Computational Geomechanics. Manuel Pastor

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Название Computational Geomechanics
Автор произведения Manuel Pastor
Жанр Физика
Серия
Издательство Физика
Год выпуска 0
isbn 9781118535301
Computational Geomechanics - Manuel Pastor
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o n normal upper Gamma equals normal upper Gamma Subscript w"/>

      It is of interest to note, as shown by Zienkiewicz (1982), that some typical soil constants are implied in the formulation. For instance, we note from (2.16) that for undrained behavior, when wi,i = 0, i.e. with no net outflow, we have (neglecting the last two terms which are of the second order).

normal d p equals minus italic upper Q alpha normal d bold epsilon Subscript italic i i

      or

normal d p equals minus italic upper Q alpha bold m Superscript normal upper T Baseline normal d bold epsilon

      and

StartLayout 1st Row normal d sigma Subscript italic i j Baseline equals normal d sigma Subscript italic i j Superscript double-prime Baseline minus italic alpha delta Subscript italic i j Baseline normal d p equals upper D Subscript italic ijkl Baseline normal d bold epsilon Subscript italic k l Baseline plus alpha squared upper Q normal d bold epsilon Subscript italic i j Baseline 2nd Row equals left-parenthesis upper D Subscript italic ijkl Baseline plus alpha squared upper Q delta Subscript italic i k Baseline delta Subscript italic j l Baseline right-parenthesis normal d bold epsilon Subscript italic k l EndLayout

      or

normal d bold sigma equals left-parenthesis bold upper D plus alpha squared bold m upper Q bold m Superscript normal upper T Baseline right-parenthesis normal d bold epsilon

      If the pressure change dp is considered as a fraction of the mean total stress change mT dσ/3 or dσii/3, we obtain the so‐called B soil parameter (Skempton 1954) as

StartLayout 1st Row upper B identical-to StartFraction minus 3 normal d p Over normal d sigma Subscript italic i i Baseline EndFraction equals StartFraction 3 italic alpha upper Q normal d bold epsilon Subscript italic k k Baseline Over upper D Subscript italic iikl Baseline normal d bold epsilon Subscript italic k l Baseline plus 3 alpha squared upper Q normal d bold epsilon Subscript italic k k Baseline EndFraction 2nd Row upper B identical-to StartFraction minus 3 normal d p Over bold m Superscript normal upper T Baseline normal d bold sigma EndFraction equals StartFraction 3 italic alpha upper Q bold m Superscript normal upper T Baseline normal d bold epsilon Over bold m Superscript normal upper T Baseline left-parenthesis bold upper D plus alpha squared bold m upper Q bold m Superscript normal upper T Baseline right-parenthesis normal d bold epsilon EndFraction EndLayout StartLayout 1st Row upper D Subscript italic ijkl Baseline equals left-parenthesis upper K Subscript upper T Baseline minus two thirds mu right-parenthesis delta Subscript italic i j Baseline delta Subscript italic k l Baseline plus mu left-parenthesis delta Subscript italic i k Baseline delta Subscript italic j l Baseline plus delta Subscript italic i l Baseline delta Subscript italic j k Baseline right-parenthesis 2nd Row upper B equals StartFraction 3 italic alpha upper Q normal d epsilon Subscript italic k k Baseline Over left-parenthesis left-parenthesis 3 upper K Subscript upper T Baseline minus 2 mu right-parenthesis delta Subscript italic k l Baseline plus 2 italic mu delta Subscript italic k l Baseline right-parenthesis normal d epsilon Subscript italic k l Baseline plus 3 alpha squared upper Q normal d epsilon Subscript italic k k Baseline EndFraction 3rd Row equals StartFraction italic alpha upper Q Over upper K Subscript upper T Baseline plus alpha squared upper Q EndFraction equals StartFraction alpha Over left-parenthesis upper K Subscript upper T Baseline slash upper Q right-parenthesis plus alpha squared EndFraction 4th Row upper B equals StartFraction 3 italic alpha upper Q bold m Superscript upper T Baseline bold m Over bold m Superscript upper T Baseline left-parenthesis bold upper D plus alpha squared bold m upper Q bold m Superscript upper T Baseline right-parenthesis bold m EndFraction equals StartFraction 9 italic alpha upper Q Over bold m Superscript upper T Baseline bold upper D m plus 9 alpha squared upper Q EndFraction 5th Row equals StartFraction 9 italic alpha upper Q Over 9 upper K Subscript upper T Baseline plus 9 alpha squared upper Q EndFraction equals StartFraction italic alpha upper Q Over upper K Subscript upper T Baseline plus alpha squared upper Q EndFraction equals StartFraction alpha Over left-parenthesis upper K Subscript upper T Baseline slash upper Q right-parenthesis plus alpha squared EndFraction EndLayout

      where KT is (as defined in equation (1.10), the bulk modulus of the solid phase and μ is once again Lamé’s constant. B has, of course, a value approaching unity for soil but can be considerably lower for concrete or rock. Further, for unsaturated soils, the value will be much lower (Terzaghi 1925; Lambe and Whitman 1969; Craig 1992).

      2.2.2 Simplified Equation Sets (u–p Form)

      The governing equation set (2.11), (2.13), and (2.16) together with the auxiliary definition system can, of course, be used directly in numerical solution as shown by Zienkiewicz and Shiomi (1984). This system is suitable for explicit time‐stepping computation as shown by Sandhu and Wilson (1969) and Ghaboussi and Wilson (1972) and later by Chan et al. (1991). However, in implicit computation, where large algebraic equation systems arise, it is convenient to reduce the number of variables by neglecting the apparently small (underlined) terms of equations (2.11) and (2.13). These contain the variable wi(w) which now can be eliminated from the system.

      The first equation of the reduced system becomes (from (2.11))

      (2.20a)sigma Subscript italic i j comma j Baseline minus rho ModifyingAbove u With two-dots Subscript i Baseline plus rho b Subscript i Baseline equals 0

      or

      (2.20b)bold upper S Superscript normal upper T Baseline bold sigma minus rho ModifyingAbove bold u With two-dots plus rho bold b equals 0

      The second equation is obtained by coupling (2.13) and (2.16) using the definition (2.14) and thus eliminating the variable wi(w). We now have, omitting density changes

      (2.21a)left-parenthesis k Subscript italic i j Baseline left-parenthesis minus p Subscript prime j Baseline minus rho Subscript f Baseline ModifyingAbove u With two-dots Subscript j Baseline plus rho Subscript f Baseline b Subscript j Baseline right-parenthesis right-parenthesis Subscript prime i Baseline plus alpha ModifyingAbove epsilon With ampersand c period dotab semicolon Subscript italic i i Baseline plus StartFraction ModifyingAbove p With ampersand c period dotab semicolon Over upper Q EndFraction plus ModifyingAbove s With ampersand c period dotab semicolon Subscript 0 Baseline equals 0

      or

      (2.21b)italic nabla Superscript upper T Baseline bold-italic k left-parenthesis minus nabla p minus rho Subscript f Baseline ModifyingAbove bold-italic u With two-dots plus rho Subscript f Baseline bold-italic b right-parenthesis plus alpha bold-italic m Superscript normal upper T Baseline ModifyingAbove bold-italic epsilon With ampersand c period dotab semicolon plus StartFraction ModifyingAbove p With ampersand c period dotab semicolon Over upper Q EndFraction plus ModifyingAbove s With ampersand c period dotab semicolon Subscript 0 Baseline equals 0

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