1290 H The Hückel Method
whereψaandψbare two of the 2pzatomic orbitals. The integralSabis anoverlap
integralifab, and is anormalization integralifab. The integralHabis a matrix
element of the effective Hamiltonian. We assume that theccoefficients are real, as are
theΨfunctions, so thatHabHbaandSabSba.
We now need to minimize this variational energy with respect to all of theccoeffi-
cients. To do this, we differentiateWiwith respect to each of theccoefficients and set
each derivative equal to zero. This gives us three simultaneous equations for the three
ccoefficients. The derivative ofWwith respect tocjis (where we temporarily omit
the superscript (i) and the limits on the sums):
∂W
∂cj
1
D
(
∑
b
cbHjb+
∑
a
caHaj
)
−
N
D^2
(
∑
b
cbSjb+
∑
a
caSaj
)
2
D
(
∑
b
cbHjb
)
−
2 N
D^2
(
∑
b
cbSjb
)
2
D
(
∑
b
cbHjb
)
−
2 W
D
(
∑
b
cbSjb
)
(H-6)
We have used the facts thatHabHbaandSabSba, and have replaced the summa-
tion indexabybin one sum (this makes no difference after summation). We set the
expression in Eq. (H-5) equal to zero to find the minimum. We multiply byD/2 and
obtain
0
∑^3
a 1
(Haj−WSaj)ca (j1, 2, 3) (H-7)
This is a set of three simultaneous linear homogeneous equations, one for each value
ofj. The equations are satisfied by the “trivial solution” in which all thec’s vanish, but
this is not the solution that we seek.
The situation is similar to that in the degenerate perturbation theory. If we divide
each equation byc 1 , we have only two unknown variables,c 2 /c 1 andc 3 /c 1 .IfWis
arbitrary, the system of equations is therefore overdetermined, with three equations for
two variables. In order for a nontrivial solution to exist, a condition must be satisfied
that makes the equations equivalent to two independent equations. This condition is
that the determinant of the matrix of the coefficients must vanish.^13 Determinants are
discussed in Appendix B. We write the condition
det(Hab−WSab) 0 (H-8)
Equation (H-8) is called asecular equation. It is similar to but not identical to the
secular equation in degenerate perturbation theory. For each value ofWthat satisfies
this equation there is a usable set of simultaneous equations, so that for each value of
Wthere is a delocalized molecular orbital.
We assume that the 2pzorbitals are normalized, so that the normalization integrals
(Saa) equal unity. We now introduce some additional assumptions and approximations
that define the Hückel method: (1) we approximate the overlap integrals (Sabwith
ab) by zero; (2) we assume thatHaahas the same value, calledα, for every atom;
(^13) I. N. Levine,op. cit., pp. 220ff, 629ff (note 6).