy of 4 free molecules. At the average separation
this mutual energy merely cancels that due to the free electrons in the
neighbourhood since the average potential is zero. Now let the two ions
approach to a distance 0-42.10 -8 cm. Their mutual energy being pro
portional to r -1 increases by 50 per cent.; and there is no corresponding
increase in the cancelling term, since the negative charge being divided
between 23 free electrons has a comparatively non-fluctuating distribution.
The increase is thus equal to the average kinetic energy of 2 free molecules,
and the 2 ions can just make the approach at the expense of all their
kinetic energy if they were originally endowed with the average amount.
Hence on the average two ions cannot approach nearer than § of their
mean distance, which means that effectively an ion is barred out from
^ of the whole volume.
When a molecule is barred from a third of the volume by finite size
of other molecules the constant b in the gas equation is %v, so that the
pressure equation becomes %pv — RT . Accordingly, the pressure is in
creased 20 per cent. But in the present case only ^ of the gas pressure
comes from the ions; the rest is from the free electrons which are not
barred from any appreciable volume. Thus the increase in the pressure
would be less than 1 per cent.
We repeat, however, that this is not a calculation of the true electro
static effect. It deals with a particular objection which arises in most
minds, viz. that ions will act as though they had large volumes. A rather
difficult mathematical investigation will show that the objection is a
phantasm (§ 184); meanwhile, we take the easier course of showing that,
phantasm or not, it is at any rate not of large order of magnitude. The
barring out of ions from close approach to one another has actually an
effect which would scarcely have been anticipated. It means that in very
small stars the ions are constrained to keep at the greatest possible distance
from one another, whilst the electrons can wander as they like. The
repulsive forces are thus kept down to a minimum, whilst the attractive
forces have a good chance of exceeding the minimum. The result is that
attractive forces predominate and assist the compression of the material.
White Dwarfs.
117. If stellar matter at the density of platinum has still the com
pressibility of a perfect gas, the limiting density must be much higher.
It is therefore possible that matter in the stars may attain densities un
paralleled in terrestrial experience. Conversely, if we can discover in the
universe matter of transcendently high density, it will be the strongest
possible confirmation of our conclusion that in the ordinary dwarf stars