Page 58 - Physical Principles of Sedimentary Basin Analysis
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40                  Linear elasticity and continuum mechanics

                                                           F
                                                  A
                                       dx
                                       θ
                                    h




                 Figure 3.2. A rectangular block is subjected to a tangential force F over its top surface with area A.
                 The shear force has moved the upper surface a distance dx relative to the lower fixed surface. The
                 height of the block is h.


                 Exercise 3.3 Show that the work needed to shear the block in Figure 3.2 by an angle θ is
                      1
                          2
                 W = Gθ V , where V = Ah is the volume of the block.
                      2


                                                3.4 Strain
                 We have seen that the strain of a stretched rod is ε = dl/l 0 , when the rod’s initial length
                 is l 0 and it is stretched a distance dl. A point x along the initial rod becomes displaced a
                 distance u(x) = xdl/l 0 by the stretching. Such a displacement function makes it possible
                 to obtain the strain locally by measuring the difference in displacement of two nearby
                 points. The strain at a position x along the rod is the difference in displacement between
                 two points x and x + dx relative to the distance dx separating the points, ε = (u(x +
                 dx) − u(x))/dx ≈ ∂u/∂x (assuming that dx is small). Notice that it is differences in
                 the displacement field that produce strain. For example, a constant displacement does not
                 result in any strain, only a pure translation. The use of a (scalar) displacement function to
                 obtain the strain can be generalized to three dimensions by use of the displacement vector
                 u i = u i (x 1 , x 2 , x 3 ), i = 1, 2, 3. The difference in displacement between two nearby points
                 separated by (dx 1 , dx 2 , dx 3 ) can now be written

                                      ∂u i
                                du i =   dx j
                                      ∂x j

                                       1  ∂u i  ∂u j   1   ∂u i  ∂u j
                                   =          +      +        −        dx j
                                       2  ∂x j  ∂x i   2   ∂x j  ∂x i

                                   = ε ij + R ij dx j .                              (3.8)

                 (Notice that the summation convention is used, where there is summation over all pairs
                 of equal indices.) The partial derivative ∂u i /∂x j has been rewritten as a sum of a
                 symmetric part
                                                 1     ∂u i  ∂u j
                                           ε ij =      +                             (3.9)
                                                 2  ∂x j  ∂x i
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