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Unit 30: Geodesic Curvature and Christoffel Symbols




                                                                                               Notes
          We can now compute K   (t),  and we get
                             N
                                                               2
                                                  
                   w cos   Fsin  2   (wcos   Fsin )sin   Esin 
          k (t)  =  L            2M                   N    .
           N
                      w E                  w 2           w 2
          We leave as an exercise to show that the above expression can be written as
                                       
                                    k (t)  = H + Acos 2+ B sin 2,
                                     N
                                                    
          where
                              GL – 2FM + EN
                          H =              ,
                                 2(EG – F )
                                       2
                              L(EG – 2F ) + 2EFM – E N
                                                 2
                                      2
                           A =
                                    2E(EG – F )
                                            2
                               EM – FL
                           B =         .
                              E EG – F 2
                          2
                       2
          Letting C =  A  B ,  unless A = B = 0, the function
                                     f() = H + Acos 2 + B sin 2
          has a maximum k  = H + C for the angles   and   + , and a minimum k  = H – C for the angles
                                                                    2
                        1
                                            0
                                                  0
                      3               A             B
            +  2   and   +   2  ,  where cos 2  =   C   and sin 2  =   C .
                                     0
                    0
                                                   0
           0
          The curvatures k  and k  play a major role in surface theory.
                             2
                        1
          Definition 1: Given a surface X, for any point p on X, letting A, B, H be defined as above, and C
               2
                  2
          =  A + B ,  unless A = B = 0, the normal curvature k  at p takes a maximum value k  and a
                                                                                 1
                                                      N
          minimum value  k   called principal curvatures at p,  where  k   = H  +  C  and  k  =  H  –  C.  The
                                                                          2
                                                            1
                         2
          directions of the corresponding unit vectors are called the principal directions at p.
                         k + k
          The average  H  =   1  2    of the principal curvatures  is called the  mean curvature,  and  the
                            2
          product K = k k  of the principal curvatures is called the total curvature, or Gaussian curvature.
                     1 2
          Observe that the principal directions   and  +     corresponding k  and k  are orthogonal.
                                                 2
                                         0
                                                                      2
                                                                 1
                                               
                                                     2
                                                             2
                                                         2
                                                 2
                                             2
             Notes   K = k k  = (H – C)(H + C) = H  – C  = H  – (A  + B ).
                          1 2
          After some laborious calculations, we get the following (famous) formulae for the mean curvature
          and the Gaussian curvature:
                              GL – 2FM + EN
                          H =              ,
                                 2(EG – F )
                                       2
                              LN – M 2
                           K =        .
                               EG – F 2
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