Nuclear Magnetic
Resonance (NMR) spectroscopy is a powerful technique employed for various
analytical purposes, especially structural characterization of organic
compounds.
NMR deals with the
behavior of nucleus under the influence of a strong magnetic field and
absorption of radiofrequency. Not all nuclei can be studied in NMR. Nuclei
having some spin can be observed with NMR spectroscopy. Spin is associated with
nuclei having an odd atomic number or mass number or both, for example 13C
has an odd mass number and even atomic number (6), 2H has an even
mass number and odd atomic number, while 1H has both the values odd.
All of these nuclei are NMR active. On the other hand 12C, 16O
have even mass number and atomic number and thus cannot be studied in NMR. Nuclei
with spin have an angular momentum and magnetic moment lending them
paramagnetism, thus acting as tiny small magnets. The ratio of the two
quantities is known as the gyromagnetic ratio (g),
which is a characteristic property of every different type of nucleus.
Spin
States
Nuclei can have several
spin states depending upon their spin quantum number. The number of possible
spin states can be calculated from the formula, 2I + 1.
For example: Proton (1H)
has a spin quantum number ½. The number of possible spin states are 2 (+1/2 and
-1/2).
2(1/2) + 1 = 2
Deuterium (2H) has spin = 1, so it can 3 spin
states.
2 (1) + 1 = 3
The frequency at which a
nucleus precesses is known as the precessional frequency or Larmor frequency (w), which is directly proportional to the
strength of the applied magnetic field (Bo)
w
= gBo
Population
of Spin states
When the nuclei are
placed in a magnetic field they align themselves in all possible spin states.
For a proton nucleus, only two states are possible. Thus a proton nucleus will
either align against the direction of the applied magnetic field or in the direction
of the field. In fact both the states are populated, but there always will be a
slight excess of population in the lower energy spin state (a). This excess is known as the Boltzmann’s
excess and can be calculated from the Boltzmann distribution law.
The magnetization of the
nuclei in both the states cancel the effect of each other, but because there is
a small excess in the lower energy state, we observe a net magnetization from
the combined effect of the excess nuclei aligned in the direction of the applied
magnetic field, shown by a net magnetization vector (Mo). Mo is by default
shown at z-axis, its equilibrium state, pointing in the direction of Bo.
Radiofrequency
pulse (Absorption of Energy)
We already know that
nuclei (proton) or the net magnetization for that matter is precessing with a
particular frequency, called the larmor frequency. When a strong pulse of
radiofrequency is applied, the frequency that matches the larmor frequency of proton
is absorbed and the nuclei flip. In other words when the radiofrequency is absorbed, the
nuclei jump from lower energy to higher energy state. The radiation thus needs
to have energy equal to the energy gap between the two states.
NMR
Signal
The nuclei need to relax
back to their equilibrium state (z-axis). This relaxation is detected by the
detector and signals are sent to the recorder which then plots the transitions
in the form of NMR signal.
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