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190                          The hydrogen atom










                                                ~
                                                ν                                     ¥
                             Figure 6.7 A typical series of spectral lines for a hydrogen-like atom shown in terms of
                             the wave number ~ í.


                               A typical series of spectral lines is shown schematically in Figure 6.7. The
                             line at the lowest value of the wave number ~ í corresponds to the transition
                             n 1 ! (n 2 ˆ n 1 ‡ 1), the next line to n 1 ! (n 2 ˆ n 1 ‡ 2), and so forth. These
                             spectral lines are situated closer and closer together as n 2 increases and
                             converge to the series limit, corresponding to n 2 ˆ1. According to equation
                             (6.83), the series limit is given by
                                                            ~ í ˆ R=n 2                        (6:85)
                                                                    1
                             Beyond the series limit is a continuous spectrum corresponding to transitions
                             from the energy level n 1 to the continuous range of positive energies for the
                             atom.
                                                                       2
                               The reduced mass of the hydrogen isotope H, known as deuterium, slightly
                                                                1
                             differs from that of ordinary hydrogen H. Accordingly, the Rydberg constants
                             for hydrogen and for deuterium differ slightly as well. Since naturally occurring
                             hydrogen contains about 0.02% deuterium, each observed spectral line in
                             hydrogen is actually a doublet of closely spaced lines, the one for deuterium
                             much weaker in intensity than the other. This effect of nuclear mass on spectral
                             lines was used by Urey (1932) to prove the existence of deuterium.




                             Pseudo-Zeeman effect
                             The in¯uence of an external magnetic ®eld on the spectrum of an atom is
                             known as the Zeeman effect. The magnetic ®eld interacts with the magnetic
                             moments within the atom and causes the atomic spectral lines to split into a
                             number of closely spaced lines. In addition to a magnetic moment due to its
                             orbital motion, an electron also possesses a magnetic moment due to an
                             intrinsic angular momentum called spin. The concept of spin is discussed in
                             Chapter 7. In the discussion here, we consider only the interaction of the
                             external magnetic ®eld with the magnetic moment due to the electronic orbital
                             motion and neglect the effects of electron spin. Thus, the following analysis
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