as Ωl and Ωr for the left and right block, respectively) that gives the number of states accessible to it at a particular energy distribution. We assume that initial energy distribution is not the final one, so that when we remove the insulation, the energy distribution of the system will spontaneously change. In other words:
Figure 2.8 (a) Probability of one of two copper blocks of equal mass in thermal equilibrium having e units of energy when the total energy of the two blocks is 20 units. (b) Ω, number of states available to the system (combinations of energy distribution) as a function of e.
where we use the superscripts i and f to denote initial and final, respectively.
When the left block has energy e, it can be in any one of Ωl = Ω(e) possible states, and the right block can be in any one of Ωr = Ω(E−e) states. Both
To make
(2.40)
and
(2.41)
As additive properties, ln
We want to know which energy distribution (i.e., values of e and E – e) is the most likely one, because that corresponds to the equilibrium state of the system. This is the same as asking where the probability function,
(2.42)
(we use the partial differential notation to indicate that, since the system is isolated, all other state variables are held constant). Substituting eqn. 2.41 into 2.42, we have:
(2.43)
(since C is a constant). Then substituting eqn. 2.40 into 2.43 we have:
(2.44)
so the maximum occurs at:
(2.45)
The maximum then occurs where the function ∂lnΩ/∂e for each of the two blocks are equal (the negative sign will cancel because we are taking the derivative ∂ƒ(−e)/∂e). More generally, we may write:
(2.46)
Notice two interesting things: the equilibrium energy distribution is the one where ln Ω is maximum (since it is proportional to P) and where the functions ∂lnΩ/∂E of the two blocks are equal. It would appear that both are very useful functions. We define entropy, S,† as:
(2.47)†
and a function β such that:
(2.48)
where k is a constant (which turns out to be Boltzmann's constant or the gas constant; the choice depends on whether we work in units of atoms or moles, respectively). The function S then has the property that it is maximum at equilibrium and β has the property that it is the same in every part of the system at equilibrium.
Entropy also has the interesting property that in any spontaneous reaction, the total entropy of the system plus its surroundings must increase. In our example, this is a simple consequence of the observation that the final probability,
(2.49)
rearranging:
The quantities in brackets are simply the entropy changes of the two blocks. Hence:
(2.50)
In other words, any decrease in entropy in one of the blocks must be at least compensated for by an increase in entropy of the other block.
For an irreversible process, that is, a spontaneous one such as thermal equilibrium between two copper blocks, we cannot determine exactly the increase in entropy. Experience has shown, however, that the increase in entropy will always exceed the ratio of heat exchanged to temperature. Thus, the mathematical formulation of the second law is:
(2.51)
