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Unit 18: Theory of Space Curves




                                                                                                Notes
                              L
                            =    x   x ds  Lr.
                                  2
                                     2
                                     2
                                 1
                              0
          Since the geometric mean of two numbers is  their arithmetic mean, it follows that
                                              1         1
                                                     2
                                           2
                                      A  r   (A   r )   Lr.
                                              2         2
          This gives, after squaring and cancellation of r, the inequality (14).
          Suppose now that the equality sign in (14) holds. A and r  have then the same geometric and
                                                          2
          arithmetic mean, so that A = r  and L = 2r. The direction of the lines g, g’ being arbitrary, this
                                   2
          means that C has the same “width” in all directions. Moreover, we must have the equality sign
          everywhere in (15). It follows in particular that
                                             2
                                                  2
                                                     2
                                      '
                                                            '2
                                           '
                                                        '2
                                  (x ,x   x x )  =  (x   x )(x  x ),
                                          2
                                      2
                                                        1
                                           1
                                                     2
                                                  1
                                                            2
                                    1
          which gives
                                                  2
                                      x 1     x 2    x  x 2 2    r.
                                                 1
                                      x ' 2  x ' 1  x  x '2 2
                                                 '2
                                                 1
          From the first equality in (15), the factor of proportionality is seen to be r, i.e.,
                                              '
                                                      '
                                         x   rx , x   rx .
                                              2
                                                      1
                                                 2
                                          1
          This remains true when we interchange x  and x , so that
                                                 2
                                           1
                                                  '
                                             x  rx .
                                                  1
                                              2
          Therefore, we have
                                             2
                                                   2
                                                2
                                            x   x  r ,
                                                2
                                             1
          which means that C is a circle.
          18.10 Summary
               A parametrized curve in Euclidean three-space e  is given by a vector function
                                                      3
          
                                       x(t) = (x (t), x (t), x (t))
                                                  2
                                                      3
                                              1
               that  assigns a  vector to every value  of a  parameter t in a  domain interval  [a, b].  The
               coordinate functions of the curve are the functions x (t). In order to apply the methods of
                                                         i
               calculus, we suppose the functions x (t) to have as many continuous derivatives as needed
                                            i
               in the following treatment.
               One of the most useful ways to parametrize a curve is by the arc length s itself. If we let
          
               s = s(t), then we have
                                      s’(t) = |x’(t)| = |x’(s)|s’(t),
               from which it follows that |x’(s)| = 1 for all s. So the derivative of x with respect to arc
               length is always a unit vector.
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