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               84                                                                               Photoelectron Spectroscopy


































               FIGURE 23 Scheme of a band structure showing the constraints
               imposed by simultaneous fulfillment of energy and momentum
               conservation.


               Consequently, energy distribution curves measured under
               differentpolarangles,butusingthesameexcitationenergy
               h ν, strongly depend on θ (Fig. 25). For two-dimensional
               lattices which occur in well-ordered adsorbates or in layer
                                                                 FIGURE 24 Energy distribution curves obtained with different ex-
               compounds, the band dispersion is only a function of k   ,
                                                                 citation energies from a InSb (100) surface under normal emission
               and the unknown change in the vertical component k ⊥ is
                                                                 (θ = 0 ). The binding energy is given with respect to the Fermi en-
                                                                     ◦
               of little importance in the analysis of the energy distri-  ergy. The photon energy is indicated on the right side. Lines are
               bution curves. For three-dimensional lattices a variety of  drawn to guide the eye only. [From Jung, Ch., and Bressler, P. R.
               methods has been developed to overcome the problems  (1996). Electron Spectrosc. 78, 503.]
               resulting from the change in k ⊥ . An experimentally deter-
               mined band structure of copper is shown in Fig. 26. The  the charge at the atom that holds the orbital. This sim-
               dashed lines show the results of theoretical predictions.  ple approximation was widely used in the early days of
               To derive the experimental band structure the polar angle  XPS. However, it is an oversimplification because it ne-
               θ and the excitation energy hν had to be varied. Because  glects not only the off-atom potential V (q B ) but also fi-
               of the latter, this kind of investigation depends on the use  nal state effects. A much better result is obtained when
               of synchrotron radiation.                         we use the method outlined at the end of Section II.B.
                                                                 From the proper combination of Auger kinetic energies
                                                                 and binding energies we can derive a close approxima-
               C. Atomic Charges
                                                                 tion to the relaxation contribution  R. Combination of
               In Section II.A we showed how core orbital energies can  Eqs. (14) and (12) allows us to take final state effects into
               be expressed in the point charge approximation (Eq. (9)].  account. We then derive quasi-experimental  ε i values
               By combining Eq. (9) with Eq. (8) we obtain       that can be used in connection with Eq. (9) and theoret-
                                                                 ically calculated atomic charges. An example of such a
                         E B (i) = k(A, i) q A +  V (q B )  (24)
                                                                 study is shown in Fig. 27. The numbers in the figure refer
                                                                 to the phosphorus compounds listed in Table VII, which
               which connects core electron binding energy shifts  E B
               with variations in atomic charges. The most drastic ap-  shows the experimental data (Auger kinetic energy shift
               proximation is to correlate binding energy shifts only with  and binding energy shifts relative to PH 3 ), the final state
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