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# Use the [http://www.hulis.free.fr/ HuLis] software to retrieve the Hückel MOs for ozone. Write a single-determinant MO wave function based on Hückel orbitals. Develop it into the basis of atomic orbitals, to get an expression in terms of VB structures (consult the hint given below).
 
# Use the [http://www.hulis.free.fr/ HuLis] software to retrieve the Hückel MOs for ozone. Write a single-determinant MO wave function based on Hückel orbitals. Develop it into the basis of atomic orbitals, to get an expression in terms of VB structures (consult the hint given below).
 
# Compute by hand the weights of the different structures (neglecting all overlaps for simplicity). What is the radical character of ozone according to simple MO theory?  <br>
 
# Compute by hand the weights of the different structures (neglecting all overlaps for simplicity). What is the radical character of ozone according to simple MO theory?  <br>
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!'''Answer'''
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# The MO orbitals in the Huckel approximation for ozone are: <br>  <math>
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\varphi_1 = \frac{1}{2}(p_1 + \sqrt{2}p_2 + p_3) </math> <br> <math>
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\varphi_2 = \frac{1}{\sqrt2}(p_1 - p_3)</math> <br> <math>
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\varphi_3 = \frac{1}{2}(p_1 - \sqrt{2}p_2 + p_3)
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</math> <br> <br> A single-determinant MO wavefunction of ozone based on these Hückel orbitals would look as follows: <br> <math>
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      \psi_{H\ddot{u}ckel} = \vert \varphi_1\bar{\varphi_1}\varphi_2\bar{\varphi_2}\vert =
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                      \vert [\frac{1}{2}(p_1 + \sqrt{2}p_2 + p_3)][\overline{\frac{1}{2}(p_1 + \sqrt{2}p_2 + p_3)]}[\frac{1}{\sqrt2}(p_1 - p_3)][\overline{\frac{1}{\sqrt2}(p_1 - p_3)]} \vert
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</math> <br> However, we can simplify the problem by using the electron/hole equivalence: [[The electron-hole equivalence|>> ''the electron-hole equivalence'']]<br>        <br> Thus, we simply replace holes by electrons and vise versa in <math> \psi_{H\ddot{u}ckel} </math> getting a function of <math> {\psi_{H\ddot{u}ckel}}^{hole} </math>, which we will then expande in terms of VB structures. Finally, we will perform the back hole-electron transformation in the VB representation to get the final result. This way we transform a 4e-3c problem into 2h-3c one.<br>                <br>  <math>
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{\psi_{H\ddot{u}ckel}}^{hole} = \vert \varphi_3\bar{\varphi_3}\vert = \frac{1}{4} \vert (p_1 - \sqrt{2}p_2 + p_3)\overline{(p_1 - \sqrt{2}p_2 + p_3)} \vert
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</math><br>  <br>  Expanding into AO determinants, we get:<br>                  <br>    <math>
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{\psi_{H\ddot{u}ckel}}^{hole} = \frac{1}{4} (\vert (p_1\overline p_3 \vert + \vert (p_3\overline p_1 \vert) - \frac{\sqrt{2}}{4}(\vert p_1\overline p_2 \vert + \vert p_2 \overline p_1 \vert) - \frac{\sqrt{2}}{4}(\vert p_2\overline p_3 \vert + \vert p_3 \overline p_2 \vert) + \frac{1}{4} \vert p_1\overline p_1 \vert + \frac{1}{4} \vert p_3\overline p_3 \vert + \frac{1}{2} \vert p_2\overline p_2 \vert
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</math><br>              <br>    Doing the electron-hole back transformation, we get: <br>  <br>    <math>
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\psi_{H\ddot{u}ckel} = \frac{\sqrt{2}}{4}\Phi_3 - \frac{1}{2}\Phi_1 - \frac{1}{2}\Phi_2 + \frac{1}{4}\Phi_6 + \frac{1}{4}\Phi_5 + \frac{1}{4}\Phi_4
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</math><br>            <br>
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#The corresponding weights while neglecting overlap (for simplicity) are therefore:<br>          <br><math>
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\psi_{H\ddot{u}ckel} =
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        25%\Phi_1 +
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        25%\Phi_2 + 12.5%\Phi_3 +
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        25%\Phi_4 + 6.25%\Phi_5 +
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        6.25%\Phi_6
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</math><br> <br>Thus, according to simple MO theory the radical character of ozone is 12.5%.
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Version du 12 juillet 2012 à 09:53

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VB applications on PI systems

In all the following exercises, <math>\pi</math> the system will be taken as active, and the <math>\sigma</math> system as inactive. In all VB calculations, the <math>\sigma</math> orbitals shall be described by MOs delocalized onto the whole molecule.




>> general guidelines for BOVB calculations