This is a member of an interesting class of compounds which are chiral, without actually containing
a define chiral centre. They are chiral because their mirror images are non-superimposable. In the case
of this molecule, there is no rotation about the bond between the two naphthol rings because of the
steric interaction between the two hydroxyl groups. ‘d’ and ‘l’ forms can be isolated and are perfectly
stable (Optical purity determination by ‘H NMR, D. P. Reynolds, J. C. Hollerton and S. A. Richards, in
Analytical Applications of Spectroscopy, edited by C. S. Creaser and A. M. C. Davies, 1988, p346).
Optically pure mandelic acid (see Structure 7.6) can be a useful chiral resolving agent where the
compound you are looking at has a basic centre, as it can form an acid-base pair with it, which is
a stronger form of association. This compound is of sparing solubility in CDCl3 however and can
precipitate out your compound if, as is often the case, its protonated form is of low solubility in CDCl3.
The technique of using resolving agents is obviously a useful one in following the synthesis of a
compound of specifie chirality. To summarise, we take our compound, which has a chiral centre of
unknown rotation and form some sort of complex by introducing it to a reagent of known optical purity.
The complexes we form have diastereoisoromeric character, which can give rise to a difference in the
chemical shifts of one or more of the substrate signals. This enables us to determine the enantiomer
ratio, either visually, or by integration, if we have sufficien signal separation.
In practise, if using one of these reagents to follow the course of a chiral separation, it is essential
to determine whether resolution is possible, by performing a test experiment either on a sample of
racemate, or at least a sample known to contain significan quantities of both enantiomers. Once useable
resolution has been established, the technique can be used to monitor solutions of unknown enantiomer
ratios with reasonable accuracy, down to normal NMR detection limits.
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t in a fairly spectacular fashion, when it is present in a molecule.
Once again, I = 1/2, so we only have two allowed states to worry about. Unlike 13C however, f uorine
has only one isotope, 19F, and as this of course, has 100 % natural abundance, we see the whole proton
signal split, instead of a couple of tiny satellites on either side of our signals!
This point is well illustrated with a spectrum of 3-fluor propanol (Spectrum 6.10), which shows
a fairly dramatic example of fluorin coupling. The F-CH2- coupling is about 47 Hz, and the
F-CH2-CH2- coupling, is 27 Hz. The coupling to the third methylene group is non-existent in this
example but can be seen sometimes (0–3 Hz).
Another example of 19F coupling, this time in an aromatic system, (4-fluor benzoic acid) is shown
in Spectrum 6.11. Note how the 19F couplings to the aromatic protons give the AA′BB′ system an
2.02.53.03.54.04.5 ppm
16
.0
0.
2
26
.5
0.
7
26
.3
26
.4
Spectrum 6.10 3-Fluoro propanol.
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Delving Deeper 85
7.307.357.407.457.507.557.607.657.707.757.807.857.907.958.008.05 ppm
15
.0
15
.0
Spectrum 6.11 4-Fluoro benzoic acid.
asymmetric appearance. The actual values in this case are 9.0 Hz (ortho) and 5.6 Hz (meta) which are
fairly typical.
More useful 19F coupling data is given in Table 6.1.
Fluorine can sometimes throw up some unexpected couplings in certain situations and spectra need
to be handled with care! Sometimes, fluorin can be seen to couple over an unfeasible number of bonds
(we have seen a seven bond coupling in the past). This is because fluorin is so electron hungry that it
can couple through space as well as through-bond!
We have also noted some strange behaviour with fluorinate pyridines, for example, 3-fluor nicotinic
acid (Structure 6.19 and Spectrum 6.12). The signal for Hc (approx. 8.1 ppm) clearly shows couplings
of 9.1, 2.9 and 1.7 Hz. The 9.1 Hz coupling must be from the fluorin as it does not appear anywhere
else in the spectrum and its chemical shift distinguishes it from either of the other two protons.
Of the other two protons, the signal at 8.82 ppm, (Hb) shows only a 2.9 Hz coupling which is also
found in Hc, whilst Ha exhibits two small couplings (2.0 and 1.7 Hz), the smallest of these also appearing
in Hc. These observations lead to the conclusion that the fluorine–proto couplings in this molecule are
as given in Table 6.2.
N
F
O
OH
HaHb
Hc
Structure 6.19 3-Fluoro nicotinic acid.
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86 Essential Practical NMR for Organic Chemistry
Table 6.1 Some typical 19F–proton couplings.
Structure 19F-1H position Typical 19F-1H coupling (Hz)
FCH3 F-CH2-F-CH2-CH2-
F-CH2-CH2-CH2-
45
24
0–3
F
HH
H
F-H (geminal)
F-H (cis)
F-H (trans)
85
20
50
CH3~C=C
H
F
F-CH3 2–4
H~C=C~CF3 F3C-H 0-1
CH3
F
F
F
F3C-CH2- 8–10
F
H
F-H (ortho)
F-H (meta)
F-H (para)
6.2–10.3
3.7–8.3
0–2.5
F
CH3
F-CH3 (ortho)
F-CH3 (meta)
F-CH3 (para)
2.5
0
1.5
F F
H
H
Faxial–Haxial
Faxial–Hequatorial
Fequatorial–Hequatorial
34
11.5
5–8
F-Hc coupling did not surprise and neither did F-Ha coupling. But the F-Hb coupling of less than a
single Hz is totally bafflin and defie obvious logic!
Having learnt the lessons from this simple little compound, it would seem reasonable to expect
similarly surprising couplings in other fluorinate heterocycles.
Tread carefully!
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Delving Deeper 87
8.058.108.158.208.258.308.358.408.458.508.558.608.658.708.758.808.858.908.95 ppm
8.
0
7.
7
7.
7
Spectrum 6.12 3-Fluoro nicotinic acid.
Table 6.2 Fluorine–proton couplings
in 3-fluoro nicotinic acid.
Position Coupling (Hz)
F-Ha 2.0
F-Hb very small, <1.0!
F-Hc 9.1
6.6.3 Coupling between Protons and 31P
Phosphorus is the other heteroatom of major coupling importance to the organic chemist. Like 19F, 31P
has a spin of 1/2 and a 100 % natural abundance, so you know what to expect! The actual size of the
couplings observed with 31P can vary considerably, depending on the oxidation state of the 31P atom.
You’ll fin some useful examples in Table 6.3.
31P shows one particularly interesting feature. The size of couplings normally decreases dramatically
with the number of intervening bonds, but this is not always the case with 31P (Table 6.3).
A proton directly bonded to a 31P atom can be split by an enormous coupling of as much as 700 Hz
(depending on the oxidation state of the phosphorus)! That means that the two parts of such a signal
would be separated by almost 3 ppm at 250 MHz! So huge is this coupling that you could easily fail to
recognise or accept it as a coupling at all, if you came across it. Structure 6.20 and Spectrum 6.13 show
an example of 31P-1H coupling.
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88 Essential Practical NMR for Organic Chemistry
Table 6.3 Some typical 31P–proton couplings.
Structure 31P-1H relative position Typical 31P-1H coupling (Hz)
(CH3)3P P-CH3 2.7
(CH3)3P=O P-CH3 13.4
(CH3)4P+I− P-CH3 14.4
(CH3-CH2)3P P-CH2-CH3
P-CH2-CH3
0.5!
13.7!
(CH3-CH2)3P=O P-CH2-
P-CH3
11.9
16.3
R P
H
H
P-H 180–200
P
O
HRO
OR
P-H 630–710
CH3 P
OR
R
R
R
P-CR2-CH3 10.5–18.0
CH3 P
OR
R
R
R
P-CR2-CH3 10.5–18.0
CH3 P
OR
OR
R
R
O
P-CR2-CH3 10.5–18.0
P
O
O CH3
P-CH2- 6
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Delving Deeper 89
P+
BrX-
Structure 6.20 Compound showing 31P-1H coupling.
1.81.92.02.12.22.32.42.52.62.72.82.93.03.13.23.33.43.53.63.73.83.94.04.1 ppm
7.
1
7.
4
7.
6
7.
1
Spectrum 6.13 31P-1H coupling.
The complex multiplet at 4.02 ppm shows a 13 Hz 2-bond 31P coupling to the firs -CH2 in the chain
and spin decoupling enables the 3-bond 31P coupling to the next -CH2 in the chain (1.86 ppm) to be
measured (8 Hz).
6.6.4 Coupling between 1H and other Heteroatoms
If you ever run a sample which is contaminated with an ammonium salt, in DMSO, you will see
14N–proton coupling, as shown in Spectrum 6.14. Note that the three lines of the multiplet are of equal
intensity (the middle line is a little bit taller than the outer ones, but this is because of the width of
the peaks at their bases. The central signal is reinforced because it stands on the tails of the outer
two). This is because 14N has a spin of I = 1, and the allowed states are therefore –1, 0 and +1.
This three line pattern with its 51 Hz splitting is highly characteristic and once seen, should never be
forgotten.
14N coupling is only observed when the nitrogen atom is quaternary. In all other cases, any cou-
pling is lost by exchange broadening, or quadrupolar broadening, both of which we’ve discussed
before. Two-bond couplings, [e.g., 14N+-(CH2)4] are not observed, even when the nitrogen is qua-
ternary, in ‘quat salts’ such as (n-butyl)4N+− Br−, presumably because the coupling is very small.
So the phenomenon is only ever observed in the +NH4 ion! Note: The -CH2- attached to the qua-
ternary nitrogen in compounds like tetra N-butyl ammonium chloride does present as a distorted
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90 Essential Practical NMR for Organic Chemistry
6.856.906.957.007.057.107.157.207.257.307.357.407.457.507.557.607.657.707.75 ppm
Spectrum 6.14 Typical appearance of +NH4 ion in DMSO.
triplet with its central line split into a narrow triplet but this has nothing to do with 14N coupling
as the same distortion can sometimes be seen in -CH2- groups next to certain other moieties, e.g.,
-SO2R. It is a non-firs order phenomenon caused by slight non-equivalence of the two protons in
question.
Boron has two isotopes, both of which have spin! 10B has a natural abundance of 18.8 %, and
a spin of I = 3 (allowed spin states –3, –2, –1, 0, +1, +2, +3; i.e., one signal will be split into
seven lines of equal intensity), whilst 11B has a natural abundance of 81.2%, and a spin of I = 3/2
(allowed spin states –3/2, –l/2, +1/2, and +3/2; i.e., one signal will be split into four lines of equal
intensity).
This gives rise to amazing effects in the borohydride, BH4− ion (Spectrum 6.15), which can some-
times be formed accidentally during borohydride reductions. Note that the 10B-H couplings are of a
different size to the 11B-H couplings. All 11 lines of the BH4− ion are to be found between 0 and
–0.7 ppm. Note that, like 14N, 11B has a quadrupolar nucleus, but once again the symmetrical envi-
ronment of the borohydride ion negates the relaxation pathway that would otherwise cause significan
line broadening. Boron coupling is not generally seen in asymmetric environments or over multiple
bonds.
-0.65-0.60-0.55-0.50-0.45-0.40-0.35-0.30-0.25-0.20-0.15-0.10-0.050.00 ppm
6.
2
8.
4
0.
8
7.
5
6.
7
Spectrum 6.15 Boron–proton coupling in the borohydride ion.
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Delving Deeper 91
-0.10.7 0.6 0.5 0.4 0.3 0.2 0.1 0.0 ppm
0.
5
4.
5
0.
4
1.
0
9.
9
1.
0
Spectrum 6.16 Mixture of two organotin compounds.
One other heteroatom worth mentioning is tin as organotin compounds are significan in organic
synthesis. Tin has no fewer than ten naturally occurring isotopes, but fortunately, only three of them
have nuclear spin. 115Sn has a natural abundance of a mere 0.32 %, which makes it spectroscopically
insignificant of course. The only isotopes of tin that need concern us, are 117Sn (natural abundance
7.67 % and I=1/2), and 119Sn (natural abundance 8.68 %, and also, I=1/2).
These two isotopes are both capable of two-bond and three-bond couplings in alkyl organotin com-
pounds. This is demonstrated in Spectrum 6.16 which shows a mixture of two organotin compounds.
The compound with a strong central peak at 0.5 ppm is thought to be (CH3)3-Sn-OH. The inner satel-
lites result from a 117Sn-CH3 coupling of 69 Hz and the outer satellites to a 119Sn-CH3 coupling
of 72 Hz.
The second compound with the major signal centred at 0.13 ppm is (CH3)3-Sn-Sn-(CH3)3. In this
case, we see once again, satellites resulting from two-bond couplings but also a second set of inner
satellites resulting from smaller three-bond couplings of about 16 Hz for both 117Sn and 119Sn (i.e.,
Sn-Sn-CH3).
Note too from the chemical shifts of these methyl groups that tin has quite a strong shielding effect.
Finally, 29Si is an isotope that you should be aware of – every time you acquire a well prepared sample
using TMS as a standard! 29Si satellites (accounting for about 4.7 % of the total signal, J 29Si – -CH3,
6.6 Hz) should be visible at the base of your TMS peak. The small coupling provides a good test of
shimming quality (Spectrum 6.17).
6.6.5 Cyclic Compounds and the Karplus Curve
As we have already mentioned, chemical shifts and couplings are heavily influence by molecular
constraint and for this reason, some guidance in dealing with cyclic (saturated) compounds might
well prove useful. We have already seen that in straightforward open-chain alkyl systems, the size of
proton-proton couplings is governed by the electronegativity of neighbouring atoms. But the most
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92 Essential Practical NMR for Organic Chemistry
-0.04-0.03-0.02-0.010.04 0.03 0.02 0.01 0.00 ppm
Spectrum 6.17 TMS showing 29Si satellites.
important factor which governs the size of couplings between vicinal protons is the dihedral angle
between them.
In open-chain systems, this angle is usually averaged by rotation about the C-C single bond, and so
is not normally of significance But in carbocyclic systems, dihedral angles are usually fi ed, since the
structures are generally rigid. It is therefore vital that we understand how the size of vicinal couplings
varies with dihedral angle. This data can be obtained by using the Karplus equation but the information
derived from this equation (or equations as there are various versions of it) is more usefully portrayed
graphically. A family of curves thus constructed makes additional allowance for factors other than
dihedral angles which influenc vicinal proton couplings, e.g., localised electronegativities (Figure 6.2)
but we have opted for a simplifie graph showing only three curves.
Selection of the best curve for a given situation is perhaps rather a matter of trial and error, but
is best approached by positively identifying an axial–axial coupling, since this arrangement ensures
(in six-membered rings at least) a dihedral angle of 180◦ between the protons. Choose the curve that
best fit the value that you observe for an axial–axial coupling in your molecule. Note that in the
absence of any extreme electronic effects, this should give rise to a coupling of about 12 Hz. Similarly,
a dihedral angle of 90◦ gives rise to a coupling of approximately 0 Hz, and where the angle is 0◦, we
may expect a coupling of about 10 Hz. Making a model of the molecule becomes very important in
the case of carbocyclic compounds, as it is important to be able to make fairly accurate estimates of
dihedral angles.
Now let us consider Structure 6.21 and Spectrum 6.18 and see how the Karplus curve can be used
to aid assignment of the spectrum. (This compound will be referred to from now on as the morpholine
compound as we will use it to demonstrate several different techniques) Note that the aromatic region
has been omitted as it contains little of interest and we wish to concentrate on the carbocyclic region of
the spectrum. It was acquired in CDCl3.
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Delving Deeper 93
θ
0
2
4
6
8
10
12
14
16
18
1801701601501401301201101009080706050403020100
Angle θ (degrees)
Co
up
lin
g
co
ns
ta
nt
(H
z)
H
H
Figure 6.2 The Karplus curve – for relating the observed splitting between vicinal protons to their dihedral
angle, θ .
To derive maximum benefi from this exercise, we recommend that you make a model of this molecule,
and refer to it as we go through the spectrum. Note that the morpholine ring falls naturally into a ‘chair’
conformation. Note also that in this example, the -CH2-Cl function will seek to minimise the morpholine
ring energy by occupying an equatorial environment as this minimises steric interactions between it, and
protons, and other substituents on the ring. All groups do this. The benzyl function will do likewise by
inversion of the nitrogen stereochemistry.
It is also worth noting that nine times out of ten, equatorial protons absorb at somewhat lower f eld
than the corresponding axial protons. This can be reversed in certain cases where the specifi anisotropies
of the substituents predominate over the anisotropies of the rings themselves but this is relatively rare.
The difference is typically 0.5–1.0 ppm, but may be more.
The structure is depicted as a Newman projection below (Figure 6.3). Aromatic protons aside, (they
give the expected fi e-proton multiplet centred at around 7.3–7.4 ppm) the firs signal we encounter as
O
N
Cl
Structure 6.21 The morpholine compound.
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94 Essential Practical NMR for Organic Chemistry
2.02.53.03.54.04.55.05.56.06.57.07.5 ppm
25
.4
43
.8
30
.2
2.12.22.32.42.52.62.72.82.93.03.13.23.33.43.53.63.73.83.94.0 ppm
Spectrum 6.18 The morpholine compound in CDCl3 with expansion.
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Delving Deeper 95
N
O
CH2Ph
CH2
Cl
Hc
Hg
Hj Hi
Hb
Hh
Hd
a e
Figure 6.3 The morpholine compound shown as a Newman projection.
we work from left to right is a complex multiplet – which is actually, a doublet of doublet of doublets
[ddd] – at 3.95 ppm. Careful measurement of the couplings reveals them to be 11.4, 3.4 and 2.0 Hz.
Since the multiplet is dominated by one large coupling, we can be safe in the knowledge that it must be
an equatorial proton.
This is because the dihedral angles between equatorial protons and both their equatorial and axial
vicinal partners are always such that they give rise to relatively small couplings (check model and the
Karplus curves). The only large coupling (i.e., 10 Hz or more) an equatorial proton can have will always
be to its geminal partner – if it has one. So in this case, the 11.4 Hz coupling is clearly a geminal
coupling. If we now make the entirely reasonable deductions that the proton giving rise to this signal is
likely to be alpha to oxygen rather than nitrogen (on the basis of chemical shift) and that as the -CH2-Cl
will be equatorial (as explained earlier), then this multiplet can only be assigned to the equatorial proton
‘b’ since there are no other equatorial protons that are alpha to oxygen in the molecule. The other two
couplings can be rationalised in terms of the equatorial–axial coupling (3.4 Hz which is reciprocated in
the ddd at 2.27 ppm) and the equatorial–equatorial coupling (2.0 Hz which is reciprocated in the dddd
at 2.71 ppm). Note: methods of unpicking couplings will be discussed at length in later sections. Such
methods are very useful when dealing with more complex spin systems like this one.
The degree of roofin of ‘b’ indicates that its geminal partner must be fairly close to it in terms of
chemical shift and sure enough, the six-line multiplet (another ddd) centred at 3.76 ppm satisfie the
requirements for this proton (‘d’). Note that the second large coupling to this signal is also 11.4 Hz, the
axial–axial coupling being the same size as the geminal coupling in this instance. The small remaining
coupling (approx. 2 Hz) is reciprocated in the dddd at 2.71 ppm and is an axial–equatorial coupling.
Proton ‘c’ can be define by the fact that it is not equatorial and it is highly coupled. The multiplet at
3.82 ppm satisfie these requirements. It is in the right ball park for chemical shift and is highly complex
in that this proton is already the X part of an ABX system coupled to both protons alpha to the chlorine
(the AB part). It is then further coupled with a 10 Hz, axial–axial coupling (reciprocated in the dd at
2.07 ppm) and with a 2 Hz axial–equatorial coupling which is reciprocated in the ddd at 2.90 ppm. Note
that ‘c’ and ‘d’ are not fully resolved from each other. Such overlap inevitably complicates the issue.
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96 Essential Practical NMR for Organic Chemistry
The N-benzyl protons are accidentally equivalent, presenting as a singlet at 3.59 ppm and overlap
with the two protons alpha to the chlorine atom which present as the heavily roofed AB part of an ABX
system (i.e., eight lines) centred at 3.55 ppm.
Without slavishly dissecting the remaining four signals (2.90, 2.71, 2.27, 2.07 ppm), we hope that the
principles of carbocyclic analysis have now been established. You should see at a glance that the 2.90
and 2.71 ppm signals must belong to equatorial protons because they are each dominated by only one
large coupling and the remaining two must correspond to their axial partners. You should now be able
to verify which equatorial proton belongs to which axial proton just by inspection.
There is one last coupling which we have not yet mentioned and that is the apparent extra small
coupling that can be seen on the equatorial protons alpha to the nitrogen (2.90 and 2.71 ppm). These
two signals are in fact coupled to each other by what is known as a W path coupling. These are 4-bond
couplings (unusual in saturated systems) which can be seen in situations where all the intervening
proton–carbon and carbon–carbon bonds lie in the same plane. You can see from the model which
you have next to you (?) that by definition such protons can only be equatorial. Note that whilst
all the assignments in this section have been made purely on the basis of observations of couplings
and multiplet appearance, this type of assignment is often simplifie by having definit ve knowledge
of coupling pathways. We will discuss the options available for acquiring this type of data in a later
chapter.
Whilst six-membered rings may often give rise to quite complex spectra, they are at least generally
rigid and based on the ‘chair’ conformation. As we have seen, this means that dihedral angles can be relied
on and the Karplus curve used with reasonable confidence Unfortunately however, the same approach
will end in tears if applied to other ring systems. Five-membered rings for example, are notoriously
difficul to deal with as they have no automatic conformational preference. They are inherently fl xible,
their conformations driven by steric factors. Cis protons on fi e-membered rings can have dihedral
angles ranging from approximately –30◦ to 0◦ to +30◦ and exhibit a range of couplings to match. Trans
protons on the other hand can range from +90◦ to +150◦. Deductions that can be made on the basis of
observed vicinal couplings are therefore limited. If the observed coupling is very small, the two protons
can only be trans to each other but if it is not, then they may be either cis or trans. We council against
reliance on molecular modelling packages to produce a valid conformation of such structures. The
energy difference between potential conformers is often small and could change in different solvents.
Modelling packages consider molecules in isolation and thus make no allowances for solvent effects.
Stereochemical assignments of such ring systems can only be confidentl made on the basis of NOE
experiments which we will cover in detail in Section 8.5.
6.6.6 Salts, Free Bases and Zwitterions
Sometimes, misunderstandings can arise when dealing with compounds containing protonatable centres.
Hopefully, in this section, we will be able to clarify a few key issues that are relevant to such compounds.
As we have already mentioned, CDCl3 should be avoided as a solvent for salts for two reasons. Firstly,
salts are unlikely to be particularly soluble in this relatively nonpolar solvent but more importantly,
spectral line shape is likely to be poor on account of relatively slow proton exchange at the protonatable
centre. The remedy is simple enough – avoid using CDCl3 and opt for one of the more polar options
instead, e.g., deuterated DMSO or MeOH and you should obtain spectra every bit as sharp as those of
free bases.
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Delving Deeper 97
In practical terms, it is invariably a nitrogen atom that is protonated in salt formation. This always
leads to a downfiel shift for protons on carbons both alpha and beta to the nitrogen concerned. In
alkyl amines, the expected shifts would be about 0.7 and 0.3 ppm respectively. Remember that some
heterocyclic compounds (e.g., pyridine) contain nitrogen atoms that are basic enough to protonate and
comparable downfiel shifts can be expected (Spectrum 5.9).
A misconception that we commonly encounter is that a spectrum can be a ‘mixture of the salt and the
free base.’ This is an excuse that is often used by chemists to explain an inconveniently messy looking
spectrum! Don’t be tempted by this idea – proton transfer is fast on the NMR timescale (or at least, it is
when you use a polar solvent!) and because of this, if you have a sample of a compound that contains
only half a mole-equivalent of an acid, you will observe chemical shifts which reflec partial protonation
and not two sets of signals for protonated and free-base forms. It doesn’t happen – ever!
Of course, whether a compound forms a salt or not depends on the degree of availability of the lone
pair of electrons on any nitrogen atoms in the compound (i.e., their pKb values) and on how strong the
acids involved in the salt formation (pKas). As a rough rule of thumb, alkyl and aryl amines do form
salts whilst amides, ureas, most nitrogen-containing heterocycles and compounds containing quaternary
nitrogen atoms do not.
It should always be remembered of course, that the NMR spectrum reflect a compound’s behaviour
in solution. It is quite possible for a compound and a weak acid to crystallise out as a stoichiometric salt
and yet in solution, for the compound to give the appearance of a free base. For this reason, care should
be taken in attempting to use NMR as a guide to the extent of protonation. If the acid has other protons
that can be integrated reliably, e.g., the alkene protons in fumaric or maleic acid, then there should be no
problem but if this is not the case, e.g., oxalic acid, then we would council caution! Do not be tempted
to give an estimate of acid content based on chemical shift. With weak acids, protonation may not occur
in a pro rata fashion though it is likely to in the case of strong acids.
Sometimes, you may encounter compounds which have more than one protonatable centre. It is often
possible to work out if either one or more than one are protonated in solution. A good working knowledge
of pKbs is useful to help estimate the likely order of protonation with increasing acidity. Assume that
the most basic centre will protonate firs and assess the chemical shifts of the protons alpha to each of
the potentially protonatable nitrogen atoms.
Zwitterionic compounds are worthy of special mention:
H2N−R − COOH ↔ H3N+−R − COO−
By their very nature, their partial charge separation can make them fairly insoluble and the degree of
this charge separation (and hence resultant NMR spectra) tends to be highly dependant on concentration
and pH. For these reasons, we recommend dealing with such compounds by ‘pushing’ them one way
or the other, i.e., by adjusting the pH of your NMR solution so that the compound in question is either
fully protonated (addition of a drop of DCl) or de-protonated (addition of a drop of saturated sodium
carbonate in D2O):
H3N+−R − COOH H2N − R − COO−
Fully protonated Fully de-protonated
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98 Essential Practical NMR for Organic Chemistry
NH+
N
N
O
A
A = Aryl
Cl-
Structure 6.22 A protonation example.
Whilst dealing with protonation issues, it is well worth considering the time dependence of the
process in the context of the NMR timescale. A compound of the type shown in Structure 6.22 provides
an interesting example.
As a free base, the Ar-CH2-N protons would present themselves as a simple singlet. The lone pair
of electrons on the nitrogen invert very rapidly on the NMR timescale and so the environment of the
two protons is averaged and is therefore identical. However, on forming a salt, the whole process of
stereochemical inversion at the nitrogen is slowed down dramatically because the sequence of events
3.33.43.53.63.73.83.94.04.14.24.34.44.54.64.74.84.95.05.1 ppm
3.
2
1.
1
0.
9
1.
0
Spectrum 6.19 Slow inversion of a protonated tertiary amine nitrogen.
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Delving Deeper 99
A
HN+
A
H
A = Aryl
Structure 6.23 Compound showing ‘pseudo enantiomeric’ behaviour.
would be; de-protonation, inversion and re-protonation. Although as we said earlier, proton transfer is
in itself a very fast process on the NMR timescale, it is the time taken for the entire process to occur that
determines the nature of the spectrum that we observe.
What we actually observe for the Ar-CH2-N protons of the salt in this molecule is a pair of broad,
featureless signals at 4.6 and 5.0 ppm. The explanation for this is simple enough once the concept of time
dependency for the inversion sequence has been appreciated. The protons in question fin themselves in
different environments (within the context of the NMR timescale) and therefore have distinct chemical
shifts. The signals are broad because the dynamic exchange process is taking place with a time period
comparable to the NMR timescale, the broadening masking the geminal coupling between them (see
Spectrum 6.19).
A logical extension of these ideas will lead you to a recognition of the fact that a phenomenon of
this type could yield species in solution which appear to behave as if they contain a chiral centre – even
when they don’t. We have seen ‘pseudo enantiomeric’ behaviour in compounds of the type shown in
Structure 6.23 (when protonated).
All the protons of the CH2s in a molecule of this type may be non-equivalent (i.e., you observe
essentially three AB systems). Note that the coupling from the alkene CH is would be small to both of
the cyclic CH2s when the spectrum is acquired in the presence of HCl (see Spectrum 6.20). When the free
3.954.004.054.104.154.204.254.304.354.404.454.504.554.604.654.704.754.80 ppm
1.
2
1.
2
2.
2
1.
1
1.
0
Spectrum 6.20 Protonated nitrogen of a tertiary amine acting as a ‘chiral centre’.
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100 Essential Practical NMR for Organic Chemistry
base is liberated, all the AB systems collapse to give singlets. The explanation follows on logically from
a consideration of the previous example. Protonation of the tertiary amine generates a chiral centre at
the nitrogen atom, forcing all the geminal pairs of protons into different environments – hence the three
AB systems. But this does not in any way imply that it would be possible to separate out enantiomers
of the compound in salt form. These ‘pseudo enantiomers’ can only be differentiated within the context
of a technique which has a timescale of a couple of seconds. Attempting to separate them on an HPLC
column for example, would be unsuccessful as this technique has a timescale of several minutes (define
by how long compounds take to travel down the column and enter the detector). During this time, proton
exchange and consequent ‘enantiomer’ interconversion would have occurred many times in the course
of the analysis. The only manifestation of this might be a slightly broader than normal (single) peak.
This whole area of spectroscopy touches on many different topics and can only be approached
confidentl with a reasonable working knowledge of basic NMR, stereochemistry and certain aspects
of physical chemistry.
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7
Further Elucidation Techniques – Part 1
If a spectrum does not yield the definit ve information that you require on inspection, there are many
other ‘tools of the trade’ that we can use to further elucidate structures. Broadly speaking, these fall into
two categories – chemical techniques and instrumental techniques.
7.1 Chemical Techniques
We will take a brief look at chemical techniques first It is true to say that the development of more and
more sophisticated instrumental techniques has to a considerable extent, rendered these less important
in recent years but they still have their place and are worthy of consideration in certain circumstances.
Before embarking on any of these chemical techniques, however, be advised that they are not without
a measure of risk as far as your sample is concerned! One of the great strengths of NMR is that it is
a nondestructive technique but that can change quite rapidly if you start subjecting your compounds
to large changes in pH or to potentially aggressive reagents like trifluoroaceti anhydride (TFAA)! Be
sure that you can afford to sacrific the sample as recovery may not be possible. In the case of precious
samples, chemical techniques should be regarded as a last option rather than a firs choice.
7.2 Deuteration
Deuteration is the most elementary of the chemical techniques available to us, but it is still useful for
assigning exchangeable protons which are not obviously exchangeable, and for locating exchangeables
masked by other signals in the spectrum. There are of course, other ways of identifying exchangeables.
The signal can be scrutinised closely to see if it has any 13C satellites associated with it, though this is
not viable in the case of broad signals. Alternatively, irradiation of the water peak in an NOE experiment
can be used as we’ll see later. Nonetheless, deuteration does provide a quick and easy method of
identificatio which is still perfectly valid.
Just to recap on the procedure, add a couple of drops of D2O to your solution, and shake vigorously
for a few seconds. Note that with CDCl3 solutions, the best results are obtained by passing the resultant
solution through an anhydrous sodium sulfate filte to remove as much emulsifie D2O as possible. (Note
Essential Practical NMR for Organic Chemistry S. A. Richards and J. C. Hollerton
© 2011 John Wiley & Sons, Ltd. ISBN: 978-0-470-71092-0
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102 Essential Practical NMR for Organic Chemistry
3.5 3.0 2.5 2.0 1.5 1.0 0.5 ppm
1.
5
1.
5
1.
0
1.
0
Spectrum 7.1 n-Butanol in CDCl3 with -OH obscured by multiplet at 1.39 ppm.
also that CDCl3 and D2O are not miscible, the CDCl3 forming the bottom layer as it is more dense than
D2O.) You then re-run the spectrum and check for the disappearance of any signals. Careful comparison
of integrations before and after addition of D2O should reveal the presence of any exchangeable protons
buried beneath other signals in the spectrum. If they are slow to exchange, like amides, a solution of
sodium carbonate in D2O, or NaOD may be used. The technique is demonstrated using n-butanol in
Spectra 7.1 and 7.2. Note the reduction in integration of the multiplet centred at 1.39 ppm.
3.5 3.0 2.5 2.0 1.5 1.0 0.5 ppm
1.
5
1.
0
1.
0
1.
0
Spectrum 7.2 n-Butanol in CDCl3 after shaking with two drops of D2O
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Further Elucidation Techniques – Part 1 103
R
O
CH3 R
OH
CH3
Structure 7.1 Keto-enol exchange.
Remember that any proton which is acidic enough is prone to undergo deuterium exchange. Methylene
protons alpha to a carbonyl for example, may exchange if left standing with D2O for any length of time,
as they can exchange via the keto-enol route (i.e., Structure 7.1).
Note that deuterium exchange of the -OH leads to incorporation of deuterium alpha to the carbonyl
in the ketone form. This may happen, even if there is no evidence of any enol signals in the spectrum
initially, i.e., it can occur even when the equilibrium is heavily in favour of the ketone. Aromatic protons
of rings which bear two or more -OH groups are also prone to undergo slow exchange, as are nitrovinyl
protons.
7.3 Basification and Acidification
This topic has been dealt with quite extensively in Section 6.6.6 so we won’t go over the material again
but there is perhaps one other type of problem that may be worth looking at with a view to solving by a
change of pH. Consider the two structures in Structure 7.2.
Whilst the preferred method of differentiating these structures would be by an NOE experiment, it
would be possible to accomplish this by running them in DMSO and then adding a drop of base to each
solution and re-running. (Note: DMSO is the preferred solvent for this experiment as both the neutral
and the charged species would be soluble in it.) In both cases, the phenoxide ion (Ar-O−) would be
formed and the extra electron density generated on the oxygen would feed into the ring and cause a
significan upfiel shift of about 0.3–0.4 ppm in any protons ortho- or para- to the hydroxyl group. In
the example above, the compound on the left would show such an upfiel shift for only a single doublet
(a), whilst the compound on the right would show an analogous upfiel shift for both a narrow doublet
(b) and a doublet of doublets (c).
Caution should be exercised if attempting any determination of this type as it is not the preferred
method and it is always safest if both compounds to be distinguished are available for study in this way.
OH
O
CH3
CH3
O
OH
CH3
CH3
bc
a
Structure 7.2 Compounds which show one or two upfield shifts.
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104 Essential Practical NMR for Organic Chemistry
7.4 Changing Solvents
If a signal of particular interest to you, is obscured by other signals in the spectrum, it is often worth
changing solvent – you might be lucky, and fin that your signal (or the obscuring signals) move
sufficientl to allow you to observe it clearly. You might equally well be unlucky of course, but it’s worth
a try.
Running a sample in an anisotropic solvent like D6-benzene or D5-pyridine, can bring about some
even more dramatic changes in chemical shifts. We tend to use benzene in a fairly arbitrary fashion, but
in some cases, there is a certain empirical basis for the upfiel and downfiel shifts we observe.
For example, benzene forms collision-complexes with carbonyl groups, ‘sitting’ above and below the
group, sandwich-style. When the carbonyl is held rigidly within the molecule, either because it forms
part of a rigid system, or because of conjugation, we can generally expect protons on the oxygen side of a
line drawn through the carbon of the carbonyl, and at right angles to the carbonyl bond to be deshielded.
Conversely, those on the other side of the line are shielded.
7.5 Trifluoroacetylation
This is quite a useful technique which can give a rapid, positive identificatio of -OH, -NH2, and -NHR
groups in cases where deuteration would be of little value. Even though the technique can be a little
time-consuming and labour-intensive in terms of sample preparation, it can nonetheless yield results in
less time than it would take to acquire definit ve 13C data – particularly if your material is limited.
Consider Spectrum 7.3. The bottom trace shows the ordinary spectrum of cyclohexanol, run in CDCl3.
Distinguishing it from chlorocyclohexane is not easy (without the use of 13C NMR) – the chemical shift
of the proton alpha to the functional group would be similar in both compounds, and in the case of the
alcohol, the -OH need not show coupling to it. Furthermore, in problems of this type, the -OH proton
itself may well be obscured by the rest of the alkyl signals or combined with the solvent water peak.
Integration of the alkyl multiplet before and after deuteration will not necessarily be very reliable, since
looking for 1 proton in a multiplet of 10 or 11, will give only a relatively small change in integral
intensity (and let us not forget that water in the CDCl3 which will absorb in this region, along with any
water that may be residual in the compound).
The top trace shows what happens when the sample is shaken for a few seconds with a few drops of
TFAA. The reaction shown in Structure 7.3 occurs.
The resultant spectrum is clearly very different from the alcohol, as the trifluoroaceti ester function
is far more deshielding with respect to the alpha proton than is the -OH group. A downfiel shift of
>1 ppm can be seen. This clearly distinguishes the alcohol from the analogous chloro compound which
would of course give no reaction.
This is a relatively quick and convenient technique, the reagent reacting quite readily (assuming no
great steric hindrance of course) with alcohols, primary and secondary amines. (Note the possibility of
complication if you react a secondary amine with TFAA – it will yield a tertiary amide!) If the reaction
is a little slow, as is often the case with phenolic -OH groups, you can ‘speed it up a little’ by gentle
warming, more shaking, and even adding a drop of D5-pyridine to base-catalyse the reaction.
Use of this reagent is however, somewhat limited. You can only use it in solvents which don’t
react with it (D4-methanol, and D2O are obviously out of the question), or contain a lot of water, i.e.,
D6-DMSO. Another slight drawback is that the cleaving of the anhydride liberates trifluoroaceti acid,
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Further Elucidation Techniques – Part 1 105
0.51.01.52.02.53.03.54.04.55.05.5 ppm
91
.27.
8
0.51.01.52.02.53.03.54.04.55.05.5 ppm
80
.77.
5
Spectrum 7.3 The use of TFAA to identify an -OH group.
which has nuisance value if your compound is very acid-sensitive, and will also protonate any unreacted
amine function present. If this salt-formation is a problem, it is worth adding sodium bicarbonate in
D2O, dropwise, to neutralise the acid. You’ll know when the excess TFA has been neutralised, as further
additions of bicarbonate fail to produce any further effervescence (shake thoroughly, and don’t forget to
release built up pressure by releasing carbon dioxide!) Dry your solution through an anhydrous sodium
sulfate filte before rerunning.
OH
O
F
F
F
O
F
F
F
O
+
O
O
F
F
F
+
O
OH
F
F
F
Structure 7.3 Using TFAA to identify an -OH group.
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106 Essential Practical NMR for Organic Chemistry
7.6 Lanthanide Shift Reagents
Unfortunately, the use of lanthanide shift reagents such as the europium compound, Eu(fod)3 is a
practise that has been largely consigned to the dustbin of history so we will say very little about them.
The problem with trying to use them in high-fiel spectrometers is that the fast relaxation times of
the collision complexes brought about by paramagnetic relaxation (courtesy of the europium or other
lanthanide atom), leads to severe line broadening. This paramagnetic broadening is very much worse in
high fiel spectrometers so if you are using a 250 MHz or above, don’t bother trying.
If, however, you are still soldiering on with a spectrometer of 100 MHz or less, then by all means try
using them to ‘stretch’ a spectrum out – if your compound is suitable. They work by coordinating with
an atom that has a lone pair of electrons available for donation. The more available the lone pair, the
greater will be the affinit (-NH2/NHR > -OH > >C=O > -O- > -COOR > -CN). Note that they will
only work in dry solvents that don’t contain available lone pairs. Good luck!
7.7 Chiral Resolving Agents
We have seen that the spectra of enantiomers, acquired under normal conditions, are identical. The NMR
spectrometer does not differentiate between optically pure samples, and racemic ones. The wording is
carefully chosen, particularly ‘normal conditions’, because it is often possible to distinguish enantiomers,
by running their spectra in abnormal conditions – in the presence of a chiral resolving agent. Perhaps
the best known of these is (–)2,2,2,trifluoro-l-(9-anthryl ethanol, abbreviated understandably to TFAE.
(W.H. Pirkle and D.J. Hoover, Top. Stereochem., 1982, 13, 263). Structure 7.4 shows its structure.
This reagent may form weak collision-complexes with both enantiomers in solution. As the reagent is
itself optically pure, these collision-complexes become ‘diastereomeric.’ That is, if we use (–)TFAE (note
that the (+) form can be used equally well), the complexes formed will be: (–)reagent – (+)substrate,
and (–)reagent – (–)substrate. These complexes often yield spectra sufficientl different to allow both
discrimination and quantificatio of enantiomers. This difference will be engendered largely by the
differing orientations of the highly anisotropic anthracene moieties in the two collision complexes.
You won’t be able to tell which is which by NMR, of course – that’s a job for polarimetry or circular
dichroism, but if you know which enantiomer is in excess, you can get a ratio, even in crude samples
which would certainly give a false reading in an optical rotation determination!
The use of TFAE is demonstrated in Spectrum 7.4, which shows the appearance of proton ‘b’, before
and after the addition of 30 mg of (+)TFAE to the solution. (This is the region of interest – it is usually
protons nearest the chiral centre, which show the greatest difference in chemical shifts in the pair of
F
F
F
H OH
Structure 7.4 Structure of TFAE.
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Further Elucidation Techniques – Part 1 107
7.5 7.0 6.5 6.0 5.5 5.0 4.5 4.0 3.5 3.0 2.5 2.0
Chemical Shift (ppm)
4.552.001.016.17
4.95 4.90 4.85 4.80 4.75 4.70 4.65 4.60 4.55 4.50 4.45 4.40 4.35 4.30 4.25 4.20 4.15 4.10 4.05 4.00
Chemical Shift (ppm)
1.01
4.95 4.90 4.85 4.80 4.75 4.70 4.65 4.60 4.55 4.50 4.45 4.40 4.35 4.30 4.25 4.20 4.15 4.10 4.05 4.00
Chemical Shift (ppm)
2mg substrate + 30mg +TFAE
NH2
OH
'b'
Spectrum 7.4 The use of TFAE as a chiral resolving agent.
complexes formed). The middle trace shows the expansion of proton ‘b’ prior to the addition of TFAE
and the top trace, its appearance after the addition of the reagent. It is clear from this trace that proton
‘b’ is no longer a simple X-part of an ABX system. Apart from shifting upfield it has broadened, and
eight lines are apparent. This is because the ‘b’ protons in the two collision complexes have slightly
different chemical shifts and we can now see them resolved from one another. (Clearly, this sample was
a racemate as the ratio of the resolved ‘X’ multiplets is 50/50.) This difference is often quite small, and
so as to exploit it to the full, experiments of this type are best performed at high fiel (e.g., 400 MHz or
more).
TFAE is a very useful reagent for this type of work, as it is very soluble in CDCl3, which is just as
well, as a considerable quantity of it is often needed to produce useful separations – even at high field
Its other advantage is that its own proton signals are generally well out of the way of the sort of substrate
signals you are likely to be looking at. It should be noted that the compound under investigation should
have at least one, and preferably two potentially lone pair donating atoms to facilitate interaction with
the reagent.
Another useful reagent of this type is ‘chiral binaphthol’ (see Structure 7.5).
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108 Essential Practical NMR for Organic Chemistry
OH
OH
Structure 7.5 (R)-(+)-1,1’-bi-2-naphthol
This is a member of an interesting class of compounds which are chiral, without actually containing
a define chiral centre. They are chiral because their mirror images are non-superimposable. In the case
of this molecule, there is no rotation about the bond between the two naphthol rings because of the
steric interaction between the two hydroxyl groups. ‘d’ and ‘l’ forms can be isolated and are perfectly
stable (Optical purity determination by ‘H NMR, D. P. Reynolds, J. C. Hollerton and S. A. Richards, in
Analytical Applications of Spectroscopy, edited by C. S. Creaser and A. M. C. Davies, 1988, p346).
Optically pure mandelic acid (see Structure 7.6) can be a useful chiral resolving agent where the
compound you are looking at has a basic centre, as it can form an acid-base pair with it, which is
a stronger form of association. This compound is of sparing solubility in CDCl3 however and can
precipitate out your compound if, as is often the case, its protonated form is of low solubility in CDCl3.
The technique of using resolving agents is obviously a useful one in following the synthesis of a
compound of specifie chirality. To summarise, we take our compound, which has a chiral centre of
unknown rotation and form some sort of complex by introducing it to a reagent of known optical purity.
The complexes we form have diastereoisoromeric character, which can give rise to a difference in the
chemical shifts of one or more of the substrate signals. This enables us to determine the enantiomer
ratio, either visually, or by integration, if we have sufficien signal separation.
In practise, if using one of these reagents to follow the course of a chiral separation, it is essential
to determine whether resolution is possible, by performing a test experiment either on a sample of
racemate, or at least a sample known to contain significan quantities of both enantiomers. Once useable
resolution has been established, the technique can be used to monitor solutions of unknown enantiomer
ratios with reasonable accuracy, down to normal NMR detection limits.
It is a good idea to keep the ratio of reagent to sample as high as possible. We recommend starting
with about 1–2 mg of compound in solution with about 10 mg of reagent. In this way, you can minimise
both the quantity of your sample and the amount of (expensive) reagent used. Keeping the initial
sample small has another advantage – it avoids line broadening associated with increased viscosity of
O
OH
OH
Structure 7.6 Mandelic acid.
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Further Elucidation Techniques – Part 1 109
very concentrated solutions, whilst at the same time leaving the option open for further increasing the
concentration of reagent, if needed.
One f nal point – the use of chiral resolving agents is restricted to nonpolar solvents, i.e., CDCl3
and C6D6, though combining these can sometimes augment separation. That just about concludes the
‘Chemical techniques’ section. As we’ve seen, some important types of problem can be tackled using
them, and if your sample is scarce, all is not lost – it can often be recovered, though this might take
some effort on your part. Deuterated samples can be back-exchanged by shaking with an excess of
water, trifluoroacetylate samples can be de-acetylated by base hydrolysis, and shift reagents can be
removed by chromatography. Now, we shall have a look at some of the most important ‘Instrumental
techniques’. . .
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