Full text: The internal constitution of the stars

34 
THERMODYNAMICS OF RADIATION 
By (25-2) the change of entropy of the gas is 
S 2 - S x = 8S = [ d ( T) dQ (27*4) 
= | 9? J d ( T ) dT + J d (T) pdv 
= §fni l2 d(T)dT + 91P T9 ( T) - ...(27-5). 
J T x JVi. v 
Now $ 2 — S x can depend only on the initial and final temperatures and 
volumes of the gas. This follows from the theory of gases according to 
which two specimens of the same gas at the same temperature and density 
are alike in all their properties. Or it can be deduced more generally from 
the reversibility. For if S 2 — S x were different according to the intermediate 
values of v and T, we could by taking the gas out by one route and back 
by another increase its entropy. Owing to the reversibility no entropy 
is created; hence the increase of entropy requires a decrease of entropy 
of our reservoirs of heat. The cycle could be repeated any number of times 
so that a small mass of gas would be able to furnish an infinite decrease 
of S (i.e. increase of organisation) to the rest of the universe. 
The expression on the right of (27-5) must therefore depend only on 
the initial and final stages. The first term evidently satisfies this; and 
therefore the second integral must in spite of appearances be independent 
of the intermediate stages. This requires that Td ( T) shall be a constant. 
To prove this, the second integral can be written 
r log v 2 
| Td ( T ) d (log v). 
• log Vi 
Consider any elementary step d (log v). During this change of volume the 
gas can have any temperature we please; so that if it is possible to vary 
Td (T) by varying T, we can vary the contribution made to the integral 
by this step. Thus the integral cannot be independent of the intermediate 
conditions of the gas unless 
Td (T) = const. 
By suitably connecting the units of entropy and temperature the 
constant may be set equal to unity so that 
d{T) = HT (27-6). 
Here T is identified with the temperature on the scale of a perfect-gas 
thermometer; but, of course, the value of d (T) here found is applicable 
to “ordinary” heat transferred from or to any kind of material in ac 
cordance with (26T). 
Equation (27-4) can now be written 
S 2 - S, = f dQ/T 
(27-7).
	        
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