|       Chapter 10   Approximate
  theories for solids with special shapes:  rods, beams, membranes, plates and shells       10.4 Exact solutions to simple problems involving
  elastic rods   This
  section lists solutions to various boundary and initial value problems
  involving deformable rods, to illustrate representative applications of the
  equations derived in Sections 10.2.2 and 10.2.3.   Specifically, we derive solutions for: 
   The natural frequencies and mode shapes for an
       initially straight vibrating beam;The buckling load for a vertical rod subjected
       to graviatational loading;The full post-buckled shape for a straight rod
       compressed by axial loads on its ends;Internal forces and moments in an initially
       straight rod that is bent and twisted into a helix;Internal forces, moments, and the deflected
       shape of a helical spring.       10.4.1 Free vibration of a straight
  beam without axial force   The
  figure illustrates the problem to be solved: an initially straight beam, with
  axis parallel to the    direction and principal axes of inertia
  parallel to    is free of external force. 
  The beam has Young’s modulus    and mass density   ,
  and its cross-section has area A and
  principal moments of area   .  Its ends may be constrained in various
  ways, as described in more detail below. 
  We wish to calculate the natural frequencies and mode shapes of
  vibration for the beam, and to use these results to write down the
  displacement    for a beam that is caused to vibrate with
  initial conditions   ,    at time t=0.   Mode
  shapes and natural frequencies: The physical significance of the mode shapes and natural frequencies
  of a vibrating beam can be visualized as follows: 
   Suppose that the
       beam is made to vibrate by bending it into some (fixed) deformed shape   ;
       and then suddenly releasing it.  
       In general, the resulting motion of the beam will be very
       complicated, and may not even appear to be periodic.However, there
       exists a set of special initial deflections   ,
       which cause every point on the beam to experience simple harmonic motion
       at some (angular) frequency   ,
       so that the deflected shape has the form   .The special
       frequencies    are called the natural frequencies
       of the beam, and the special initial deflections    are called the mode shapes.   Each mode shape has a wave
       number   ,
       which characterizes the wavelength of the harmonic vibrations, and is
       related to the natural frequency by   
 
   The mode shapes    have a very useful property (which is
       proved in Section 5.9.1):   
     The
  mode shapes, wave numbers and corresponding natural frequencies depend on the
  way the beam is supported at its ends. 
  A few representative results are listed below   Beam
  with  free ends: The wave numbers for each mode are given by the
  roots of the equation    The mode shapes are   
 where    are arbitrary constants.   Beam
  with pinned ends: The wave numbers for each mode are    The mode shapes are   ,
  where    are arbitrary constants   Cantilever
  beam (clamped at   ,
  free at   :   The wave numbers for each mode are given by the
  roots of the equation    The mode shapes are   
 where    are arbitrary constants.     Vibration
  of a beam with given initial displacement and velocity   The
  solution for free vibration of a beam with given initial displacement and
  velocity can be found by superposing contributions from each mode as follows   
 where   
     Derivation:  We will
  derive the equations for the natural frequencies and mode shapes of a beam
  with free ends as a representative example. 
  This is a small deflection problem and can be modeled using
  Euler-Bernoulli beam theory summarized in Section 10.3.2. 1.       The deflection of the beam must satisfy the equation
  of motion given in Sect 10.3.2   
 2.       The general solution to this equation (found, e.g.
  by separation of variables, or just by direct substitution) is   
 where the frequency and wave number must be related
  by    to satisfy the equation of motion. 3.       The coefficients    and the wave number    must be chosen to satisfy the boundary
  conditions at the ends of the bar.  
  For a beam with free ends, the boundary conditions reduce to   ,    at   .  Substituting the formula from (2) into the
  four boundary conditions, and writing the resulting equations in matrix form
  yields   
 4.       For a nonzero solution, the matrix in this equation
  must be singular.  This implies that
  the determinant of the matrix  is  zero, which gives the governing equation
  for the wave-number   
 5.       Since the equation system in (3) is now singular, we
  may discard any one of the four equations and use the other three to
  determine an equation relating    to   .  Choosing to discard the last row of the
  matrix, and taking the first column to the right hand side shows that   
 Solving this equation system shows that   .  Substituting these values back into the
  solution in step (2) gives the mode shape. 6.       To understand the formula for the vibration of a
  beam with given initial conditions, note that the most general solution
  consists of a linear combination of all
  possible mode shapes, i.e.   
 Formulas
  for    found by substituting   ,
  multiplying both sides of the equation by    and integrating over the length of the
  beam.   We know that   
 so
  the result reduces to   
 The
  formula for    is found by differentiating the general
  solution with respect to time to find the velocity, substituting   ,
  and then proceeding as before to extract each coefficient   .       10.4.2 Buckling of a column subjected
  to gravitational loading   The
  problem to be solved is illustrated in the figure.  A straight, vertical elastic cantilever
  beam with mass density    and elastic modulus    is clamped at its base and subjected to
  gravitational loading. The beam has length L, cross-sectional area A
  and principal moments of area   .  The straight, vertical rod is always an
  equilibrium configuration, but this configuration is stable only if   .   Our
  objective is to show that the critical buckling length is      A
  number of different techniques can be used to find buckling loads.  One of the simplest procedures (which will
  be adopted here) is to identify the critical conditions where both the
  straight configuration (with    ), and also the deflected configuration
  (with a small transverse deflection    ) are possible equilibrium shapes for the
  rod.   This
  problem can be solved using the governing equations for a beam subjected to
  large axial forces, listed in Section 10.3.3.    For the present case, we note that 1.       The external forces acting on the rod are   ,   ,
  where g is the gravitational
  acceleration; 2.       The acceleration is zero (because the rod is in
  static equilibrium) 3.       The equilibrium equations therefore reduce to              
 4.       These equations must be solved subject to the
  boundary conditions    
 5.       Integrating the second equation of (3) and using the
  boundary condition    at    reduces the first equation of (3) to   
 6.       Integrating this equation with respect to    and imposing the boundary condition    at    shows that   
 7.       This equation can be solved for    using a symbolic manipulation program, which
  yields   
 where
     are special functions called `Airy Wave
  functions of order zero’ 8.       The remaining boundary conditions are    at   ,
  and    at   .  Substituting (7) into the boundary
  conditions and writing the results in matrix form gives   
 where
     and    are Airy wave functions of order 1. 9.       For this system of equations to have a nonzero
  solution, the determinant of the matrix must vanish, which shows that    must satisfy   .  This equation can easily be solved
  (numerically) for   .  The smallest value of    that satisfies the equation is   . 10.   The buckling length follows as   
       10.4.3  Post-buckled shape of an initially
  straight rod subjected to end thrust   The
  figure illustrates the problem to be solved. 
  An initially straight, inextensible elastic rod, with Young’s modulus E, length L and principal in-plane moments of area     (with    ) is subjected to end thrust.  The ends of the rod are constrained to
  travel along a line that is parallel to the undeformed rod, but the ends are
  free to rotate.   We wish to calculate
  the deformed shape of the rod.   You
  are probably familiar with the simple Euler buckling analysis that predicts
  the critical buckling loads.  Here, we
  derive the full post-buckling solution.   The
  rod is assumed to bow away from its straight configuration as shown: the
  deflected rod lies in the plane perpendicular to   .  The basis    and the Euler angle    that characterize the rotation of the rod’s
  cross sections are shown in the picture; the remaining Euler angles are   .   Solution: Several possible equilibrium solutions may exist,
  depending on the applied load P. 1.       The straight rod, with    is always an equilibrium solution.  It is stable for applied loads   . 2.       For applied loads   ,
  with n an integer, there are n+1 possible equilibrium
  solutions.  One of these is the
  straight rod; the rest are possible buckling modes.  The shape of each buckling mode depends on
  a parameter    which satisfies   
 where K
  denotes a complete elliptic integral of the first kind   .  Note that K has a minimum value    at k=0,
  and increases monotonically to infinity as   .  The equation for    has no solutions for   ,
  and n solutions for   ,
  as expected.  If multiple solutions
  exist, only the solution with n=1
  is stable. 3.      
  The shape of
  the deformed rod can be characterized by the Euler angle   ,
  which satisfies   
 where sn(x,k)
  denotes a Jacobi-elliptic function called the `sine-amplitude:’ its second
  argument k is called the `modulus’
  of the function. 4.       The coordinates of the buckled rod can also be
  calculated.  They are given by   
 Here am(x,k)
  and cn(x,k) denote Jacobi elliptic
  functions called the `amplitude’ and `cosine amplitude’, and E(x,k) denotes an incomplete elliptic
  integral of the second kind   .  The shape of the deflected rod for the
  stable buckling mode (n=1) is shown
  in the figure above.   Derivation:  This
  is a large deflection problem and must be treated using the general equations
  listed in Sections 10.7-10.9. 
   The equilibrium
       equation    immediately shows that T=constant along the rod’s
       length.  The boundary conditions
       at the end of the rod give   ,
       so that the components of T
       in    follow as   .ÂSubstituting the
       expressions for    into the moment balance equations shows
       that    and   Finally, note that
       the curvatures are   ,
       and recall that   ,
       so that the angle    satisfies   This is the equation
       that governs oscillations of a pendulum, and its solution is well known.
       The equation is satisfied trivially by    (this is the straight configuration),
       and also by two one-parameter families of functions of the form   
 Here,    and    are parameters whose values must be
  determined from the boundary conditions. 
  The first of these two functions is called an `inflexional’ solution,
  because the curve has points where   .
   The second is called `non-inflexional’
  because it has no such points.  For the
  pendulum, inflexional solutions correspond to periodic swinging motion; the
  non-inflexional solution corresponds to the pendulum whirling around the
  pivot. 
   The bending moment
       must satisfy    at both ends of the rod, which requires
       that    at    and   .  Only the inflexional solution can
       satisfy these boundary conditions.  
       For this case, we have   
 The cosine amplitude cn is a periodic function (it
  is a generalized cosine) and satisfies    at   .  We may therefore satisfy the boundary
  conditions by choosing    and   .  This leads to the defining equations for   . 
   Finally, the formula
       for the coordinates follows by integrating    and    subject to boundary conditions    at    and    at s=0.Finally, the
       (global) stability of the various solutions can be checked by comparing
       their potential energy.       10.4.4 Rod bent and twisted into a
  helix   We
  consider an initially straight rod with Young’s modulus E and shear modulus   .  The cross-section of the rod has area   ,
  principal in-plane moments of inertia    and an effective torsional inertia   .  The 
  rod is initially straight and unstressed, and is then subjected to
  forces and moments on its ends to bend and twist it into a helical shape.  The geometry of the deformed rod can be
  characterized by: 1.      
  The radius r of the cylinder that generates the
  helix 2.      
  The number of
  turns per unit axial length    in the helix 3.      
  The helix angle
    ,
  which is related to n by    4.       The twist curvature   ,
  which quantify the distorsion induced by twisting the rod about its deformed
  axis.  For the rod to be in
  equilibrium,    must be constant. 5.      
  The stretch
  ratio   .  For the rod to be in equilibrium,    must be constant.   The
  geometry and forces in the deformed rod are most conveniently described using
  a cylindrical-polar coordinate system    and basis    shown in the figure.  In terms of these basis vectors, we may
  define 
   The tangent vector to the rod   The binormal vector is      In terms of these
  variables: 
   The internal moment in the rod is   The internal force
       in the rod is    For the limiting case of an inextensible rod, the
  quantity    should be replaced by an indeterminate axial
  force   .   The
  forces acting on the ends of the rod must satisfy    and    at    and       at s=0.   A
  variety of force and moment systems may deform the rod into a helical shape,
  depending on the twist and stretch.  An
  example of particular practical significance consists of a force    and moment    acting at s=L (with equal and opposite forces at s=0), where   
 This force system is
  statically equivalent to a wrench with force    and moment    acting at r=0.   Finally
  note that this analysis merely gives conditions for a helical rod to be in
  static equilibrium.  The configuration
  may not be stable.     Derivation   
   We take    at s=0,
       so that the cylindrical polar coordinates are related to arc-length by   .
       Note also that the basis vectors satisfy   ,   ,
       so that           
 
   The position vector of a point on the axis of
       the rod can be expressed as   ;The tangent vector follows as   ;By definition, the
       curvature vector is   ,
       which can be expressed in terms of the binormal vector as   ;The moment-curvature relations then give the
       internal moment   ;The equilibrium
       equation    shows that T=constant.  We may
       express this constant internal force vector in terms of its components
       as   The internal forces
       and moments must satisfy the moment equilibrium equation, which shows
       that   
 Taking the dot product of both sides of this
  equation with    shows that   .
  It then follows that    and   
 
   Finally, the
       force-stretch relation requires that   .  This equation can be solved together
       with the final result of (7) for the components of internal force in the
       rod.       10.4.5 Helical spring   The
  behavior of a helical spring can be deduced by means of a simple extension of
  the results in the preceding section. 
  We assume that the spring is made from a material with Young’s modulus
  E and shear modulus   .  The cross-section of the rod has principal
  in-plane moments of inertia    and an effective torsional inertia   .  The rod is assumed to be inextensible, for
  simplicity.  The geometry of the
  undeformed spring can be characterized as follows 
   The length of the
       rod L, radius    of the cylinder that generates the
       helix; the height    of the spring, the number of turns in
       the coil   ,
       and the helix angle   The variables characterizing the undeformed
       spring are related as follows   
 
   It is helpful to select a basis    to characterize the orientation of the
       initial spring. Since    we may select    and    arbitrarily. It is convenient to choose    and    to be parallel to the normal vector n and binormal vector b of the undeformed spring,
       respectively, which gives   The initial curvature components can be
       calculated from the condition that 
          and follow as   .   The
  end of the spring at s=0 is held fixed (so it cannot move or rotate).  The end of the spring at    is subjected to a combination of a force    and moment    which act at the axis of the helical
  coil.   The
  solution can be calculated in exactly the same way as the derivation in
  Section 10.3.5.  It can be shown  that 
   The spring remains
       helical: its deformed shape can be characterized by new values of r,    and    after deformation.The spring may tend
       to twist about the axis of the helix when it is subjected to load.  The twisting can be quantified by the
       change in cylindrical-polar coordinates of the point at s=L on the spring.  In the undeformed state, these
       are    ;
       after deformation, they are   .  The twisting can be characterized by
       the rotation     The point where the load is applied
       therefore displaces through a distance   ,
       and rotates through the angle    about the axis of the cylinder.The displacement and
       rotation are related to the rod’s length L, the coil radius r
       and helix angle    by   
 
   The vectors    and    after deformation are given by   .The curvatures after
       deformation follow as   The internal moment
       and force in the spring are related to the curvatures and external force
       and moment by   
   
 
   The external force
       and moment applied to the axis of the spring are related to the helix
       angle and coil radius before and after deformation by   
 8.       If the spring is subjected a prescribed force and
  moment, these equations can be solved for    and   ,
  and the results can be substituted into (3) to calculate the extension    and rotation    of the spring.  The results cannot be expressed in closed
  form for large shape changes.  If    and    are small, however, the relations can be
  linearized to yield   
 where
  the spring stiffnesses are   
       |