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August 18, 2010 11:36      9in x 6in     b985-ch09     Elementary Physical Chemistry





                               102                   Elementary Physical Chemistry

                               9.8. Structure, Transitions and Selection Rules

                               We have already mentioned that in a hydrogenic atom, the electron can have
                               three quantum numbers n, l,and m l . We must now also add m s .Thus,

                                                     n =1, 2,...
                                                     l =0, 1,... ,n − 1
                                                   m l =0, +1, −1, +2, −2,...
                                                   m s =+1/2, −1/2

                               Note that l cannot exceed n − 1, although it may be smaller.
                                                                                         2
                                                    2
                                  Each energy level is n -fold degenerate, meaning that there are n states
                               which have the same energy. This rule is true only for hydrogenic atoms
                               and does not apply to other atoms.


                               9.9. Many-Electron Atoms
                               The Schr¨odinger equation can only be solved exactly for hydrogenic atoms,
                               yielding exact analytic expressions for the wave-functions. In all other cases,
                               solutions are approximate.
                                  As a first approximation, one can think of the wave-function of the
                               atom as the product of the wave-functions of the individual electrons, i.e.

                                                    Ψ atom = ψ(1)ψ(2)ψ(3)...              (9.10)
                               where ψ(1) is the orbital of electron 1, ψ(2) the orbital of electron 2, etc. but
                               with nuclear charge that is modified by the presence of all other electrons.
                               This effective nuclear charge, Z eff , is the charge of the nucleus shielded by
                               the other electrons. Thus, the nuclear charge an electron “sees” is not the
                               actual charge, Z e (e being the absolute value of an electronic charge) but
                               Z e−σ = Z eff ,where σ is a shielding constant that can be approximated.
                                  The Z eff values are different for s, p, d, etc. orbitals. For example, the
                               s electron has greater penetration to the nucleus than the p electron; the
                               p electron has greater penetration than the d electron, etc. But there are
                               exceptions; for example, 4s precedes 3d.


                               9.10. Pauli Exclusion Principle
                               This Principle states that no more than two electrons can occupy the same
                               orbital. Actually, the Pauli Exclusion Principle really states that in an atom
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