/*! This file is auto-generated */ .wp-block-button__link{color:#fff;background-color:#32373c;border-radius:9999px;box-shadow:none;text-decoration:none;padding:calc(.667em + 2px) calc(1.333em + 2px);font-size:1.125em}.wp-block-file__button{background:#32373c;color:#fff;text-decoration:none} Q. 6.42 In problem 6.20 you computed the... [FREE SOLUTION] | 91Ó°ÊÓ

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In problem 6.20 you computed the partition function for a quantum harmonic oscillator :Zh.o.=11-e-βε, where ε=hfis the spacing between energy levels.

(a) Find an expression for the Helmholtz free energy of a system of Nharmonic oscillators.

(b) Find an expression for the entropy of this system as a function of temperature. (Don't worry, the result is fairly complicated.)

Short Answer

Expert verified

part (a): F=NkT1-e-βε

part (b):role="math" localid="1647054975548" S=-Nkln1-e-βε+NkεkTeβε-1

Step by step solution

01

Part (a): Step 1. Given information

The partition function of a single harmonic oscillator is given by

Zh.o.=11-e-βε...................(1)
02

Part (a): Step 2. Calculation

The formula to calculate the Helmholtz free energy for th single harmonic oscillator is given by

F=-kTlnZ.....................(2)

Substitute the value of Zfrom equation (1) into equation (2) to calculate the free energy for single harmonic oscillator.

F=-kTln11-e-βε=kTln1-e-βε.......................(3)

Since, Helmholtz free energy is an extensive property, multiply both sides of equation (3) by Nto obtain the required free energy for Nharmonic oscillators.

role="math" localid="1647054790522" FN=NF=NkTln1-e-βε

Here,FNis the Helmholtz free energy forNharmonic oscillator.

03

Part (b): Step 1. Calculation of entropy

The formula to calculate the entropySof the system is given by

S=-∂F∂TN..........................(4)

Substitute the formula for Helmholtz free energy from equation (3) into equation (4) and simplify to obtain the required entropy of the system.

role="math" localid="1647054991723" S=-∂∂TNkTln1-e-βε=-Nkln1-e-βε-NkT1-e-βε-1εe-βε∂β∂ε=-Nkln1-e-βε+NkεkTeβε-1

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Most popular questions from this chapter

Consider a large system of Nindistinguishable, noninteracting molecules (perhaps an ideal gas or a dilute solution). Find an expression for the Helmholtz free energy of this system, in terms of Z1, the partition function for a single molecule. (Use Stirling's approximation to eliminate the N!.) Then use your result to find the chemical potential, again in terms ofZ1.

Prove that, for any system in equilibrium with a reservoir at temperature T, the average value of E2 is

E2¯=1Z∂2Z∂β2

Then use this result and the results of the previous two problems to derive a formula for σEin terms of the heat capacity, C=∂E¯/∂T

You should findσE=kTC/k

In the numerical example in the text, I calculated only the ratio of the probabilities of a hydrogen atom being in two different states. At such a low temperature the absolute probability of being in a first excited state is essentially the same as the relative probability compared to the ground state. Proving this rigorously, however, is a bit problematic, because a hydrogen atom has infinitely many states.

(a) Estimate the partition function for a hydrogen atom at 5800 K, by adding the Boltzmann factors for all the states shown explicitly in Figure 6.2. (For simplicity you may wish to take the ground state energy to be zero, and shift the other energies according!y.)

(b) Show that if all bound states are included in the sum, then the partition function of a hydrogen atom is infinite, at any nonzero temperature. (See Appendix A for the full energy level structure of a hydrogen atom.)

(c) When a hydrogen atom is in energy level n, the approximate radius of the electron wavefunction is a0n2, where ao is the Bohr radius, about 5 x 10-11 m. Going back to equation 6.3, argue that the PdV term is Tot negligible for the very high-n states, and therefore that the result of part (a), not that of part (b), gives the physically relevant partition function for this problem. Discuss.

For a COmolecule, the constant €is approximately 0.00024eV.(This number is measured using microwave spectroscopy, that is, by measuring the microwave frequencies needed to excite the molecules into higher rotational states.) Calculate the rotational partition function for a COmolecule at room temperature (300K), first using the exact formula 6.30 and then using the approximate formula 6.31

Prove that the probability of finding an atom in any particular energy level is P(E)=(1/Z)e-F/kT, whereF=E-TS and the "'entropy" of a level is k times the logarithm of the number of degenerate states for that level.

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