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8.1  Buckling                                             137



                                                                         2
                                                     P cr (  1mode  )     2  EI L
                                 This critical bucking load corresponds to the first mode shape.
                                            For the second mode, the beam shape is similar to an S-
                                 curve  as  shown  in  the  following  figure.    The  corresponding
                                 buckling load is,
                                                                         2
                                                     P cr (  2mode  )    4 2  EI L

                                                             E,  I
                                                                                       P


                                                             L

                                 For higher modes, the beam shapes behave in the same fashion but
                                 are more complicated.
                                            The example above contains only a single beam, deter-

                                 mination  of  its  mode  shapes  and  critical  buckling  loads  is  not
                                 difficult.  For a complicated structure with many beams and plates,
                                 the classical method cannot provide solution effectively.  The finite
                                 element method offers a convenient way to yield the mode shapes
                                 with critical buckling loads.  The method starts from deriving finite
                                 element equations for all elements in the structural model.  These
                                 element equations are in the algebraic form of,
                                                       M          K      0

                                                                                         
                                 where   is the  mass matrix;   is the stiffness  matrix;   is
                                                               K
                                        M
                                                                           
                                 the vector containing nodal unknowns; and     is the vector con-
                                 taining nodal accelerations.
                                            Then, the eigenvalue problem is solved from,
                                                         K  2      0
                                                               M
                                 where   denotes the natural frequency.  The equations above lead
                                 to the eigenvalues   and corresponding eigenvectors.  Details for
                                                    i
                                 finding the eigenvalues and eigenvectors can be found in advanced
                                 finite element textbooks, including the book written by the author.
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