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The Equations for the Orbitals

The orbitals are the solution of a Schrodinger-like equation
$\displaystyle F\phi_i=\epsilon_i\phi_i$
    (31)
 where $\epsilon_i$ is the orbital energy, F is the hamiltonian (in the molecular orbital approximation). If we substitute the MO-LCAO expression we get
$\displaystyle (F-\epsilon_i)\sum c_{ri}\eta_r=0$
    (32)
 Multiply on the left $\eta_s$ and integrate to give
$\displaystyle \sum_r^M\langle\eta_s\vert F-\epsilon_i\vert\eta_r\rangle c_{ri}=0$
    (33)
 where we have introduced the notation
$\displaystyle \langle\eta_s\vert F\vert\eta_r\rangle=\int\eta_sF\eta_rdv=F_{sr}=F_{rs}$
    (34)
$\displaystyle \langle\eta_s\eta_r\rangle=\int\eta_s\eta_rdv=S_{sr}=S_{rs}$
    (35)
 We can therefore write the equations
$\displaystyle \sum_r^M(F_{sr}-\epsilon_i S_{sr})c_{ri}=0$
    (36)
 or
$\displaystyle {\bf (F-\epsilon_{\rm i} S) c_{\rm i}=0}$
    (37)
 These are of course the secular equations and they have been written in an eigenvector notation. 
next up previous
Next: Valence-Bond Theory Up: Contents - Previous: The Molecular Orbital Wavefunction

Nicholas Handy

1998-09-23