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74                    Finite Element Modeling and Simulation with ANSYS Workbench



              We conclude that the stiffness matrix for the simple beam element is

                                                 L
                                                   T
                                             k = ∫  B EI dx                            (3.10)
                                                      B
                                                 0
              Applying the result in Equation 3.10 and carrying out the integration, we arrive at the
            same stiffness matrix as given in Equation 3.5.


            3.4.3  Treatment of Distributed Loads
            To convert a distributed load into nodal forces and moments (Figure 3.12), we consider
            again the work done by the distributed load q

                                  L             L                  L
                                1             1      T         1
                           W q =  ∫ vxqxdx =    ∫ (Nu )  q xdx =  u T ∫ N T q xdx
                                    ()
                                                        ()
                                       ()
                                                                       ()
                                2             2                2
                                  0             0                  0
              The work done by the equivalent nodal forces (and moments) is
                                                           F 
                                                            q
                                                           i
                                                            
                                                            q
                                       1                  M    1
                                                            i
                                     =  [      i θ            =  uf
                                                                   T
                                 W f q   v i      v j   j θ  ]  q   q
                                       2                   F j   2
                                                          M q
                                                           j 
              By equating W q =  W f q , we obtain the equivalent nodal force vector as
                                                 L
                                             f q = ∫ N qx dx                           (3.11)
                                                    T
                                                      ()
                                                 0
            which is valid for arbitrary distributions of q(x). For constant q, we have the results shown
            in Figure 3.13. An example of this result is given in Figure 3.14.


                                                  q(x)
                                                               x
                                           i       L        j

                                           F i q             F j q

                                      M i q                   M j q
                                           i                j

            FIGURE 3.12
            Conversion of the distributed lateral load into nodal forces and moments.
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