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24.8: The Vibrational Partition Function of A Diatomic Ideal Gas

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    152806
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    We base the electronic potential energy for a diatomic molecule on a model in which the nuclei are stationary at the bottom of the electronic potential energy well. We now want to expand this model to include vibrational motion of the atoms along the line connecting their nuclei. It is simple, logical, and effective to model this motion using the quantum mechanical treatment of the classical (Hooke’s law) harmonic oscillator.

    A Hooke’s law oscillator has a location, \(r_0\), at which the restoring force, \(F\left(r_0\right)\), and the potential energy, \(\epsilon \left(r_0\right)\), are zero. As it is displaced from \(r_0\), the oscillator experiences a restoring force that is proportional to the magnitude of the displacement, \(dF=-\lambda \ dr\). Then, we have

    \[\int^r_{r_0}{dF}=-\lambda \ \int^r_{r_0}{dr} \nonumber \]

    so that \(F\left(r\right)-F\left(r_o\right)=-\lambda \left(r-r_0\right)\). Since \(F\left(r_o\right)=0\), we have \(F\left(r\right)=-\lambda \left(r-r_0\right)\). The change in the oscillator’s potential energy is proportional to the square of the displacement,

    \[\epsilon \left(r\right)-\epsilon \left(r_o\right)=\int^r_{r_0}{-F\ dr}=\lambda \ \int^r_{r_0}{\left(r-r_0\right)dr\ }=\frac{\lambda }{2}{\left(r-r_0\right)}^2 \nonumber \]

    Since we take \(\epsilon \left(r_o\right)=0\), we have \(\epsilon \left(r\right)={\lambda {\left(r-r_0\right)}^2}/{2}\). Taking the second derivative, we find

    \[\frac{d^2\epsilon }{{dr}^2}=\lambda \nonumber \]

    Therefore, if we determine the electronic potential energy function accurately near \(r_0\), we can find \(\lambda\) from its curvature at \(r_0\).

    In Chapter 18, we note that the Schrödinger equation for such an oscillator can be solved and that the resulting energy levels are given by \({\epsilon }_n=h\nu \left(n+{1}/{2}\right)\) where \(\nu\) is the vibrational frequency. The relationship between frequency and force constant is

    \[\nu =\frac{1}{2\pi }\sqrt{\frac{\lambda }{m}} \nonumber \]

    where the oscillator consists of a single moving mass, \(m\). In the case where masses \(m_1\) and \(m_2\) oscillate along the line joining their centers, it turns out that the same equations describe the relative motion, if the mass, \(m\), is replaced by the reduced mass

    \[\mu =\frac{m_1m_2}{m_1+m_2} \nonumber \]

    Therefore, in principle, we can find the characteristic frequency, \(\nu\), of a diatomic molecule by accurately calculating the dependence of the electronic potential energy on \(r\) in the vicinity of \(r_0\). When we know \(\nu\), we know the vibrational energy levels available to the molecule. Alternatively, as discussed in Section 24.7, we can obtain information about the molecule’s vibrational energy levels from its infrared absorption spectrum and use these data to find \(\nu\). Either way, once we know \(\nu\), we can evaluate the vibrational partition function. We have

    \[z_v=\sum^{\infty }_{n=0} \mathrm{exp} \left[-\frac{h\nu }{kT}\left(n+\frac{1}{2}\right)\right] =\frac{\mathrm{exp} \left(-h\nu /2kT\right)}{1- \mathrm{exp} \left(-h\nu /kT\right)} \nonumber \]

    where we take advantage of the fact that the vibrational partition function is the sum of a geometric series, as we show in Section 22.6.


    This page titled 24.8: The Vibrational Partition Function of A Diatomic Ideal Gas is shared under a CC BY-SA 4.0 license and was authored, remixed, and/or curated by Paul Ellgen via source content that was edited to the style and standards of the LibreTexts platform; a detailed edit history is available upon request.