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Unit 31: Joachimsthal's Notations




          Nevertheless, from the theory of ordinary differential equations, the following lemma showing  Notes
          the local existence of geodesics can be shown :
          Lemma 1: Given a surface X, for every point p = X(u, v) on X, for every non-null tangent vector
           
           v T (u,v)  (X) at p, there is some  > 0 and a unique curve  : ] –, [  E  on the surface X, such
                                                                    3
            
                                          
          that  is a geodesic, (0) = p, and ’(0) =  v.
                                                                                  
          To emphasize that the  geodesic  depends on the initial direction  v,  we often write (t,  v )
          instead of (t).
          The geodesics on a sphere are the great circles (the plane sections by planes containing the center
          of the sphere).
          More generally, in the case of a surface  of revolution (a surface generated by  a plane curve
          rotating around an axis  in the  plane  containing the  curve and  not meeting  the curve),  the
          differential equations for geodesics can be used to study the geodesics.


                 Example: The meridians are geodesics (meridians are the plane sections by planes through
          the axis of rotation: they are obtained by rotating the original curve generating the surface).

          Also, the parallel circles such that at every point p, the tangent to the meridian through p is
          parallel to the axis of rotation, is a geodesic.
          It should be noted that geodesics can be self-intersecting or closed. A deeper study of geodesics
          requires a study of vector fields on surfaces and would lead us too far.
          Technically, what is needed is the exponential map, which we now discuss briefly.
          The idea behind the exponential map is to parameterize locally the surface X in terms of a map
          from the tangent space to the surface, this map being defined in terms of short geodesics.
          More precisely, for every point p = X(u, v) on the surface, there is some open disk B  of center
                                                                              
          (0, 0) in   (recall that the tangent plane T (X) at p is isomorphic to  ), and an injective map
                  2
                                                                  2
                                            p
                                         exp  : B   X(),
                                            p
                                               
                                    
          such that for every  v B     with  v  0,
                                                   
                                          exp (v)   (1,v),
                                             p
                                                                    
          where  (t,v)   is the unique geodesic segment such that  (0,v)    p  and  (0,v) '   v.  Furthermore,
                                                                  
          for B  small enough, exp  is a diffeomorphism. It turns out that  exp (v)  is the point q obtained
                             p                                 p
                                      
          by “laying off” a length equal to  v  along the unique geodesic that passes through p in the
                  
          direction  v.
                                                   
                                       3
                                                         2
          Lemma 2: Given a surface X :   E , for every  v  0  in  , if
                                            
                                                  
                                                
                                          ( ,v) :] – , [ E 3
                                          
          is a geodesic on the surface X, then for every  > 0, the curve
                                          
                                       
                                       ( , v) :] – / , / [ E 3
                                              
                                                 
                                                   
                                         
                                                     
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