Page 20 - Phase Space Optics Fundamentals and Applications
P. 20

CHAPTER1





                                     Wigner Distribution



                                                        in Optics





               Martin J. Bastiaans
               Technische Universiteit Eindhoven, Faculteit Elektrotechniek
               Eindhoven, Netherlands





          1.1 Introduction
                            1
               In 1932 Wigner introduced a distribution function in mechanics that
               permitted a description of mechanical phenomena in a phase space.
                                                                    2
               Such a Wigner distribution was introduced in optics by Dolin and
               Walther 3,4  in the 1960s, to relate partial coherence to radiometry. A few
               years later, the Wigner distribution was introduced in optics again 5–11
               (especiallyintheareaofFourieroptics),andsincethen,agreatnumber
               of applications of the Wigner distribution have been reported.
                 While the mechanical phase space is connected to classical mechan-
               ics, where the movement of particles is studied, the phase space in
               optics is connected to geometrical optics, where the propagation of
               optical rays is considered. Whereas the position and momentum of a
               particle are the two important quantities in mechanics, in optics we are
               interested in the position and the direction of an optical ray. We will
               see that the Wigner distribution represents an optical field in terms of
               a ray picture, and that this representation is independent of whether
               the light is partially coherent or completely coherent.
                 We will observe that a description by means of a Wigner distribu-
               tion is, in particular, useful when the optical signals and systems can
               be described by quadratic-phase functions, i.e., when we are in the
               realm of first-order optics: spherical waves, thin lenses, sections of
               free space in the paraxial approximation, etc. Although formulated




                                                                        1
   15   16   17   18   19   20   21   22   23   24   25