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Complex Analysis and Differential Geometry




                    Notes          and
                                                               g    = [ ; ] + [ ; ].
                                                                |
                                   From all this, we get
                                                             2[ ; ] = g   + g   – g  .
                                                                       |  |  |
                                   As before, the Christoffel symbols [ ; ] and    are related via the Riemannian metric by the
                                                                         
                                                                         
                                   equations
                                                                    g 11  g 12   1
                                                                         [ ; ].
                                                                                
                                                                    g 21  g 22 
                                   This seemingly bizarre approach has the advantage to generalize to Riemannian manifolds.
                                   30.2 Principal Curvatures, Gaussian Curvature, Mean Curvature


                                   We will now study how the normal curvature at a point varies when a unit tangent vector varies.
                                   In general, we will see that the normal curvature has a maximum value k  and a minimum value
                                                                                            1
                                   k , and that the corresponding directions are orthogonal. This was shown by Euler in 1760.
                                    2
                                   The quantity K = k k  called the Gaussian curvature and the quantity H = (k  + k )/2 called the
                                                                                                1
                                                                                                   2
                                                  1 2
                                   mean curvature, play a very important role in the theory of surfaces.
                                   We will compute H and K in terms of the first and the second fundamental form. We also classify
                                   points on a surface according to the value and sign of the Gaussian curvature.
                                   Recall that given a surface X and some point p on X, the vectors X , X  form a basis of the tangent
                                                                                      u
                                                                                         v
                                   space T (X).
                                        p
                                                   
                                   Given a unit vector  t  = X x + X y, the normal curvature is given by
                                                        u
                                                            v
                                                                 
                                                              k ( t ) = Lx  + 2Mxy + Ny ,
                                                                       2
                                                                                  2
                                                               N
                                   since Ex  + 2Fxy + Gy  = 1.
                                                    2
                                         2
                                   Usually, (X ,X ) is not an orthonormal frame, and it is useful to replace the frame (X ,X ) with an
                                                                                                       v
                                              v
                                                                                                     u
                                           u
                                   orthonormal  frame.
                                                                
                                   One verifies easily that the frame  (e ,e )  defined such that
                                                                  2
                                                                1
                                                                 X      EX  FX
                                                               1 e   u  ,  2 e   v  u  .
                                                                   E      E(EG F )
                                                                                 2
                                                                               
                                   is indeed an orthonormal frame.
                                                                                              
                                   With respect to this frame, every unit vector can be written as  t   cos  1 e   sin   2 e ,  and expressing
                                     
                                   (e 1,e )  in terms of X  and X , we have
                                       2
                                                   u
                                                         v
                                                              w cos   Fsin   E sin
                                                          t              X       X ,
                                                                                      v
                                                                            u
                                                                w E            w
                                                  2
                                   where w =  EG F .
                                                
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