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
:
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
:
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.
 
Search WWH ::




Custom Search