Spherical Harmonics and Rigid Rotor Problem, Lecture notes of Physics

The mathematical formula for spherical harmonics and their eigenfunctions for the rigid rotor problem. It also discusses the orthonormality and orthogonality of the eigenfunctions and their energies. The degeneracy of each state and the spacing between states are also explained. The document concludes with the observation of transitions between rotational states through spectroscopy.

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5.61 F all 2007 Lecture # page
1
SPHERICAL HARMONICS
(
θ
,
φ
)
= Θ
l
θ
( )
Y
l
m m
( )
Φ
m
φ
1
!
2
m
m im
φ
Y
l
(
θ
,
φ
)
=
2
4
l
π
+ 1
(
(
l
l
+
m
m
)
)
!
P
l
(
cos
θ
)
e
l = 0, 1, 2,... m = 0, ± 1, ± 2, ± 3,... ± l
Y
l
m
’s are the eigenfunctions to
H
ˆ
ψ
= E
ψ
for the rigid rotor problem.
1
Y0
0 = 1
(
4
π
)
1 2 Y2
0 =
16
5
π
2
(
3cos2
θ
1
)
1 1
Y
1
0 =
4
3
π
2
cos
θ
Y2
±1 =
8
15
π
2
sin
θ
cos
θ
e±i
φ
1 1
3 2 15 2
Y
1
1 =
8
π
32
π
sin2
θ
e±2i
φ
sin
θ
ei
φ
Y2
±2 =
1
2
Y
1
1 = 3 i
φ
8
π
sin
θ
e
m
Y
l
’s are orthonormal:
1 if l = l1 if m = m normalization
Krönecker delta
δ
ll
=
δ
mm
=
0 if l l0 if m m orthogonality
ˆm
)Energies: (eigenvalues of
HYl
m = ElmYl
Switch
l J
conventional for molecular rotational quantum #
2IE
Recall
β
= = l l
(
+ 1
)
J J
(
+ 1
)
J = 0, 1, 2,...
!
2
20
pf3
pf4
pf5

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5.61 Fall 2007 Lecture # page 1

SPHERICAL HARMONICS

θ, φ

l

θ

Y

l

m

m

m

φ

1

2

m

m

im φ

Y

l

θ, φ

l

π

l

l

m

m

P

l

cos θ

e

l = 0, 1, 2,... m = 0, ± 1, ± 2, ± 3,... ± l

Y

l

m

’s are the eigenfunctions to

H

ψ = E ψ for the rigid rotor problem.

1

Y

0

0

4 π

1 2

Y

2

0

π ⎠

2

3cos

2

θ − 1

1 1

Y

1

0

π ⎠

2

cos θ Y

2

± 1

π ⎠

2

sin θ cos θ e

± i φ

1 1

2

2

Y

1

− 1

8 π ⎠

32 π ⎠

sin

2

θ e

± 2 i φ

sin θ e

i φ

Y

2

± 2

1

2

Y

1

1

i φ

8 π ⎠

sin θ e

m m ′∗ m

Y

l

’s are orthonormal:

Y

l

θ, φ

Y

l

θ, φ

sin θ d θ d φ = δ

ll

δ

mm

1 if l = l

1 if m = m ′ normalization

Krönecker delta δ

ll

δ

mm

0 if ll

0 if mm

orthogonality

m

Energies: (eigenvalues of HY )

l

m

= E

lm

Y

l

Switch lJ conventional for molecular rotational quantum #

2 IE

Recall β = = l l

≡ J J

J = 0, 1, 2,...

2

20

5.61 Fall 2007 page 2

E

2

E

J

= J J + 1

2 I

2

0 ± 1 ± 2 ± 3

Y

3

, Y

3

, Y

3

, Y

3

7x degenerate

J = 3

E

3

I

2

0 ± 1 ± 2

J = 2 E

2

= Y

2

, Y

2

, Y

2

5x degenerate

I

2

0 0

J = 1 E

1

= Y

1

, Y

1

2x degenerate

I

0

J = 0

E

0

= 0 Y

0

nondegenerate

Degeneracy of each state g

J

= ( 2 J + 1

from m = 0, ± 1, ± 2,..., ± J

Spacing between states ↑ asJ ↑

2

2

E =

J + 1

− E

J

2 I

J + 1

− J J + 1

I

J + 1

J + 2

Transitions between rotational states can be observed through

spectroscopy, i.e. through absorption or emission of a photon

δ+

δ-

Absorption

E

J

δ+

δ-

E

J+

δ+

δ-

E J

Emission

δ+

δ-

E J- 1

or

Lecture # 20

00 E =

01 ν→

12 ν→ 23 ν→ 34 ν→ 45 ν→ 56 ν→

5.61 Fall 2007 page 4

E

E

3

= 12 Bhc

E

2

= 6 Bhc

E

1

= 2 Bhc

J = 1

J = 2

J = 3

Δ E

0 → 1

= 2 Bhc

Δ E

2 → 3

= 6 Bhc

Δ E

1 → 2

= 4 Bhc

This gives rise to a rigid rotor absorption spectrum with evenly spaced lines.

J = 0

ν

ν

0 → 1

ν

1 → 2

ν

2 → 3

ν

3 → 4

ν

4 → 5

ν

5 → 6

2 B

Spacing between transitions is 2 B (Hz) or 2 B (cm

ν

J + 1 → J + 2

−ν

JJ + 1

= 2 B

J + 1

− 2 B J + 1

= 2 B

Use this to get microscopic structure of diatomic molecules directly from

the absorption spectrum!

Get B directly from the separation between lines in the spectrum.

Use its value to determine the bond lengthr 0

!

Lecture # 20

5.61 Fall 2007 page 5

h

2

m

1

m

2

2 B =

4 π

2

cI

Ir

0

μ =

m

1

  • m

2

1 1

h

2

h

2

( B in cm

) or r

0

r = ( B in Hz)

0

8 π

2

8 π

2

cB μ B μ

Lecture # 20