Page 206 - Rock Mechanics For Underground Mining
P. 206

METHODS OF STRESS ANALYSIS

                                        Introducing equation 6.41,
                                                   %                   %              %
                                               e        T       e           T  0           T
                                             [q ] =   [B] [D][B][u ]dV +  [B] [  ]dV −   [N] [b]dV    (6.42)
                                                    V e                 V e            V e
                                        Examining each component of the RHS of this expression, for a triangular element
                                               &    T
                                        the term  [B] [D][B]dV yields a 6 × 6 matrix of functions which must be inte-
                                                V e
                                                                               &    T  0
                                        grated over the volume of the element, the term  [B] [  ]dV a6 × 1 matrix, and
                                                                                V e
                                        &    T
                                          [N] [b]dV a6 × 1 matrix. In general, the integrations may be carried out using
                                         V e
                                        standard quadrature theory. For a constant strain triangular element, of volume V e ,
                                        the elements of [B] and [N] are constant over the element, and equation 6.42 becomes
                                                      e
                                                               T
                                                                                   0
                                                                                           T
                                                                               T
                                                                       e
                                                    [q ] = V e [B] [D][B][u ] + V e [B] [  ] − V e [N] [b]
                                        In all cases, equation 6.42 may be written
                                                                                 e
                                                                            e
                                                                  e
                                                                         e
                                                                 [q ] = [K ][u ] + [f ]               (6.43)
                                                                                  e
                                        In this equation, equivalent internal nodal forces [q ] are related to nodal displace-
                                                                               e
                                               e
                                        ments [u ] through the element stiffness matrix [K ] and an initial internal load vector
                                                            e
                                          e
                                                                   e
                                        [f ]. The elements of [K ] and [f ] can be calculated directly from the element ge-
                                        ometry, the initial state of stress and the body forces.
                                        6.6.4 Solution for nodal displacements
                                        The computational implementation of the finite element method involves a set of
                                                                                                    e
                                                                              e
                                        routines which generate the stiffness matrix [K ] and initial load vector [f ] for all
                                        elements. These data, and applied external loads and boundary conditions, provide
                                        sufficient information to determine the nodal displacements for the complete element
                                        assembly. The procedure is illustrated, for simplicity, by reference to the two-element
                                        assembly shown in Figure 6.8.
                                          Suppose the applied external forces at the nodes are defined by
                                                              T
                                                           [r] = [r x1 r y1 r x2 r y2 r x3 r y3 r x4 r y4 ]
              Figure 6.8  A simple finite element
              structure to illustrate the relation be-
              tween nodal connectivity and con-
              struction of the global stiffness matrix.














                                        188
   201   202   203   204   205   206   207   208   209   210   211