Introduction Electric Quadrupole and Nuclear magnetic moments NMR experiments Energy consideration Chemical shift scale 11/07/2012 Organic Spectroscopy 1 Lecture 6 & 7 011 th November 2012
Introduction
Electric Quadrupole and Nuclear magnetic moments
NMR experiments
Energy consideration
Chemical shift scale
11/07/2012Organic Spectroscopy 1
Lecture 6 & 7
011th November 2012
Nuclear magnetic resonance is an importantspectroscopic technique which uses thelonger wavelengths (radio frequency)absorption to give information about numberof each type of nuclei (hydrogen/carbon) alsothe nature of its chemical environment.
An absorption spectrum is recorded byvarying the energy of radiation incident on asample and monitoring how much radiation isabsorbed at each energy level.
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Radiation can be absorbed when its energy
corresponds to the difference in energy
between energy levels in a molecule.
Energy transition in NMR technique; for
electron spin, ∆E corresponds to energy in
microwave region and for nuclear spin, ∆E
corresponds to the energy of radio waves.
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Any atomic nucleus which possesses eitherodd mass or odd atomic number or both hasa quantized spin angular momentum and amagnetic moment.
Thus, proton and carbon-13 have the spinquantum number I = ½ and has two allowedspin states. i.e +½ and –½.
Recall that I is a physical constant for eachnucleus, and there are 2I + 1 allowed spinstate which range with integral differencesfrom +I to -I
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i.e -I (-I + 1), …, (I –1), I;
For proton, Allowed spin state =2I + 1
Then, 2(½) + 1 = 2
Allowed spin states for proton is 2.
So, an applied magnetic field nuclei spins in
+½ (a-state) or -½ (b- state).
Whereas, the spin state of any given nucleus
are degenerate and equally populated in
absence of applied magnetic field
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Nuclear spin
(I)
Half integer
I = ½, 3/2 , 5/2,
Have
Odd
Atomic mass
Odd or Even
Atomic number
Integer
I = 1
Have
Even
Atomic mass
Odd
Atomic number
For zero
I = 0
Have
Even
Atomic mass
Even
Atomic number
I =1/2 : 1H, 13C, 19F
I= 3/2: 11B
I= 5/2: 17O
I =1: 2H, 14NI = 0: 12C, 16O
Spin state of some isotopic elements with respect to
atomic number and atomic masses
NMR involve absorption of Radio frequencies
on EMS.
A signal in an NMR spectrum is referred to as
resonance.
1H and 13CNMR spectroscopic experiment
gives information about number, type and
connectivity of hydrogen and carbon atoms in
a molecule
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NMR data are commonly acquired from 1D & 2D
experiments
The NMR spectra give information about the nature
of the chemical environment of each magnetically
active nucleus in the molecule
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H3C
C
O
O
H2C
C
CHH3C
H2C
O
H
3 types of H atomsNumber of H atoms= 6
5 types of C atomsNumberof C atoms = 5
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Nucleus may have spherical chargedistribution or non-spherical (prolate oroblate) charge distribution.
That is, all nucleus with I = 0 or I = ½ haveapproximately spherical charge distributionwithin their nuclei hence small electricquadrupole moment.
Those with I > ½ have non-spherical(ellipsoidal) charge distribution within theirnucleus hence large electric quadrupolemoment as shown below.
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Intrinsic magnitude of the generated dipole is
expressed in nuclear magnetic moment, μ.
The magnetic moment is generated by the charge
and spin of a charged particle.
Many moving charge generates a magnetic field
of its own and a weak secondary field (Bsec) due
movement of electron around it that opposes
applied field that shields the proton nucleus.
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All nuclei with non-zero spin (I >0) have
magnetic moment, μ, but the non-spherical
nuclei also have eQ.
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1H 12C 16O 19F 2H < 14N << 35Cl, 37Cl << 79Br,81Br 127I
eQ negligible Increasing eQ (absolute value)
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When the frequency of the oscillating electric
field component of the incoming radiation
just matches the frequency of the electric
field generated by the precessing nucleus the
two fields can couple, and energy can be
transformed from the incoming radiation to
the nucleus thus causing spin change. This
situation is called Resonance
The strong applied magnetic field (Bo) induces
the electrons to circulate around the nucleus
(left hand rule)
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e-
Bo
The induced circulation of electrons sets up a
secondary (induced) magnetic field (Bi) that
opposes the applied field (Bo) at the nucleus
(right hand rule)
Therefore, the effective field (Beff) is the difference
between Bo and Bsec . That is, Beff = Bo - Bsec
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e-
Bi
Bo
Hydrogen nucleus may have +½ or –½ spin
with μ. These two cases are in opposite
In an applied magnetic field, Bo all protons
will have their μ either aligned with the field
or opposed to it.
Thus, hydrogen nuclei can adopt either +½ or –½ with respect to the applied field
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Consider hydrogen nuclei acting like a tiny bar magnet (having North pole (N) and South pole (S) when placed in magnetic field, like-poles repeals each other and opposite poles attracts each other.
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Proton spinning in an
external magnetic field,
where the magnetic axis
of the proton precesses
about z axis of the
stationary magnetic field
Bo.
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protons in a molecule are shielded hence resonate at differentfrequencies.
Alignment of proton spin states when an external magnetic field, Bo is applied.
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Aplied magnetic
field, Bo
spin + ½
aligned to Bo
spin - ½
oppose Bo
Spinning proton has electron which also do spin and both generatemagnetic field.
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There is excess spin state in a-state because of lower inenergy.
The difference in energy, DE betweenthe two states (+½ and –½) dependson strength of the applied field, Bo.
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A nucleus is in resonance when it absorbs radio frequency radiations and spin flip to a high energy state
Energy absorbed is a quantized process and most equal the energy different between two state involved
Eabsorbed = (E -1/2 state – E +1/2 state) = h
In practice DE = f (bo)
The stronger the applied magnetic fields, the greater the energy difference between possible spin.
i.e the magnitude of the energy level separation depend on the
particular nuclear involved
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Magnetogyric ratio, is constant for eachnucleus and determines the energydependence on the MF
DE = f (bo) = h
bx
D =l
where l = 1/2
bx
The charge distribution which is slightly excess ina state (a lower energy level) is explain byBoltzmann charge distribution, N α > Nβ
Nα / Nβ = e-ΔE/kT
where k is Boltmann constant and T is temp (K) and change in energy is given by;
∆E = (hγ/2π)βo Where h - Planck’s constant, γ – nuclear constant (magnetogyric ratio).
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Spin states of proton in absence and in presence of Bo
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Spin states of chlorine in absence and in presence of Bo
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Once two levels for the proton have beenestablished energy in form of radiofrequency(rf or v1) can be introduced to effect thetransition between energy levels in astationary magnetic field of a given strengthBo;
Then, this equation (∆E = (hγ/2π)βo ) have tobe modified due to secondary magnetic field
by the nucleus i.e ν = βo (1- d)/2π; d isshielding factor
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DE =h
2_
Bo1 =
2_
Bo
Obtainable is the fundamental NMR equation correctingthe applied radiofrequency, 1 (MHz) with the Bo,
since DE = hν.
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1. NMR spectroscopy uses radiofrequency absorption to giveinformation about number of each type of nuclei and theconnectivity
2. Proton and carbon-13 have the spin quantum number I = ½and has two allowed spin states. i.e +½ (α sate) and –½ (βstate) which important for NMR techniques
3. The spin state of any given nucleus are degenerate andequally populated in absence of applied magnetic field
4. A signal in an NMR spectrum is referred to as resonance
5. The NMR spectra give information about the nature of thechemical environment of each magnetically active nucleus inthe molecule
6. All nuclei with non-zero spin (I >0) have magnetic moment,μ, but the non-spherical nuclei also have electricalquadrupole moment.
7. Spinning proton has electron which also do spin and both generate magnetic field The strong Bo induces the electrons to circulate around the nucleus (left hand rule)
which sets up secondary MF (Bi) that opposes Bo (Right hand rule)
8. The difference in energy, DE between the two states (+½ and –½) depends on strength of the applied field, Bo
9. Protons in a molecule are shielded hence resonate at different frequencies
10. There is excess spin state in a-state because of lower in energy
11. ∆E = (hγ/2π)βo ; since ∆E = hv
v = (γ/2π)βo
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