Molecular Orbital (MO) Calculations
O2, OCS, and m-xylene
By: Peter Michalski and Presley Neuman
University of Wisconsin- Oshkosh
Abstract
Successful molecular orbital calculations for O2, OCS, and m-xylene were
completed. It was found that out of the 6-21G, 6-31G, and DZV basis
sets, DZV yielded the most accurate energy prediction for each of the
molecules since the geometry optimizations using the DZV basis set
yielded the lowest energies for systems. The software used successfully
calculated geometries, vibrational frequencies, electronic transitions
frequencies, dipole moments, and many other properties, and many
calculations were compared to literature values.
Introduction1
Reactivity of molecules can be determined by electronic structure. Ab initio quantum chemistry methods, which are computational methods based on quantum
chemistry, were used to calculate information about three different molecules O2, OCS, and m--xylene.
These basis sets are built from the linear combination of atomic
orbitals. Three
different basis sets were used to calculate the optimized geometry of
these molecules. In
increasing size of the basis set there are 6-21G, 6-31G, and DZV. The
larger the basis set is the
more accurate the predictions tend to be. The molecule is modified in
these calculations until the
geometries and bond lengths have the lowest potential energy. The more
accurate the calculated
geometry is the better the predicted electronic structure will be.
Therefore, a better optimized
geometry will have more accurate predictions such as molecular dipole
moment, polarizability,
vibrational frequency, probability of absorption of visible light, and
if reactions will occur. Molecular orbitals may be characterized by
wavefunctions for electrons. The variational principle allows
approximate true wavefunctions with linear combinations of trial
wavefunctions to be made. Trial wavefunctions are not eigenfunctions of
the Hamiltonian, however, thus the expectation value of the energy must
be calculated. The "basis set" wavefunctions that are used to form the
trial wavefunction is normalized, but the total wavefunction must be
normalized, putting additional constraints on coefficient values.
Experimental1
In this experiment the Avogodro
2 program was used to built structures for
each of the molecules. Molecular mechanics optimizations were then
completed on the structures and saved as .xyz files. The wxMacMolPlt
3 software used the .xyz files to generate AM1 and PM3 geometry optimizations (.inp) files for the Gamess
4 computation package.
If calculations worked molecules they were saved as .log files. These .log
files could then be used in Jmol
5 to observe structure and make
calculations. The
ab initio molecular calculations were carried out using Gamess and the Gaussian type basis sets: 6-21G, 6-31G, and DZV.
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Jmol0 will appear here.
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O2
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By clicking the link underneath the following display, you
will be taken to molecular orbital calculations completed for O2.
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Jmol1 will appear here.
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OCS |
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By clicking the link underneath the following display, you
will be taken to molecular orbital calculations completed for OCS.
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By clicking the link underneath the following display, you
will be taken to molecular orbital calculations completed for m-xylene.
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References
1. J. Mihalick, J. Gutow. Molecular Orbital (MO) Calculations, UW Oshkosh 2013.
2. Avogodra software. http://sourceforge.net/projects/avogadro/ (accessed February 13, 2014).
3. Bode, B. M. and Gordon, M. S. J. Mol. Graphics Mod., 16, 133-138(1998).
4. M.W. Schmidt, K. K. Baldridge, J. A. Boatz, S.T. Elbert, M.S. Gordon,
J.H. Jensen, S. Koseki, N. Matsunaga, K.A. Nguyen, S.J. Su, T.L.
Windus, M. Dupuis, J.A. Montgomery J. Comput. Chem. 14, 1347-1363(1993).
5. The Jmol Development Team. http://www.jmol.org, accessed February 2014.
Based on template by A. Herráez as modified by J. Gutow
Using directory /Users/student/Desktop/jmolpp/Intropage for all molecules
adding JmolPopIn.js
...jmolApplet0
...adding O2_picture.png
copying and unzipping jsmol.zip directory into /Users/student/Desktop/jmolpp/Intropage for all molecules
...copying
file:/Users/student/Desktop/PeterPresley/02_DVZ_geo_opt_UHF.log
to
/Users/student/Desktop/jmolpp/Intropage for all molecules/02_DVZ_geo_opt_UHF.log
...adding O2_picture.spt
...jmolApplet1
...adding ocs_picture.png
copying and unzipping jsmol.zip directory into /Users/student/Desktop/jmolpp/Intropage for all molecules
...copying
file:/Users/student/Desktop/PeterPresley/ocs_DVZ_geo_opt.log
to
/Users/student/Desktop/jmolpp/Intropage for all molecules/ocs_DVZ_geo_opt.log
...adding ocs_picture.spt
...jmolApplet2
...adding m-xylene_picture.png
copying and unzipping jsmol.zip directory into /Users/student/Desktop/jmolpp/Intropage for all molecules
...copying
file:/Users/student/Desktop/PeterPresley/mxylene_DZV_geo_opt-3.log
to
...compressing large data file to
/Users/student/Desktop/jmolpp/Intropage for all molecules/mxylene_DZV_geo_opt-3.log.gz
/Users/student/Desktop/jmolpp/Intropage for all molecules/mxylene_DZV_geo_opt-3.log.gz
...adding m-xylene_picture.spt