Quantum Mechanics - Prof. Eric R. Bittner - University of Houston
Quantum Mechanics - Prof. Eric R. Bittner - University of Houston
Quantum Mechanics - Prof. Eric R. Bittner - University of Houston
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• Method development: The development and implementation <strong>of</strong> new theories and computational<br />
strategies to take advantage <strong>of</strong> the increaseing power <strong>of</strong> computational hardware.<br />
(Bigger, stronger, faster calculations)<br />
• Application: The use <strong>of</strong> established methods for developing theoretical models <strong>of</strong> chemical<br />
processes<br />
Here we will go in to a brief bit <strong>of</strong> detail into various levels <strong>of</strong> theory and their implementation<br />
in standard quantum chemical packages. For more in depth coverage, refer to<br />
1. <strong>Quantum</strong> Chemistry, Ira Levine. The updated version <strong>of</strong> this text has a nice overview <strong>of</strong><br />
methods, basis sets, theories, and approaches for quantum chemistry.<br />
2. Modern Quanutm Chemistry, A. Szabo and N. S. Ostlund.<br />
3. Ab Initio Molecular Orbital Theory, W. J. Hehre, L. Radom, P. v. R. Schleyer, and J. A.<br />
Pople.<br />
4. Introduction to <strong>Quantum</strong> <strong>Mechanics</strong> in Chemistry, M. Ratner and G. Schatz.<br />
8.4.1 The Born-Oppenheimer Approximation<br />
The fundimental approximation in quantum chemistry is the Born Oppenheimer approximation<br />
we discussed earlier. The idea is that because the mass <strong>of</strong> an electron is at least 10 −4 that <strong>of</strong><br />
a typical nuclei, the motion <strong>of</strong> the nuclei can be effectively ignored and we can write an electronic<br />
Schrödinger equation in the field <strong>of</strong> fixed nuclei. If we write r for electronic coordinates and R<br />
for the nuclear coordinates, the complete electronic/nuclear wavefunction becomes<br />
Ψ(r, R) = ψ(r; R)χ(R) (8.80)<br />
where ψ(r; R) is the electronic part and χ(R) the nuclear part. The full Hamiltonian is<br />
H = Tn + Te + Ven + Vnn + Vee<br />
(8.81)<br />
Tn is the nuclear kinetic energy, Te is the electronic kinetic energy, and the V ’s are the electronnuclear,<br />
nuclear-nuclear, and electron-electron Coulomb potential interactions. We want Ψ to be<br />
a solution <strong>of</strong> the Schrödinger equation,<br />
HΨ = (Tn + Te + Ven + Vnn + Vee)ψχ = Eψχ. (8.82)<br />
So, we divide through by ψχ and take advantage <strong>of</strong> the fact that Te does not depend upon the<br />
nuclear component <strong>of</strong> the total wavefunction<br />
1<br />
ψχ Tnψχ + 1<br />
ψ Teψ + Ven + Vnn + Vee = E.<br />
On the other hand, Tn operates on both components, and involves terms which look like<br />
Tnψχ = �<br />
n<br />
− 1<br />
(ψ∇<br />
2Mn<br />
2 nχ + χ∇ 2 nψ + 2∇χ · ∇nψ)<br />
232