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10   Chapter One


               light can be written in the form

                                                
 t
                          
               r 1 + r 2  G 1  −iH  r 1 + r 2
                (r 1 , r 2 ) = 2  det G 1 exp −        t
                                        2 r 1 − r 2  −iH   G 2  r 1 − r 2
                                                                    (1.18)
               where we have chosen a representation that enables us to determine
               the Wigner distribution of such light in an easy way. The exponent
               shows a quadratic form in which a four-dimensional column vector
                      t
                              t t
               [(r 1 +r 2 ) , (r 1 −r 2 ) ] arises together with a symmetric 4×4 matrix. This
                                                                  t
               matrix consists of four real 2×2 submatrices G 1 , G 2 , H, and H , where,
               moreover, matrices G 1 and G 2 are positive definite symmetric. The
               special form of the matrix is a direct consequence of the fact that the
               cross-spectral density is a nonnegative definite Hermitian function.
               The Wigner distribution of such Gaussian light takes the form 20,21
                                            
 t        −1  t     −1
                            det G 1        r   G 1 + HG H    −HG 2    r
                                                       2
                W(r, q) = 4       exp −2               −1  t     −1
                            det G 2        q        −G H        G 2  q
                                                       2
                                                                    (1.19)
                 In a more common way, the cross-spectral density of general
               Gaussian light (with 10 degrees of freedom) can be expressed in the
               form
                                
                      t
                                              1
                       (r 1 , r 2 ) = 2  det G 1 exp −  (r 1 − r 2 ) G 0 (r 1 − r 2 )
                                              2
                                          t      1      t
                               × exp −  r 1  G 1 − i (H + H ) r 1
                                                 2
                                          t      1      t
                               × exp −  r 2  G 1 + i (H + H ) r 2
                                                 2

                                         t       t
                               × exp −  r i(H − H ) r 2             (1.20)
                                         1
               where we have introduced the real, positive definite symmetric 2 × 2
               matrix G 0 = G 2 − G 1 . Note that the asymmetry of matrix H is a mea-
               sure for the twist 22–26  of Gaussian light, and that general Gaussian
               light reduces to zero-twist Gaussian Schell-model light 27,28  if the
                                       t
               matrix H is symmetric, H−H = 0. In that case, the light can be consid-
               eredasspatiallystationarylightwithaGaussiancross-spectraldensity
                √
                             1
                                      t
               2 det G 1 exp[−  (r 1 − r 2 ) G 0 (r 1 − r 2 )], modulated by a Gaussian
                             2
                                                       t
               modulator with modulation function exp[− r (G 1 − iH) r]. We re-
               mark that such Gaussian Schell-model light (with nine degrees of
               freedom) forms a large subclass of Gaussian light; it applies, for in-
               stance, in
                                                   t
                  • the completely coherent case (H = H , G 0 = 0, G 1 = G 2 )
                  • the (partially coherent) one-dimensional case (g 0 = g 2 − g 1 ≥ 0)
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