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Chemistry LibreTexts

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=eEi/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=iEieEi/kTQ

Where Q is the partition function:

Q=ieEikT

We can take the derivative of lnQ with respect to temperature, T:

(lnQT)=1kT2iEieEi/kTQ

Comparing Equation ??? with ???, we obtain:

E=kT2(lnQT)

It is common to write these equations in terms of β, where:

β=1kT

The partition function becomes:

Q=ieβEi

We can take the derivative of lnQ with respect to β:

(lnQβ)=iEieβEiQ

And obtain:

E=(lnQβ)

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.

 


5.3: The Average Ensemble Energy is shared under a CC BY-NC-SA 4.0 license and was authored, remixed, and/or curated by LibreTexts.

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