Second Order Spectra
BCMB/CHEM 8190
Second Order Spectrum Example: Acrylonitrile
1H
C
1H
A
N≡C
1H
B
•
•
•
•
•
A
B
C
AMX first order spectrum
Twelve lines,
lines all equal intensities if first order
JAB = -2 Hz, δC = 5.6 ppm
JAC = 11 H
Hz, δB = 6.1
6 1 ppm
JBC = 16 Hz, δA = 6.3 ppm
Actual spectrum is more complex, field dependent
Field dependence of second order spectra
60 MHz
250 MHz
90 MHz
490 MHz
Line Intensities and Transition Probabilities
• What if spin system cannot be cleanly described as being in
one state? ψ = c1 αα + c2 αβ + c3 βα + c4 ββ = ∑j cj φj
• What is the probability of being in one of the basis states?
Probability in space is proportional to ψ* ψ. Hence,
probability: ρjj = c*jcj
• Similarly, c*kck c*lcl is the probability of starting in k and
ending in l
• If we know we start in k, c*
c kck = 1, just need cl
• Schrodinger’s time dependent equation allows us to solve
for dcj/dt by substituting ∑k ck φk, multiplying from left by φl*
g
g H ψ(
ψ(t)) = - i ((h/2π)
π) d(ψ(t))/dt
(ψ( ))
and integrating:
• from Schrodinger equation: dcl /dt ∝ <φl|H’|φk>
g
g from t = 0 and combining
g with c*l
• Integrating
• Pk->l ∝ |<φl|H’|φk>|2 … gives line intensities
Understanding second order spectra
• A2 vs AX or H2O
•
•
•
•
vs HF
For HF ..
Pββ->αβ ∝ |<ββ|γ
|<ββ| B1(Ix1 + Ix2)|αβ>|
| β>|2 ; Ix = (I+ + I-)/2
this is finite and same for all Pij
implies same line intensities
ββ
αβ
βα
αα
E
For an A2 system:
• αα, αβ, βα, ββ are not good wave functions
• Imply distinguishability
• Use: αα, (αβ+βα)/√2, (αβ-βα)/√2, ββ
• <ββ|
<ββ|γB1(Ix1 + Ix2)| (αβ+βα)/
( β+β )/√2 > = (½ + ½)/√2
• <ββ|γB1(Ix1 + Ix2)| (αβ-βα)/√2 > = (½ -½ )/√2 =0
• Outer transitions are not allowed
ββ
E
(αβ+βα)/√2
αα
(αβ-βα)/√2
Intermediate behavior of 2nd order spectra
• H 2O
• AB
• HF
Outer lines are not
Observed
Couplings still exist
Second order effects can be important
H5
Base
O
φ
C
H4
HO
J45
4 ?
H5'
OH
X
OH
• Coupling of H4 and H5
H5, H5’
H5 protons in ribose rings – an
ABX system
• Karplus equation might be used to deduce torsion angle,
but can couplings be measured from
f
multiplet?
?
• For degenerate H5, H5’, see a triplet, but splitting is
((J45+J45
45’))/2
• Cannot conclude that J45 = J45’
• Answer: simulate spectra
• See:
S
S A Smith,
S.A
S ith JJ. M
Magn R
Res, 166,
166 75 (1994)
(1994); M
M.Veshtort,
V ht t
R.G.Griffin, J Magn. Res., 178, 248-282 (2006)
Operators in Matrix Notation
(an alternate way of handling second order spectra)
If we stay with one basis set, properties vary only because of
changes in the coefficients weighting each basis set function
μx = γ(h/2π)<ψ| Ix |ψ>
ψ= c1 αα + c2 αβ + c3 βα + c4 ββ = ∑j cj φj
<ψ|
ψ| Ix |ψ
|ψ> = ∑j,k
φj| Ix |φk>
j k cj* ck <φ
We need calculate <φj| Ix |φk> only once if we stay
with this basis set – these can be put in a n x n matrix
matrix.
Matrix equivalent: <ψ| Ix |ψ> = (c1, c2, …)* ⎡ ⎤ ⎛c1⎞
⎟ Ix⎟⎟ ⎟ c2⎟⎟
⎣ ⎦ ⎝ •⎠
Special Case: Pauli Spin Matrices
0
|Ix| =
½
½
0
0
|Iy| =
i½
-i½
0
Note: < α | Ix | α> = ½ < α | β > = 0
< α | Ix | β > = ½ < α | α > = ½
½
|Iz| =
0
0
½
How do they work? Try something we know: Ix | α > = ½ β
0
½
½
0
1
0
=
0
½
0
=½
1
= ½ β
Operators are a matrix of numbers, Spin functions a vector of numbers
Larger Collections of Spin ½ Nuclei
IAx =
αα
βα
αβ
ββ
?
?
?
?
?
?
?
?
?
?
?
?
?
?
?
?
|β =
<αα|| IAx|βα>
<αα| ½ |αα> = ½
αα βα αβ ββ
0 1/ 2 0
=
1/ 2 0
0 0
0
0
0 0
0 1/ 2
0 1/ 2 0
0
IXx =
0 1/ 2 0
0 0
1/ 2 0
0 1/ 2
0 0
0 1/ 2 0
0
Easier way: direct products: E ⊗ IAx with 2X2 matrices
Density Matrices and Observables
f an Ensemble
for
E
bl off Spins
S i
Expectation values pertain to single spin properties;
we observe net behavior of an ensemble of spins. For
a particular system (two spin ½ nuclei) operator
representations are the same; all variations are in basis set
coefficients. We need to average over these coefficients.
< | Ix
<ψ|
I |ψ>
| > = (c1,
( 1 c2,
2 …)*
)* ⎡ ⎤ ⎛c1⎞
⎛ 1⎞
⎟ Ix⎟ ⎟ c2⎟
⎣ ⎦ ⎝ •⎠
= ∑j,k cj* ck Ix
I jk
Products of averaged coefficients can also be collected
and used in matrix form. This is called a density matrix, ρ.
<ψ| Ix |ψ> = Tr |cjck*| | Ix | = Tr | ρ | | Ix|