Environmental Engineering Reference
In-Depth Information
nuclei behave like tiny bar magnets. Some nuclei will align with the magnetic field (at a
lower energy level), whereas others will align against the field (at a higher energy
level). Since the nucleus energy is quantized, there will be no other spin states. The
energy difference between the two nuclear spin states is as follows:
gh
2p
B
0
E ¼
ð12
:
1Þ
where h is the Planck's constant, B
0
is the strength of the magnetic field in the unit of
tesla (T), and g is the gyromagnetic ratio in the unit of rad/T/s. One tesla (T) is actually
a relatively strong field—the earth's magnetic field is of the order of 0.0001 T.
When an electromagnetic radiation is introduced, the nucleus is resonated if the
applied radiation energy (E ¼ hn) is equal to the energy difference (
E) noted in
Eq. 12.1. This frequency can be calculated by
g
2p
B
0
n ¼
ð12
:
2Þ
At the resonance frequency, nuclei in the lower energy (þ½) flip to the higher energy
state (½). Since the value of gyromagnetic ratio (g) depends on a particular kind of
nucleus, different energies are required to bring different kinds of nuclei into
resonance. Hence, an NMR signal (rf absorption) can be obtained as a function of the
changing frequency. Such a relationship is the basis of an NMR spectrum.
Note that only certain atomic nuclei have the NMR signals. Nuclei with an even
mass number and an even charge number (
12
C) have spin quantum numbers of zero.
Nuclei with an even mass number and an odd charge number (e.g.,
2
H) have integer
spin quantum number of one. Neither
12
C nor
2
H produces NMR signals. Only
nuclei with odd mass numbers and half-integer spin quantum numbers (I ¼ ½),
such as
1
H,
13
C,
15
N,
19
F, and
31
P can be used to obtain NMR spectra. Among
these,
1
H and
13
C are the most common, hence the name
1
H-NMR (proton NMR)
and
13
C-NMR (carbon thirteen NMR).
From Table 12.2, it is clear that the most abundant isotope of carbon (
12
C),
unfortunately, cannot be used to obtain an NMR spectrum. The NMR responsive
Table 12.2 Properties of selected nuclei that are important in NMR spectroscopy
a
Natural
Gyromagnetic
NMR frequency
Relative
(MHz)
b
sensitivity
c
Nucleus
Spin (I)
abundance (%)
ratio (rad/T/s)
1
H
½
99.99
2:675210
8
100
1
2
H
1
0.01
4:106610
7
15.35
9:6510
3
12
C
0
98.9
-
-
-
13
C
½
1.1
6:728310
7
25.15
1:5910
2
14
N
1
99.6
1:933810
7
7.23
1:0110
3
15
N
½
0.4
2:712610
8
10.14
1:0410
3
19
F
518210
8
3210
1
½
100
2
:
94.09
8
:
31
P
1:084010
8
6:6510
2
½
100
40.48
a
Values adapted from Friebolin (2005).
b
NMR resonance frequency is calculated at B
0
¼ 2:3488 T.
c
Selectivity is expressed relative to
1
H at a constant field for an equal number of nuclei.
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