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Compressibility and Consolidation - notes and formulae

Coefficient of Compressibility (av)

av = (e1 - e2)/(σ2 - σ1)

Here, e1 is the void ratio corresponding to effective stress σ1 and e2 is the void ratio corresponding to effective stress σ2. The coefficient of compressibility expresses change of volume (or void ratio) per unit change in effective stress.

Coefficient of Compressibility (av)
Coefficient of Compressibility (av)
Coefficient of Compressibility (av)

Relationship between volume change and thickness change:

ΔV/V0 = ΔH/H0

  • ΔV = change in volume (m3 or cm3).
  • V0 = initial volume (m3 or cm3).
  • ΔH = change in depth (m or cm).
  • H0 = original depth (m or cm).

Coefficient of Compression (Cc)

The coefficient of compression (Cc) is used with void ratio-log stress plots (e-log σ′) to estimate primary consolidation settlement.

  • Empirical and approximate relations (useful for quick estimates):
    • Cc = 0.009(WL - 10) for undisturbed soil of medium sensitivity, where WL is liquid limit (%) .
    • Cc = 0.009(WL - 7) for remoulded soil of low sensitivity.
    • Cc = 0.40(e0 - 0.25) for undisturbed soil of medium sensitivity, where e0 is initial void ratio.
    • Cc = 1.15(e0 - 0.35) for remoulded soil of low sensitivity.
    • Cc = 0.115 w where w is water content (expressed in the same units as required by the empirical relation).
Coefficient of Compression (Cc)
Coefficient of Compression (Cc)
Coefficient of Compression (Cc)

Overconsolidation Ratio (O.C.R.)

O.C.R. = Maximum past effective stress (preconsolidation stress) / Current effective stress

  • O.C.R. > 1 → overconsolidated soil.
  • O.C.R. = 1 → normally consolidated soil.
  • O.C.R. < 1 → underconsolidated (usually not encountered in static natural soils).
Overconsolidation Ratio (O.C.R.)

Differential Equation of One-Dimensional Consolidation

Differential Equation of One-Dimensional Consolidation

The governing differential equation for one-dimensional consolidation (Terzaghi) is written in terms of excess pore pressure u(z,t):

∂u/∂t = Cv2u/∂z2

where:

  • u = excess pore pressure (function of depth z and time t).
  • ∂u/∂t = rate of change of pore pressure with time.
  • 2u/∂z2 = curvature of pore pressure distribution with depth.
  • Cv = coefficient of consolidation (m2/s or cm2/s).

Coefficient of Volume Compressibility and Compression Modulus

Coefficient of volume compressibility mv is related to av by

mv = av / (1 + e0)

where e0 is the initial void ratio.

Compression modulus Ec is the reciprocal of mv:

Ec = 1 / mv

Degree of Consolidation (U)

  • Formulation from excess pore pressure:

    %U = (1 - u/u1) × 100%

    Here u is the excess pore pressure at time t and u1 is the initial excess pore pressure (at t = 0). At t = 0, %U = 0%; as t → ∞, u → 0 and %U → 100%.

    Degree of Consolidation (U)
  • Formulation using void ratio:

    %U = [(e0 - e)/(e0 - ef)] × 100%

    where e is void ratio at time t, e0 is initial void ratio (t = 0) and ef is void ratio at 100% primary consolidation (t = ∞).

  • Formulation using settlement:

    %U = (Δh / ΔH) × 100%

    where Δh is settlement at time t and ΔH is final total settlement due to primary consolidation (settlement at t = ∞).

Time Factor, Tv, and Relations with Degree of Consolidation

The time factor Tv is defined as:

Tv = Cv t / d2

where:

  • Cv = coefficient of consolidation (m2/s or cm2/s).
  • t = time (s).
  • d = length of drainage path (m or cm). For two-way drainage d = H0/2; for one-way drainage d = H0.
  • H0 = thickness of consolidating layer or sample.

Approximate relations between Tv and degree of consolidation U (useful for hand calculations and laboratory curve fitting):

  • For U ≤ 60%: Tv ≈ (π/4) U2. A commonly used value is T50 ≈ 0.196 for U = 50%.
  • For U > 60%: Tv ≈ -0.9332 log10(1 - U) - 0.0851.

Methods to Determine Cv from Consolidation Tests

  • Square-root of time fitting method:

    Cv = (T90 × d2) / t90

    where T90 is the time factor corresponding to 90% consolidation and t90 is the observed time for 90% consolidation. d is the drainage path.

  • Logarithm-of-time fitting method:

    Cv = (T50 × d2) / t50

    where T50 is the time factor for 50% consolidation and t50 is the observed time for 50% consolidation.

Compression Ratios

  • Initial Compression Ratio

    Defined from dial gauge readings; typical notation uses initial reading Ri, zero consolidation reading R0 and final reading Rf after secondary compression.

    Compression Ratios
  • Primary Consolidation Ratio

    Measured as the change in dial gauge reading corresponding to 100% primary consolidation (R100).

    Compression Ratios
  • Secondary Consolidation Ratio

    Ratios for initial, primary and secondary components satisfy ri + rp + rs = 1 for partitioning of total compression.

    Compression Ratios

Total Settlement

Total settlement S is the sum of initial, primary and secondary settlements:

S = Si + Sp + Ss

  • Initial settlement (Si)

    For cohesionless soils, initial settlement may be estimated using empirical bearing capacity or elastic approaches. An approximate factor given is Cs = 1.5 (Cr0) where Cr is a static resistance and σ0 reference stress. H0 denotes the depth of influence.

    Total Settlement

    For cohesive soils, initial elastic settlement may be estimated using a shape (influence) factor It and loaded area A.

    Total Settlement
  • Primary settlement (Sp)

    Primary consolidation settlement is obtained from e-logσ′ relations or from mv:

    S = ΔH = mv H0 Δσ′ for normally consolidated ranges, or by integrating changes in void ratio from initial to final effective stress.

    Total Settlement
    Total Settlement
    Total Settlement
    Total Settlement
    Total Settlement
    Total Settlement
    Total Settlement= Settlement for normally consolidation stage
    Total Settlement

    Note: separate plots and formulae are used for normally consolidated and overconsolidated stages; the images above correspond to common consolidation and settlement diagrams.

  • Secondary settlement (Ss)

    Secondary compression (creep) occurs after primary consolidation is essentially complete. It is often estimated from a secondary compression index and logarithmic time relations. Typical symbols include H0 ~ H100 (thickness after 100% primary consolidation), e100 (void ratio after 100% consolidation) and t2 the period over which secondary compression is calculated.

    Total Settlement

Permeability of Soils

Definition

Permeability is a measure of the ease with which water flows through a soil. The coefficient of permeability is usually denoted by K (or k).

Darcy's Law

For laminar flow in a porous medium (Darcy conditions): the discharge per unit time is proportional to the hydraulic gradient and cross-sectional area and inversely proportional to the length.

Rate of flow: q = K i A

Darcy`s Law
  • q = rate of flow (m3/s).
  • K = coefficient of permeability (m/s).
  • i = hydraulic gradient = HL/L = (H1 - H2)/L.
  • A = cross-sectional area of flow.

Seepage velocity and percolation coefficient

  • Seepage velocity Vs = V / n where V is the average pore water velocity and n is porosity.
  • Coefficient of percolation KP = K / n.

Laboratory permeability tests

  • Constant head test (suitable for coarse-grained soils):

    K = Q L / (t HL A)

    Q = volume collected in time t; L = sample length; HL = head loss; A = cross sectional area.

    Laboratory permeability tests
  • Falling head (variable head) test (suitable for finer soils):

    K = (2.303 a L) / (A t) log10(h1/h2)

    a = cross-sectional area of standpipe; A = area of specimen; t = time interval; L = length of specimen; h1, h2 = head readings at start and end of interval.

    Laboratory permeability tests

Kozeny-Carman equation and particle geometry

The Kozeny-Carman type relations connect permeability with particle shape, specific surface and porosity. The general form uses a shape coefficient C and specific surface S:

Kozeny-Carman equation and particle geometry
  • C is a shape coefficient (order of magnitude depends on particle shape; a value around a few mm is often used in empirical forms).
  • S = specific surface (surface area per unit volume or mass).
Kozeny-Carman equation and particle geometry

For spherical particles, relations for specific surface and characteristic dimensions are often simplified; R denotes particle radius. The input images show geometric relations and typical substitutions for S and particle sizes.

Kozeny-Carman equation and particle geometry

Empirical relations

  • Hazen (Allen Hazen) equation:

    K = C × D102

    D10 = effective grain size (cm). C ≈ 100 to 150 for clean sands (K in cm/s).

  • Lioudens equation:

    log10(K S2) = a + b n

    S = specific surface; n = porosity; a and b are empirical constants.

  • Relation with consolidation parameters:

    K = Cv mv γw

    This relates permeability with coefficient of consolidation Cv, coefficient of volume compressibility mv and unit weight of water γw.

Permeability of partially saturated soil (capillary permeability)

Permeability of partially saturated soil (capillary permeability)

In partially saturated soils the hydraulic behaviour depends on degree of saturation S; capillary heights and retained suction influence flow. Typical relations include a head distribution i = (h0 + hc)/x for certain simplified geometries where hc is capillary height and x is distance. Permeability K generally increases with saturation and reaches maximum at S = 100%.

Permeability of partially saturated soil (capillary permeability)
Permeability of partially saturated soil (capillary permeability)

Note: Ku (permeability for unsaturated soil) ∝ S; for S = 100% K = maximum.

Permeability of stratified soils

  • When flow is parallel to layers (bedding), the equivalent permeability keq can be approximated by a weighted arithmetic mean; the expressions in the images give the appropriate averaging.
  • When flow is perpendicular to the layers, keq is influenced by harmonic averaging of layer permeabilities; the images illustrate the formula forms.
  • For 2-D and 3-D flows similar averaging rules apply; for 3-D isotropic combination keq = (kx·ky·kz)1/3 is commonly used.
Permeability of stratified soils
Permeability of stratified soils
Permeability of stratified soils
Permeability of stratified soils
Permeability of stratified soils
Permeability of stratified soils

Effective Stress, Capillarity and Seepage

Seepage pressure and seepage force

Seepage pressure is the pressure exerted by moving water on soil particles as a result of flow. Seepage force acts in the direction of flow and is due to frictional drag of water on the soil skeleton.

Seepage pressure: Ps = h γw, where h is head loss and γw is unit weight of water (≈ 9.81 kN/m3).

Seepage force over a volume: Fs = h A γw.

Seepage force per unit volume: fs = i γw, where i is hydraulic gradient (i = h/z).

Quicksand condition

When upward seepage through a cohesionless soil produces a hydraulic gradient large enough to counteract the effective weight of soil, the net effective vertical stress becomes zero and the soil may behave as quick sand.

Critical hydraulic gradient is given by:

ic = (G - 1)/(1 + e)

  • G is specific gravity of solids (typical range 2.65-2.70).
  • e is void ratio (typical 0.65-0.70 in the example values given).

To avoid a floating (piping/quick) condition the actual gradient i must satisfy i < ic. A factor of safety against quick condition can be expressed as F.O.S. = ic/i > 1.

Two-Dimensional Flow: Laplace Equation and Flow Nets

The potential function ∅ and total head H are related for seepage in homogeneous isotropic soil: ∅ = k H.

Two-Dimensional Flow: Laplace Equation and Flow Nets
Two-Dimensional Flow: Laplace Equation and Flow Nets

For isotropic homogeneous soil the 2-D Laplace equation applies to H or ∅ and flow nets (orthogonal families of streamlines and equipotential lines) provide graphical solutions.

Seepage discharge from flow net

For unit length in the out-of-plane direction, seepage discharge q is given by:

q = k h (Nf / Nd)

  • h = total head difference between upstream and downstream.
  • Nf = number of flow channels (≈ number of flow nets between upstream and downstream boundaries).
  • Nd = number of equipotential drops.
  • Shape factor = Nf/Nd.
  • Nf = Nψ - 1, where Nψ is total number of flow lines.
  • Nd = N - 1, where N is total number of equipotential lines.

Hydrostatic (pore) pressure at a point: U = hw γw, where hw is pressure head.

An expression for seepage pressure using equipotential drops: Ps = h′ γw, where h′ = h - (2h/Nd) in the specific diagrammatic formulation shown in the images.

Seepage discharge from flow net

Exit gradient

The exit gradient at the downstream face of a porous medium (e.g., in an exit flow field of dimensions b × b shown in the figure) is approximated from flow net geometry. The equipotential drop ΔH = h / Nd is used in that evaluation.

Exit gradient

Phreatic Line

The phreatic line is the topmost streamline in an earth dam seepage profile; it represents the free surface of flow and follows a parabolic path in many simple geometries. Pressure on the phreatic line is atmospheric, while pressure below it is hydrostatic.

Phreatic line with filter (permeable blanket)

Phreatic line with filter (permeable blanket)
Phreatic line with filter (permeable blanket)

The phreatic line follows the base parabola; positions and radii of characteristic arcs (e.g., CF as radius of a circular arc) are shown in the figure. Typical notations: C = entry point of base parabola, F = junction of permeable and impermeable surfaces, S = focal length (distance between focus and directrix), FH = S, etc.

Relevant relations from the diagrams and analysis include discharge per unit length q = k s (where s is the seepage path length component shown), and other geometric relations shown in the images.

Phreatic line with filter (permeable blanket)
Phreatic line with filter (permeable blanket)
Phreatic line with filter (permeable blanket)

Phreatic line without filter

Phreatic line without filter

For a simple dam geometry with downstream slope angle α the approximate discharge expressions shown in the diagrams are:

  • For α < 30°: q = k a sin2α (diagram and derivation shown).
  • For α > 30°: q = k a sin α tan α (diagram and derivation shown).
Phreatic line without filter
Phreatic line without filter
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FAQs on Compressibility & Consolidation of Soils - Soil Mechanics - Civil Engineering (CE)

1. What is compressibility of soils?
Ans. Compressibility of soils refers to the ability of a soil to undergo volume change under applied load or stress. It is a measure of how much a soil can be compressed or compacted under load.
2. How is compressibility of soils determined?
Ans. The compressibility of soils is typically determined through laboratory tests, such as the oedometer test or consolidation test. These tests involve applying a load to a soil sample and measuring the resulting settlement or deformation over time.
3. What is consolidation of soils?
Ans. Consolidation of soils is the process by which a saturated soil undergoes a decrease in volume due to the expulsion of water from its pores under the influence of an applied load. It is a time-dependent process that occurs in fine-grained soils, such as clay.
4. How does consolidation affect the behavior of soils?
Ans. Consolidation significantly affects the behavior of soils by causing settlement. As water is expelled from the soil pores, the soil particles come closer together, resulting in a reduction in volume. This can lead to settlement of structures built on top of the soil and can also affect the stability of slopes.
5. What factors influence the compressibility and consolidation of soils?
Ans. Several factors influence the compressibility and consolidation of soils, including soil type, initial water content, applied load, duration of load application, and the presence of any preexisting soil layers or strata. These factors play a crucial role in determining the rate and magnitude of settlement that may occur in a soil.
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