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Complex Analysis and Differential Geometry




                    Notes          or, equivalently,
                                                           E (t) = cos((t))E (t) + sin((t))E (t)
                                                            2
                                                                                    3
                                                                        2
                                                           E (t) = sin((t))E (t) + cos((t))E (t) .
                                                                        2
                                                            3
                                                                                   3
                                   From these two representations, we may derive an important formula:
                                                                        '
                                                             E (t) . E (t) = E (t) . E (t) –  '(t)
                                                              '
                                                                                  
                                                                             3
                                                              2
                                                                   3
                                                                        2
                                   Expressed in the form of differentials, without specifying parameters, this formula becomes:
                                                                 dE E  = dE E  – d.
                                                                          2
                                                                           3
                                                                    2
                                                                     3
                                   Since E (t) = T(t) × E (t), we have:
                                                   2
                                        3
                                                             E (t) . E (t) = [E (t), E (t), T(t)]
                                                                         '
                                                              '
                                                              2
                                                                              2
                                                                   3
                                                                         2
                                   or, in differentials:
                                                                 dE E  = –[dE ,E ,T] .
                                                                             2
                                                                   2
                                                                     3
                                                                           2
                                   More generally, if z(t) is a unit vector in the normal space at x(t), then we may define a function
                                   w(t) = –[z’(t), z(t),T(t)]. This is called the connection function of the unit normal bundle. The
                                   corresponding differential form w = –[dz, z,T] is called the connection form of the unit normal
                                   bundle.
                                   A vector function z(t) such that |z(t)| = 1 for all t and z(t) . x’(t) = 0 for all t is called a unit normal
                                   vector field along the curve x. Such a vector field is said to be parallel along x if the connection
                                   function w(t) = –[z’(t), z(t),T(t)] = 0 for all t. In the next section, we will encounter several unit
                                   normal vector fields naturally associated with a given space curve. For now, we prove some
                                   general theorems about such objects.
                                   Proposition 2. If E (t) and E (t) are two unit normal vector fields that are both parallel along the
                                                 2
                                                         2
                                   curve x, then the angle between E (t) and E (t) is constant.
                                                                     2
                                                              2
                                   Proof. From the computation above, then:
                                                       '
                                                      E (t)· (–E (t) × T(t)) = E (t)· (–E (t) × T(t)) –  '(t).
                                                                        '
                                                                                        
                                                                              2
                                                                        2
                                                       2
                                                             2
                                   But, by hypothesis,
                                                         '
                                                                            '
                                                        E (t)· (–E (t)xT(t)) = 0 = E (t)(–E (t) × T(t))
                                                               2
                                                         2
                                                                            2
                                                                                 2
                                   so it follows that ’(t) = 0 for all t, i.e., the angle (t) between E (t) and E (t) is constant.
                                                                                    2
                                                                                            2
                                   Given a closed curve x and a unit normal vector field z with z(b) = z(a),
                                   we define
                                                               1                   1
                                                      (x, z) =     [z'(t),z(t),T(t)]dt    [dz,z,T].
                                                              2                  2
                                   If z is another such field, then
                                                  1
                                                                 
                                   (x, z) – (x, z) =     [z'(t),z(t),T(t)] [z'(t),z(t),T(t)]dt
                                                  2
                                      1           1
                                                    
                                   =      '(t)dt    [ (b)   (a)].
                                      2         2
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