This reduces to:
(12.32)
Using the relationships
x=rsinθcosφ
y=rsinθsinφ (12.33)
e±iφ=cosφ±isinφ
it is easy to show that the p orbitals can be rewritten as
(12.34)
(12.35)
These combinations have the zcomponent of angular momentum can-
celing and have the same basic form as for p 0. These versions of the
orbitals yield the conventional representation shown
in Figure 12.7.
d Orbitals
The d orbitals represent the l=2 orbitals and arise when
nis at least 3; then=3 shell contains one 3s orbital,
three 3p orbitals, and five 3d orbitals. The electrons in
the 3d orbitals have an angular momentum with
mlequal to −2, −1, 0, +1, and +2. As was found for the
p orbitals, the wavefunctions with opposite values of
mlcan be combined in pairs to give rise to conventional
standing orbitals (Figure 12.8), expressed as:
dxy=xy f(r) (12.36)
dyz=yz f(r)
dzx=zx f(r)
dx (^2) −y 2 =
dz 2 =
1
23
()() 3 zrfr^22 −
1
2
()()xyfr^22 −
6 Z
p
i
y=+∝()pp yr+−
2
11
pppxrx= ()
−
+−−∝
1
2
11
p
a
± = re±i
⎛
⎝
⎜
⎜
⎞
⎠
⎟
(^10) ⎟
52
1
8
1
sin
/
5
π
θ φ
252 PART 2 QUANTUM MECHANICS AND SPECTROSCOPY
z
pz py
px
y
x
Figure 12.7A representation of p
orbitals of the hydrogen atom. A nodal
plane separates the two lobes of each
orbital.