Each of the hydrogen atom states shown in Figure 6.2 is actually twofold degenerate, because the electron can be in two independent spin states, both with essentially the same energy. Repeat the calculation given in the text for the relative probability of being in a first excited state, taking spin degeneracy into account. Show that the results are unaffected.

Short Answer

Expert verified

Therefore,

PE2PE1=4e-E2-E1/kT

Step by step solution

01

Given information

Each of the hydrogen atom states shown in Figure 6.2 is actually twofold degenerate, because the electron can be in two independent spin states, both with essentially the same energy.

02

Explanation

With n = 2, if E1 is the ground state energy and E2 is the first excited state energy, the probability is:

P(s)=1Ze-E/kT

There are four states in E2 and one state in E1, thus their probabilities are P(s2) multiplied by eight and P(s1) multiplied by two when we add the spin. Thus, the probability of E2 equals Ps2multiplied by eight and the probability of E1 equals Ps1multiplied by two when we include the spin.

PE2=8Ze-E2/kTPE1=2Ze-E1/kT

The ratio of these probabilities is:

role="math" localid="1647300792412" PE2PE1=8e-E2/kT2e-E1/kTPE2PE1=4e-E2-E1/kT

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Most popular questions from this chapter

Suppose you have 10 atoms of weberium: 4 with energy 0 eV, 3 with energy 1 eV, 2 with energy 4 eV, and 1 with energy 6 eV.

(a) Compute the average energy of all your atoms, by adding up all their energies and dividing by 10.

(b) Compute the probability that one of your atoms chosen at random would have energy E, for each of the four values of E that occur.

(c) Compute the average energy again, using the formulaE¯=sE(s)P(s)

For an O2molecule, the constant is approximately 0.00018eV. Estimate the rotational partition function for an O2molecule at room temperature.

The dissociation of molecular hydrogen into atomic hydrogen, H22Hcan 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.

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

E2¯=1Z2Zβ2

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

Use Boltzmann factors to derive the exponential formula for the density of an isothermal atmosphere, already derived in Problems 1.16 and 3.37. (Hint: Let the system be a single air molecule, let s1 be a state with the molecule at sea level, and let s2 be a state with the molecule at height z.)

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