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116   Applied Petroleum Geomechanics


          that after reaching the peak stress the strength decreases to a residual value
          determined by frictional sliding (Schöpfer et al., 2013). The difference
          between the peak and residual strengths is the stress drop (Fig. 3.25). At a
          high confining pressure, however, no stress drop occurs, and the rock is in
          elastic perfectly plastic deformation. The transition of the confining pressure
          at which no loss in strength occurs is a possible definition of the brittlee
          ductile transition (Schöpfer et al., 2013).
             Astudy by Singh et al. (2011), involving reanalysis of thousands of
          reported triaxial tests, has revealed the astonishing simplicity of the
          following equality: UCS z s crti (i.e., critical s 3 ) for the majority of rock
          types. In other words, the two Mohr circles referred to in Fig. 3.24 are
          touching at their circumference. The curvature of peak shear strength
          envelopes is more correctly described, so that few triaxial tests are
          required, only needed to be performed at low confining stress, to
          delineate the whole strength envelope. This simplicity does not of course
          apply to the case, where triaxial tests are required over a wide range of
          confining stress, to correct the envelope, usually to adjust to greater local
          curvature.
             Singh et al. (2011) basically modified the MohreCoulomb criterion
          by absorbing the critical state defined in Barton (1976) and then
          quantifying the necessary deviation from the linear form, using a large
          body of experimental test data. This modified MohreCoulomb
          nonlinear failure criterion may be written in the effective stress form as
          follows:
                                           2 sin 4
                           0    0                   0     0 2
                          s   s ¼ UCS þ           s   As              (3.47)
                           1    3                   3     3
                                          1   sin 4
          where A is an empirical constant for the rock type under consideration. Eq.
          (3.47) is the linear MohreCoulomb failure criterion (Eq. 3.41) except the
                       0 2
          last team  As . For 0   s   s , Singh et al. (2011) found that param-
                                        0
                                   0
                       3           3    crti
          eter A has the following form:
                                        1   sin 4
                                   A ¼                                (3.48)
                                       s 0 crti  1   sin 4
          where s crti is the critical effective confining stress and s crti z UCS.
                                                           0
                  0
             In the tensile stress area (i.e., s 3 < 0) in Fig. 3.24, the Griffith failure
          criterion described by a parabolic Mohr envelope can be used (refer to
          Section 3.4.9, Eq. (3.83) and Fig. 3.31 for details).
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