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Rays and Waves    275



          8.11 Concluding Remarks
               The field estimates presented in this chapter were derived through the
               same generic procedure: an ansatz is substituted into the Helmholtz
               equation, leading to conditions that the functions in the ansatz must
               satisfy. Note, however, that an alternative procedure for deriving
               some of these results exists where, instead of using the (differential)
               Helmholtz equation, one considers an infinite succession of prop-
               agation integrals over infinitesimally short distances. For each in-
               finitesimally thin slice of space, the propagation integral amounts to a
               Rayleigh-Sommerfeld-like superposition of secondary waves, where
               for each of these waves the refractive index is approximated as that
               at the secondary source position. This description of wave propaga-
               tion is analogous to Feynman’s path integral formulation of quantum
               mechanics 48  as a “sum of all possible histories.” The ray-based esti-
               mates can then be obtained by approximating the integrals asymptoti-
               cally, where k is used as the asymptotic parameter. The position-based
               estimate in particular results from applying the method of stationary
               phase 49  to all the integrals. The resulting leading contribution to the
               field at a point is associated with a trajectory (or a set of trajectories) ar-
               riving at this point from the initial plane. The optical path length of this
               trajectory is stationary with respect to infinitesimal variations, so it sat-
               isfies Fermat’s theorem. These stationary paths are therefore the rays
               of geometrical optics. Since the method of stationary phase consists of
               approximating the rapidly varying phase as a quadratic polynomial
               around a stationary point, the short-wavelength limit studied here
               has something in common with the paraxial and quasi-homogeneous
               limits mentioned in Sec. 8.1: they all lead to field estimates consistent
               with ray optics through the quadratic approximation of phases inside
               integrals, so that these integrals can be approximated analytically.
                 The author acknowledges support from the National Science Foun-
               dation under grant 0449708, and from an anonymous donor under an
               internal grant from The Institute of Optics.



          References
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                2. R. K. Luneburg, Mathematical Theory of Optics, University of California Press,
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                3. A. Sommerfeld, Optics, Lectures on Theoretical Physics, vol. IV, Academic Press,
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                4. Yu. A. Kravtsov and Yu. I. Orlov, Geometrical Optics of Inhomogeneous Media,
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                5. Yu. A. Kravtsov and Yu. I. Orlov, Caustics, Catastrophes, and Wave Fields, 2d ed.,
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