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198                                                  Essentials of Physical Chemistry


                           TABLE 9.2
                           Nuclear Screening of the K Shell and a Partial
                           L Shell in Selected Elements
                           Element   Z     L a (eV)  l L a  (Å)  Z eff  KL screen
                           Sn        50    3.444     3.600   42.6904   7.3096
                           Cs        55    4.286     2.892   47.6302   7.3698
                           Nd        60    5.230     2.370   52.6147   7.3853
                           Tb        65    6.2728    1.977   57.6074   7.3926
                           Yb        70    7.4140    1.672   62.6417   7.3538
                           Re        75    8.6150    1.433   67.6641   7.3359
                           Hg        80    9.987     1.241   72.7103   7.2897
                           Rn        86    11.724    1.057   78.7851   7.3149
                           Th        90    12.966    0.956   82.8424   7.1576
                           Pu        94    14.279    0.868   86.9404   7.0560



              This can be interpreted as the effective charge out of the bare nuclear charge of 49 that is not
            covered by the K shell and what there is of the L shell. Thus, (49   41.7057) ¼ 7.2943 so the clean
            formula of the one-electron Bohr atom is now muddled up with internal electron–electron repulsion
            and the idea that as the shell radius gets large the electrons get spread out more and cannot
            completely cover up the nuclear charge on a 1:1 basis. The same effect is almost constant across
            the periodic chart for the L a transitions from atomic number 49 (In) to the data for Pu (Z ¼ 94) as
            seen for selected elements in Table 9.2. This result also indicates that the electron giving off the
            x-ray energy is not falling into an empty L shell and that may be a function of how hard the atom
            was hit with the incoming electron, because this effective charge number indicates there are
            definitely some other electrons in the L shell. Assuming the number of electrons is an integer, the
            noninteger effective charge means that as the electrons move they cannot be everywhere at once.
            Thus, even if the electrons are very fast, both the K shell and what there is of the L shell cannot
            completely cover an integer amount of the nuclear charge. These considerations are useful to
            increase our appreciation of what is going on inside an atom. Historically, this is probably as far
            as one can push the Bohr model without including electron–electron repulsion and a better
            description of the orbitals but it is interesting to see that the K- and L-Auger transitions behave
            almost like the one-electron Bohr model when the model is adjusted for an effective nuclear charge.
              Although our short list implies that the average value of the screening might be 7.3, previous
            work by Moseley soon after 1913 preferred a value of 7.4 [6]. Mosely was a brilliant British chemist
            who was tragically killed in action in WWI at the Battle of Gallipoli at the age of 27. Some writers
            have said that Bohr’s shell model was not believed until the work of Mosely; note concurrent dates
            of discovery.

            X-RAY FLUORESCENCE

            While Auger processes do lead to x-ray emission, there is a variation in the technique that offers
            more sensitivity and generality. Overall, x-ray emission techniques are not as sensitive as some
            other analytical methods but offer simple sample preparation and simultaneous imaging of very
            small samples and elemental analysis. An application combining these advantages is the ability to
            check the elemental composition of doped microelectronic devices. Forensic samples such as shot or
            bullets offer an abundant sample size, so the element ratios within a strong signal is the desired
            information. These examples can use the Auger emission of the SEM beam or reduce the voltage to
            measure L a transitions. With the standard SEM method, scattered Auger electrons require a
            grounding connection to the sample in some cases to bleed off the secondary scattered electrons
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