For a CO molecule, the constant ϵis 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.

Short Answer

Expert verified

The rotational partition function for a CO molecule at room temperature is 107.7.

The exact value of rotational partition function of a CO molecule is 108.03.

Step by step solution

01

Step 1. Given Information.

We are given that the value of constantεis 0.00024eV.

02

Step 2. Calculating rotational partition function.

The rotational partition function of a heterogeneous diatomic molecule is,

Zrot=j=0(2j+1)exp-j(j+1)kT

At higher temperatures, for kT>, the rotational partition function becomes as follows,

Zrot=kTϵ

Substitute 8.617×10-5eV/K for k, 300K for T, and 0.00024eVin the equation Zrot=kTϵ, we get

Zrot=8.617×10-5eV/K(300K)0.00024eV=107.7

Therefore, the rotational partition function of a CO molecule is 107.7.

03

Step 3. Calculating the exact rotational partition function.

The rotational partition function of a heterogeneous diatomic molecule is,

Zrot=j=0(2j+1)exp-j(j+1)kT

Expand the above summation from j=0to j=50,

role="math" Zrot=1+3exp-2ϵkT+5exp-6ϵkT+7exp-12ϵkT+101exp-2550ϵkT

Substitute 107.7for kTϵ in the above equation,

Zrot=1+3exp-2107.7+5exp-6107.7+7exp-12107.7=108.03

Hence, the exact value of rotational partition function of a CO molecule is 108.03.

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Most popular questions from this chapter

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?

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.

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

Show explicitly from the results of this section thatG=Nμfor an ideal gas.

Use the Maxwell distribution to calculate the average value of v2for the molecules of an ideal gas. Check that your answer agrees with equation 6.41.

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