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              Photoelectron Spectroscopy                                                                   67

              process 3 in Fig. 2 and, in a further extension of the above  valence orbitals and the vibrational structure of the cor-
              ideas, is called a “shake-off” process. Since the second  responding photoemission bands (Section II.G), shake-up
              electron is no longer bound, shake-off excitations lead to  structures in the valence region are more difficult to ob-
              a continuum. This corresponds to the continuum following  serve. Figure 3 shows an example where it was possible to
              discrete excitations in the optical spectrum of the ion.  detectashake-upstructure(indicated2h1p)bycomparison
                Examples of the processes discussed above are seen in  with the optical spectrum of the ion. A transition from the
              the photoemission spectrum of neon (Fig. 1a). The first  ion ground state M to this particular 2h1p state is allowed
                                                                               +
                                                                              0
              line appears at 21.6 eV, corresponding to photoionization  and leads to a strong band in the absorption spectrum of
              of one of the six 2p electrons. The second line, at 49 eV,  the ion. In the PE spectrum, which starts from M 0 instead
                                                                    +
              corresponds to photoionization of a 2s electron and the  of M , the 2h1p final state gives rise to only a weak struc-
                                                                    0
              third line, at 870 eV, to photoionization of a 1s electron.  ture. From the PE spectrum alone it would be difficult to
              On an enlarged intensity scale (Fig. 9) shake-up satellites  detect this weak structure as a result of an independent
              are seen at the high binding energy side of the Ne 1s line,  transition. Comparison with the UV spectrum of the ion,
              which result from transitions into 2h1p states. The lines  however, allows an unambiguous assignment.
              designated 3, 5, 6, and 7, for example, have been identified  In the examples shown, the shake-up transitions only
              as transitions into states where, in addition to the creation  lead to weak structures in the PE spectrum. This is a very
              of the 1s hole, a 2p electron is excited to 3p,4p,5p,  general observation. Only in special cases can shake-up
              and so on. In addition, a shake-off continuum underlies  satellites reach an intensity comparable to that of the main
              the high-energy part of the 1s shake-up spectrum. Shake-  line (see Section IV.D and Fig. 28). Why are shake-up tran-
              up satellites are especially common for the 2p spectra  sitions usually weak? In the FOA, transitions are allowed
              of metals with d-electrons, as for example in the Cu 2p  only when the initial and final states differ by one electron.
              spectrum of copper(II) oxide shown in Fig. 10a, and in  Transitions that involve more than one electron are forbid-
              the spectra of aromatic organic compounds where they  den. Since all 2h1p states differ from the initial state by at
              result from transitions between bonding and antibonding  least two electrons (Fig. 8), transitions from M 0 to 2h1p
              π-orbitals. Much weaker shake-up satellites have been  states (and also to shake-off states) are strictly forbidden
              reported for the σ → σ transitions in aliphatic organics.  in the FOA. Only transitions to final single-hole states are
                                ∗
                The appearance of shake-up structures is not restricted  allowed. When degenerate orbitals are counted only once,
              to the core region. Because of the close spacing of the  the number of lines or bands observable in a PE spectrum


































                     FIGURE 9  Shake-up satellites accompanying Ne 1s photoionization; hν = 1486.7 eV. [From Siegbahn, K. (1974). J.
                     Electron Spectrosc. 5, 34.]
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