The following appendices contain detailed specific calculations associated with each chapter of the main text which are too long or too cumbersome to remain in the main text.
When thermal dissipation is negligible or fixed, compared with another term (Φ2 ≃ 0, or even Φ2 constant), under given T, the minimum of is the minimum of Φ1.
This appendix is related to sections 1.2.4 and 1.2.5 of Chapter 1 and focused on the determination of distributions of elementary contact actions tensors within the granular mass in motion, achieving a minimal dissipation in equation [1.16].
The dissipation rate being minimal for the lowest possible value of the internal feedback rate R(A) = 0, the solutions investigated are the distributions of contact actions tensors p(c) satisfying the condition [1.18]: .
Note that the proof given here through simple summations on discrete distributions representing a discrete finite set of contact actions tensors p(c) can be extended to integration over a continuous set representing a continuous statistical distribution of contact actions tensors (see Chapter 2, section 2.1.2).
For any distribution of elementary contact actions p(c), numbered from 1 to n, with random mutual orientations, we obtain the following:
Note that the sum is a tensor with positive trace, being a sum of positive trace tensors p(k) (property of elementary contact actions tensors); so, P owns at least one positive eigenvalue. Ordering the eigenvalues of tensor P by descending values, the following table summarizes all possible combinations, their connection with the “cases” analyzed further on, and the possibility of solutions.
Signature of (P1, P2, P3) | Case analyzed | Possible solution |
(+,−,−) | A | Yes: Mode I |
(+,0,−) | A and B | Yes: Border Mode |
(+,+,−) | B | Yes: Mode II |
(+,+,0) | C | No |
(+,+,+) | C | No |
(+,0,0) | C | No |
In the eigen referential of each of the p(k), we take the following numbering convention: p1(k) = p+(k) > 0, p2(k) = 0, p3(k) = p−(k) < 0
and we note the coordinates of direction
In the above expression, the positive terms correspond only to p+(k), all other terms being negative; moreover, the trigonometric coefficients are all ≤ 1, thus .
The only solution is that for all k, are verified, i.e. that and the direction bearing p+(k) are identical.
However, this inversion, which is not easy in any referential, is simpler in the natural basis of stresses, because in this stress referential the components verify . Then, resolving these relations, the following expression is obtained in the natural stress referential:
This expression becomes simpler in the case of coaxiality of the three tensors (note that if σ and are coaxial, then π is also coaxial with the two others, as a result of the definition [1.2.2]), as in the common eigen referential, only diagonal terms are not null in the above expression.
However, as outlined in the main text, note that the validity of this particular expression of strain rates is subordinate to the validity of the assumption that fluctuations in the local covariances of stress and strain rates may be neglected relative to the average, which is stronger than the assumption that is strictly required for the global validity of the approach developed in this book.
As a result, the relation [1.22] is no longer directly invertible, and the above expression of strain rate will also be corrected to account for these covariances.
Here, we treat in three dimensions the question treated in two dimensions in the main text (section 2.1.2.1): given a tensor of internal actions in a granular mass P, satisfying the dissipation equation, which conditions will satisfy a distribution of local contact actions tensors p in order to have tensor P as resultant?
Each local contact actions tensor p can be referenced in the global natural basis of the resultant P by the Euler angles of its local contact actions natural basis. The matrix for a change of basis (from local coordinates to global basis coordinates) is given by classical formulas (using the extrinsic convention 3-1-3 or Z-X-Z, with angles ψ,θ,φ, and abbreviated notations cψ, for cosψ, etc.)
In its own natural basis, the local contact actions tensor p is
In the global resultant tensor natural basis, whether the motion is in Mode I or Mode II, the internal actions of the granular mass P are
with , this parameter α represents the participation of eigenvalue no. 2, to P− in Mode I (as P− is borne by eigendirections no. 2 and 3), and to P+ in Mode II.
Calling f(ψ,θ,φ) the participation in the global dissipation of all the local tensors of contact actions found between ψ and ψ+dψ, θ and θ+dθ, φ and φ+dφ, their contribution to the global tensor P will be given by , where the tensor components tij are the components of local tensor transformed by the change of basis from local to global natural basis: , and the function f(ψ,θ,φ) is the density of dissipation by local contact actions, as a function of their orientation. This function can vary with time during motion.
Then, by integrating over ψ,θ,φ (between 0 and 2π for ψ and φ, 0 and π for θ)
Thus, after explicit formulation of all the relevant terms, in the natural basis of the global tensor of internal actions in the granular mass P (or the natural basis of the average tensor), the distribution f(ψ,θ,φ), density of dissipation by local contact actions as a function of their orientation, satisfies at any time of motion the system of seven conditions given on the next page.
Note that for a given R, the set of solutions f(ψ,θ,φ) satisfying this system of seven conditions is again a convex set, and that given a particular solution f0, any other solution f will be of the form: , where is a solution of the homogeneous linear system of the six last conditions with zero on their right-hand side, and may be again interpreted as a distribution of fluctuations, or deviations around f0.
However, given the complexity of this system of seven conditions, the detailed analysis of its solutions, in a similar way to how it is displayed in the main text for 2D granular materials (Chapter 2), is yet to be developed.
(The simplest way to get the condition on internal feedback is on the eigendirection of its unique sign, which ever the Mode: direction no.1 for Mode I, no.3 for Mode II).
Here, we show that a wide range of usual experimental conditions, provided that the response of the material is coaxial to the exerted solicitation, naturally satisfy the following conditions [2.11]:
As in the usual interpretation of these experiments, we neglect the effect of gravity.
Consider the tensor formed by the symmetrical product of external forces and velocities of their points of application on the external boundary of domain . In the following, we will term this tensor as “tensor of external actions”; note that this trace is the work rate of external forces: , and analyze the contributions brought by the faces of our specimen to this tensor of external actions.
The diagonal term can be transformed by taking into account the following:
Examine non-diagonal terms, such as :
The eigenvalues of TE (as those of ) can be interpreted as fluxes of mechanical energy as the outside exchanges with our material domain through its boundaries. In our quasi-static conditions, and for physical consistency, these fluxes will balance 2 by 2, with the corresponding fluxes of the internal actions tensor, i.e. in our conditions of Mode I (, only of its sign), the flux of mechanical energy provided by external actions to the domain along the eigendirection no. 1, which is , will be equal to the flux of mechanical energy received by the domain on this eigendirection no. 1, which is our “input power” . So, .
Complementing the reasoning along the other eigendirections and forming the corresponding summations, we arrive at the following equation:
Similarly, with the norm .
These are the intended conditions [2.11], but naturally satisfied (QED).
Here, we show that the local compliance with the dissipation equation also implies its verification by average values of stresses and strain rates on the material domain despite the presence of heterogeneities as defined in section 2.2.1.3.
By taking into account the second of the above observations, the integrals on both sides may be condensed, leading to
Here, we discuss the analysis of consequences of conditions [2.11] on , for each mode:
Ordering the eigendirections by descending values of eigenvalues, we obtain , with the complementary conditions of null Trace (c22 + c33 = 0), symmetry (c32 = c23) and conservation of mode signature and .
Here, we investigate, for each mode of minimal dissipation, the surfaces within the material in motion, which satisfy the following conditions:
We begin with the situations very close to theoretical minimum dissipation (with confounded with ϕµ) and later discuss the situations belonging to the wider neighborhood of minimal dissipation.
with , the parameter α representing the repartition of P− between the eigendirections nos 2 and 3.
α cos2 θ + (1 − α)sin2 θ = 1 which yields , with .
Now, consider the situations not so close to theoretical minimum dissipation, with no longer confounded with ϕμ, because of the internal feedback R(A) ≠ 0. As the motions we consider remain in a certain neighborhood of minimum dissipation, the polarization of the distribution of local contact actions tensors, although somewhat fuzzy, will nevertheless remain pronounced (see section 2.1.2). Therefore, the main orientation of the localization surface remains, although some dispersion in local contacts sliding will appear inside the corresponding shear band, leading to some diffusion of the movement toward outside the shear band, this being the subject of section 3.3 in Chapter 3.
In conclusion, the orientation of the shear band is the one found for situations very close to theoretical minimum dissipation, the orientation of localization surfaces is both at off the direction bearing P+, and at off the direction bearing P−, the general motion being in plane strain near this surface. This orientation corresponds to Rankine’s slip lines orientations (QED).
Here, we show that the orientation of chains of active forces is symmetric to the orientation of the localization surface, relative to the direction bearing π+. We again begin with situations very close to theoretical minimum dissipation (with confounded with ϕμ) and later discuss the situations belonging to the wider neighborhood of minimal dissipation.
The analysis of all possible situations for a given shows that there is only one solution for the direction of , the direction symmetric to , relative to the axis bearing π+.
Here, we set the detailed energy balance inside the shear band stationary structure, in the framework of section 3.3.3, together with Figure 3.8 in the main text.
This leads to the energy balance for the cell in layer (n):
This relation is the equation of energy dissipation diffusion, by internal feedback effect (a discretized form of a second-order linear ordinary differential equation). It defines a classical recurrent sequence whose solutions are linear combinations of two independent particular solutions: , where these particular solutions ω1, ω2 are the roots of the following equation:
For R <1/2, sin ϕμ about 0.5, and α > 0, the above expression [C] is generally far greater than 1. A limited series expansion provides , then: leading to equation [3.8] in section 3.3.3.
Let us prove this compatibility in the case of Mode I, with signature (+,−,−):
Here, we analyze the variance of strain rates in the case of the n parallel shear bands system of section 3.5.2: where the average shear rate , material parameter k, and the width of domain L, are fixed quantities, and ΣLi = L.
So, the minimum is reached when all the ui are null, i.e. when the parallel shear bands are of equal width .
In this appendix, the different strain modes allowed at a critical state are analyzed extensively, under three-dimensional stress states, for the least shear-resistant solutions, and the least dissipative ones, leading to the Failure Criterion. As this analysis requires wide algebraic development, we note for simplification .
The condition of positive dissipation Tr{π} > 0 results in the elimination of Reverse strain Modes I and II. For Mode I Reverse (only ), as here only the last term of is positive, and as σ1 ≥ σ2 ≥ σ3 > 0 it implies that and as , it would imply Tr{π} ≤ 0, excluded by the positive dissipation condition. For Mode II Reverse (only ), the same relation is found, leading to the same conclusion.
Another consequence of the dissipation relation is that under isotropic stresses it is written , which is not compatible with the critical state condition , so here under critical state conditions, it is σ1 > σ3.
To ease the analysis, it appears useful to express principal stresses and strains in function of deviatoric parameters and (note that the convention on the order in principal stresses σ1 ≥ σ2 ≥ σ1 > 0 makes that 0 ≤ b ≤1, there are no restrictions on values for c, and the constant volume condition has no incidence on the deviatoric parameter c)
For each of the modes defined in Table 4.1, we investigate the eventuality of a minimum of the ratio , for all allowed values of deviatoric parameters b, c.
This mode corresponds to −1 ≤ c ≤ ½.
As and ; the internal work rate is here , always > 0, the dissipation condition Tr {π} > 0 does not bring further restriction in this Mode I Direct.
The dissipation equation [1.30b] becomes ; then, by substituting to σi, and with their expressions in function of b and c, the above equality, after simplification, becomes: .
Let us observe that for 0≤b≤1 and :
In conclusion, we have shown that under strain Mode I Direct, for all allowed parameters b (0 ≤ b ≤ 1) and c (−1 ≤ c ≤ ½), provided that , this condition represents the limit of tensile stress conditions; then:
This mode corresponds to ½ ≤ c < 2.
As and ; the internal work rate is here , always > 0, the dissipation condition Tr {π} > 0 does not bring further restriction in this Mode II Direct.
The dissipation equation becomes: ; then, by substituting to σi, and with their expressions in function of b and c, the above equation, after simplification, becomes: .
Let us observe that, for 0 ≤ b ≤ 1 and :
In conclusion, under this strain Mode II Direct for all allowed parameters b and c:
This mode corresponds to
As and ; the internal work rate is here , which will be positive only if ; then, by substituting σi, and with their expressions in function of b and c, this inequality reduces to (for c ≤ –1 or c ≥ 2). This is the restriction to be verified in this Mode I Transverse in order to satisfy the dissipation condition Tr{π} > 0.
The dissipation relation here becomes: ; then, by substituting σi, and with their expressions in function of b and c, the above equation, after simplification, becomes: , with the condition , in which the numerator and denominator are maintained with the same sign corresponding to the limit of the tensile stress condition (i.e. becomes ∞), more restrictive than the above condition for Tr{π} > 0.
In conclusion, under this Mode I Transverse strain for allowed parameters b and c:
This mode again corresponds to .
As and the internal work rate is here , which will be positive only if ; then, by substituting σi, and with their expressions in function of b and c, this inequality reduces to (for c ≤ –1 or c > 2). This is the restriction to be verified in this Mode II Transverse in order to satisfy the dissipation condition Tr{π} > 0.
The dissipation relation here becomes: , then, by substituting σi, and with their expressions in function of b and c, the above equation is simplified as: , with again the condition corresponding to the limit of the tensile stress condition (i.e. becomes ∞), more restrictive than the above condition for Tr{π} > 0.
As σ1 > σ3, the above dissipation relation becomes an inequality
, so except if and σ2 = σ3.
In conclusion, under this Mode II Transverse strain for all allowed parameters b and c:
For the modes defined in Table 4.2, we investigate the eventuality of a minimum of the ratio , for all allowed values of deviatoric parameters b and c, where Tr{π} is the internal work rate for each of the strain modes investigated, and Tr{π0} is the internal work rate of the reference plane strain solution under the same boundary conditions as the considered strain mode.
In addition to the useful relations displayed in Appendix A.4.1, other relations bind the dissipated energy rate, resulting from the dissipation equation, which always links the dissipated energy rate Tr{π} to the input power π+, sum of positive eigenvalues of the tensor π, i.e. , and the output power π–, sum of negative eigenvalues of the tensor π, i.e.
As and , the above ratio becomes .
For the three allowable strain modes Mode I, Mode II Direct, and Mode II Transverse, we will now compare the dissipated energy rate Tr{π} > 0 with the dissipated energy rate of reference plane strain solution Tr{π0} > 0 under the same boundary conditions.
This mode corresponds to –1 ≤ c ≤ 1/2.
The energy dissipation rate is given here by and relative to the reference plane strain mode:
Therefore, the minimum of the ratio under this strain Mode I Direct is identical to the minimum of the ratio , already determined in section 4.1.
This mode corresponds to 1/2 ≤ c < 2.
The energy dissipation rate is given by . As may be expressed as a function of given boundary condition by , then , and relative to the plane strain reference solution Tr{π0}, it is simplified to which is always ≥ 1 as here 1/2 ≤ c < 2, the equality being reached only for c = 1/2 (i.e. plane strain ).
Therefore, we have shown here that under our given boundary conditions, whatever the parameters b and c satisfying 1/2 ≤ c < 2 under this strain Mode II Direct:
This mode again corresponds to .
The energy dissipation rate is given by . As may be expressed as a function of given boundary condition by , then , and relative to plane strain reference solution Tr{π0}, it yields .
We observe that
In conclusion, under this strain Mode II Transverse, only one particular solution realizes a relative minimum of dissipated rate: it is confounded with the axisymmetric stresses σ2 = σ3 (i.e. b = 0), associated with plane strain = 0.
This mode corresponds to −1 ≤ c ≤ ½.
The energy dissipation rate here is . Then, relative to reference plane strain (for c = 1/2) under the same boundary conditions : , hence Therefore, the minimum of the ratio under this strain Mode I Direct is the minimum of for −1 ≤ c ≤ 1/2, i.e. for c = 1/2 (plane strain ) whatever the value of b, otherwise the ratio is > 1.
In conclusion, under our given boundary conditions, whatever the parameters b and c satisfying ½ ≤ c < 2 under this strain Mode I Direct:
This mode corresponds to ½ ≤ c < 2.
The energy dissipation rate here is , and reference plane stain . Then, .
Here, the minimum of the ratio under this strain Mode II Direct is the minimum of . As the initial conditions of these boundary conditions are under isotropic stresses , this stress ratio can decrease until it is physically limited by the shear Failure Criterion : once it is reached, the material can experience large strains under quasi-static conditions, and the resulting ratio is equal to 1. The ratio could be forced to be further reduced, however the motion would no longer remain quasi-static and would enter into dynamic behavior, out of our present scope.
In conclusion, under our given boundary conditions B, whatever the parameters b and c satisfying ½ ≤ c < 2 under this strain Mode II Direct:
The treatment of Mode I Transverse, similar to the above treatment of Mode II Transverse under boundary conditions A, although submitted to stronger restrictions due to dissipation condition (see section 4.1), does not bring further significant features.
The deviatoric relation selected here, and represented in Figure 4.8(a), is
Here, we show the basic inequalities listed in Table 5.1 taking into account the dilatancy rate d as defined in section 5.1.
We treat first the situation 0 < b < 1, which implies that both
The dissipation relation yields , substituting σ2 to σ3, as σ2 > σ3, the above equality becomes which can also be written as or with the dilatancy rate . As , the above inequality also means: if then . Similarly, now substituting σ3 to σ2 yields , hence . Therefore, when 0 < b < 1, we have (QED).
Note that these last two inequalities transform into simple equalities either when the substitutions become indifferent, which occurs when σ2 = σ3, i.e. axisymmetric stresses b = 0, or when one of the principal internal actions or disappears from the dissipation relation, which occurs when or , i.e. plane strain. For b = 1, these last two inequalities remain valid without a change (except that here ).
The dissipation relation yields , so substituting here σ1 and σ3, we have
Note that these last two inequalities transform into simple equalities either when the substitutions become indifferent, which occurs when , i.e. isotropic stresses, or when one of the principal internal actions, or , disappears from the dissipation relation, which occurs when or , i.e. plane strain.
The dissipation relation yields , so substituting here σ1 and σ2, we have
Note that these last two inequalities transform into simple equalities either when the substitutions become indifferent, which occurs when σ1 = σ2, i.e. axisymmetric stresses b = 1, or when one of the principal internal actions, or , disappears from the dissipation relation, which occurs when or , i.e. plane strain.
Mode II Direct, Transverse, and Reverse can be treated similarly, particularizing the strain rate unique of its sign (here negative) and substituting the principal stresses borne by the two other eigendirections. In Mode II Direct, we also have the property: if then .
These are the same as in Appendix A.4 for the expression of intermediate principal stresses in a function of the deviatoric parameter and the dissipated energy rate.
For the plane strain reference solution π0 with and (d0 dilatancy rate)
For the allowable strain modes Modes I and II Direct, and Modes I and II Transverse, we will now compute the principal stress ratio , and for the allowable strain modes under boundary conditions A, we will compare the dissipated energy rate Tr{π} > 0 with the dissipated energy rate of reference plane strain solution Tr{π} > 0 under the same boundary conditions ( and σ3).
Combining the definition of the generalized dilatancy rate with the definition of deviatoric parameter c provides the following expressions of :
The constraints on parameters for this mode are
This is a homographic function of each of the parameters b, c, and d whose numerator and denominator are always > 0, provided that , this last inequality corresponding to the limit of the tensile stress condition (i.e. becomes ∞). This homography is an increasing function relative to b and d, and a decreasing function relative to c; given the above constraints on parameters b, c, and d, it has a minimum for b = 0 (axisymmetric stresses), or (Plane Strain ), that minimum being , which constitutes the least shear strength criterion under this Mode I Direct with dilatancy, this Failure Criterion being the critical state one, enlarged by the dilatancy rate (QED).
The above expression transforms into
This is the generalized stress–dilatancy relation for this Mode I Direct (QED).
Then,
As outlined above, this homographic function of b, c, and d has a minimum for b = 0 (axisymmetric stresses) or (plane strain ), and that minimum is equal to d. So,
except for b = 0 (axisymmetric stresses), or (plane strain ) for which the inequalities become equalities. So:
Combining the definition of the generalized dilatancy rate , with the definition of deviatoric parameter c, provides the following expressions of :
Constraints on parameters are
Then, by substituting σi, and with their expressions in function of b, c, and d, the above equality, after simplification, becomes
The condition is required to maintain the numerator and denominator with the same sign, this condition being the limit of tensile stress on σ3.
In conclusion, the least shear strength criterion under this Mode I Transverse with dilatancy is the critical state one, enlarged by the dilatancy rate (QED).
Combining the definition of the generalized dilatancy rate: with the definition of parameter c, provides the following expressions of :
Then, by substituting σi, and with their expressions in function of b, c, and d, the above equality after simplification becomes:
This is a homographic function of each parameter b, c, and d, whose numerator and denominator are always > 0, provided that , this last inequality corresponding to the limit of the tensile stress condition (i.e. becomes ∞). It is an increasing function relative to c and d, and decreasing relative to (1 − b); given the above constraints on the parameters b, c, and d, it has a minimum for b = 1 (axisymmetric stresses) or (plane strain ), that minimum being , which constitutes the least shear strength criterion under this Mode II Direct with dilatancy, this Failure Criterion being the critical state one, enlarged by the dilatancy rate (QED).
The above expression transforms into
This is the generalized stress–dilatancy relationship for this Mode II Direct (QED)
Combining the definition of the generalized dilatancy rate: , with the definition of parameter c, gives expressions of
Constraints on parameters for this mode are:
By substituting σi, and with their expressions in function of b, c, and d, the above becomes after simplification: . This relation is again a homographic function of each parameter b, c, and d, whose numerator and denominator are always >0, provided that , this inequality corresponding to the limit of tensile stress conditions. This homography is an increasing function relative to b and c. Given the constraints on c, two minima are to be considered:
In conclusion, the least shear strength criterion under this Mode II Transverse with dilatancy is the critical state one, enlarged by the dilatancy rate (QED).
We observe that:
In conclusion, under this strain Mode II Transverse, only one particular solution realizes a relative minimum of energy dissipation rate, which is confounded with the axisymmetric stresses σ2 = σ3, associated with plane strain ; this provides the same result as the least shear strength criterion (QED).
To find this limit, we analyze the algebraic configuration of the dissipation equation for the six strain modes allowed, through a procedure similar to Appendix A.5.1.
The dissipation equation yields: .
Substituting σ3 to σ2, as σ2 ≥ σ3, the above equation becomes , and as , this inequality becomes .
Similarly, substituting σ2 to σ3, as σ2 ≥ σ3, the above relation becomes , then .
The dissipation equation yields: .
So, according to the substitutions between σ1 and σ3, .
The dissipation equation yields: .
So, according to the substitutions between σ1 and σ2, .
Similar conditions can be drawn for Mode II, particularizing here the negative strain rate. All the resulting inequalities may be gathered in the recapitulative table (Table A.1).
Note that if , as σ1 ≥ σ2 ≥ σ3 > 0, then we obtain .
Thus, in all strain modes, there will be volume contraction provided that . On the other side of this limit, when dilatancy is impossible in Modes I and II Reverse, and with restrictions in Modes I and II Transverse (QED).
The “internal friction angle,” the quantity widely used in Soil Mechanics practice, is defined at peak shear resistance by . Reworking this definition with the stress–dilatancy equation [5.4], we have at peak shear resistance , this relation allows us either to compute Φ in the function of the maximum dilatancy rate and apparent inter-granular friction , or to adjust a value for on the basis of a set of experimental data , as shown in Figure 6.1(c).
With the specific coordinates provided by relation [6.1], we have
, and as the stress–dilatancy relations provided in Table 5.3 is written as: in Direct motion and for Reverse motion, it becomes with specific coordinates: for Direct motion and for Reverse motion. Note that in the specific dilatancy diagram, the corresponding theoretical curves are hyperbolic arcs, crossing at point {–1, –3/2} in Figure 6.3.
For Direct movement in plane strain , the dissipation relation is written with specific notations given in the main text (relation [6.2]).
This transforms into a specific form of stress–dilatancy relation: .
Observe that with these coordinates, the theoretical curve becomes a hyperbolic arc passing at points {1, −1} and {−1, 1} in the specific dilatancy diagram shown in Figure 6.4.
For Reverse movement, the dissipation relation is written as and the corresponding specific stress–dilatancy relation becomes . The theoretical curve is another hyperbolic arc passing at points {1, −1} and {−1, 1} in the specific dilatancy diagram.
In the following, details of calculations leading to the features shown in Figure 6.5 are described, these calculations are performed here with the value S ≈ 0.485 or adjusted on the energy diagram [Figure 6.5(c)]:
Observe that the specific coordinates defined by relations [6.3] are very similar to the coordinates already defined for simple shear (relations [6.2]) and worked in section 6.3. In this specific dilatancy diagram, it will thus yield for the Direct motion and for the Reverse motion.
Observe that, in specific dilatancy diagram, the corresponding theoretical curves are hyperbolic arcs crossing here at {1,1} and {−1,−1}, as drawn in Figure 6.6.
Here, we draw the relations for cyclic compaction under alternate simple shear motion in plane strain:
and as , we get for the cycle which transforms into: or conversely: .
These formulas allow building the diagrams in Figure 7.3.
Here, we describe the composite local micromechanical motions resulting into the bulk mono-dimensional settlement, associated with the geostatic stress-building in the development of geostatic equilibrium, and the elements sustaining the comparison with the Jaky formula.
The global internal actions tensor π, which is uniaxial of vertical axis, is decomposed into two components of the same axis, but with opposite signatures: , which allows for a null resultant in principal directions 2 and 3, those components being in Mode I Direct (+,−,−) and Mode II Reverse (−,+,+):
with a typical value , it gives a participation of 75% in total dissipation to the main component in Mode I Direct. Note that the higher the apparent inter-granular friction, the higher this participation of the main component in the total dissipation.
Table A.3. Correspondence between stress states and volume change conditions
Stress state | |||
Main component Mode I | Volume contraction | Volume contraction | Dilatancy (in horizontal directions) |
Secondary component Mode II | Dilatancy (in vertical direction) | Volume contraction | Volume contraction |
Total motion | Volume contraction | Volume contraction | Volume contraction |
The process of equilibrium build-up under the action of gravity being associated with densification of the material is the reason why the comparison is done for dense to medium dense granular materials.
The relationship between “internal friction” Φ of the Jaky formula, measured by classical laboratory tests and our apparent inter-granular friction is: where DMax is the maximum observed of the dilatancy rate during the test (relation valid for “triaxial” or plane strain tests, see also Appendix A.6.1). Systematic measurements have provided the following orders of magnitude, for various granular materials sheared under moderate confining stress, and for the usual range of apparent inter-granular friction (approximately from 23° to 45°):
These elements allow computing the data summarized in Figure 8.3.
Here, we develop the micro-mechanical proof of the “Scale Effect Rule” detailed in Chapter 9.
Before entering into a more general situation, let us first consider the particles from two sets of particles A and B issued from the same homogeneous mineral stock, with similar grain shapes, and characteristic diameters dA and dB, which satisfy the relations displayed in section 9.1.2:
Here, we will again consider the Love–Weber relation for average stresses in granular media, which expresses the stresses from local contact forces and branch vectors between fixed material points inside the grains in contact (see section 1.3.2 in Chapter 1)
where f(n/p) is the contact force exerted by particle n on particle p, l(n / p) is the branch vector joining the centroids of particles in contact, from particle n toward particle p, and N is the total number of particles occupying the volume V in the sample granular material.
Let us now consider two geometrically similar granular materials A and B issued from the same homogenous mineral stock (Figure A.2) and let us analyze the relations resulting from this similarity, assumed to be a perfect one.
First, these two similar granular media display similar grain shapes, the same density, and parallel grain size distributions in the classical gradation diagrams, where the abscissae are in logarithmic scale (Figure A.3).
The geometric correspondence between the two similar granular media A and B is ruled by a geometric similarity ratio DB/DA, where DA and DB are the given characteristic sizes for media A and B, respectively (e.g. maximum grain size DMax, or mean grain size D50 or any other given characteristic diameter).
For instance, the diameters dA(p) and dB(p) for two homologous particles number p, or the branch vectors between particles n and p in contact, or the volumes VA and VB occupied by homologous representative subsets of particles in the granular media A and B are linked by
With regard to the forces and internal equilibrium in both similar materials, the following basic assumptions are recalled:
Consider now our similar granular media submitted to macroscopic stresses, close to the limit equilibrium, inducing slow motion inside both our granular media: the contact forces in our granular media in slow motion induce some grain breakage. Consider the probability of failure of homologous particles number p in our similar granular media under the effect of contact forces exerted by homologous particles n.
The relation [A9.1] shows that, in order to secure the same probability of grain breakage, the homologous contact forces should be in proportion to the crushing resistances of homologous particles .
As the scaling ratio is the same for all contact forces, this relation valid locally for each contact force f(n/p) also holds globally for the complete sets of contact forces {f}
Macroscopic stresses in our similar granular materials A and B are derived from equation [A9.2]
From equations [A9.2] to [A9.4], all terms in the stress tensor formula for granular media B may now be expressed as a function of corresponding terms belonging to the similar granular media A, resulting in the following relation [FRO 09)]:
Equation [A9.5] sets the relationship between the macroscopic stress state tensors to be applied to granular media A and B in order to obtain the same probability of grain breakage during mechanical loading, and thus statistically the same amount of grain breakage during motion (QED).
Here, we treat the simplified three-dimensional analysis of the kinematics of settlements in dam body at impounding, leading to the equation [10.8].
The valley is schematized by a trapezoidal vertical section, with a width of L0 at its base, and with a vertical dammed section at dam height H, of Sv. As , observe that the horizontal width of this valley L(h), may be expressed at any level by , and that .
Under the impounding water pressure over the upstream impervious face, the dam body will settle perpendicularly to its facing [Figure A.4(a)] and the magnitude of this settlement in the central section along the valley is (neglecting the deformations of the foundation compared to dam body settlements):
Under the effect of a vertical component δv(h) of these settlements:
This modulus at impounding ERI can be related to the apparent rigidity modulus at the end of the construction ERC (the only rigidity modulus known before impounding) by using the statistical correlations developed in [HUN 03], which also displays some dependence on valley shape (arching effects, etc.). With some safety margin, it leads to select a value ERI ≃ 2.7ERC. Replacing in the above expression of , this leads directly to the relation [10.8] (QED).
Here, we handle the question of substitution of another p-norm to octahedral norm N for numerical applications of dissipation equation.
The mathematical difficulties mentioned in Chapter 11 are linked to the lack of continuity of derivatives of this octahedral norm N; this lack of continuity also manifests in the geometry of its unit ball: an octahedron with sharp edges and sharp vertices.
Therefore, if, instead of the tensor octahedral norm N, , we consider the following tensor norm with 0 < α ≪ 1: