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              Electron Spin Resonance                                                                     335

              where m S and m I refer to the electron and nuclear spin
              quantum numbers, respectively.
                If we examine Fig. 3 we see that only two of the four
              possible transitions are allowed, namely, those in which
              the nuclear spin does not change its orientation. The en-
              ergy difference between these two transitions is defined as
              the hyperfine constant, usually symbolized by A in units of
              megahertz (MHz) or gauss (G). Since 
m I = 0, the effect
              of the nuclear Zeeman term in the spin Hamiltonian will
              always cancel out for first-order spectral transitions. Thus,
              this term can be neglected in the Hamiltonian when one is
              considering only first-order spectra. However, it should be
              cautioned that if one considers spectra in which the per-
              turbation theory approach must be carried out to second
              order or if one considers spin relaxation, which will be
              discussed later, the full spin Hamiltonian must be used.
                Figure  4  shows  the  energy-level  diagram  based  on
                                                      N
              Eq. (8) for a hypothetical NH species where A and
                                       +
               H
                                                 H
                                            N
              A are assumed to be positive and A > A . Any sub-
              script refers to the location of the nucleus in the molecule.
              Figure 4 shows the energy levels of the spin system and  FIGURE 5 Stick diagram for an ESR spectrum of hypothetical
                                                                  +
              the allowed transitions between sets of two energy levels.  NH .
                                                                So that the actual ESR spectrum can be represented in a
                                                                simple way, a stick diagram is often used. Figure 5 shows
                                                                a stick diagram for hypothetical NH . Each line repre-
                                                                                              +
                                                                sents an observed ESR line. The stick diagram, looks like
                                                                half of the energy-level diagram, except that the separation
                                                                between lines in the actual spectrum is equal to the hyper-
                                                                fine constant rather than to some fraction of it. If no lines
                                                                overlap, the total number of lines is given by   n (2I n + 1).
                                                                  Aslightlymorecomplicatedsituationforhyperfinecou-
                                                                pling exists when several nuclei have the same coupling
                                                                constants.Suchnucleiarecalledequivalent.ConsiderCH 3
                                                                and CD 3  as examples; stick diagrams are shown in Figs. 6























              FIGURE 4 First-order hyperfine energy levels and allowed tran-
                                                H
                                            N
              sitions for a hypothetical NH radical with A > A > 0.  FIGURE 6 Stick diagram for an ESR spectrum of the CH 3 radical.
                                 +
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