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Unit 30: Geodesic Curvature and Christoffel Symbols




          Introduction                                                                          Notes

          In this unit, we focus exclusively on the study of Geoderic Curvature. In this unit, we will go
          through the properties of the curvature of curves on a surface. The study of the normal and of the
          tangential components of the curvature will lead to the normal curvature and to the geodesic
          curvature. We will study the normal curvature, and this will lead us to principal curvatures,
          principal directions,  the Gaussian  curvature, and the  mean curvature.  In  turn, the  desire to
          express the geodesic curvature in terms of  the first fundamental form alone will lead to  the
          Christoffel symbols. The study of the variation of the normal at a point will lead to the Gauss
          map and its derivative, and to the Weingarten equations.

          30.1 Geodesic Curvature and the Christoffel Symbols

                                                                                    
          We showed that the tangential part of the curvature of a curve C on a surface is of the form k n .
                                                                                     g
                                                                                   g
          We now show that k  can be computed only in terms of the first fundamental form of X, a result
                           n
          first proved by Ossian Bonnet circa 1848.
          The computation is a bit involved, and it will lead us to the Christoffel symbols, introduced in
          1869.
               
          Since  n  is in the tangent space T (X), and since (X , X ) is a basis of T (X), we can write
                g
                                     p
                                                   u
                                                      v
                                                                  p
                                           
                                         k g  g n  = AX  + BX ,
                                                  u
                                                       v
          form some A, B  .
          However,
                                                   
                                         kn = k N + k g  g n ,
                                               N
          and since N is normal to the tangent space,
             .
                   .
          N X  = N X  = 0, and by dotting
              u
                     v
                                           
                                         k g  g n  = AX  + BX v
                                                  u
          with X  and X , since E = X u  .  X , F = X u  .  X , and G = X v  .  X , we get the equations:
                                                        v
                                            v
                                   u
                     v
               u
                                          
                                             .
                                         kn X  = EA + FB,
                                              u
                                          
                                             .
                                         kn X  = FA + GB.
                                              v
          On the other hand,
                             
                           kn  = X” = X u” + X v” + X (u’)  + 2X u’v’ + X (v’) .
                                                     2
                                                                    2
                                                         uv
                                                 uu
                                     u
                                                                 vv
                                           v
          Dotting with X  and X , we get
                            v
                      u
            
              .
          kn X  = Eu” + Fv” + (X uu  .  X )(u’)  + 2(X uv  .  X )u’v’ + (X vv  .  X )(v’) ,
                                      2
                                                              2
                                                          u
                                  u
                u
                                               u
            
          kn   .  Xv = Fu” + Gv” + (X uu  .  X )(u’) + 2(X uv  .  X )u’v’ + (X vv  .  X )(v’) .
                                      2
                                                               2
                                  v
                                               v
                                                           v
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