By Daniel Kleppner (auth.), W. Hanle, H. Kleinpoppen (eds.)

ISBN-10: 1461339359

ISBN-13: 9781461339359

ISBN-10: 1461339375

ISBN-13: 9781461339373

W. HANLE and H. KLEINPOPPEN In 1919, within the first version of Atombau and Spektrallinien, Sommerfeld spoke of the significant quantity of knowledge which have been accumu­ lated in the course of the first interval of 60 years of spectroscopic perform. Sommer­ feld emphasised that the names of Planck and Bohr will be hooked up perpetually with the efforts that were made to appreciate the physics and the idea of spectral strains. one other interval of virtually 60 years has elapsed because the first version of Sommerfeld's recognized monograph. because the editors of this monograph, development in Atomic Spectroscopy, we suppose that the current interval is better characterised via the massive number of new spec­ troscopic equipment which were invented within the final many years. Spectroscopy has consistently been serious about the sphere of analysis on atomic constitution and the interplay of sunshine and atoms. the improvement of recent spectroscopic tools (i.e., new in comparison to the conventional optical equipment) has ended in many notable achievements, which, including the rise of task during the last many years, look as one of those renaissance of atomic spectroscopy.

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D2, 37 (1970). 26. U. Fano, J. Opt. Soc. Am. 65, 979 (1975); K. T. Lu and U. Fano, Phys. Rev. A 2, 81 (1970). 27. P. Esherick, Phys. Rev. A 15, 1920 (1977). 28. P. Esherick, J. J. Wynne, and J. A. Armstrong (to be published). 29. R. W. Solarz, C. A. May, L. R. Carlson, E. F. Worden, S. A. Johnson, J. A. Paisner, and L. J. , Phys. Rev. A 14, 1129 (1976). 30. J. R. Rubbmark, S. A. Borgstrom, and K. Bockasten, J. Phys. B 10,421 (1977). -JURGEN KLUGE 1. Introduction This chapter will concentrate on a special branch of the large field of optical spectroscopy, namely, the study of hyperfine structure (hfs) and isotope shift (IS) of short-lived isotopes.

Gallagher, R. M. Hill, and S. A. Edelstein, Phys. Rev. A 14, 744 (1976). 12. R. R. Freeman and D. Kleppner, Phys. Rev. A 14, 1614 (1976). 13. T. W. Ducas and M. L. Zimmerman, Phys. Rev. A 15,1523 (1977). 14. T. W. Ducas, M. G. Littman, R. R. Freeman, and D. Kleppner, Phys. Rev. Lett. 35, 366 (1975). 15. R. F. Stebbings, C. J. Latimer, W. P. West, F. B. Dunning, and T. B. Cook, Phys. Rev. A 12, 1453 (1975). 16. A. F. J. van Raan, G. Braum, and W. Raith, J. Phys. B 9, L173 (1976). 17. D. Herrick, J.

These are high-energy proton (or deuteron, or alpha particle) reaction, fission, and high-energy heavy ion reaction. Until now, only the first two of these methods have been used to produce short-lived isotopes for investigation by optical spectroscopy. The most powerful means for a large-scale production of neutrondeficient nuclei is spallation as induced by high-energy protons. However, the large energy deposited in the nucleus opens many reaction channels and a mixture of elements and isotopes is obtained.

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Progress in Atomic Spectroscopy: Part B by Daniel Kleppner (auth.), W. Hanle, H. Kleinpoppen (eds.)

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