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Self-Imaging in Phase Space    295


               will allow us to extend the context of our discussion and further high-
               light the importance of the fractional Talbot.



          9.7 Matrix Formulation of the Fractional
                Talbot Effect
               In Sec. 9.6 we made no assumption regarding the groove shape of the
               grating structure to illustrate that the fractional Talbot effect can be
               expressed as a superposition of shifted and modulated copies of the
               grating’s transmission function.
                 We will now consider the case in which each period of the input
               function can be written as

                                            Q−1
                                            ,          qd
                              u p (x) = u int (x) ∗  a q   x −      (9.28)
                                                       Q
                                            q=0
               with Q being an integer number. We can interpret Eq. (9.28) as
               a sampling expansion with u int (x) defining the interpolation func-
               tion. In particular, with u int (x) = sinc(xQ/d), Eq. (9.28) turns into
               the well-known Shannon-Whitaker sampling theorem. For u int (x) =
               rect(xQ/d) we obtain a model most suitable to describe binary diffrac-
               tive optical elements or images with rectangular pixels.
                 We are again at liberty to explore Fresnel diffraction without speci-
               fying the interpolation function explicitly. It is sufficient to investigate
               Fresnel propagation of the discrete sampled version of the input func-
               tion. Given our discussion in Sec. 9.6, we expect to find fractional
               Talbot planes where the diffraction amplitude is described as a su-
               perposition of Q copies laterally shifted by a multiple of d/Q. This,
               in turn, implies that for an input function consisting of modulated
               functions at intervals d/Q, the output function also has to be a mod-
               ulated comb function with the same spacing between pulses. With
               the interpolation functions remaining unaffected, each period of the
               Fresnel diffracted wave can be expressed as

                                              Q−1
                                              ,          qd
                           u p (x, z M,N ) = u int (x) ∗  b q   x −  (9.29)
                                                          Q
                                              q=0
               In other words, we can solve the propagation problem by express-
               ing coefficients b q as a linear superposition of the coefficients a q .
               This, in turn, means we can interpret the a q and b q as vectors in a
                Q-dimensional vector space and determine a linear discrete trans-
               formation to relate both sets of coefficients. 14,15  The transformation
               matrix has to be a function of the respective Talbot coefficients which
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