Page 233 - PRINCIPLES OF QUANTUM MECHANICS as Applied to Chemistry and Chemical Physics
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224                      Systems of identical particles
                                                             á(1)á(2)
                                                             â(1)â(2)
                                                    2 ÿ1=2 [á(1)â(2) ‡ á(2)â(1)]

                             and one antisymmetric spin wave function
                                                    2 ÿ1=2 [á(1)â(2) ÿ á(2)â(1)]
                             where the factors 2 ÿ1=2  are normalization constants. When the spatial and spin
                             wave functions are combined, there are four antisymmetric combinations: a
                             singlet state (S ˆ 0)
                                          1 [ö a (1)ö b (2) ‡ ö a (2)ö b (1)][á(1)â(2) ÿ á(2)â(1)]
                                          2
                             and three triplet states (S ˆ 1)
                                                                  8
                                                                    á(1)á(2)
                                                                  <
                                    2 ÿ1=2 [ö a (1)ö b (2) ÿ ö a (2)ö b (1)]  â(1)â(2)
                                                                  :  ÿ1=2
                                                                    2    [á(1)â(2) ‡ á(2)â(1)]
                             These four antisymmetric wave functions are normalized if the single-particle
                             spatial wave functions ö n (r i ) are normalized. If the two fermions are in the
                             same state ö a (r i ), then only the singlet state occurs
                                               2 ÿ1=2 ö a (1)ö a (2)[á(1)â(2) ÿ á(2)â(1)]
                               The helium atom serves as a simple example for the application of this
                             construction. If the nucleus (for which Z ˆ 2) is considered to be ®xed in
                                                           ^
                             space, the Hamiltonian operator H for the two electrons is
                                                     " 2            Ze9 2  Ze9 2  e9 2
                                              ^            2    2
                                             H ˆÿ       (= ‡ = ) ÿ       ÿ      ‡              (8:54)
                                                                2
                                                           1
                                                    2m e             r 1    r 2   r 12
                             where r 1 and r 2 are the distances of electrons 1 and 2 from the nucleus, r 12 is
                             the distance between the two electrons, and e9 ˆ e for CGS units or
                             e9 ˆ e=(4ðå 0 ) 1=2  for SI units. Spin±orbit and spin±spin interactions of the
                             electrons are small and have been neglected. The electron±electron interaction
                             is relatively small in comparison with the interaction between an electron and a
                             nucleus, so that as a crude ®rst-order approximation the last term on the right-
                                                                                      ^
                             hand side of equation (8.54) may be neglected. The operator H then becomes
                             the sum of two hydrogen-atom Hamiltonian operators with Z ˆ 2. The
                             corresponding single-particle states are the hydrogen-like atomic orbitals ø nlm
                             discussed in Section 6.4. The energy of the helium atom depends on the
                             principal quantum numbers n 1 and n 2 of the two electrons and is the sum of
                             two hydrogen-like atomic energies with Z ˆ 2
                                                      2
                                                  m e Z e9 4     1  1              1   1
                                             ˆÿ               ‡      ˆÿ54:4eV       ‡
                                       E n 1 ,n 2            2    2                2    2
                                                    2" 2    n    n                n    n
                                                             1    2                1    2
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