Vibrational partition function

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The vibrational partition function[1] traditionally refers to the component of the canonical partition function resulting from the vibrational degrees of freedom of a system. The vibrational partition function is only well-defined in model systems where the vibrational motion is relatively uncoupled with the system's other degrees of freedom.

Definition

For a system (such as a molecule or solid) with uncoupled vibrational modes the vibrational partition function is defined by

Q_{vib}(T) =\prod_j{\sum_n{e^{-\frac{E_{j,n}}{k_B T}}}}

where  T is the absolute temperature of the system,  k_B is the Boltzmann constant, and  E_{j,n} is the energy of j'th mode when it has vibrational quantum number  n= 0, 1, 2, \ldots . For an isolated molecule of n, atoms the number of vibrational modes (i.e. values of j) equals 3n − 5 or 3n − 6 dependent upon whether the molecule is linear or nonlinear respectively.[2] In crystals, the vibrational normal modes are commonly known as phonons.

Approximations

Quantum harmonic oscillator

The most common approximation to the vibrational partition function uses a model in which the vibrational eigenmodes or normal modes of the system are considered to be a set of uncoupled quantum harmonic oscillators. It is a first order approximation to the partition function which allows one to calculate the contribution of the vibrational degrees of freedom of molecules towards its thermodynamic variables.[1] A quantum harmonic oscillator has an energy spectrum characterized by:

E_{j,n}=\hbar\omega_j(n_j +\frac{1}{2})

where j runs over vibrational modes and  n_j is the vibrational quantum number in the j 'th mode,  \hbar is Planck's constant, h, divided by  2 \pi and  \omega_j is the angular frequency of the j'th mode. Using this approximation we can derive a closed form expression for the vibrational partition function.

Q_{vib}(T) =\prod_j{\sum_n{e^{-\frac{E_{j,n}}{k_B T}}}} = \prod_j e^{-\frac{\hbar \omega_j}{2 k_B T}} \sum_n \left( e^{-\frac{\hbar \omega_j}{k_B T}}   \right)^n
= \prod_j \frac{e^{-\frac{\hbar \omega_j}{2 k_B T}}}{ 1 -  e^{-\frac{\hbar \omega_j}{k_B T}}   } 
= e^{- \frac{E_{ZP}}{k_B T}} \prod_j \frac{1}{ 1 -  e^{-\frac{\hbar \omega_j}{k_B T}} }

where  E_{ZP} = \frac{1}{2} \sum_j \hbar \omega_j is total vibrational zero point energy of the system.

Often the wavenumber, \tilde{\nu} with units of cm−1 is given instead of the angular frequency of a vibrational mode[2] and also often misnamed frequency. One can convert to angular frequency by using  \omega = 2 \pi c \tilde{\nu} where c is the speed of light in vacuum. In terms of the vibrational wavenumbers we can write the partition function as


Q_{vib}(T) = e^{- \frac{E_{ZP}}{k_B T}} \prod_j \frac{1}{ 1 -  e^{-\frac{ h c \tilde{\nu}_j}{k_B T}} }

References

  1. 1.0 1.1 Donald A. McQuarrie, Statistical Mechanics, Harper & Row, 1973
  2. 2.0 2.1 G. Herzberg, Infrared and Raman Spectra, Van Nostrand Reinhold, 1945

See also


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