5.3: The Average Ensemble Energy
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We will be restricting ourselves to the canonical ensemble (constant temperature and constant pressure). Consider a collection of N molecules. The probability of finding a molecule with energy Ei is equal to the fraction of the molecules with energy Ei. That is, in a collection of N molecules, the probability of the molecules having energy Ei:
Pi=niN
This is the directly obtained from the Boltzmann distribution, where the fraction of molecules ni/N having energy Ei is:
Pi=niN=e−Ei/kTQ
The average energy is obtained by multiplying Ei with its probability and summing over all i:
⟨E⟩=∑iEiPi
Equation ??? is the standard average over a distribution commonly found in quantum mechanics as expectation values. The quantum mechanical version of this Equation is
⟨ψ|ˆH|ψ⟩
where Ψ2 is the distribution function that the Hamiltonian operator (e.g., energy) is averaged over; this equation is also the starting point in the Variational method approximation.
Equation ??? can be solved by plugging in the Boltzmann distribution (Equation ???):
⟨E⟩=∑iEie−Ei/kTQ
Where Q is the partition function:
Q=∑ie−EikT
We can take the derivative of lnQ with respect to temperature, T:
(∂lnQ∂T)=1kT2∑iEie−Ei/kTQ
Comparing Equation ??? with ???, we obtain:
⟨E⟩=kT2(∂lnQ∂T)
It is common to write these equations in terms of β, where:
β=1kT
The partition function becomes:
Q=∑ie−βEi
We can take the derivative of lnQ with respect to β:
(∂lnQ∂β)=−∑iEie−βEiQ
And obtain:
⟨E⟩=−(∂lnQ∂β)
Replacing 1/kT with β often simplifies the math and is easier to use.
It is not uncommon to find the notation changes: Z instead of Q and ˉE instead of ⟨E⟩.