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               338                                                                               Electron Spin Resonance


                      H
               where Q is a constant with a value of about −25 G. Equa-  The difference between the allowed transitions shown
               tion (10) applies to protons bonded to any atom, except  in Fig. 8 is not changed from the first-order situation at
                    H
               that Q is dependent on the atom. It has been most exten-  constant magnetic field. However, in an actual ESR spec-
               sively tested for protons bonded to carbon and to a lesser  trometer the magnetic field is swept, and since the second-
               extent for protons bonded to nitrogen.            order correction term depends on the magnetic field, the
                 Although proton hyperfine interactions are by far the  “apparent” splitting will change in second order. This ob-
               most common in aromatic radicals, a great deal of in-  served apparent splitting will be larger than the actual hy-
               formation about spin densities can also be derived from  perfine splitting, and for the case of hydrogen atoms this
                                     13
                                        14
                                               17
                                            19
               hyperfine interactions with C, N, F, O, and so forth.  difference is about 2 G.
               The simple relation of Eq. (10) for protons does not gen-  The second-order effect on the hydrogen-atom spec-
               erally apply to these nuclei because the interactions of the  trum is a subtle one, in the sense that the nominal appear-
               unpaired spin with spin density on adjacent nuclei and  ance of the spectrum does not change. Generally in more
               with lone-pair π electrons must be considered.    complex paramagnetic systems additional lines in the ESR
                                                                 spectrum appear that are due to second-order effects in the
                                                                 energy-level diagram. These types of transitions must be
               V. SECOND-ORDER HYPERFINE EFFECTS                 identified in order to interpret a spectrum well enough to
                                                                 assign the structure of a radical. The “extra” lines that
               When the hyperfine coupling constants are large and the  commonly occur due to second-order hyperfine effects
               linewidth is small, second-order hyperfine effects must be  can be divided into two classes. One class arises from the
               considered to explain the observed spectra in many cases.  splitting of some of the degeneracies of the inner lines
               A simple example is the spectrum of a hydrogen atom.  of a hyperfine pattern involving several equivalent nuclei.
               The second-order effects in the hydrogen spectrum cause  The second class involves forbidden transitions where the
               a shift of the center of the spectrum to lower field and  nuclear spin selection rule is violated and transitions cor-
               cause the observed hyperfine splitting to be larger than  responding to 
m I =±1 are observed.
               the actual value for a field-swept spectrum. Second-order  In general, extra spectral lines due to the splitting of
               analysis is required because the hyperfine splitting of 507  the degeneracies of equivalent nuclei occur when the
               G is a significant fraction of the typical 3300-G magnetic  second-order hyperfine correction magnitude is greater
               field used to observe the spectrum. The second-order per-  than the linewidth. This has been observed only in liquid-
               turbation theory correction factor to the energy levels is  phase spectra. To second order, the transition energies for
               proportional to the square of the hyperfine coupling con-  a system with one unpaired electron and one type of de-
               stant divided by the observing field. This causes a second-  generate nuclei of nuclear spin I is given by
               order shift in two of the four hydrogen-atom energy levels,              2
                                                                                                      2
               as shown in Fig. 8. The two transition energies are in-  E n = gβH + AM I +  1 A   I(I + 1) − M ,  (11)

                                                                                                      I
               creased, so the entire spectrum is shifted to lower field due          2 gβH
               to this effect. For hydrogen atoms the shift is about 18 G,  where M I is the total nuclear spin quantum number for the
               which corresponds to a change in the apparent g factor of  set of equivalent nuclei. For n equivalent nuclei in general
                                                                       2
                                                                  2
               0.0108.                                            I  = M , so from Eq. (11) one can see that some splitting
                                                                       I
                                                                 ofthefirst-orderdegeneracywillresult.Anexampleofthis
                                                                 situation occurs for the trifluoromethyl radical in solution,
                                                                 where the first-order spectrum would predict four equally
                                                                 spaced lines with relative intensities of 1 : 3 : 3 : 1. Since
                                                                  A iso for  19 F is 145 G, which is a large value, second-
                                                                 ordereffects are observable. In the actual spectrumat suffi-
                                                                 ciently high resolution six lines are observed with relative
                                                                 intensities 1 : (1 : 2) : (1 : 2) : 1, where the (1 : 2) lines are
                                                                 two closely spaced lines whose splitting is due to second-
                                                                 order shifts. All lines are shifted slightly to low field, but
                                                                 different energy levels are shifted by different amounts,
                                                                 which leads to the additional splitting of about 9 G in this
                                                                 case.
                                                                   The other result of second-order hyperfine effects is to
               FIGURE 8 Schematic of the first- and second-order energy lev-
               els of a hydrogen atom, the first-order allowed ESR transitions,  mix the first-order wave functions as shown in Fig. 8 so
               and the first- and second-order spin wave functions. The magni-  as to partially allow some forbidden transitions that in-
                                       2
               tude of the second-order shift is A [4(gβH + g N β N H)] −1 .  volve flipping of nuclear spins. When the first-order wave
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