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Rotational partition function

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The rotational partition function relates the rotational degrees of freedom to the rotational part of the energy.

Definition

The total canonical partition function of a system of identical, noninteracting atoms or molecules can be divided into the atomic or molecular partition functions [1] .

with

Where is the degeneracy of the j'th quantum level of an individual particle, is the Boltzmann constant, and is the absolute temperature of system. for molecules, under the assumption that that total energy levels can be partitioned into its contributions from different degrees of freedom (weakly coupled degrees of freedom)[2]

and the number of degenerate states are given as products of the single contributions

where "trans", "ns", "rot", "vib" and "e" denotes translational, nuclear spin, rotational and vibrational contributions as well as electron excitation, the molecular partition functions

can be written as a product itself

Rotational energies are quantized. For a diatomic molecule like CO or HCl or a linear polyatomic molecule like OCS in its ground vibrational state, the allowed rotational energies in the Rigid rotor approximation are

J is the quantum number for total rotational angular momentum and takes all integer values starting at zero,i.e. is the rotational constant, and is the Moment of inertia. Here we are using B in energy units. If it is expressed in frequency units, replace B by hB in all the expression that follow, where h is Planck's Constant. If B is given in units of , then replace B by hcB where c is the speed of light in vacuum.

For each value of J, we have rotational degeneracy, = (2J+1), so the rotational partition function is therefore

For all but the lightest molecules or the very lowest temperatures, . This suggests we can approximate the sum by replacing the sum over J by an integral of J treated as a continuous variable.

This approximation is known as the high temperature limit. It is also called the classical approximation as this is the result for the canonical partition function for a classical rigid rod.

Using the Euler-Maclaurin formula an improved estimate can be found [3]

.

For the CO molecule at , the (unit less) contribution to turns out to be in the range of .

The mean thermal rotational energy per molecule can now be computed by taking the derivative of with respect to temperature . In the high temperature limit approximation, the mean thermal rotational energy of a linear rigid rotor is .

A rigid, nonlinear molecule has rotational energy levels determined by three rotational constants, conventionally written and , which can often be determined by Rotational spectroscopy. In terms of these constants, the rotational partition function can be written in the high temperature limit as [4]

with the rotational symmetry number [5] which equals the number ways a molecule can be rotated to overlap itself in an indistinguishable way, i.e. that at most interchanges identical atoms. The expression works for asymmetric, symmetric and spherical top rotors.

References

  1. ^ Donald A. McQuarrie, Statistical Mechanics, Harper \& Row, 1973
  2. ^ Donald A. McQuarrie, ibid
  3. ^ G. Herzberg, Infrared and Raman Spectra, Van Nostrand Reinhold, 1945, Equation (V,21)
  4. ^ G. Herzberg, ibid, Equation (V,29)
  5. ^ G. Herzberg, ibid; see Table 140 for values for common molecular point groups

See also