Page 153 - Intro to Tensor Calculus
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               Another form of equation (1.5.104) is obtained by using the equation (1.5.83) together with the relation
                        σγ
               a αβ = −a   σα   βγ . It is left as an exercise to verify the resulting form

                                                  −Ka αβ = c αβ − a σγ b σγ b αβ .                   (1.5.106)

                   Define the quantity
                                                             1  σγ
                                                        H =   a  b σγ                                (1.5.107)
                                                             2
               as the mean curvature of the surface, then the equation (1.5.106) can be written in the form


                                                  c αβ − 2Hb αβ + Ka αβ =0.                          (1.5.108)

                                                         β
                                                      α
               By multiplying the equation (1.5.108) by du du and summing, we find
                                                     C − 2HB + KA =0                                 (1.5.109)

               is a relation connecting the first, second and third fundamental forms.


               EXAMPLE 1.5-2
                   In a two dimensional space the Riemann Christoffel tensor has only one nonzero independent component
               R 1212 . ( See Exercise 1.5, problem number 21.) Consequently, the equation (1.5.104) can be written in the
                      √    √
               form K ae 12 ae 12 = b 22b 11 − b 21 b 12 and solving for the Gaussian curvature K we find

                                                    b 22 b 11 − b 12 b 21  b  R 1212
                                               K =                =   =      .                       (1.5.110)
                                                   a 11 a 22 − a 12 a 21  a  a



               Surface Curvature
                                      α
                                           α
                                                                                     2
                                                                               i
                                                                           i
                                                                                  1
                   For a surface curve u = u (s),α =1, 2 lying upon a surface x = x (u ,u ),i =1, 2, 3, we have a two
                                                                                 du α
                                                                             α
               dimensional space embedded in a three dimensional space. Thus, if t =  is a unit tangent vector to
                                                                                  ds
                                         α
                                       du du β      α β
               the surface curve then a αβ    = a αβ t t =1. This same vector can be represented as the unit tangent
                                       ds ds
                                                                                           i
                                                                dx i                     dx dx j
                                             1
                                                   2
                                                                                                        j
                                      i
                                                             i
                                                                                                      i
                                           i
               vector to the space curve x = x (u (s),u (s)) with T =  . That is we will have g ij  = g ij T T =1.
                                                                 ds                      ds ds
                                                       i
                                 α
               The surface vector t and the space vector T are related by
                                                            i
                                                          ∂x du α    i α
                                                      i
                                                    T =          = x t .                             (1.5.111)
                                                                     α
                                                         ∂u α  ds
                                 α
                                                           α β
               The surface vector t is a unit vector so that a αβ t t =1. If we differentiate this equation intrinsically with
               respect to the parameter s, we find that a αβ t α δt β  =0. This shows that the surface vector  δt α  is perpendicular
                                                       δs                                    δs
                                          α
                                   α
               to the surface vector t . Let u denote a unit normal vector in the surface plane which is orthogonal to the
                             α                 α                      α β
               tangent vector t . The direction of u is selected such that   αβ t u =1. Therefore, there exists a scalar κ (g)
               such that
                                                         δt α      α
                                                            = κ (g) u                                (1.5.112)
                                                         δs
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