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28   Chapter One



               It is not difficult to show now that M can be represented in the general
               form

                            10            cos ϑ     exp(i ) sin ϑ

                    M = Q 0      + Q                                (1.67)
                            01        exp(−i ) sin ϑ   − cos ϑ
               where the angles ϑ and   follow from the relations Q cos ϑ = Q 1 (with
               0 ≤ ϑ ≤  ) and Q exp(i ) sin ϑ = Q 2 + iQ 3 .
                 A phase-space rotator will only change the values of the angles ϑ
               and  , but does not change the invariants Q 0 and Q. To transform a
               diagonal matrix M with diagonal entries Q 0 + Q and Q 0 − Q into

               the general form (1.67), we can use, for instance, the phase-space ro-
                                                      1
                                    1
                                1
                                                   1
                                           1
               tating system 81  F(  , −  ) R(− ϑ) F(−  ,  ); see also Sec. 1.6.2
                                2   2      2       2  2
               and Eq. (1.48). Moreover, from Eq. (1.65), we easily derive 80  that
               for a separable fractional Fourier transformer F(  x ,   y ), Q 1 is an
               invariant and Q 2 + iQ 3 undergoes a rotation-type transformation:
               (Q 2 + iQ 3 ) o = exp[i(  x −   y )] (Q 2 + iQ 3 ) i . Similar properties hold
               for a gyrator G(
), for which Q 2 is an invariant and (Q 3 + iQ 1 ) o =
               exp(i2
)(Q 3 + iQ 1 ) i , and for a rotator R(−
), for which Q 3 is an
               invariant and (Q 1 + iQ 2 ) o = exp(i2
)(Q 1 + iQ 2 ) i .
               1.7.3 Symplectic Moment Matrix—The
                      Bilinear ABCD Law
               If the moment matrix M is proportional to a symplectic matrix, it can
               be expressed in the form 77
                                          −1        −1
                                        G          G H
                               M = m      −1        −1              (1.68)
                                      HG     G + HG H
               with m a positive scalar, G and H real symmetric 2 × 2 matrices, and
               G positive definite; the two positive eigenvalues of MJ are now equal
               to +m, and the two negative eigenvalues are equal to −m.
                 We recall that for a symplectic moment matrix, the input-output
                                 t
               relation M o = TM i T can be expressed equivalently in the form of the
               bilinear relationship
                     H o ± iG o = [C + D(H i ± iG i )][A + B(H i ± iG i )] −1  (1.69)

               This bilinear relationship, together with the invariance of det M, com-
               pletely describes the propagation of a symplectic matrix M through
               a first-order optical system. Note that the bilinear relationship (1.69)
               is identical to the ABCD law for spherical waves: for spherical waves
                                             −1
               we have H o = [C + DH i ][A + BH i ] , and we have only replaced the
               (real) curvature matrix H by the (generally complex) matrix H±iG.We
               are thus led to the important result that if matrix M of second-order
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