Page 306 - Rock Mechanics For Underground Mining
P. 306

ENERGY, MINE STABILITY, MINE SEISMICITY AND ROCKBURSTS


                                        that the excavation boundary be traction free, for t > 0. Simplifying the expressions
                                        for the case   = 0, equations 10.58 and 10.59 yield
                                                                      3
                                                               A =−a p/4G
                                                                              a p/4G
                                                               B =−(1 − 2	) 1/2 3
                                        The expression for f (equation 10.57) then becomes

                                                   3
                                                                                                 3
                                            f = (−a p/4G) exp(−  0 T )[cos   0 T + (1 − 2	) 1/2  sin   0 T ] + (a p/4G)
                                                                                                     (10.60)
                                        The various partial derivatives of the function f required to establish displacement
                                        and strain components around the spherical opening are given by
                                                                       2

                                                      f =−(1 − 2	) 1/2 (a p/2G) exp(−  0 T ) sin   0 T  (10.61)

                                           f = [(1 − 2	)/(1 − 	)](ap/2G) exp(−  0 T )[cos   0 T − (1 − 2	) 1/2  sin   0 T ]
                                                                                                     (10.62)

                                        Since the radial displacement is given by
                                                                                2

                                                                u r = (1/r) f − (1/r ) f
                                        the strain components are given, for the spherically symmetric problem, by
                                                                        2
                                                                                           3

                                                      ε rr =−∂u r /∂r = (2/r ) f − (1/r) f − (2/r ) f  (10.63)

                                                                                     2
                                                                            3
                                                           ε 

 =−u r /r = (1/r ) f − (1/r ) f       (10.64)
                                        Thetotalstressesinthemediumareobtaineddirectlyfromtheinducedstrains,through
                                        application of the stress–strain relations and superposition of the field stresses; i.e.
                                                                  rr =    + 2Gε rr + p               (10.65)
                                                                 

 =    + 2Gε 

 + p                (10.66)
                                        where

                                                                     = ε rr + 2ε
                                        Introduction of the expressions for ε rr and ε 

 in equations 10.65 and 10.66, and sub-
                                        sequent substitution of the expressions for the function f and its derivatives (equations
                                        10.60, 10.61 and 10.62), produce, after some simplification

                                                        a    a             a   a   2a          1/2
                                                         3    
                 3    2
                                                  −  0 T
                                            rr = pe        −    cos   0 T +  +   −      (1 − 2	)  sin   0 T
                                                        r 3  r             r   r 3  r 2
                                                         3
                                                        a
                                               + p 1 −                                               (10.67)
                                                        r 3
                                                            	   a    a                	   a   a    a
                                                                      3  
                     3     2
                                            

 = pe −  0 T  −     +      cos   0 T +        −    +
                                                          (1 − 	) r  2r  3          (1 − 	) r  2r  3  r  2
                                                                #
                                                                          a
                                                                            3
                                               ∗       1/2
                                                (1 − 2	)  sin   0 T + p 1 +                          (10.68)
                                                                          2r 3
                                        288
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