W.Brząkała: CEB007361 Lecture no.7
1 THE METHOD OF CORRESPONDING STATES OF STRESSES
for cohesive soils in the limit state of stresses
1. The essence of the problem
How to find a solution for the limit state stresses in the Coulomb-Mohr medium in cohesive soil (c > 0), if a solution to the same problem is known,
but for non-cohesive soil (c = 0)?
The term "the same problem" means that all mechanical and physical parameters are the same (ex- cept for cohesion), as well as the shape of the medium - boundary surfaces, given external loads, etc.
A non-cohesive medium that meets these requirements is called a corresponding medium; it differs from the considered cohesive medium by only one parameter: c = 0.
2D cases are considered in the plane state of displacements; so, only transversal cross-sections of a
"very long" geotechnical structures are considered, like long retaining walls, slopes, and foundation beams.
2. Governing equations and the procedure
There are 3 components of stresses σ
z, σ
x, τ in a real cohesive medium which fulfil:
1. Static equilibrium equations in 2D
+ = (1a) + = 0 (1b) 2. Algebraic limit condition for cohesive Coulomb-Mohr media
− + 4 ∙ − + ∙ sin = 2 ∙ ∙ cos . (2)
Fig.1. Limit state condition.
1. Static equilibrium equations in 2D
∗ + ∗ = (1a*)
∗ + ∗ = 0 (1b*) 2. Algebraic limit condition for non-cohesive Coulomb-Mohr media
∗ − ∗ + 4 ∙ ∗ − ∗ + ∗ ∙ sin = 0 (2*) By making a horizontal shift of the axis τ, to the left by the value of σ
H= c⋅ctg (ϕ) = const > 0, the stress state components in the new coordinate system σ*, τ* are as follows:
σ
z* = σ
z+ σ
H, σ
x* = σ
x+ σ
H, τ * = τ , or in the reverse order
σ
z= σ
z* - σ
H, σ
x= σ
x* - σ
H, τ = τ *.
In the shifted system of axes σ *, τ *, we deal with the corresponding non-cohesive medium in the limit state of stresses; this is seen in (1*) and (2*), derived from equations (1) and (2).
ϕ
τ
c
τ=σ⋅tgϕ
σ, σ *
0
τ *
σ
H= c ⋅ ctg ϕ
W.Brząkała: CEB007361 Lecture no.7
2 The procedure can be summarized as follows.
a) Define the region occupied by the real cohesive medium.
Known loads τ
oand σ
oare applied to a part of the boundary B
oof the cohesive medium; it can be q, σ
zor σ
x, or also τ , i.e. for an inclined load. On the rest of the boundary B
1determine which load is unknown (to be found), like σ
1, sometimes also τ
1or some relationships between them
1; it can be for example the ratio τ
1/ σ
1= tg δ depending on the so-called frictional roughness of the wall surface
2.
b) Formulate the identical (corresponding task in the corresponding non-cohesive medium (*), modifying the acting loads applied to the boundary B
o, i.e. taking τ
o* = τ
oand σ
o* = σ
o+ σ
H. Solve this problem using relevant known methods, i.e. having τ
o* and σ
o* along B
o,
find τ
1* and σ
1* along B
1, taking c* = 0.
c) Return to the real cohesive medium using the inverse transformation:
τ
1= τ
1* and σ
1= σ
1* - σ
H. This way the solution is found for the cohesive medium.
3. Examples Example #1. The Coulomb solution
The method of corresponding states of stresses is exact and gives the same result as the exact Coulomb-Mohr method (discussed in Lecture 6). For the active pressure:
= ∙ ∙ + − 2 ∙ ∙ , where = !"#$ %
&"#$ % = ' &"#$ % ()" % * .
For the Coulomb wall and active soil pressure, direct application of the procedure is as follows.
Point a)
B
o= horizontal ground surface z = 0 which is loaded vertically τ
o= 0, σ
o= q = const;
B
1= vertical smooth wall, τ
1= 0, σ
1= e
a= ? Point b)
τ
o* = τ
o= 0 and σ
o* = σ
o+ σ
H= q + σ
H= q* are applied to the horizontal surface of
the corresponding (non-cohesive) medium, the parameters z, γ, ϕ and K
akeep unchanged;
∗ = ∗ = + ∙ ∙ + ∗ = + ∙ ∙ + + + ∙ , and τ
1* = 0.
Point c)
Reverse transformation : τ
1= τ
1* = 0 and σ
1= σ
1* - σ
H= e
a* - σ
H= e
a, therefore
= + ∙ ∙ + + + ∙ , − , = + ∙ ∙ + − , ∙ 1 − + .
= + ∙ ∙ + − ∙ cos sin ∙ 1+sin 2∙sin = + ∙ ∙ + − 2 ∙ ∙ + , because ()" %
&"#$ % = ! "#$ %
/&"#$ %
/= !"#$ % ∙ &"#$ %
&"#$ % ∙ &"#$ % = .
Example #2. The bearing capacity coefficient N
cfor a shallow foundation beam (EC7-1) For non-cohesive soils the following formula holds: 0 = ∙ 1 2 + ½ ⋅γ⋅B⋅ 1 3 [kPa], and the bearing capacity coefficient N
qyields form the Prandtl solution.
Point a)
The considered region is just the half-plane B0A, being a special case of the Prandtl wedge; it has the horizontal boundary and vertical loading, Fig.2.
1 σ
1does not mean - exceptionally - principal stress, but generally just a normal stress along B0.
2 The angle δ is usually a fraction of the angle ϕ being constant in this method, therefore the angle δ also does
not change.
W.Brząkała: CEB007361 Lecture no.7
3 B
o= 0B, τ
o= 0, σ
o= q (known),
B
1= 0A, τ
1= 0, σ
1= q
f= ? Point b)
τ
o* = τ
o= 0 and σ
o* = σ
o+ σ
H= q + σ
H= q* , τ
1* = 0.
Therefore for c* = 0 there is ∗ = 0 ∗ = ∗ ∙ 1 2 + ½⋅γ⋅ B ⋅1 3 = ∙ 1 2 + 4 ∙ 1 2 + ½⋅γ⋅ B ⋅1 3 . Point c)
Reverse transformation: = 0 = 0 ∗ − 4 = ∙ 1 2 + ∙ 1 5 + ½⋅γ⋅ B ⋅1 3 ,
where the following coefficient is introduced 1 5 = 67 ∙ 81 2 − 19, the same as in EC7-1.
The other bearing capacity coefficients N
q, N
γare not changed during this procedure, because they depend only on the angle ϕ which is constant.
Fig.2. Bearing capacity problem in the corresponding medium (c*= 0).
Example #3. Pressure of a weightless cohesive soil on a retaining wall
This situation recalls the general case of the weightless Prandtl wedge and shows significant effects of the vector nature of the pressure
3.
Symbols and sign convention are taken as previously by Coulomb-Prandtl.
Fig.3. The Prandtl wedge.
For c > 0, the active soil pressure q
1< q is to be found in its vector form (both value and angle).
Point a)
The weightless wedge A0B loaded by a constant q along A0 is considered.
Given: ϕ , c
,q, α
o ,β , ε , δ = η⋅ϕ , where η ≤ 1 is a certain constant.
3 The previous issues were actually scalar ones, because there was τ = 0 along the boundary, that is, only one component of the soil pressure vector was of interest – the normal component σ
1.
q *
q f * q f *
B A
B
wA
w0
β
ε
q
q
1+
+ ∞
+ ∞ δ 0
α o
A
B
c > 0, γ = 0
δ
W.Brząkała: CEB007361 Lecture no.7
4 B
o= 0A: τ
o= q⋅sin(α
o), σ
o= q⋅cos(α
o).
B
1= 0B: q
1= ? Point b)
σ
H= c ⋅ ctg( ϕ ) increases the normal component of the boundary load σ
o* = σ
o+ σ
Hand – keeping unchanged τ
o* = τ
o– generates a new vectorial boundary load along 0A
∗ = : ∗ + : ∗
Comment:
for the corresponding medium along 0A, the angle of q* to the normal is reduced; instead of the real value α
o =arctg( τ
o/ σ
o) for q, there is a virtual value α
o* = arctg( τ
o*/ σ
o*) ≤ α
ofor q* (in absolute values of both angles α , of course).
The problem is being solved in the corresponding medium, so the formulae (4),(5) from Lecture 7 (Coulomb-Prandtl) can be used.
Taking ϕ , c = 0
,q*, α
o*
,β , ε , δ = η⋅ϕ one gets the solution q
1* = const along 0B, which has two following components σ
1* = q
1*⋅cos(δ) and τ
1*= q
1*⋅sin(δ).
Point c)
The reverse transformation goes as usually: σ
1= σ
1* - σ
H, τ
1= τ
1*. This solution defines a vectorial loading q
1= const along 0B
= + = ;<=6
which has an angle δ
cto the normal; this angle is greater than the frictional roughness δ , because tg( δ
c) = τ
1/ σ
1= τ
1*/( σ
1* - σ
H) > τ
1*/ σ
1* = tg( δ ).
As the effect:
cohesion c > 0 causes a reduction of the length of the vector q
1and increases its angle to the normal;
but this is potentially possible that δ = ϕ, therefore, this inclination can be greater in cohesive soils than the internal friction angle
4.
Example 4. Pressure of a heavy cohesive soil on a retaining wall
The procedure is similar to the previous example, but the matter is complicated by the lack of an exact solution for the non-cohesive soil - necessary step in Point b). In general, it cannot be even the standard Poncelet solution from Lecture 6, because it concerns only the vertical load q applied to the ground surface ( α
o= -ε ); for the angle |α
o* | < |α
o| it will no longer be a vertical load on the
corresponding medium (unless ε = 0).
However, it is easy to predict the features of such a solution for soil pressure on the wall: along the wall 0B soil pressure will increase, both τ
1* = τ
1and σ
1*. Thus σ
1= σ
1* - σ
Hwill also increase, but the influence of this σ
Hcorrection will decrease relatively, because σ
His a constant value.
So tg ( δ
c) > tg ( δ ) but tg ( δ
c) → tg ( δ ).
Of course, there is nothing special about it, because the same yields from the Coulomb condition τ = σ⋅ tg ϕ + c; the cohesion c becomes of little importance if σ is "very large".
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