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Wigner Distribution in Optics   11


                  • the (partially coherent) rotationally symmetric case (H = hI,
                    G 1 = g 1 I, G 2 = g 2 I, G 0 = (g 2 − g 1 )I, with I the 2 × 2 identity
                    matrix)

                 Gaussian Schell-model light reduces to so-called symplectic Gaus-
                       21
               sian light, if matrices G 0 , G 1 , and G 2 are proportional to one another.
                                   −1
               Now G 1 = 
G, G 2 = 
 G, and thus G 0 = (
 −1  − 
)G, with G a real,
               positive definite symmetric 2 × 2 matrix and 0 < 
 ≤ 1. The Wigner
               distribution then takes the form


                                         
 t       −1        −1
                                        r   G + HG H     −HG      r
                            2
                 W(r, q) = 4
 exp −2 
             −1        −1
                                        q       −G H        G     q
                                                                    (1.21)
               The name symplectic Gaussian light (with six degrees of freedom) orig-
               inates from the fact that the 4 × 4 matrix that arises in the exponent of
               the Wigner distribution (1.21) is symplectic. We will return to symplec-
               ticity later in this chapter. We remark that symplectic Gaussian light
               forms a large subclass of Gaussian Schell-model light; it applies again,
               for instance, in the completely coherent case, in the (partially coherent)
               one-dimensional case, and in the (partially coherent) rotationally sym-
               metric case. And again, symplectic Gaussian light can be considered
               as spatially stationary light with a Gaussian cross-spectral density,
               modulated by a Gaussian modulator [cf. Eq. (1.20)], but now with the
               real parts of the quadratic forms in the two exponents described—up
               to a positive constant—by the same real, positive definite symmetric
               matrix G.


               1.3.4 Local Frequency Spectrum
               The Wigner distribution can be considered as a local frequency spec-
               trum; the marginals are correct


                    (r, r) =  W(r, q) dq  and    ¯  (q, q) =  W(r, q) dr

                                                                    (1.22)

               Integrating over all frequency values q yields the intensity  (r, r)of
               the signal’s representation in the space domain, and integrating over
               all space values r yields the intensity ¯  (q, q) of the signal’s repre-
               sentation in the frequency domain. To operate easily in the mixed rq
               plane, the so-called phase space, we will benefit from normalization
                                          −1
               to dimensionless coordinates W r =: r and Wq =: q, where W is a
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