In the real world, most oscillators are not perfectly harmonic. For a quantum oscillator, this means that the spacing between energy levels is not exactly uniform. The vibrational levels of an H2 molecule, for example, are more accurately described by the approximate formula

Enϵ1.03n-0.03n2,n=0,1,2,

where ϵ is the spacing between the two lowest levels. Thus, the levels get closer together with increasing energy. (This formula is reasonably accurate only up to about n = 15; for slightly higher n it would say that En decreases with increasing n. In fact, the molecule dissociates and there are no more discrete levels beyond n 15.) Use a computer to calculate the partition function, average energy, and heat capacity of a system with this set of energy levels. Include all levels through n = 15, but check to see how the results change when you include fewer levels Plot the heat capacity as a function of kT/ϵ. Compare to the case of a perfectly harmonic oscillator with evenly spaced levels, and also to the vibrational portion of the graph in Figure 1.13.

Short Answer

Expert verified

Therefore,

C=nNkβϵ1.03n-0.03n22eβϵ1.03n-0.03n2eβϵ1.03n-0.03n2-12

Step by step solution

01

Given information

In the real world, most oscillators are not perfectly harmonic. For a quantum oscillator, this means that the spacing between energy levels is not exactly uniform. The vibrational levels of an H2 molecule, for example, are more accurately described by the approximate formula

Enϵ1.03n-0.03n2,n=0,1,2,

where ϵ is the spacing between the two lowest levels. Thus, the levels get closer together with increasing energy. (This formula is reasonably accurate only up to about n = 15; for slightly higher n it would say that En decreases with increasing n. In fact, the molecule dissociates and there are no more discrete levels beyond n15.)

02

Explanation

In actual life, most oscillators are not perfect harmonic oscillators; the energy of real oscillators is provided by:

En=ϵ1.03n-0.03n2

Where

ϵis the energy difference between the first two levels.

The partition function is:

Z=ne-βEn(1)

Substitute with energy

localid="1647451366905">Z=ne-βϵ1.03n-0.03n2(2)

Using python the summation is found with the code:

03

Explanation

The average energy is given as:

E¯=-1ZZβ

Substitute from (1),

role="math" localid="1647451769495" E¯=-1-e-βEnβ11-e-βEnE¯=1-e-βEnEne-βEn1-e-βEn2E¯=Ene-βEn1-e-βEnE¯=EneβEn-1

Substituting the energy,

E¯=nϵ1.03n-0.03n2eβϵ1.03n-0.03n2-1

The partial derivative of total energy with respect to temperature equals the heat capacity, which is:

C=UT=βTUβC=βTβNEneβEn-1C=Tβ-1-NEn2eβEneβEn-12

But β=1/kTT=1/kβ

Tβ-1=-kβ2

Therefore,

C=NkβEn2eβEneβEn-12

Substitute the energy:

role="math" localid="1647452008304" C=nNkβϵ1.03n-0.03n22eβϵ1.03n-0.03n2eβϵ1.03n-0.03n2-12CNk=nβϵ1.03n-0.03n22eβϵ1.03n-0.03n2eβϵ1.03n-0.03n2-12

If x=1/βϵ, then

CNk=n1.03n-0.03n2/x2e1.03n-0.03n2/xe1.03n-0.03n2/x-12

04

Explanation

Using python to plot the function for different values of nmax. The code is given below:

In the graph below, the red curve is for harmonic oscillator:

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Most popular questions from this chapter

A lithium nucleus has four independent spin orientations, conventionally labeled by the quantum number m = -3/2, -1/2, 1/2, 3/2. In a magnetic field B, the energies of these four states are E = mμB, where μ the constant is 1.03 x 10-7 eV/T. In the Purcell-Pound experiment described in Section 3.3, the maximum magnetic field strength was 0.63 T and the temperature was 300 K. Calculate the probability of a lithium nucleus being in each of its four spin states under these conditions. Then show that, if the field is suddenly reversed, the probabilities of the four states obey the Boltzmann distribution for T =-300 K.

Cold interstellar molecular clouds often contain the molecule cyanogen (CN), whose first rotational excited states have an energy of 4.7x 10-4 eV (above the ground state). There are actually three such excited states, all with the same energy. In 1941, studies of the absorption spectrum of starlight that passes | through these molecular clouds showed that for every ten CN molecules that are in the ground state, approximately three others are in the three first excited states (that is, an average of one in each of these states). To account for this data, astronomers suggested that the molecules might be in thermal equilibrium with some "reservoir" with a well-defined temperature. What is that temperature?

Consider a classical particle moving in a one-dimensional potential well ux, as shown. The particle is in thermal equilibrium with a reservoir at temperature T, so the probabilities of its various states are determined by Boltzmann statistics.

{a) Show that the average position of the particle is given by

x=xe-βuxdxe-βuxdx

where each integral is over the entire xaxis.

A one-dimensional potential well. The higher the temperature, the farther the particle will stray from the equilibrium point.

(b) If the temperature is reasonably low (but still high enough for classical mechanics to apply), the particle will spend most of its time near the bottom of the potential well. In that case we can expand u(z) in a Taylor series about the equilibrium point

ux=ux0+x-x0dudxx0+12x-x02d2udx2x0+13!x-x03d3udx3x0+........

Show that the linear term must be zero, and that truncating the series after the quadratic term results in the trivial prediction x=x0.

(c) If we keep the cubic term in the Taylor series as well, the integrals in the formula for xbecome difficult. To simplify them, assume that the cubic term is small, so its exponential can be expanded in a Taylor series (leaving the quadratic term in the exponent). Keeping only the smallest temperature-dependent term, show that in this limit x differs from by a term proportional to kT. Express the coefficient of this term in terms of the coefficients of the Taylor series ux

(d) The interaction of noble gas atoms can be modeled using the Lennard Jones potential,

ux=u0x0x12-2x0x6

Sketch this function, and show that the minimum of the potential well is at x=x0, with depth u0. For argon, x0=3.9Aand u0=0.010eV. Expand the Lennard-Jones potential in a Taylor series about the equilibrium point, and use the result of part ( c) to predict the linear thermal expansion coefficient of a noble gas crystal in terms of u0. Evaluate the result numerically for argon, and compare to the measured value α=0.0007K-1

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

E¯=-1ZZβ=-βlnZ

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

Calculate the most probable speed, average speed and rms speed for OxygenO2molecules at room temperature.

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