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Modern Spectroscopy

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106 5 ROTATIONAL SPECTROSCOPY<br />

for the rotational energy levels E r of a diatomic molecule, in the rigid rotor approximation,<br />

was introduced. In this equation, I is the moment of inertia [equal to mr 2 , where the reduced<br />

mass m is equal to m 1m 2=ðm 1 þ m 2ÞŠ and the rotational quantum number J ¼ 0; 1; 2; ....<br />

The same expression applies also to any linear polyatomic molecule but, because I is likely<br />

to be larger than for a diatomic molecule, the energy levels of Figure 1.12 tend to be more<br />

closely spaced.<br />

In practice, what is measured experimentally is not energy but frequency, in the millimetre<br />

wave and microwave regions, or wavenumber, in the far infrared. Therefore we convert the<br />

energy levels of Equation (5.10) to what are known as term values FðJÞ having dimensions<br />

of either frequency, by dividing by h, or wavenumber, by dividing by hc, giving<br />

or<br />

FðJÞ ¼ E r<br />

h<br />

h<br />

¼<br />

8p2 JðJ þ 1Þ ¼BJðJ þ 1Þ ð5:11Þ<br />

I<br />

FðJÞ ¼ Er h<br />

¼<br />

hc 8p2 JðJ þ 1Þ ¼BJðJ þ 1Þ ð5:12Þ<br />

cI<br />

The use of the symbols FðJÞ and B for quantities which may have dimensions of frequency<br />

or wavenumber is unfortunate, but the symbolism is used so commonly that there seems<br />

little prospect of change. In Equations (5.11) and (5.12) the quantity B is known as the<br />

rotational constant. Its determination by spectroscopic means results in determination of<br />

internuclear distances and represents a very powerful structural technique.<br />

Figure 5.2 shows a set of rotational energy levels, or, strictly, term values, for the CO<br />

molecule.<br />

The transition intensity is proportional to the square of the transition moment, which is<br />

given by<br />

ð<br />

Rr ¼ c 0<br />

r*mc 00<br />

r dt ð5:13Þ<br />

analogous to Equation (2.13). The rotational selection rules constitute the conditions for<br />

which the intensity, and therefore R r, is non-zero and are:<br />

1. The molecule must have a permanent dipole moment (m 6¼ 0).<br />

2. DJ ¼ 1.<br />

3. DM J ¼ 0, 1, a rule which is important only if the molecule is in an electric or magnetic<br />

field (see Equation 1.61).<br />

Rule 1 shows that transitions are allowed in heteronuclear diatomic molecules such as CO,<br />

NO, HF and even 1 H 2 H (for which m ¼ 5:9 10 4 D compared with, say, HF, for which<br />

m ¼ 1.82 D), 1 but not in H 2,Cl 2 and N 2. Similarly, ‘unsymmetrical’ linear polyatomic<br />

1 1D’ 3.335 64 6 10 730 Cm.

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