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Spatiotemporal  Geometry                    49
        EXAMPLE 2.16:  The  Euclidean metric  in a rectangular coordinate system—see
        Equation  2.12—is obtained  from  Equation  2.17  by setting gy  =  Sij,  etc.



        COMMENT  2.5 : Assume   that   a   transformation   ca n b e established  from   a


        given  coordinate   system   {s^}   t o a  rectangular  coordinate   system   {s^},  an d

        let J   —  (dUi/dsi)  be   the  Jacobian   matrix   of   this   transformation.   Then,

        the matrix g = (gij)  o f  the Euclidean  metric   in  th e  {sj} coordinate   system

                               T
        can be  expressed  as  g  — J  J.

        EXAMPLE   2.17:  Consider the transformation  of systems from  cylindrical {sj}
        coordinates to  rectangular  {~s j}  coordinates in  Equation  2.7.  The  Jacobian is



        and,  hence, the  Euclidean metric  for  cylindrical  coordinates  is given by







        i-e., gn  =  933 =  1, 922  =  s\,  and g^  =  0 (i  =£  j),  which is the same  result
        as  that  obtained  in  Example 2.13.  Of  course,  other  (non-Euclidean)  metrics
        could  be considered for  the cylindrical  coordinate system, as well.

        COMMENT  2.6: Suppose   that   a  transformation  between   a  system  o f gener-


        alized curvilinear  coordinates  {s^}   and   an   underlying   system   of   rectangular

        coordinates  {¥,} exists.  Then,   th e metric  coefficients   ca n  be expressed  a s




            In  Equation  2.16  above we  used  the  metric  coefficients g^  to  represent
        the  coefficients  in  the  distance  \ds\  for  a  general  coordinate  system.  The
        metric  coefficients g^  play  an  important  role  in  several  other  operations  of
        spatiotemporal  geometry  related to  the  modeling  of  natural  phenomena, such
        as  the  determination  of  a  suitable  metric  (the  issue  is  discussed  also  in  the
        section  entitled  "Restrictions  on spatiotemporal  geometry  imposed by physical
        laws"  on  p.  56).  The  gradient,  Laplacian,  and  divergence  operators  for  a
        scalar field X(p)  and a vector  field X(p)  can be expressed  in terms of  general
        curvilinear  coordinates as follows
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