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diffuse molecular orbitals are more susceptible to polarisation.
If a diatomic is rotating at frequency , then
using a classical picture we can say that '
its polarisability oscillates with frequency 2'
because of symmetry.
_
=
= [
+ sin(2p2't)]
sin(2't)
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(5) |
Using the Trigonometric relation:
_ |
|
sinAsinB = ½ {cos(A - B) - cos(A + B)} |
(6) |
_
=
sin(2't)
+
[cos2(
- 2')
- cos2(
+ 2')
t ] |
(7) |
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