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V - MSpace at the University of Manitoba

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��<br />

�<br />

E �<br />

NR<br />

DFT<br />

NI �R� � Ek<br />

� Een<br />

� Eee<br />

Exc<br />

With <strong>the</strong><br />

22<br />

Coul<br />

(2–6)<br />

NI<br />

Ek term accounting for <strong>the</strong> kinetic energy <strong>of</strong> <strong>the</strong> non-interacting model<br />

system <strong>of</strong> <strong>the</strong> same density, and <strong>the</strong> remaining interacting kinetic energy being accounted<br />

for within <strong>the</strong> Exc term.<br />

With this ingenious and ground-breaking step, Kohn and Sham introduced <strong>the</strong><br />

new concept <strong>of</strong> using a non-interacting reference system, with <strong>the</strong> exact same density as<br />

<strong>the</strong> real system, to account for almost all <strong>of</strong> <strong>the</strong> kinetic energy, instead <strong>of</strong> <strong>the</strong> exact<br />

amount accounted for by <strong>the</strong> Schrödinger equ<strong>at</strong>ion. The remaining small amount <strong>of</strong><br />

kinetic energy is <strong>the</strong>n merged into <strong>the</strong> only unknown term in equ<strong>at</strong>ion (2–6), Exc. In order<br />

to solve for this term an appropri<strong>at</strong>e method <strong>of</strong> approxim<strong>at</strong>ion must be chosen.<br />

The most commonly used approach to determining approxim<strong>at</strong>ions for Exc is to<br />

separ<strong>at</strong>e it into an exchange term Ex and a correl<strong>at</strong>ion term Ec, and approxim<strong>at</strong>e each <strong>of</strong><br />

<strong>the</strong>se terms separ<strong>at</strong>ely.<br />

E �<br />

xc<br />

� Ex<br />

Ec<br />

(2–7)<br />

Given an expression for Exc one can formul<strong>at</strong>e a one-electron Schrödinger<br />

equ<strong>at</strong>ion (2–8) analogous to <strong>the</strong> HF equ<strong>at</strong>ion (2–4). This allows us to use <strong>the</strong> well-<br />

established HF SCF technique.<br />

ˆ<br />

f KS � i � � i� i (2–8)

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