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Rotations in Phase Space    99


               and as well as the HG mode can be associated with the point
               ( /2, 0) on the orbital Poincar´e sphere. By performing the appro-
               priate phase-space rotations, the entire sphere can be populated.
               The signal f  ,  at point ( ,  ) is characterized by the vector Q =
               (m xx −m yy )(sin   cos  , sin   sin  , cos  ),whichdefinesthesignalsym-
               metry. Thus signal with Q = (Q 1 , 0, 0) is better described in the Carte-
               sian coordinates; meanwhile for Q = (0, 0,Q 3 ) polar coordinates are
               the best choice for signal analysis. Moreover, in the last case the signal
                f 0,  possesses a longitudinal component of the OAM (m xx − m yy ).
                 Let us consider a signal f (x, y) presented as a superposition of the
               HG modes
                                 ,                  ,
                                                           2
                          f (x, y) =  a mn H mn (x, y)  |a mn | = 1  (3.98)
                                  m,n               m,n
               Based on the expressions for the signal second-order moments, 75  we
               derive its Q components.
                            ,                      ,
                                   2                      2
                       Q 0 =   |a mn | (m + n + 1) = 1 +  |a mn | (m + n)
                            m,n                    m,n
                            ,
                                   2
                       Q 1 =   |a mn | (m − n)
                            m,n

                                 ,
                       Q 2 = 2Re    a m,n+1 a  ∗  (m + 1)(n + 1)
                                          m+1,n
                                 m,n

                                 ,
                       Q 3 = 2Im    a m,n+1 a  ∗  (m + 1)(n + 1)    (3.99)
                                          m+1,n
                                 m,n
               We observe that Q 2 = Q 3 = 0 if in the signal decomposition Eq. (3.98)
               there are no subsequent terms a m,n+1 and a m+1,n . Moreover Q 3 = 0if
               the signal is real.
                 The stable beams that do not change their form under the propaga-
               tion in free space contain in the decomposition Eq. (3.98) only the HG
               modes with the same index sum m + n. Then since the signal decom-
               position is normalized, they have integer parameter Q 0 = m + n + 1,
               which is related to the Gouy phase of the beam.
                 If a signal corresponds to a circular harmonic c l (r, 
) [see Eq. ( 3.90],
                                                               l
               it has the same parameter Q = (0, 0,l) as the LG mode L .
                                                               p
                 Representing signals on the orbital Poincar´e spheres, we simplify
               the analysis and processing as well as the comparison with other sig-
               nals. Since the search of the CT T c is related to the diagonalization of
               the moment matrix, the signal presentation on the Poincar´e sphere is
               valid for coherent as well as partially coherent beams.
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