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G. Raithel, M. Fauth, and H. Walther, Phys. Rev. A 44, 1898 (1991); 47, 419 (1993); G. Raithel, H. Held, L. Marmet, and H. Walther, J. Phys. B 27, 2849 (1994); G. Raithel and M. Fauth, ibid. 28, 1687 (1995); R. C. Hilborn, L. R. Hunter, K. Johnson, S. K. Peck, A. Spencer, and J. Watson, Phys. Rev. A 50, 2467 (1994); E. Flöthmann, Ph.D. thesis, University of Bielefeld, 1994; R. Ubert, Ph.D. thesis, University of Bielefeld, 1995; E. A. Solov'ev, Zh. Éksp. Teor. Fiz. 82, 1762 (1982) [Sov. Phys. JETP 55, 1017 (1982)]; 85, 109 (1983) [58, 63 (1983)]; J. von Milczewski and T. Uzer, Phys. Rev. E 55, 6540 (1997); Related works are J. von Milczewski, G. H. F. Dierckson, and T. Uzer, Phys. Rev. Lett. 76, 2890 (1996); M. J. Gourlay, T. Uzer, and D. Farrelly, Phys. Rev. A 47, 3113 (1993); 48, 2508(E) (1993); J. von Milczewski, G. H. F. Diercksen, and T. Uzer, Int. J. Bifurcation Chaos Appl. Sci. Eng. 4, 905 (1994); D. Sadovskii and B. Zhilinskii, Phys. Rev. A 57, 2867 (1998).
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This work could straightforwardly be generalized to m ≠ 0 by allowing the initial wave function to be φ dependent. The classical trajectories would be approximately unchanged, though their weights and phases would be modified. See, for example, J. Goetz and J. B. Delos (listed in Ref. [4]); G. J. Kuik, A. Kips, W. Vassen, and W. Hogervorst, J. Phys. B 29, 2159 (1996); A. Kips, W. Vassen, W. Hogervorst, and P. A. Dando, Phys. Rev. A 58, 3043 (1998); A. Kips, Ph.D. thesis, Vrije Universiteit Amsterdam, 1999.
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This work could straightforwardly be generalized to m ≠ 0 by allowing the initial wave function to be φ dependent. The classical trajectories would be approximately unchanged, though their weights and phases would be modified. See, for example, J. Goetz and J. B. Delos (listed in Ref. [4]); G. J. Kuik, A. Kips, W. Vassen, and W. Hogervorst, J. Phys. B 29, 2159 (1996); A. Kips, W. Vassen, W. Hogervorst, and P. A. Dando, Phys. Rev. A 58, 3043 (1998); A. Kips, Ph.D. thesis, Vrije Universiteit Amsterdam, 1999.
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Ph.D. thesis, Vrije Universiteit Amsterdam
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This work could straightforwardly be generalized to m ≠ 0 by allowing the initial wave function to be φ dependent. The classical trajectories would be approximately unchanged, though their weights and phases would be modified. See, for example, J. Goetz and J. B. Delos (listed in Ref. [4]); G. J. Kuik, A. Kips, W. Vassen, and W. Hogervorst, J. Phys. B 29, 2159 (1996); A. Kips, W. Vassen, W. Hogervorst, and P. A. Dando, Phys. Rev. A 58, 3043 (1998); A. Kips, Ph.D. thesis, Vrije Universiteit Amsterdam, 1999.
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