Beam and Fiber Optics by J. A. Arnaud

By J. A. Arnaud

Beam And Fiber Optics

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G. Toraldo Di Francia, Opt. Ada 1, 157 (1955). E. A. J. Marcatili and R. A. Schmeltzer, Bell Syst. Tech. J. 43, 1783 (1964). H. G. Booker and W. Walkinshaw, in "Meteorological Factors in Radio-Wave Propaga­ tion," p. 80. Physical Soc, London, 1946. S. Kawakami and J. Nishizawa, IEEE Trans. Microwave Theory Tech. MTT16, 814 (1968). D. W. Berreman, Bell Syst. Tech. J. 43, 1469 (1964); 44, 2117 (1965). K. C. Kao and G. A. Hockham, Proc. IEE London 113, 1151 (1966). W. G. French, A. D. Pearson, G. W.

34 The optical-wave equation follows from the substitutions t —> z, m/h —» /c(0), — eU(x)/h -» k(x) in the Schrödinger equation, using conven­ tional notations. 5 This analogy is for a given color of the ray or a given energy of the particle. Dynamical effects such as radiation pressure are not essential in principle to understand problems of linear propagation. They are often deemed too small to be of much interest in optics. 36"38 After a brief historical review, we shall discuss the dynamical aspects of light waves and compare them to those of matter waves.

20, 239 (1972). W. A. Gambling, D. N. Payne, and H. Matsumura, Electron. Lett. 8, 568 (1972). R. Kompfner, Appl. Opt. 11, 2412 (1972). S. E. Miller, E. A. J. Marcatili, and T. Li, Proc. IEEE 61, 1703 (1973). H. F. Taylor, / . Appl. Phys. 44, 3257 (1973). P. Kaiser, E. A. J. Marcatili, and S. E. Miller, Bell Syst. Tech. J. 52, 265 (1973). E. A. J. Marcatili, Bell Syst. Tech. J. 53, 645 (1974). J. A. Arnaud, Bell Syst. Tech. J. 53, 675, 1379 (1974). H. Kogelnik, in Proc. Symp. , p. 333. Polytech.

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