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In the low-temperature limit (kT<<∈), each term in the rotational partition function is much smaller than the one before. Since the first term is independent of T, cut off the sum after the second term and compute the average energy and the heat capacity in this approximation. Keep only the largest T-dependent term at each stage of the calculation. Is your result consistent with the third law of thermodynamics? Sketch the behavior of the heat capacity at all temperature, interpolating between the high-temperature and low- temperature expressions.

Short Answer

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The graph is as follows,

Step by step solution

01

Step 1. Given Information

We are given that in the low-temperature limit (kT<<∈), each term in the rotational partition function is much smaller than the one before.

02

Step 2. Expanding the partition function 

Expanding the partition function by neglecting all higher order terms in the low temperature limit (kT<<∈).

Zrot=1+(2(1)+1)e-1(1+1)∈/kT=1+3e-2e/kT

The average energy of the system is given as follows:

Erot=-1Zrot∂Zrot∂β=-11+3e-2β∈∂∂β(1+3e-2β∈)=-11+3e-2β∈(3e-2β∈(-2∈))=6∈e-2β∈1+3e-2β∈

Neglecting the term 3e-2β∈in the denominator of 6∈e-2β∈1+3e-2β∈,

Since the function 3e-2β∈approaches to zero as β→∞because e-∞=0.

Therefore, the average energy of the system is 6∈e-2β∈.

03

Step 3. Specific heat capacity of the system

The specific heat capacity of the system is given by,

C=∂Erot∂T=∂∂T(6∈e-2β∈∈)=6∈∂∂T(e-2∈/kT)=6∈(e-2∈/kT)-2∈k-1T2=12∈2kT2e-2∈/kT=3k2∈kT2e-2∈/kT

Therefore, the heat capacity of the system in the low temperature limit is C=3k2∈kT2e-2∈/kT.

In the low temperature limit, the heat capacity of the system decreases exponentially to zero.

04

Step 4. Behavior ho heat capacity

The low and high temperature limit of Ckare plotted against the dimensionless parameter kT∈.

The graph is as follows,

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Most popular questions from this chapter

Estimate the probability that a hydrogen atom at room temperature is in one of its first excited states (relative to the probability of being in the ground state). Don't forget to take degeneracy into account. Then repeat the calculation for a hydrogen atom in the atmosphere of the starγ UMa, whose surface temperature is approximately 9500 K.

The dissociation of molecular hydrogen into atomic hydrogen, H2→2Hcan be treated as an ideal gas reaction using the techniques of Section 5.6. The equilibrium constant K for this reaction is defined as

K=PH2P0PH2

whereP0is a reference pressure conventionally taken to be1bar,and the other P's are the partial pressures of the two species at equilibrium. Now, using the methods of Boltzmann statistics developed in this chapter, you are ready to calculate K from first principles. Do so. That is, derive a formula for K in terms of more basic quantities such as the energy needed to dissociate one molecule (see Problem 1.53) and the internal partition function for molecular hydrogen. This internal partition function is a product of rotational and vibrational contributions, which you can estimate using the methods and data in Section 6.2. (AnH2 molecule doesn't have any electronic spin degeneracy, but an H atom does-the electron can be in two different spin states. Neglect electronic excited states, which are important only at very high temperatures. The degeneracy due to nuclear spin alignments cancels, but include it if you wish.) Calculate K numerically atT=300K,1000K,3000K,and6000K. Discuss the implications, working out a couple of numerical examples to show when hydrogen is mostly dissociated and when it is not.

Use a computer to sum the rotational partition function (equation 6.30) algebraically, keeping terms through j = 6. Then calculate the average energy and the heat capacity. Plot the heat capacity for values ofkT/ϵ ranging from 0 to 3. Have you kept enough terms in Z to give accurate results within this temperature range?

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

E¯=-1Z∂Z∂β=-∂∂βlnZ

where β=1/kT. These formulas can be extremely useful when you have an explicit formula for the partition function.

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.)

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