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Z
lδφ = r sin( θ ) δφ
δφ
r
δθ
l
θ
δr
δθ
r
φ
Y
X
δτ = rlδrδθδφ
= r 2 sin( θ ) δrδθδφ
Figure A9.6 Geometry required to define a small volume element
δτ
in spherical polar coor-
dinates according to the small changes
. The sides of the small element shown
can be found using the definition of radians as the ratio of the arc length subtended by the
angle and the radius.
δ
r,
δθ
and
δφ
In effect, this proceedure sums the probability around a thin spherical shell of radius r and
thickness
r , as illustrated in Figure 7.12. The limits of the integrals in this equation can
be understood with reference to Figure A9.1. The
δ
θ
derivative runs from 0 to
π
(or 180 )
φ
sweeping out a half circle with its diameter on the Z -axis. Then, the
integral covers a
full circle from
π
to
, ensuring that the half circle defined by
θ
is swept through a full
π
sphere.
Our atomic orbital functions are products of radial and angular terms, and so this type
of multiple integral can be treated as a product of integrals over each of the coordinates.
For the 1s orbital, for example:
δ
π
π
χ 100 χ 100 r 2 sin(
P 100 ( r )
δ
r
=
θ
)d
θ
d
φ
r
(A9.56)
π
0
Taking the angular and radial functions from Tables A9.1 and A9.2:
Z eff
a 0
3 / 2
π
π
1
π
A 2 r 2 exp(
P 100 ( r )
δ
r
=
ρ
r )
δ
r
d
φ
sin
(θ)
d
θ
with
A
=
(A9.57)
π
0
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