berkeley pile in liquefied soil

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    AbstractSoil liquefaction and associateddeformation is a major cause of earthquake-related

    damage to piles and pile-supported structures.

    Computational procedures for nonlinear soil-pile

    interaction response commonly employ a 1D pile-soil

    system, and simplify the effect of soil pressure by

    linear or nonlinear p-y springs.

    This paper presents a pilot 3D Finite Element

    study of dynamic pile response in liquefied ground.

    The numerical model is formulated using CYCLIC, a

    geomechanics nonlinear finite element program

    developed to analyze cyclic mobility and liquefaction

    problems. In the current analysis, the pile and soil

    domains are discretized using 3D brick elements. The

    soil stress-strain behavior is represented by aplasticity-based, effective-stress constitutive model.

    This constitutive model is capable of simulating the

    essential response characteristics of saturated

    cohesionless soils, including shear-induced pore-

    pressure generation (dilatancy) and cyclic mobility.

    The computed results are compared to related

    centrifuge testing results. Special attention is given to

    the change in pile response characteristics due to

    liquefaction and lateral spreading of the surrounding

    soil.

    KeywordsFinite Element Analysis, Pile,

    Liquefaction

    INTRODUCTION

    Liquefaction and associated shear deformation is a

    major cause of earthquake-related damage to piles andpile-supported structures. Pile foundation damage due to

    lateral spreading induced by liquefaction is documented

    in numerous reports and papers [1-3].

    The recognition of the importance of lateral ground

    displacement on pile performance has led to thedevelopment of analytical models capable of evaluating

    the associated potential problems [4]. Modeling lateral

    ground displacement and pile response involves complex

    aspects of soil-structure interaction and soil behaviorunder large strains. Currently computational procedures

    for nonlinear soil-pile interaction response commonlyemploy a 1D pile-soil system, and simplify the effect of

    soil pressure by linear or nonlinear p-y springs. There is

    not much effort devoted to the study of the piles inliquefaction-induced lateral spreading using finite element

    method (FEM).

    This paper presents a pilot three-dimensional (3D)

    Finite Element study of dynamic pile response in liquefiedground. The numerical model is formulated using

    CYCLIC, a geomechanics nonlinear finite element

    program developed to analyze cyclic mobility andliquefaction problems [5,6]. In CYCLIC, the soil stress-

    strain behavior is represented by a plasticity-based,

    effective-stress constitutive model. This constitutivemodel is capable of simulating the essential response

    characteristics of saturated cohesionless soils, including

    shear-induced pore-pressure generation (dilatancy) and

    cyclic mobility. Extensive calibration of CYCLIC hasbeen conducted with results from experiments and full-

    scale response of earthquake simulations involving ground

    liquefaction [7].

    In this paper, salient features of the constitutive modeland the finite element formulation are presented first.

    Thereafter, the numerical simulation procedures and

    results are described and discussed.

    FINITE ELEMENT FORMULATION

    In CYCLIC, the saturated soil system is modeled as a

    two-phase material based on the Biot [8] theory for porous

    media. A numerical formulation of this theory, known as

    u-p formulation (in which displacement of the soilskeleton u, and pore pressurep, are the primary unknowns

    [9,10]), was implemented [5,6,11]. This implementation

    is based on the following assumptions: small deformation

    and rotation, density of the solid and fluid is constant inboth time and space, porosity is locally homogeneous and

    constant with time, incompressibility of the soil grains,

    and equal accelerations for the solid and fluid phases.

    The u-p formulation is defined by Chan [9] as twoequations: i) the equation of motion for the solid-fluid

    mixture, and ii) the equation of mass conservation for the

    fluid phase, incorporating equation of motion for the fluidphase and Darcy's law. These two governing equations

    may be expressed in the following finite element matrix

    form [9]:

    0fQpdBUM s

    T =&& (1a)0fHppSUQ

    pT =&& (1b)where M is the total mass matrix, U the displacement

    vector, Bthe strain-displacement matrix, the effectivestress tensor (determined by the soil constitutive model

    described below), Q the discrete gradient operatorcoupling the solid and fluid phases, p the pore pressure

    Three-Dimensional Finite Element Analysis of Dynamic Pile Behavior in

    Liquefied Ground

    Jinchi Lu1, Liangcai He1, Zhaohui Yang1, Tarek Abdoun2and Ahmed Elgamal11Department of Structural Engineering, University of California, San Diego, USA

    2Geotechnical Centrifuge Research Center, Rensselaer Polytechnic Institute, Troy, NY

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    vector, S the compressibility matrix, and H the

    permeability matrix. The vectorss

    f andp

    f representthe effects of body forces and prescribed boundaryconditions for the solid-fluid mixture and the fluid phase

    respectively.In equation (1a) (equation of motion), the first term

    represents inertia force of the solid-fluid mixture,

    followed by internal force due to soil skeletondeformation, and internal force induced by pore-fluid

    pressure. In equation (1b) (equation of mass

    conservation), the first two terms represent the rate of

    volume change for the soil skeleton and the fluid phaserespectively, followed by the seepage rate of the pore

    fluid. Equations (1a) and (1b) are integrated in the time

    domain using a single-step predictor multi-correctorscheme of the Newmark type [5,9]. In the current

    implementation, the solution is obtained for each time

    step using the modified Newton-Raphson approach [5].

    SOIL CONSTITUTIVE MODEL

    The second term in equation (1a) is defined by thesoil stress-strain constitutive model. The finite element

    program incorporates a soil constitutive model [5,11-13]

    based on the original multi-surface-plasticity theory forfrictional cohesionless soils [14]. This model was

    developed with emphasis on simulating the liquefaction-induced shear strain accumulation mechanism in clean

    medium-dense sands [6,7,12,13,15]. Special attention

    was given to the deviatoric-volumetric strain coupling(dilatancy) under cyclic loading, which causes increased

    shear stiffness and strength at large cyclic shear strain

    excursions (i.e., cyclic mobility).

    The constitutive equation is written in incrementalform as follows [14]:

    )(: pE &&& = (2)

    where & is the rate of effective Cauchy stress tensor, & the rate of deformation tensor,

    p& the plastic rate of

    deformation tensor, and E the isotropic fourth-order

    tensor of elastic coefficients. The plastic rate of

    deformation tensor is defined by:p& = P L , where Pis

    a symmetric second-order tensor defining the direction of

    plastic deformation in stress space, L the plastic loading

    function, and the symbol denotes the McCauley's

    brackets (i.e., L =max(L, 0)). The loading functionLis

    defined as: L = Q:& /H where H is the plasticmodulus, and Q a unit symmetric second-order tensor

    defining yield-surface normal at the stress point (i.e., Q=

    ff / ), with the yield function f selected of the

    following form [16]:

    0

    )())((:))((2

    3 20

    200

    =

    +++= ppMppppf ss (3)

    in the domain of 0p . The yield surfaces in principal

    stress space and on the deviatoric plane are shown in Fig.

    1. In equation 3, s p is the deviatoric stresstensor, p the mean effective stress, a second-orderkinematic deviatoric tensor defining the surfacecoordinates, and M dictates the surface size. For

    cohesionless soil, 0p is a small positive value (1.0 kPa inthis paper) such that the yield surface size remains finite at

    0p for numerical convenience (Fig. 1). For cohesive

    soil, 0p is related to cohesion. In the context of multi-surface plasticity, a number of similar surfaces with a

    common apex form the hardening zone (Fig. 1). Each

    surface is associated with a constant plastic modulus.

    Conventionally, the low-strain (elastic) moduli and plastic

    moduli are postulated to increase in proportion to the

    square root of p [14].The flow rule is chosen so that the deviatoric

    component of flow P = Q (associative flow rule in thedeviatoric plane), and the volumetric component P defines the desired amount of dilation or contraction in

    accordance with experimental observations. Consequently,

    P defines the degree of non-associativity of the flowrule and is given by [5]:

    P1)/(

    1)/(2

    2

    +

    =

    (4)

    Where p/2/1):)2/3(( ss is effective stress ratio, a material parameter defining the stress ratio along the

    phase transformation (PT) surface [17], and a scalar

    function controlling the amount of dilation or contraction

    depending on the level of confinement and/or accumulated

    plastic deformation [12]. The sign of 1)/(2

    dictates dilation or contraction. If negative, the stress pointlies below the PT surface and contraction takes place

    (phase 0-1, Fig. 2). On the other hand, the stress point lies

    above the PT surface when the sign is positive and dilationoccurs under shear loading (phase 2-3, Fig. 2). At low

    confinement levels, accumulation of plastic deformation

    may be prescribed (phase 1-2, Fig. 2) before the onset of

    dilation [12].

    A purely deviatoric kinematic hardening rule ischosen according to [14]:

    bp =& (5)

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    Fig. 1: Conical yield surfaces for granular soils in principal

    stress space and deviatoric plane (after [5,11,14,18])

    Fig. 2: Shear stress-strain and effective stress path under

    undrained shear loading conditions (after [5,11])

    where is a deviatoric tensor defining the direction oftranslation and b is a scalar magnitude dictated by the

    consistency condition. In order to enhance computational

    efficiency, the direction of translation is defined by anew rule [5,12], which maintains the original Mroz [19]

    concept of conjugate-points contact. Thus, all yield

    surfaces may translate in stress space within the failureenvelope.

    SIMULATION OF CENTRIFUGE EXPERIMENT

    Centrifuge Experiment

    In the centrifuge test reported by Abdoun [4], a single

    pile model (model 3, Fig. 3) was tested to simulate theresponse of the pile foundation subjected to the lateral

    pressure of a liquefied soil due to lateral spreading. The

    experiment was conducted using the rectangular, flexible-

    wall laminar box container shown in Fig. 3. The soilprofile consist s of two layers of fine Nevada sand

    saturated with water: a top liquefiable layer of relative

    density, Dr = 40% and 6m prototype thickness, and abottom slightly cemented nonliquefiable sand layer with

    a thickness of 2m. The prototype single pile is 0.6m in

    Fig. 3: Lateral spreading pile centrifuge model in two-layer soil

    profile, model 3 (modified after [20])

    diameter, 8m in length, has a bending stiffness, EI = 8000kN/m2, and is free at the top. The model has an inclination

    angle of 2 and is subjected to a predominantly 2Hz

    harmonic base excitation with a peak acceleration of 0.3g.The results of the test were documented in [4].

    Numerical Modeling

    The centrifuge test was simulated using the above-

    described three-dimensional finite element programCYCLIC. As shown in Fig. 4, the soil domain and the

    single pile were discretized using 3D 8-node brick

    elements. A half mesh configuration is used due togeometrical symmetry. The boundary conditions were (i)

    dynamic excitation was defined as the recorded baseacceleration, (ii) at any given depth, displacement degrees

    of freedom of the downslope and upslope boundaries were

    tied together (both horizontally and vertically using the

    penalty method) to reproduce a 1D shear beam effect [5],(iii) the soil surface was traction free, with zero prescribed

    pore pressure, and (iv) the base and lateral boundaries

    were impervious.A static application of gravity (model own weight)

    was performed before seismic excitation. The resultingfluid hydrostatic pressures and soil stress-states served as

    initial conditions for the subsequent dynamic analysis [7].

    Fig. 4: Finite element mesh of model 3

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    With a mild inclination of 2, model 3 attempts to

    simulate an infinite slope subjected to shaking parallel tothe slope [21]. However, it was noted that, in the

    centrifuge test, the soil surface gradually lost the slope

    and became level during the shaking phase. To simulatesuch behavior of losing the surface slope, a horizontal

    component of gravity varying with time was applied to

    the finite element simulation. The load-time history of theapplied horizontal gravity component was calculated

    based on the recorded lateral displacement at ground

    surface (the second subplot in Fig. 7).Figs. 5-8 display the computed and recorded lateral

    accelerations, displacement, and pore pressures. In

    general, good agreement was achieved between thecomputed and recorded responses. At 2m depth,

    accelerations virtually disappeared after about 4 seconds

    due to liquefaction (A4, Fig. 6). Liquefaction wasreached down to a depth of 5.0m (Fig. 8), as indicated by

    the pore-pressure ratio ru approaching 1.0 (ru = ue/v

    where ueis excess pore pressure, and vinitial effectivevertical stress). The Nevada sand layer remained liquefied

    until the end of shaking and beyond. Thereafter, excesspore pressure started to dissipate.

    The mild inclination of model 3 imposed a static

    shear stress component (due to gravity), causingaccumulated cycle-by-cycle lateral deformation. The

    recorded and computed ue histories both displayed anumber of instantaneous sharp pore pressure drops after

    initial liquefaction (Fig. 8). These drops coincided with

    the observed and computed acceleration spikes thatoccurred exclusively in the negative direction.

    -0.2

    0

    0.2

    A1 (3.0m)

    Experimental

    Computed

    -0.2

    0

    0.2

    LateralAcceleration(g)

    A2 (7.0m)

    0 5 10 15 20 25 30

    -0.2

    0

    0.2

    A3 (Input)

    Time (sec)

    Fig. 5: Model 3 recorded and computed acceleration time

    histories (along the laminar box boundary)

    -0.2

    0

    0.2

    A4 (2.0m)

    Experimental

    Computed

    -0.2

    0

    0.2

    LateralAcceleration(g)

    A5 (4.0m)

    0 5 10 15 20 25 30

    -0.2

    0

    0.2

    A6 (7.0m)

    Time (sec)

    (Experimental data unavailable)

    Fig. 6: Model 3 recorded and computed acceleration time

    histories (in the soil)

    0

    10

    20

    30

    40

    LVDT1 (Pile head)

    Experimental

    Computed

    0

    20

    40

    60

    80

    100

    Surface (near LVDT2(.25m))

    0

    20

    40

    60

    80

    LateralDisplacement(cm)

    2.0m (near LVDT3(2.5m))

    0

    20

    40

    60

    80

    4.0m (near LVDT4(3.75m))

    -8

    -4

    0

    4

    8

    LVDT5 (6.0m)

    0 5 10 15 20 25

    -8

    -4

    0

    4

    8

    LVDT6 (7.0m)

    Time (sec)

    Fig. 7: Model 3 recorded and computed lateral displacement

    time histories

    The permanent lateral displacement of the ground

    surface after shaking is approximately 100cm. All lateral

    displacements occurred in the top 6.0m within the

    liquefiable sand layer. The top graph of Fig. 7 shows the

    recorded and computed pile lateral displacement at the soilsurface during and after shaking. The computed pile

    lateral pile lateral displacement increased to 40cm, and

    decreased to approximately 20cm at the end of shaking,indicating relative movement between pile and soil. The

    bottom slightly cemented sand layer, as indicated in Fig.

    7, did not slide with respect to the base of the laminar box.

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    0

    2

    4

    6

    8

    10

    12ru= 1.0

    Excessporepressure(KPa)

    PP1 (1.0m)

    Experimental

    Computed

    0 5 10 15 20 25 30

    0

    10

    20

    30

    40

    50

    PP2 (5.0m)

    Time (sec)

    Fig. 8: Model 3 recorded and computed excess pore pressure

    time histories

    CONCLUSIONS

    A 3D finite element study of dynamic pile response inliquefied ground was presented in this paper. The results

    from numerical simulation were compared to relatedcentrifuge testing results. In general, good agreement was

    achieved between the computed and recorded responses.

    The calibrated numerical model will be useful inconducting additional parametric investigations.

    ACKNOWLEDGMENTS

    The reported research was supported in part by thePacific Earthquake Engineering Research (PEER) Center,

    under the National Science Foundation Award Number

    EEC-9701568, and by the National Science Foundation

    (Grant No. CMS0084616). This support is most

    appreciated.

    REFERENCES

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