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Complex Analysis and Differential Geometry




                    Notes          is also a geodesic, and

                                                                           
                                                                          
                                                                     
                                                                   (t,  v) =  ( t, v).
                                                                           
                                                          
                                   From lemma 2, for  v  0,  if  (1,v)  is defined, then
                                                          
                                                                       
                                                                     v    
                                                                     v ,      (1,v).
                                                                      v 
                                                                        
                                   This leads to the definition of the exponential map.
                                   Definition 2: Given a surface X :   E  and a point p = X(u, v) on X, the exponential map expp
                                                                  3
                                   is the map
                                                                   exp : U  X()
                                                                     p
                                   defined such that

                                                                           
                                                                       v    
                                                             exp (v)     v ,      (1,v),
                                                                p
                                                                          v 
                                                                           
                                                                                                            
                                                                                                    v
                                                                        2
                                   where  (0,v)    p  and U is the open subset of  (= T (X)) such that for every  v   0,      v ,      is
                                                                           p
                                                                                                         v  
                                                    
                                   defined. We let  exp (0) = p.  It is immediately seen that U is star-like. One should realize that in
                                                  p
                                   general, U is a proper subset of .
                                          Example: In the case of a sphere, the exponential map is defined everywhere. However,
                                                                                               
                                   given a point p on a sphere, if we remove its antipodal point –p, then  exp (v)  is undefined for
                                                                                              p
                                   points on the circle of radius .
                                   Nevertheless, expp is always well-defined in a small open disk.

                                   Lemma 3: Given a surface X :   E , for every point p = X(u, v) on X, there is some  > 0, some
                                                               3
                                   open disk B  of center (0, 0), and some open subset V of X() with p  V, such that the exponential
                                            
                                   map exp  : B  V is well defined and is a diffeomorphism.
                                          p
                                   A neighborhood of p on X of the form exp (B) is called a normal neighborhood of p.
                                                                     p
                                   The  exponential  map  can  be  used  to  define  special  local  coordinate  systems  on  normal
                                   neighborhoods, by picking special coordinates systems on the tangent plane.
                                   In particular, we can use polar coordinates (, ) on  . In this case, 0 <  < 2. Thus, the closed
                                                                              2
                                   half-line corresponding to  = 0 is omitted, and so is its image under exp . It is easily seen that in
                                                                                            p
                                   such a coordinate system, E = 1 and F = 0, and the ds  is of the form
                                                                             2
                                                                  ds  = dr  + G d .
                                                                              2
                                                                        2
                                                                    2
                                   The image under exp  of a line through the origin in   is called a geodesic line, and the image
                                                                               2
                                                    p
                                   of a circle centered in the origin is called a geodesic circle. Since F = 0, these lines are orthogonal.





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