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function of the orbital exponent c s . The too attractive h ss has its bad
minimum at c s ¼ 1
5 (see Table 4.2) and is contrasted by the repulsive
E pn so as to give the best variational minimum of
:
« w ¼ 0
:
1234E h
occurring for c s ¼ 0
:
4222. This result is within 98.7%of the exact result,
E 2s ¼ 0
:
125E h . Even without doing orbital exponent optimization
ð c s ¼ 0
1192E h would be obtained
(about 95% of the exact value), showing the crucial importance of
Schmidt's orthogonalization in assessing a reasonable variational approx-
imation to the 2s excited state.
:
5 Þ , the remarkable result of
« w ¼ 0
:
4.2.3 The First Excited 2p State of the Hydrogenic System
We can take as an appropriate variational function for this case the
normalized 2p z STO:
! 1 = 2
c p
p
w ¼
exp ð c p r Þ r cos
u
ð 4
:
20 Þ
orthogonal to
c 0 by symmetry. The orthogonality constraint is now
satisfied from the outset, and simple calculation gives the upper bound
(Equation 3.66):
1
2 r
Z
r
1
2 ð c p Zc p Þ E 2p
2
« w ¼
2p z
2p z
¼
ð 4
:
21 Þ
giving upon c p optimization the exact value for the excited 2p energy level
of the H-like system:
« w
dc p ¼ c p
Z 2
8
d
Z
2 ¼ 0 ) c p ð best Þ¼
Z
2 ) « w ð best Þ¼
ð 4
:
22 Þ
4.2.4 The Ground State of the He-like System
With reference to Figure 4.4, the two-electron Hamiltonian (in atomic
units) for the He-like system is
1
r 12 ;
1
2 r
Z
r
H ¼ h 1 þ h 2 þ
h ¼
2
ð 4
:
23 Þ
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