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332 RESERVOIR COMPACTION, SUBSIDENCE AND WELL DAMAGE

                                                                        (11.7)

            where σ' is the effective stress tensor, α is a material parameter referred to as the
            effective stress coefficient, p is the fluid pressure in the pores, and I is the second
            order identity tensor.
              In considering finite, elastoplastic deformations and using the Kirchhoff total
            stress  tensor,  defined  by  in  the  balance  of  mechanical  energy  of  a  mixture  of
                                                      56
            incompressible solids and fluids, Borja and Alarcón  showed that the effective
            stress, is defined as
                                                                        (11.8)

                  f
            where τ =pI is a rational concept for effective stress. They showed that, since the
            fluid is assumed to be incompressible and has no shear strength, the component
            of  stress  in  the  fluid  phase,  does  not  perform  mechanical  work  on  the  system,
                                                     f
            which is a clear distinction from the partial stress τ . Thus, the effective stress is
            intuitive  and  provides  a  rational  and  convenient  framework  for  describing  the
            stress  within  a  saturated  solid.  Since  the  Kirchhoff  stress  will  be  used  below,
            note that it is defined with reference to the undeformed configuration, while the
            Cauchy stress is defined with respect to the deformed configuration.
                           61
              Nur and Byerlee  showed that for linear, isotropic theory of the mechanics of
            porous media, the effective stress can be defined and written exactly as:

                                                                        (11.9)


            where the term in parentheses is identified by the effective stress coefficient α of
            Equation  (11.7).  The  form  of  Equation  (11.9)  adopts  the  notation  proposed  by
                            62
            Zimmerman, et al.,  in which C  is the compressibility of the rock matrix and
                                       r
            C  is the compressibility of the bulk rock under the action of the confining stress
             bc
            in  a  drained  test.  In  an  analysis  of  the  linearized  theory  of  Biot 63–67  and  the
            development  of  solutions  to  problems  using  that  theory,  Rice  and  Cleary 68
            showed that while the effective stress law of Equation (11.9) occurs naturally in
            the equations of equilibrium, it arrives from the constitutive assumption, not from
            considering the pore pressure p in an analysis of equilibrium.
              In  the  development  that  follows  for  finite  deformation,  elastoplastic  finite
            element analysis, the effective stress law is taken to be:

                                                                       (11.10)

            where χ is an effective stress coefficient dependent upon saturation and surface
            tension between the pore fluid and solid. The coefficient χ is assumed to be 1.0
            for a fully saturated medium. It may be noted that the effective stress coefficient
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