Chemistry 29b M. Walker
N.M.R. SPECTROSCOPY
1. Introduction
Nuclear Magnetic Resonance (NMR) is a property of the nucleus of an atom, concerned with what is known as nuclear spin (I). This is equivalent to the nucleus acting like a miniature bar magnet. Although isotopes can have a variety of values for I (including zero), the most useful for spectroscopy are those nuclei which have I = 1/2 . Fortunately this includes hydrogen-1 (1H), carbon-13, fluorine-19 and phosphorus-31, so that some of the commonest elements in organic chemistry can be analyzed using NMR.
When a nucleus with I = 1/2 is placed in a magnetic field, it can either align itself with the field (lower energy) or against it (higher energy). If radio waves are
applied, nuclei in the lower energy state can absorb the energy and jump to the higher energy state. We can observe either the absorption of energy, or the subsequent release of energy as the nucleus "relaxes" back to the lower energy state. Traditionally this was done by scanning slowly through a range of radio wave frequencies (this is called continuous wave, CW). However this has largely been replaced by the faster Fourier Transform (FT) method where one big, broad pulse of radio waves is used to excite all nuclei, then the results are analyzed by computer.
2. Chemical shift
In a real molecule, the effective magnetic field "felt" by a particular nucleus (Beff) includes not only the applied field B0, but also the magnetic effect of nearby nuclei and electrons. This causes the signal to absorb at a slightly different frequency than for a single atom; it is convenient to reference this resonant frequency to a standard (usually tetramethylsilane, TMS, defined as zero). The difference (in parts per million, ppm) is referred to as the chemical shift (
d). A typical range for d is around 12 ppm for 1H and around 220 ppm for 13C. It is customary to have the zero point at the right hand end of the spectrum, with numbers increasing to the left ("downfield") as shown in Fig. 2:</i>
It should be noted that the positions given in Fig. 2 may be only approximate, though for simple molecules they are fairly accurate. Where a wide range of d is observed, this is indicated by use of a double-headed arrow showing the range. Additional nearby electron-withdrawing groups will tend to move the signals downfield. Nearby p-bonds may move the signal either upfield or downfield, depending on orientation. In 13C spectra steric factors can have a major effect.
Exercise 1. Predict approximate chemical shifts for all the carbon and hydrogen atoms which are explicitly shown in the following molecules:
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3. Equivalence If two or more protons (or indeed with two or more carbons) are in an equivalent environment, then they will have the same chemical shift and appear as one signal. A common example of this is a CH3 group, where all three protons are always equivalent. In a CH2 group, the two protons are also equivalent, unless adjacent to a chiral center. Look for any plane of symmetry in the molecule, which will render the two halves equivalent. In the examples below, the different types of atom are given a subscript; atoms which are equivalent will have the same subscript.
Exercise 2. Predict how many peaks you would expect to see in the 1H and 13C NMR spectra of the following molecules:
4. Integration
A valuable aspect of 1H NMR is that the area under each peak is proportional to the number of hydrogens that are giving rise to that peak
* . A convenient way of analyzing these peak areas is to electronically "integrate" the peak, to convert the area into a distance. This distance is routinely printed onto a 1H NMR spectrum as a line, such that the vertical distance of the integration line is proportional to the number of hydrogens. We need to compare the ratios of these vertical distances, and from this we can find the ratio of the numbers of hydrogens. This ratio can be very helpful in determining the structure of an unknown substance using NMR, but be careful- integrations are only approximate!For example:
Cyclohexene
tert
-Butyl 2-hydroxy-2-methylpropanoateExercise 3: What is the ratio of the hydrogens in the following 1H spectrum?
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5. Coupling (1H only) As mentioned in section 2 above, the chemical shift is determined by Beff, which is affected by nearby nuclei and electrons. However, the nearby nuclei are themselves being excited to the higher energy state by the radio waves. It turns out that any particular 1H will spend about 50% of the time in the lower energy state, and about 50% of the time in the upper energy state. Consider two neighboring protons in the following system:
If we consider Beff for Ha, we will find that 50% of the time Hb will be increasing Beff for Ha (because Hb is aligned with the field), and 50% of the time Hb will be decreasing Beff for Ha (see above). The net result is that 50% of the signal for Ha will be shifted slightly downfield by Hb, while 50% of the signal for Ha will be shifted upfield by Hb. This process is called coupling, and it leads to a splitting of the signal into a doublet.
If now we turn to Hb, we will find that Ha has the exact same effect on Hb that Hb had on Ha. Thus the signal for Hb will be split by the same amount as Ha.
Now let us consider a more complicated system. If Ha has two neighboring Hb nuclei which are equivalent, the effect of these Hb nuclei may cancel out or not, as shown in the diagram below. This leads to the Ha signal being split into a triplet, with the three parts of the peak having areas in the ratio 1 : 2 : 1
(i.e., 25% : 50% : 25%). [However Hb will only be a simple doublet, as in the previous situation, because there is only one neighboring Ha affecting it.]
How do things work out in practice?
Consider the following examples:
A.
B.
Exercise 4. Predict the coupling patterns in the following molecules:
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6. Decoupling a 13C spectrum
Since 13C makes up only 1% of natural carbon, coupling between carbon atoms is rarely observed. However coupling by nearby hydrogens would very often make 13C spectra very hard to read, so we routinely use a technique called decoupling to eliminate all coupling effects from all hydrogens. This is done by blasting the sample with radio waves which excite in the 1H region (this scrambles all of the hydrogens), while observing in the 13C region. There is a price to pay: integration can no longer be done accurately. However there is also a benefit: the hydrogens transfer some of their energy to the carbons and this improves the otherwise feeble absorption of energy by the 13C nuclei. A side effect of this is that carbons which have no hydrogens attached to them tend to be considerably smaller than the other carbons, and such carbons can easily be identified in a 13C spectrum.
Therefore in a decoupled 13C spectrum we see no coupling (except in the CDCl3 solvent, which is split into three peaks by the deuterium). This means that each carbon gives rise to a single sharp peak, and in a clear 13C spectrum the total number of such peaks (excluding TMS and solvent) is equal to the number of types of carbon in the molecule.
7. Putting it all together: determining a structure from an NMR spectrum
Interpreting an NMR spectrum is a skill acquired through much practice, and there are few hard and fast rules since every spectrum is different. However there are a few general guidlines which are usually helpful. I personally follow this procedure:
Exercise 5. Try it out on these NMR spectra:
All spectra from the Sigma-Aldrich Handbook of FT-NMR Spectra.
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