Page 154 - Intro to Tensor Calculus
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               where κ (g) is called the geodesic curvature of the curve. In a similar manner it can be shown that  δu α
                                                                                                           δs
                                              α
                                                             α
               is a surface vector orthogonal to t . Let  δu α  = αt where α is a scalar constant to be determined. By
                                                      δs
                                           α β
               differentiating the relation a αβ t u = 0 intrinsically and simplifying we find that α = −κ (g) and therefore
                                                        δu α       α
                                                            = −κ (g) t .                             (1.5.113)
                                                        δs
               The equations (1.5.112) and (1.5.113) are sometimes referred to as the Frenet-Serret formula for a curve
               relative to a surface.
                   Taking the intrinsic derivative of equation (1.5.111), with respect to the parameter s, we find that

                                                  δT i   i  δt α  i  du β  α
                                                      = x α   + x α,β   t .                          (1.5.114)
                                                   δs      δs        ds
               Treating the curve as a space curve we use the Frenet formulas (1.5.13). If we treat the curve as a surface
               curve, then we use the Frenet formulas (1.5.112) and (1.5.113). In this way the equation (1.5.114) can be
               writteninthe form
                                                                       β α
                                                               α
                                                         i
                                                     i
                                                  κN = x κ (g) u + x i  t t .                        (1.5.115)
                                                         α          α,β
               By using the results from equation (1.5.71) in equation (1.5.115) we obtain
                                                                     i α β
                                                      i
                                                              i
                                                   κN = κ (g) u + b αβ n t t                         (1.5.116)
                      i
                                                                      α
               where u is the space vector counterpart of the surface vector u . Let θ denote the angle between the surface
                                                                             i
                       i
                                                i
               normal n and the principal normal N , then wehavethatcos θ = n i N . Hence, by multiplying the equation
               (1.5.116) by n i we obtain
                                                                  α β
                                                       κ cos θ = b αβ t t .                          (1.5.117)
                                                                                α
               Consequently, for all curves on the surface with the same tangent vector t ,the quantity κ cos θ will remain
               constant. This result is known as Meusnier’s theorem. Note also that κ cos θ = κ (n) is the normal component
               of the curvature and κ sin θ = κ (g) is the geodesic component of the curvature. Therefore, we write the
               equation (1.5.117) as
                                                                  α β
                                                        κ (n) = b αβ t t                             (1.5.118)
                                                                             α
               which represents the normal curvature of the surface in the direction t . The equation (1.5.118) can also be
               writteninthe form
                                                               α
                                                             du du β   B
                                                    κ (n) = b αβ     =                               (1.5.119)
                                                              ds ds    A
               which is a ratio of quadratic forms.
                   The surface directions for which κ (n) has a maximum or minimum value is determined from the equation
               (1.5.119) which is written as
                                                                  α β
                                                   (b αβ − κ (n) a αβ )λ λ =0.                       (1.5.120)
               The direction giving a maximum or minimum value to κ (n) must then satisfy

                                                                   β
                                                    (b αβ − κ (n) a αβ )λ =0                         (1.5.121)
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