After more than a century of study, the hydrogen atom still presents challenges and opportunities to theoretical as well as to experimental physicists. The discovery of the Lamb shift in the late nineteen forties, followed by the development of QED and the introduction of powerful new experimental techniques in the nineteen sixties and seventies, have preserved for hydrogen its central place in atomic physics. Part I of this book, a reprint of the work published in 1957, covers the period from the earliest days up to the late nineteen fifties. Part II, a collection of progress reports written by well-known specialists on hydrogen and hydrogen-like systems, presents the advances in theory and experiment that have occurred since that time.
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ATOMIC spectra furnish material for testing theories of atomic structure. Since hydrogen is the simplest kind of atom, the interpretation of its spectrum has been of the greatest interest to theorists, particularly since all but the most recent theories can be applied with mathematical rigour to the two-body problem which the hydrogen atom presents…
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IT had been known for over twenty-five years before Bohr’s theory that the Balmer lines were not single, but appeared to be close doublets under instruments of high resolving power There was, however, considerable disagreement as to the separation between the doublet peaks. It was particularly important to the early spectroscopists to know whether the doublet separation remained constant throughout the Balmer series, or whether it gradually decreased, since this is an important distinction in alkali spectra between the sharp and diffuse series on the one hand, and the principal series on the other. In fact, each Balmer line is a blend of sharp, principal and diffuse doublets. Complete resolution even in the most favourable case of Hα has not yet been achieved.
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PASCHEN’S study [102] of the lines of ionized helium, and, in particular, of the line 4686 Å (n = 4→ n = 3) was claimed to provide striking experimental support for Sommerfeld’s theory. The fine structure of the Balmer series, as far as it was resolved at that time, also supported the theory, and further weighty evidence came from measurements of X-ray fine structure. In the following sections we shall briefly review these lines of argument.
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THE selection rules of the new quantum theory allow electric dipole transitions between levels of the same n but since the probability of spontaneous transition depends on the cube of the frequency such transitions in hydrogen are exceedingly improbable. Stimulated transitions, on the other hand, may take place under quite small alternating electric fields of the appropriate frequency. Absorption and emission of energy by the atom are equally probable, so that a change in an assembly of atoms may only be detected if the two states between which transitions are taking place are unequally populated at the outset…
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THE confirmation by Lamb and Retherford of the inadequacy of the Dirac theory stimulated a re-examination of a theoretical problem to which only a very incomplete solution had so far been found: the problem of the interaction between charged particles and the electromagnetic field. We shall briefly refer to the problem as it presented itself in classical physics, and then (following Weisskopf [135]) notice the further difficulties which the quantum theory introduces. Finally we shall see how these difficulties have been circumvented by the new quantum electrodynamics, and how a small correction is thereby introduced to the energy levels predicted by Dirac’s theory. The new theory, however, is not a complete and logically satisfactory solution to the problems we shall state: a difficulty of principle remains now, as formerly.
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DEVIATIONS from the Dirac theory have now been found in the levels n = 1,2 and 3 of deuterium, n = 2 of tritium, and n = 2, 3 and 4 of He+ by optical spectroscopy. Shifts in the level n = 3 of hydrogen and n = 2 of He+ have been measured by radio-frequency spectroscopy.
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IT is well known that hyperfine structure in spectra arises from the interaction of nuclear magnetic dipoles and the magnetic field due to the electron cloud. In the case of hydrogen the interaction energy is appreciably greater than the natural width of the energy levels only in the case of the ground level and the abnormally narrow (metastable) 22S½ level. The hyperfine structure of both these levels has been measured with great precision by atomic beam magnetic resonance methods. The ground level in particular has been repeatedly examined by this technique, and also by the method of paramagnetic absorption of microwaves.
Calculation of the hyperfine structure requires knowledge of the magnetic moment of the proton. If this were a Dirac particle, its moment would be eh/4πMc (one nuclear magneton), which stands in conflict with the value 2.79275 nuclear magnetons measured by a variety of methods. This experimental value, used in the simplest hyperfine structure formula, leads to substantial agreement between experiment and theory. Even so, there remains a discrepancy of about 0.1 per cent, which is greatly in excess of the experimental errors. This discrepancy is closely related to the interactions which give rise to the Lamb shift, as we shall now see.
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THE system comprised of one electron and one positron can exist in bound states for times sufficiently long to allow the measurement of energy differences between them. Positronium*, as this substance is called, thus allows a further test of the theory of the two-particle atom. Details of the theory were worked out before there was experimental proof of the existence of positronium.
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