Computational Geomechanics. Manuel Pastor
Читать онлайн книгу.will also be used for the same quantity in vectorial notation.
Similarly, we shall use wi and vi or w and v to denote the velocities of water and air relative to the solid components. These velocities are calculated on the basis of dividing the appropriate flow by the total cross sectional area of the solid–fluid composite.
As mentioned in Chapter 1, σij and
Similarly, εij or ε refers to the strain components. Further, pa, pw, and p = χw pw + χa pa will stand for air and water pressure and the “effective” pressure defined in the effective stress concept in Equation (1.11) when two fluids are present.
Sa and Sw are the relative degrees of saturation and ka and kw are the permeabilities for air and water flow.
Other symbols will be added and defined in the text as the need arises.
The derivation of the equations in this chapter follows a physical approach which establishes clearly the interactions involved in the manner presented by Zienkiewicz and Shiomi (1984), Zienkiewicz (1982), Zienkiewicz et al. (1990a, 1990b), etc. This is a slightly different approach from that used in the earlier presentations of Biot (1941, 1955, 1956a, 1956b, 1962) and Biot and Willis (1957) but we believe it is slightly easier to follow as it explores the physical meaning of each term.
Later, it became fashionable to derive the equations in the form of the so‐called mixture theories (see Green and Adkin 1960; Green 1969; Bowen 1976). The equations derived were subsequently recast in varying forms. Here an important step forward was introduced by Morland (1972) who used extensively the concept of volume fractions. Derski (1978) introduced a different derivation of coupled equations and Kowalski (1979) compared various parameters occurring in Derski’s equations with those of Biot’s equations. A full discussion of the development of the theory is given in the paper by de Boer (1996).
For completeness, we shall include such mixture derivations of the equations in Section 2.5. If correctly applied, the mixture theory establishes, of course, identical equations with appropriately chosen parameters and rheological relations.
It seems that despite much sophistication of various sets of coupled equations, most authors limited their works to conventional, linear elastic, behavior of the solid. Indeed, de Boer and Kowalski (1983) found it necessary to develop a special plasticity theory for porous, saturated solids. In the equations of Zienkiewicz (1982) and Zienkiewicz et al. (1990a), any nonlinear behavior can be specified for the skeleton and, therefore, realistic models can be incorporated. Indeed we shall find that such models are essential if practical conclusions are to be drawn from this work.
2.2 Fully Saturated Behavior with a Single Pore Fluid (Water)
2.2.1 Equilibrium and Mass Balance Relationship (u, w, and p)
We recall first the effective stress and constitutive relationships as defined in Equation (1.16) of Chapter 1 which we repeat below.
or
(2.1b)
This effective stress is conveniently used as it can be directly established from the total strains developed.
However, it should be remembered here that this stress definition was derived in Chapter 1 as a corollary of using the effective stress defined as below:
(2.2a)
or
(2.2b)
which is responsible for the major part of the deformation and certainly for failure.
In soils, the difference between the two effective stresses is negligible as α ≈ 1. However, for such materials as concrete or rock, the value of α in the first expression can be as low as 0.5 but experiments on tensile strength show that the second definition of effective stress is there much more closely applicable as shown by Leliavsky (1947), Serafim (1954), etc.
For soil mechanics problems, to which we will devote most of the examples, α = 1 will be assumed. Constitutive relationships will still, however, be written in the general form using an incremental definition
(2.3a)
(2.3b)
The vectorial notation used here follows that corresponding to stress components given in (1.1). We thus define the strains as
(2.4)
In the above, D is the “tangent matrix” and dε0 is the increment of the thermal or similar autogenous strain and of the grain compression
If large strains are encountered, this definition needs to be modified and we must write
(2.5)