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6

                                                    The hydrogen atom
















                             A theoretical understanding of the structure and behavior of the hydrogen atom
                             is essential to the ®elds of physics and chemistry. As the simplest atomic
                             system, hydrogen must be understood before one can proceed to the treatment
                             of more complex atoms, molecules, and atomic and molecular aggregates. The
                                                                                      È
                             hydrogen atom is one of the few examples for which the Schrodinger equation
                             can be solved exactly to obtain its wave functions and energy levels. The
                             resulting agreement between theoretically derived and experimental quantities
                             serves as con®rmation of the applicability of quantum mechanics to a real
                             chemical system. Further, the results of the quantum-mechanical treatment of
                             atomic hydrogen are often used as the basis for approximate treatments of more
                                                                            È
                             complex atoms and molecules, for which the Schrodinger equation cannot be
                             solved.
                               The study of the hydrogen atom also played an important role in the
                             development of quantum theory. The Lyman, Balmer, and Paschen series of
                             spectral lines observed in incandescent atomic hydrogen were found to obey
                             the empirical equation

                                                           1    1
                                                  í ˆ Rc     ÿ     ,     n 2 . n 1
                                                          n 2  n 2
                                                            1    2
                             where í is the frequency of a spectral line, c is the speed of light, n 1 ˆ 1, 2, 3
                             for the Lyman, Balmer, and Paschen series, respectively, n 2 is an integer
                             determining the various lines in a given series, and R is the so-called Rydberg
                             constant, which has the same value for each of the series. Neither the existence
                             of these spectral lines nor the formula which describes them could be explained
                             by classical theory. In 1913, N. Bohr postulated that the electron in a hydrogen
                             atom revolves about the nucleus in a circular orbit with an angular momentum
                             that is quantized. He then applied Newtonian mechanics to the electronic
                             motion and obtained quantized energy levels and quantized orbital radii. From

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