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Lecture 17: Chap. 5, Sect. 8: Rigid Rotator - model for molecular rotation Chap. 4, Sect. 2: Angular momentum properties MathChap. C, pp. 111-2 Angular momentum vectors MathChap. D, pp. 147-8 Spherical coordinates
Lecture 18: Chap. 5, Section 9: Rigid Rotator, continued energy levels microwave spectroscopy
Chem 4502 Quantum Mechanics & Spectroscopy (Jason Goodpaster)
Chapter 5 (continued): Rigid Rotator
2
�Trying to capture the physicists� precise mathematical description of the quantum world with our crude words and mental images is like playing Chopin with a boxing glove on one hand and a catcher�s mitt on the other.�
George Johnson, New York Times, 1996
Quantum quote of the day, submitted by 3502 student David:
3
Assuming that H79Br has a vibrational frequency of
∼2560 cm-1, predict its gas phase IR absorption spectrum.
Figure 13.2 p. 500
There is a gap centered at ∼2560 cm-1.
On either side, absorption lines are spaced by ∼17 cm-1.
These are due to rotational transitions (plus ∆v = 1). 4
Classical Rotational Motion
Consider a mass, m, rotating about a point at radius r:
r Moment of inertia (I)
I = m r2
I corresponds to m in linear motion.
Consider 2 masses separated by r, rotating about their center of mass:
Fig. 5.9 p. 174
I = µ r2
µ = reduced mass = m1 m2 m1 + m2 (for 2 masses)
5
Classical Rotational Motion
Center of mass (CM) : defined by
m1 m2
XCM
X1 X2
m1 > m2
XCM (m1+m2) = m1X1+m2X2
If m1 = m2, then XCM = ½ (X1+X2) right in the middle
and µ = ½ (m1) = ½ (m2)
mass-weighted average position of all of the masses
XCM position of the center of mass
6
Classical Rotational Motion
Angular momentum (magnitude)
L = I ω
L = angular momentum
I = moment of inertia (µr2)
ω (�omega�) = rotational speed or angular velocity radians/sec
In the absence of an external torque (force causing rotation), angular momentum is conserved.
Example: figure skater brings arms in
(reducing I) → L remains constant so ω increases (spins faster).
7
Classical Rotational Motion
Angular momentum (direction)
MathChapter C pp. 111-112
right hand rule
p = mv = linear momentum
L = r x p → → →
→ →
8
Classical Rotational Motion
Relate our two expressions for angular momentum, L:
L = r x p → → →
Since r and p are perpendicular for circular motion, magnitude of L is:
L = r p = r mv
→ →
ω (rad/s) = v (m/s) 2 π (rad/cycle) 1 / (2 π r) (cycle/m) = v/r
Substituting,
L = m r2 (v / r) = m r v Same as above
L = m r v
L = I ω = m r2 ω
We also had (for one rotating mass):
9
Classical Rotational Motion
Rotational kinetic energy
Erot = ½ I ω2 Analogous to: E = ½ mv2
= ½ (I ω)2 / I = L2 / 2I = p2 / 2m
Is skater�s Erot conserved when brings arms in?
No: Erot = L2 / 2I
L is the same, but I is reduced so Erot is increased
To bring arms in, skater has to do work against the �centrifugal force� pulling arms outward.
This compensates for the increased rotational kinetic energy.
10
p. 120
r
Lz
rotation in x-y plane
Classical Rotational Motion
QM Rotation:
Complementary observables (uncertainty relation) x, px Φ, Lz
where Φ is (azimuthal) angle in xy plane
(v)
mv2
(ω=v/r) (I = mr2)
; L= r p = r mv
11
Quantum Mechanical Rotational Motion
Extend to 3-D. Applications:
Particle constrained to move on surface of a sphere
Gas phase molecule rotating freely about its center of mass
2-D (planar) motion (in an inherently 3-D system) forbidden
Uncertainty Principle: if molecule were to rotate only in the xy plane, both z and pz would be zero
Model: Rigid (fixed r) rotator
12
Quantum Mechanical Rotational Motion
Schrödinger equation for the rigid rotator:
Ĥ Ψ = E Ψ All the energy is kinetic
∇2 LaPlacian Operator in Cartesian coordinates
�Convenient� to convert to spherical coordinates
(since r is constant)
13
Quantum Mechanical Rotational Motion
Spherical Coordinates (MathChapter D p. 147)
Φ (�phi�) �azimuthal� angle (in xy plane)
θ �theta� angle from z axis
r distance from origin
0 ≤ Φ ≤ 2 π 0 ≤ θ ≤ π
0 ≤ r < ∞ generally but here r is fixed
14
Quantum Mechanical Rotational Motion
Using the chain rule, convert ∇2 from Cartesian to spherical coordinates:
∇2 = ∂2/∂x2 + ∂2/∂y2 + ∂2/∂z2 Cartesian
Since r is constant, can omit first term:
Chap. 5 #30-32, not assigned Eqn. 5.49
15
Quantum Mechanical Rotational Motion
∇2 = We had:
Hamiltonian operator in Cartesian coordinates:
Factoring out 1/r2 and using I = µ r2 , obtain
Hamiltonian operator in spherical coordinates (fixed r)
16
Lecture 18: Chap. 5, Sect. 9: Rigid Rotator, continued energy levels; microwave spectroscopy Lecture 19: Chapter 6: Hydrogen Atom
17
Quantum Mechanical Rotational Motion
Schrödinger equation for the rigid rotator:
call wave functions Y(θ, Φ) �spherical harmonics�
Ĥ E = rotational kinetic energy
So, a rotating molecule in a state characterized by one of the Y(θ,Φ) eigenfunctions will have a well-defined rot. kinetic energy.
Will any of its other properties also be well-defined?
18
Quantum Mechanical Rotational Motion
Ĥ Y(θ,Φ) = E Y(θ,Φ) We had:
Are the spherical harmonics also eigenfunctions of any other operator?
Recall for kinetic energy (here, call it �K�): K = ½ I ω2 = L2 / 2 I for rotational motion
Analogous to: K = ½ mv2 = p2 / 2m for linear motion
L2 = 2 I K
Write the operator corresponding to L2 :
L2 = 2 I Ĥ ˆ since have no potential energy K = Ĥ ˆ So, L2 = 2 I K ˆ ˆ
19
Quantum Mechanical Rotational Motion
We had:
L2 = 2 I Ĥ ˆ Also, since
ˆ L2 = -�2
The spherical harmonics, Y(θ,Φ), will also be eigenfunctions of with eigenvalues L2 = 2I E. ˆ L2
Ĥ Y(θ,Φ) = E Y(θ,Φ) Y(θ,Φ) = 2I E Y(θ,Φ) ˆ L2
unitless Natural unit of angular momentum is � (i.e., J•s).
20
Ĥ Y(θ,Φ) = E Y(θ,Φ)
Rigid Rotator
Apply boundary conditions Y(θ, Φ) = Y(θ, Φ+2π)
Schrödinger equation Use separation of variables.
Solution yields 2 quantum numbers:
also determines magnitude of angular momentum
in rigid rotator, J determines total (= kinetic) energy
J = 0, 1, 2, ...
(we will call this ℓ for H atom)
m = 0, ±1, ±2, ... ±J (so, 2J+1 degenerate states for a given J)
determines direction of angular momentum vector
21
Rigid Rotator
Look at the lowest energy solution:
J=0, m=0 Y(θ,Φ) = 1 / (4π)½ E=0
J=0 no rotation so rotational kinetic energy = 0
angular momentum = 0
(also linear momentum = 0)
Does this violate the uncertainty principle?
Y(θ,Φ) is a constant; spherically symmetric No.
The position (angular orientation) is completely unknown. 22
Rigid Rotator
The energy levels turn out to be:
EJ = ћ2 J (J+1) 2I
J = 0, 1, 2, ...
where I = µr2 moment of inertia
Rotational energy levels are quantized.
In contrast, classically the rotational kinetic energy can have a continuous range of values:
Erot = ½ I ω2 ω (�omega�) = rotational speed (rad/sec)
23
EJ = ћ2 J (J+1) 2I
Rigid Rotator
where I = µr2
We had:
µ = m1 m2 m1 + m2
Model for rotating diatomic molecule
So, by measuring the rotational energy levels EJ ,
we can determine r, the bond length of the molecule.
For polyatomics, can also measure bond angles.
24
Rigid Rotator
EJ = ћ2 J (J+1) 2I
We had:
In units of wave numbers (cm-1),
EJ = EJ / hc = ћ2 J (J+1) 2I hc
∼ ћ = h/2π
= h J(J+1) 8 π2 I c
B ∼ Rotational
constant (cm-1) EJ (cm-1) = B J (J+1) ∼ ∼
In units of E/h, B = h / ( 8 π2 I )
25
Rigid Rotator
EJ (cm-1) = B J (J+1) ∼ ∼
Selection rule for absorption or emission of a photon:
∆J = ± 1
Fig. 5.10 p. 178
J
0
E ∼ (cm-1)
2B ∼
6B ∼
20B ∼
12B ∼
g
1 3
5
7
9
Rotational spectrum shows absorption lines separated by 2B ∼
Degeneracy g = 2J+1
since m = 0, ±1, ..., ±J 26
Rigid Rotator
Selection rule
to absorb or emit a photon and change rotational level,
the molecule must have a permanent dipole moment.
Homonuclear diatomics (O2, N2)
or symmetric molecules (e.g., benzene, methane)
do not have a microwave (pure rotational) spectrum
(but they do have discrete rotational levels).
27
Rigid Rotator
The linked image cannot be displayed. The file may have been moved, renamed, or deleted. Verify that the link points to the correct file and location.
Engel p. 143
Selection rule (classical picture):
a molecule with a permanent dipole moment can absorb rotational energy from the oscillating electric field of the (microwave) radiation.
28
Rigid Rotator
Calculate the J=0 to J=1 rotational energy spacing of 12C16O, and its rotational constant, in cm-1. The equilibrium bond length is 1.13 Å.
EJ (cm-1) = B J (J+1) ∼ ∼ B = h / 8 π2 I c
I = µr2
µ = m1 m2 / (m1+m2)
Answer: µ = m1 m2 / (m1+m2) = [12•16/28] amu = 6.9 amu = 1.14 x 10-26 kg
1.66 x 10-27 kg/amu
B = h / 8 π2 I c = 6.63 x 10-34 Js / ((8 π2 1.46x10-46 kg m2)( 3.00 x 1010 cm/s)) = 1.9 cm-1 = rotational constant
∼
∼ h = 6.63 x 10-34 Js
I = µr2 = 1.14 x 10-26 kg (1.13 x 10-10 m)2 = 1.46 x 10-46 kg m2
c = 3.00 x 108 m/s
For J=0, E=0 cm-1; for J=1, E = 2B = 3.8 cm-1 = energy spacing ∼
29
Rigid Rotator
Calculate the J=0 to J=1 rotational energy spacing of 12C16O, and its rotational constant, in cm-1. The equilibrium bond length is 1.13 Å.
We had:
2B = 3.8 cm-1 ∼
Rotational transitions occur in the microwave (and far IR) regions of the electromagnetic spectrum.
If measure rotational energy spacings, can deduce precise bond length (12C16O re = 1.128229 ± 0.000001 Å).
Rot. spacings are typically much smaller than vibrational: (12C16O vibrational frequency: 2169.7559 cm-1)
30
Microwave spectroscopy (�radio astronomy�)
of interstellar molecules
Almost all of the molecules known to occur in the interstellar medium were detected by rotational spectroscopy.
�As of 2001, over 120 different chemical compounds have been identified in interstellar clouds, circumstellar matter, and comets.�
(Nummelin article, WebCT)
31
Ken�s group�s Fourier transform microwave spectrometer, in 29 Smith Hall http://www.chem.umn.edu/groups/kleopold/
32
Ken Leopold�s Research Program: Microwave Spectroscopy of Gas Phase Complexes (trimethylamine trimethylborane, a Lewis acid-base complex)
33
Rigid Rotator
Energy level diagram showing the rotational energy levels associated with each vibrational state for a diatomic molecule
Figure 13.2 p. 500
H79Br
Fig. 13.1 p. 499
The IR absorption spectrum of a gas phase molecule shows transitions from a specific rot. level of the lower vib. state to a specific rot. level of the upper vib. state
(For HBr, ∆ J = ± 1) 34
Rigid Rotator
Does rigid rotor �obey� the Correspondence Principle:
expect energy levels to be nearly continuous at high quantum numbers
EJ (cm-1) = B J (J+1) ∼ ∼
Spacings between adjacent levels:
EJ+1 – EJ = B (J+1)(J+2) - B J(J+1) = B (2J +2) ∼ ∼ ∼ ∼ ∼
Energy spacing 2B (J+1) 2 Energy B J(J+1) J
= = → 0 as J → ∞
Yes: energy spacings are ≈ continuous at high J
35
Rigid Rotator
Recall: The spherical harmonics, Y(θ,Φ), are also eigenfunctions of with eigenvalues L2 = 2I E. ˆ L2
Ĥ Y(θ,Φ) = E Y(θ,Φ) Y(θ,Φ) = 2I E Y(θ,Φ) ˆ L2
Angular momentum
Angular momentum is also quantized.
(Classically, L = I ω = r mv can have a continuum of values.)
E = ћ2 J (J+1) 2I
L2 = ћ2 J (J+1)
For J=1, L2 = 2 ћ2 and the length of the angular momentum vector │L│ = √2 ћ. →
L →