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Lecture 34

Rotational spectroscopy: intensities

Rotational spectroscopy

 In the previous lecture, we have considered the rotational energy levels.

 In this lecture, we will focus more on selection rules and intensities.

Selection rules and intensities (review)

 Transition dipole moment m = ò y *

f

y

i d

t  Intensity of transition

I

µ m 2

Rotational selection rules

Oscillating electric field (microwave) Transition moment m

fi

= = ò ò e

Y J f f v f Y J f M J

,

f

ˆ e

i v i Y J i M J

,

i

(

M J

, ò e

i v i

e

i v i d

t

e d

t

d

t

v f

)

e d

t

v d

t

Y J i M J

,

i r d

t

r

µ permanent dipole m

ev

= m

ev

ò

Y J f M J

,

f

ˆ

Y J i M J

,

i d

t

r

No electronic / vibrational transition

Rotational selection rules

Gross selection rule:

nonzero permanent dipole

      Does H 2 O have microwave spectra?

Yes Does N 2 No have microwave spectra?

Does O 2 No have microwave spectra?

Quantum in nature

Microwave spectroscopy How could astrochemists know H 2 O exist in interstellar medium?

Public image NASA

Selection rules of atomic spectra(review)

TDM µ òò

Y

¢

l

*

m l

¢ (

Y

10 or

Y

1 ± 1 )

Y lm l

sin q

d

q

d

j ´ d

m s

¢

m s

 From the mathematical properties of spherical harmonics, this integral is zero unless D

m l

D

l

= = ¢ -

m

D

l

¢

m s

-

l

= ± =

m l

0 = 1 0, ± 1

Rotational selection rules

Specific selection rule:

D

J

D

M J

= ± 1 = 0, ± 1 m

fi

= m

ev

ò

Y J f M J

,

f

ˆ

Y J i M J

,

i d

t

r

Spherical & linear rotors

 In units of wave number (cm –1 ):   1   2

BJ

Nonrigid rotor: Centrifugal distortion

 Diatomic molecule  ( ) =

J

2  ( )  2

D J

» 4

B

3 n 2 Vibrational frequency

B

= 4 p

cI I

=

m m A m B A

+

m B R

2

Nonrigid rotor: Centrifugal distortion

 Nonrigid 

D J J

2 

J

 1  2 ( ) = Rigid ( )

Appearance of rotational spectra

 Rapidly increasing and then decreasing intensities Transition moment 2 Degeneracy

g J

 m

J

+ 1,

J

      2 2

J J

2

J

  µ  1 1 1  2 m 2

ev

 Boltzmann distribution (temperature effect)

e

-

E J

/

kT

=

e

-

hcBJ

(

J

+ 1)/

kT

Rotational Raman spectra

Gross selection rule:

polarizability changes by rotation

Specific selection rule: x

2 +

y

2 +

z

2

~ Y

0,0

xy

, etc. are essentially

Y

0,0 ,

Y

2,0 ,

Y

2, ± 1 ,

Y

2, ± 2

I

µ å

k

ò

Y J f

* ,

M J

,

f

ˆ Y

k

(0)

E

0 (0) -

d

t ò

E k

(0) Y

k

(0)* ±

h

n ˆ

J i

,

M J

,

i d

t Linear rotors: Δ

J

= 0, ± 2 2 Spherical rotors: inactive (rotation cannot change the polarizability)

Rotational Raman spectra

 Anti-Stokes wing slightly less intense than Stokes wing – why?

 Boltzmann distribution (temperature effect)

Rotational Raman spectra

 Each wing ’ s envelope is explained by the competing effects of   Degeneracy Boltzmann distribution (temperature effect)

H 2 rotational Raman spectra

 Why does the intensity alternate?

H 2 rotational Raman spectra

 Why does the intensity alternate?

Answer:

odd

J

levels are triply degenerate (triplets), whereas even

J

levels are singlets.

Nuclear spin statistics

  Electrons play no role here; we are concerned with the rotational motion of nuclei.

The hydrogen’s nuclei (protons) are

fermions

and have

α

/

β

spins .

 The rotational wave function (including nuclear spin part) must be

antisymmetric

with respect to interchange of the two nuclei.

 The molecular

rotation through 180

° amounts to

interchange

.

Para and ortho H 2

Singlet (

para-

H 2 ) Y µ { Sym.

spatial part of rotation } Antisym.

{ a (1) b (2) b (1) a (2) } Nuclear (proton) spins Triplet (

ortho-

H 2 ) Y µ Antisym.

{ spatial part of rotation } ¢ ¢ Sym.

a (1) a (2) b (1) b (2) a (1) b (2) + b (1) a (2) With respect to interchange (180 ° molecular rotation)

Spatial part of rotational wave function

 By 180 degree rotation, the wave function changes sign as ( –1)

J

(cf. particle on a ring )

Para and ortho H 2

Y Y Singlet (

para-

H 2 ) µ {

J

Sym.

= even } { Antisym.

a (1) b (2) b (1) a (2) } µ Antisym.

{

J

= odd } ¢ ¢ Sym.

a (1) a (2) b (1) b (2) a (1) b (2) + b (1) a (2) Triplet (

ortho-

H 2 )

Summary

 We have learned the gross and specific selection rules of rotational absorption and Raman spectroscopies.

 We have explained the typical appearance of rotational spectra where the temperature effect and degeneracy of states are important.

 We have learned that nonrigid rotors exhibit the centrifugal distortion effects.

 We have seen the striking effect of the antisymmetry of proton wave functions in the appearance of H 2 rotational Raman spectra.