00:01
For a, you want to find the probabilities p0 of t and p1 of t.
00:07
So for a system in thermal equilibrium at temperature t, the probability that a system is in a particular state follows the boltzmann distribution.
00:19
So the probability pi that a particle is in state i with energy epsilon i is given by pi equals e to negative epsilon i over kb times t over z, where kb is boltzmann's constant, and z is the partition function for a single particle, which sums over all possible states of the particle.
00:51
So for our two -state system, we have epsilon 0 equals 0, epsilon 1 equals epsilon, and the partition function z is therefore e to negative epsilon 0 over kb t plus e to negative epsilon 1 over kb t, which is equal to 1 plus e to negative epsilon over kb t.
01:21
So the probabilities are for p0 of t, this is the particle being in the lower energy level, so energy equals 0.
01:32
This is equal to e to negative 0 over kb times t over z which is equal to 1 over 1 plus e to negative epsilon k over kb times t and p1 of t is equal to e to negative epsilon epsilon over kb t over z or equals to e to negative epsilon over kb times t over 1 plus e to negative epsilon over kb times t.
02:22
Okay, now we're gonna do part.
02:25
We're gonna calculate the total energy u and the heat capacity c.
02:29
So the total energy u of the system is the sum of the expected energies of all particles.
02:35
Since the particles are non -interacting and identical, the total energy is simply n times the expected energy of a single particle...