Page 196 - Shigley's Mechanical Engineering Design
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                                                                                              Deflection and Stiffness  171
                                                  Combining the four terms gives the total strain energy

                                                                M dθ      F Rdθ       MF θ dθ     CF Rdθ
                                                                  2         2                        2
                                                                                                    r
                                                                           θ
                                                         U =          +          −           +                 (4–37)
                                                                2AeE       2AE          AE          2AG
                                               The deflection produced by the force F can now be found. It is
                                                              ∂U        M    ∂M          F θ R     ∂F θ
                                                          δ =     =              dθ +              dθ
                                                              ∂F       AeE   ∂F          AE    ∂F
                                                                         1 ∂(MF θ )       CF r R  ∂F r

                                                                    −              dθ +               dθ       (4–38)
                                                                        AE    ∂F           AG    ∂F
                                               This equation is general and may be applied to any section of a thick-walled circular
                                               curved beam with application of appropriate limits of integration.
                                                  For the specific curved beam in Fig. 4–12b, the integrals are evaluated from 0 to π.
                                               Also, for this case we find
                                                                                      ∂M
                                                                 M = FR sin θ             = R sin θ
                                                                                      ∂F
                                                                                      ∂F θ
                                                                 F θ = F sin θ            = sin θ
                                                                                      ∂F
                                                                                   ∂(MF θ )
                                                                       2    2                      2
                                                               MF θ = F R sin θ           = 2FR sin θ
                                                                                     ∂F
                                                                                      ∂F r
                                                                 F r = F cos θ            = cos θ
                                                                                      ∂F
                                               Substituting these into Eq. (4–38) and factoring yields

                                                       FR 2     π  2     FR     π  2     2FR     π  2
                                                   δ =         sin θ dθ +      sin θ dθ −        sin θ dθ
                                                       AeE  0            AE  0            AE   0
                                                                                         CF R     π  2
                                                                                       +          cos θ dθ
                                                                                          AG   0
                                                       π FR 2  π FR   π FR   πCF R    π FR 2   π FR   πCF R    (4–39)
                                                    =        +      −      +        =       −       +
                                                       2AeE    2AE     AE     2AG      2AeE    2AE     2AG
                                               Because the first term contains the square of the radius, the second two terms will be
                                               small if the frame has a large radius.
                                                  For curved sections in which the radius is significantly larger than the thickness, say
                                               R/h > 10, the effect of the eccentricity is negligible, so that the strain energies can be
                                               approximated directly from Eqs. (4–17), (4–23), and (4–25) with a substitution of Rdθ
                                               for dx. Further, as R increases, the contributions to deflection from the normal force
                                               and  tangential force becomes negligibly small compared to the bending component.
                                               Therefore, an approximate result can be obtained for a thin circular curved member as

                                                                      2
                                                                .   M
                                                             U =        Rdθ                   R/h > 10         (4–40)
                                                                    2EI

                                                                 ∂U .     1     ∂M
                                                              δ =    =        M      Rdθ      R/h > 10         (4–41)
                                                                 ∂F       EI    ∂F
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