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6.4 Atomic orbitals                       181
                                                                        7=2
                                                             1      Z
                                                                            2
                                                                                 2
                        j3d 2  2i  2 ÿ1=2 (j3d 2 i‡j3d ÿ2 i) ˆ            (x ÿ y )e ÿ( Zr=3a 0 )
                          x ÿ y
                                                         81(2ð) 1=2  a 0
                                                                                         (6:64d)
                                                             2 1=2     7=2
                                                                    Z
                           j3d xy i ÿi2 ÿ1=2 (j3d 2 iÿj3d ÿ2 i) ˆ         xye ÿ( Zr=3a 0 )  (6:64e)
                                                            81ð 1=2  a 0

                        In forming j3d 2  2i and j3d xy i, equations (A.37) and (A.38) were used. Graphs
                                     x ÿ y
                        of the square of the angular part of these ®ve real functions are shown in Figure
                        6.3 and the mathematical expressions are listed in Table 6.2.






                        Radial functions and expectation values
                        The radial functions R nl (r) for the 1s, 2s, 2p, 3s, 3p, and 3d atomic orbitals are
                        shown in Figure 6.4. For states with l 6ˆ 0, the radial functions vanish at the
                        origin. For states with no angular momentum (l ˆ 0), however, the radial
                        function R n0 (r) has a non-zero value at the origin. The function R nl (r) has
                        (n ÿ l ÿ 1) nodes between 0 and 1, i.e., the function crosses the r-axis
                        (n ÿ l ÿ 1) times, not counting the origin.
                          The probability of ®nding the electron in the hydrogen-like atom, with the
                        distance r from the nucleus between r and r ‡ dr, with angle è between è and
                        è ‡ dè, and with the angle j between j and j ‡ dj is

                                                        2
                                                                  2 2
                                          2
                                     jø nlm j dô ˆ [R nl (r)] jY lm (è, j)j r sin è dr dè dj
                        To ®nd the probability D nl (r)dr that the electron is between r and r ‡ dr
                        regardless of the direction, we integrate over the angles è and j to obtain

                                                    ð 2ð
                                                  … …
                                                                 2
                                               2
                                       2
                                                                                         2
                                                                                 2
                           D nl (r)dr ˆ r [R nl (r)] dr  jY lm (è, j)j sin è dè dj ˆ r [R nl (r)] dr
                                                   0 0
                                                                                          (6:65)
                        Since the spherical harmonics are normalized, the value of the double integral
                        is unity.
                          The radial distribution function D nl (r) is the probability density for the
                        electron being in a spherical shell with inner radius r and outer radius r ‡ dr.
                        For the 1s, 2s, and 2p states, these functions are
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