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INTERNATIONAL JOURNAL OF CIVIL AND STRUCTURAL ENGINEERING
Volume 2, No 1, 2011
© Copyright 2010 All rights reserved Integrated Publishing services
Research article ISSN 0976 – 4399
Received on July 2011 published on November 2011 176
Soil structure interaction analysis methods - State of art-Review Siddharth G. Shah
1, Solanki C.H.
2, Desai J.A.
3
1, Research Scholar
2 Associate Professor,
SV National Institute of Technology Surat, Gujarat, India.
1 Asst. Prof, 3 Director & Professor
C G Patel Institute of Technology, Uka Tarsadia University, Bardoli, Gujarat, India.
doi:10.6088/ijcser.00202010101
ABSTRACT
Soil flexibility has to be considered in the analysis of massive structures to avoid failure
and ensure safe service. Post failure analysis of massive structures realized the
importance of SSI-soil structure interaction. In the literature as many as half dozen
methods are available but researches and designers are not clear about the history &
development in this field. Current paper attempts to review the stat of art about soil
structure interaction analysis methods. The review reveals that for simple analysis direct
methods-Global procedures are physible while for non linear analysis substructure
method is effective and simple to apply.
Keywords: Soil structure interaction, global procedure, local procedure, thin layer
method, boundary layer method, finite element method, transmitting boundary, infinite
element, absorbing boundary.
1. Introduction
Soil conditions have a great deal to do with damage to structures during earthquakes.
Foundation motions deviate from free-field motions for two principal reasons: (1) the
imposition of stiff foundation systems on (or in) a geologic medium experiencing
nonuniform shaking will result in foundation motions being reduced relative to those in
the free-field and (2) inertial forces developed in the structure will cause base shear and
moment, which in turn will induce relative foundation/free-field motions due to the
foundation compliance. These phenomena are commonly termed Soil-Structure
Interaction (SSI). The general SSI problem is subdivided into kinematic SSI, which is
concerned with first factor identified above, and inertial SSI, which is concerned with the
second factor. Depending mainly on the relative stiffness of the soil and structure, SSI
can have an impact on the response of the structure.
Over the last four decades, various methods have been proposed for the solution of wave
equations in unbounded domains. This paper summarizes briefly the existing literature
with particular emphasis on the dynamic soil-structure interaction. In general, these
approaches fall into two broad categories: global and local procedures. Global procedures
in Section 2 are divided into sub-sections presenting the boundary element method, thin
layer method, exact non-reflecting boundary conditions and the scaled boundary finite-
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177
element method. Local procedures in Section 3 are grouped as transmitting boundary
conditions, infinite elements and absorbing layers. An investigation on the capacity of
popular commercial finite-element packages for modeling unbounded domains is
presented in Section 4.
2. Global procedures
Global procedures have been proposed for the dynamic analysis of unbounded domains
from 1970s. They are constructed through integral operators with respect to space or time
leading to globality in space or time. This is consistent with the physical nature of wave
propagation. the global procedures are generally rigorous. Due to their high accuracy,
they can be placed immediately beyond the structure-media interface leading to a
reduction of the number of degrees of freedom in the bounded domain and thus total
computational time. However, because of the spatially and temporally global formulation
the computational effort in global procedures increases with the size of the problem.
Generally speaking, extension to unbounded domains of general anisotropic and non-
homogeneous media with arbitrary geometry increases the complexity of the global
procedures.
2.1 Boundary Element Method
The well known boundary element method based on boundary integral equations presents
an attractive computational framework especially for problems involving singularity and
unbounded domains. The basic idea of this method is to formulate the equation of motion
of the unbounded domain in the form of an integral equation instead of a differential
equation. Finally, this integral equation is solved numerically. The method has been
applied in various areas of engineering and science. A detailed literature on the
formulation of the method and its applications in different fields is addressed in the book
by Brebbia et al. (1984). A full literature review on the method is beyond the scope of
this paper.
Firstly, essential features of the method are summarized. Secondly, a brief review of the
recent researches for the dynamic soil-structure interaction analysis with the particular
emphasis on anisotropic and non-homogeneous soils is presented. Finally, new
developments for improving the efficiency of the method are summarized.
In the boundary element method (Beskos, 1987, 1997; Hall and Oliveto, 2003) (Figure
2.1) rather than throughout the interior domain (Ω), as its name suggests, only the
boundary (Γ) is discretized resulting in a reduction of the spatial discretization by one.
For instance, for a three-dimensional problem only a two-dimensional surface has to be
addressed. Surface and line elements are used to discretize the structure-soil interface in
three- and two-dimensional problems, respectively. Over each element the functions
under consideration, for example displacement in elastodynamics, can vary in much the
same manner as in finite elements. They are interpolated in terms of the nodal values by
the so-called shape functions in a local coordinate system. The weighting functions are
chosen as fundamental solutions, or Green’s functions, satisfying rigorously the radiation
condition at infinity and the governing equations. Generally speaking, the exact solution
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of the governing equation subjected to a concentrated unit load in an infinite domain
represents the fundamental solution.
Figure 2.1: Spatial discretization in boundary element method for an unbounded domain
The boundary element method is applicable to problems for which the fundamental
solutions can be calculated. Determining the fundamental solutions for general
anisotropic media is very complicated and sometimes even impossible. Applying the
fundamental solutions and the method of weighted residual to the governing equations
followed by integration by parts, yields the boundary integral equation. For example, a
typical boundary integral equation in the frequency domain is in the form
=
+
Where,
and are the corresponding displacements and tractions respectively,
describing the fundamental solutions.
B j (ω) is the body load.
U j (ω) and Pj (ω) are the boundary displacement and tractions respectively.
As can be observed in Eq. (2.1), only the contribution of body load B j (ω) is represented
by an integration over the domain Ω. Two other terms are expressed by the integration
over the boundary Γ. The boundary integral equation (Eq. (2.1)) is discretized into
boundary elements. Generally, the integrals involving fundamental solutions are
performed by using numerical integration schemes. The fundamental solutions are
generally the response to a concentrated force. They are singular. Special techniques have
to be applied to compute their integrals. Having calculated the integrations and
discretized Eq. (2.1) for different nodes, a global system of linear algebraic equations is
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derived. After imposing the prescribed boundary conditions, the system of linear
algebraic equations can be solved by direct or iterative solvers for unknown nodal values.
The coefficient matrices are fully populated and non-symmetric. This leads to a high
storage requirement and computational costs. Boundary integral equation can also be
formulated in the time domain.
=
+
Convolution integrals are encountered. Evaluation of these convolution integrals leads to
a large amount of computational costs. The fundamental solutions for full-plane or full-
space are derived without satisfying any boundary condition. Using these fundamental
solutions, one has to discretize the free surfaces (half-planes or half-spaces) (Figure 2.2a).
In the boundary element method, the interface between two different materials when non-
homogeneity is encountered, has to be discretized (Figure 2.2a) too. Obviously, the
infinite extent of these boundaries requires a special treatment in any numerical scheme.
The most straightforward approach consists in restricting the discretization to a finite part
of the boundary, thereby truncating the boundary integrals leading to modeling errors. To
reduce the computational efforts, in addition to fundamental solutions for full-space or
full-plane in three- and two-dimensional problems, fundamental solutions for half-space
or half-plane may also be determined. These fundamental solutions satisfy the boundary
conditions on the free surfaces of half-plane or half-space. Doing so, the free-surfaces
need not to be discretized reducing considerably the amount of numerical work involved
in the solution of the problem (Figure 2.2b). An infinite boundary element has also been
developed by Zhang et al. (1989, 1991) for dynamic problems of three-dimensional half-
space by making use of the transformation technique from an infinite domain to a finite
domain. A decay-type shape function based on the asymptotic behavior of fundamental
solutions for three-dimensional dynamic problems was used in the element. The coupled
finite-element/boundary element method has been used in wave propagation problems as
well. In this case, the bounded domain is modeled by finite elements and the unbounded
domain by boundary element method.
Figure 2.2: (a) boundary discretization in the boundary element method when
fundamental solutions for full-plane are used and the discretization of interface between
different materials when non-homogeneity is encountered; (b) boundary discretization
when fundamental solutions for half-plane are used.
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The earliest works on applying boundary element method to soil-structure interaction
problems address the homogeneous isotropic unbounded domains. Luco and Westmann
(1971) studied the dynamic response of a rigid circular footing on the surface of an
isotropic half-space using the mixed boundary value problem. Wong and Luco (1976)
computed the dynamic compliance of a surface rigid mass-less foundation of arbitrary
shape on an elastic half-space by dividing the soil-foundation interface into rectangular
elements. They used the integration of Lamb’s point load solution to obtain the relation
between the tractions over an element and the displacements on the soil surface. It was
actually a boundary element method with a half-space fundamental solution. Dominguez
(1978) applied for the first time the boundary element method to dynamic soil-structure
interaction problems. Using a frequency-domain formulation he obtained the dynamic
stiffness of rectangular foundations resting on, or embedded in, a viscoelastic half-space.
From the early 1970s the boundary integral methods have been used for the dynamic
analysis of soil-structure interaction problems in anisotropic soils. A brief literature
review for the frequency-domain analysis is included here. Freedman and Keer (1972)
studied the response of a body resting on the surface of a transversely isotropic half-plane
and presented exact solutions in terms of dual integral equations. Wang and Rajapakse
(1991) studied the dynamic response of rigid strip foundations embedded in orthotropic
elastic soils. Rajapakse and Wang (1993) presented a boundary integral solution for the
dynamic response of three-dimensional problems in a transversely isotropic elastic half-
space. They applied the Fourier expansion with respect to the circumferential coordinate
and Hankel integral transforms with respect to the radial coordinates to derive general
solutions for equations of equilibrium expressed in terms of displacements. These general
solutions are used to derive the explicit solutions for Green’s functions corresponding to
a set of time-harmonic circular ring loads acting inside a half-space. Wang and
Achenbach (1995) obtained Green’s functions in an anisotropic medium by using the
Radon transform. This transformation reduces a three- or two-dimensional partial
differential equation to one-dimensional differential equations of the same kind. Having
solved the one-dimensional problem, the 3D and 2D solutions follow from the inverse
Radon transform. Dravinski and Zhang (2000) utilized the Radon transform to develop an
efficient algorithm for evaluation of time-harmonic Green’s functions for an orthotropic
full-space. Wang and Rajapakse (2000) used the boundary element method to investigate
the dynamic response of rigid mass-less cylindrical and hemispherical foundations
embedded in transversely isotropic elastic soils. Ahmad et al. (2001) analyzed the time-
harmonic two-dimensional elastodynamic problems of anisotropic media. They used the
full- and half-space Green’s functions developed by Rajapakse and Wang (1991), higher
order isoparametric curvilinear boundary elements and the self-adapting numerical
integration technique to deal with problems of orthotropic and non-orthotropic solids
with arbitrary geometries. They illustrated the effect of soil anisotropy on the compliance
of a rigid strip foundation resting on a two-layered media through an extensive
parametric study. Dravinski and Niu (2002) developed three-dimensional time-harmonic
Green’s functions based on Radon transform for the most general anisotropic material,
i.e., for a triclinic material. They used a symbolic computation system to efficiently
evaluate the finite integrals of the Green’s function. One- and two-dimensional Gauss-
Legendre quadratures were used. Niu and Dravinski (2003) used the time-harmonic
Green’s functions proposed in Dravinski and Niu (2002) to study the scattering of elastic
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waves in 3D general anisotropic media (triclinic). They formulated the scattering
problems for scatterer in form of a cavity only. Denda et al. (2003) investigated two-
dimensional time harmonic response of solids of general anisotropy. They split the
fundamental solution obtained by Radon transform into static singular and dynamic
regular parts. The boundary integrals for the static singular part are evaluated analytically
and those for the dynamic regular part numerically over a unit circle. They also applied
the developed boundary element method to an eigen-value analysis. Arias and Achenbach
(2004) proposed a simple approach to correct the error introduced by the truncation of the
infinite boundary in the boundary element method modeling of elastodynamic wave
propagation in semi-infinite domains when Green’s functions of a full-space are used.
They exploited the asymptotic behavior of the solution and invoked the reciprocity
theorem of elastodynamics to adequately correct the boundary element method results.
Chen and Dravinski (2007) derived the displacement and stress Green’s functions for a
general anisotropic 2D half-space with embedded harmonic line load. Both displacement
and stress fields were expressed in terms of double Fourier integrals. The integrals were
evaluated by using contour integrations and a composite Gauss-Legendre quadrature over
a finite domain. Only a limited number of boundary element method studies have taken
into account the non-homogeneity of soils in a dynamic soil-structure interaction analysis.
Most of them are for cases when the foundation is located at the surface of the unbounded
soil. A summary of the existing literature is presented here. Guzina and Pak (1998)
studied the vertical vibration of a rigid circular footing resting on an elastic half-space
with a linear wave velocity profile in the vertical direction. Using a displacement-
potential representation and integral transforms, the problem is formulated as a set of dual
integral equations which are reducible to a Fredholm’s integral equation. Pak and Guzina
(1999) derived a regularized format of the time-harmonic direct boundary element
formulations for the three-dimensional elastodynamics for general anisotropic materials.
As in the conventional direct boundary element methods the evaluation of the Cauchy
principal values leads to mathematical and numerical complexities, they derived the
regularized boundary integral equation based on the decomposition of Green’s functions
into their singular and regular parts. This alternative form of the conventional boundary
integral equation involves weakly singular integrals only. They extended their
formulations to the general soil-structure interaction problems in the semi-infinite
domains including inhomogeneous and anisotropic media. Vrettos (1999) investigated the
vertical and rocking response of rigid rectangular foundations resting on a linear elastic
non-homogeneous half-space utilizing semi-analytical solutions for mixed boundary-
value integrations. Using the boundary integral method, Muravskii (2001) studied the
dynamic response of surface footings on a heterogeneous isotropic and transversely
isotropic elastic half-space. The variation of shear modulus with depth as linear functions
and as exponential functions to a finite or infinite depth are addressed.
Most of the studies for the dynamic analysis of soil-structure interaction problems in non-
homogeneous anisotropic soils using the boundary element method have been carried out
in the frequency domain. Here a summary of works done in the time domain is presented.
Wang and Achenbach (1992, 1993) developed two- and three-dimensional Green’s
functions for general anisotropic media based on Radon transform. Rajapakse and Gross
(1995) investigated the time-domain response of an orthotropic elastic half-plane
containing a cavity of arbitrary shape using the Laplace transformation. Wang et
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al.(1996) presented a two-dimensional transient boundary element method using the
Green’s functions presented by Wang and Achenbach (1993) to solve elastodynamic
boundary initial-value problems in solids of general anisotropy. Richter and Schmid
(1999) derived the transient Green’s functions of the elastodynamic half-plane for cases
where source and observation points are situated beneath the traction-free surface. The
derivations are based on Laplace transform methods and the Cagniard-de Hoop inversion.
In the conventional boundary element approaches, the storage requirements and
computational time will tend to grow according to the square of the problem size. This is
because of the dense and non-symmetric nature of the boundary element matrix. To
improve the efficiency in terms of computational time and memory requirement, several
fast algorithms have been proposed in the past 20 years. Fast multi-pole method was first
introduced by Rokhlin (1983). It was developed for potential problems based on iterative
algorithms. It has been shown that this approach is efficient for the integral equations of
second kind. For the integral equations of first kind, appropriate matrix conditioning
techniques are necessary to result in similar computational costs because of the
unboundedness of the condition number of the matrix. Alpert et al. (1993) proposed
wavelet-based methods. They transformed the coefficient matrix to wavelet-like
coordinates leading to a sparse matrix. Grigoriev and Dargush (2004b) proposed a fast
multi-level boundary element method for the two-dimensional solution of Laplace
equation with mixed boundary condition. They used double-noded corners to facilitate
the implementation of a patch-by patch boundary element. They employed a bi-conjugate
gradient method as an iterative solver and also utilized the multi-grid method to
accelerate the convergence rate of the proposed iterative solver. They later extended the
fast multi-level boundary element into Helmholtz (Grigoriev and Dargush, 2004a) and
Stokes problems (Grigoriev and Dargush,2005). Wang et al. (2005) recently applied the
fast multi-level boundary element into the transient diffusion. In addition to fast
algorithms, the symmetric Galerkin boundary element methods have been proposed. The
symmetry property of the coefficient matrices permits the employment of efficient
symmetric solvers. The symmetric Galerkin boundary element methods are beneficial
from the point of view of coupling with finite elements as well. The main difficulty
associated with the symmetric Galerkin boundary element methods is the existence of
hyper singular integrals leading to more complex fundamental solutions. A fairly
extensive recent review on symmetric Galerkin boundary element methods can be found
in Bonnet et al. (1998). Perez-Gavilan and Aliabadi (2001) presented a symmetric
Galerkin boundary element formulation for the frequency-domain solution of two-
dimensional viscoelastic problems. Kallivokas et al. (2005) introduced a symmetric
Galerkin boundary element method for the solution of interior problems based on an
energy-based variational framework.
In summary, in the boundary element method only the boundary is discretized reducing
the spatial discretization by one. The fundamental solutions satisfy rigorously the
governing equations and the radiation condition at infinity. Although the boundary
element method in last four decades has gained the recognition as the logical tool for
dealing with unbounded domain problems, difficulties are encountered in its application
to many practical engineering problems owing to its reliance on the fundamental solution.
For instance, when the material is general anisotropic, the complexity of the fundamental
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solution increases dramatically. Furthermore, in the conventional boundary element
methods the coefficient matrices are densely populated and unsymmetric. It leads to
expensive computations. Fictitious frequencies embedded in singular integral equations
are encountered in the frequency-domain analysis (Brebbia et al., 1984) too.
2.2 Thin layer method
The rigorous thin layer method, also known as consistent boundary or hyperelement, was
first developed by Lysmer and Waas (1972) for the dynamic analysis of unbounded
domains subjected to anti-plane loads. This method discretizes the boundary in the
vertical direction only consistent with that used for finite elements (Figure 2.3). The
displacement functions in the horizontal direction are expressed analytically to satisfy the
radiation condition at infinity. This semi-analytical technique is well suited to model
horizontal layers Layered medium.
Figure 2.3: Spatial discretization in thin layer method
Absorbing boundaries with material properties varying in the vertical direction. The
boundary conditions on the free surfaces and on the interfaces between adjacent layers
are rigorously satisfied with the same computational effort as for a homogeneous
horizontal layer. Thin layer method can be easily implemented in a finite-element
analysis. Applying the semi-discretization to the governing equations of motion and
enforcing the relevant boundary conditions, result in a complex-valued quadratic eigen-
value problem in the frequency domain. After solving the complex eigen-value problem,
the wave numbers and the corresponding mode shapes of the waves in the medium are
determined yielding the dynamic-stiffness matrix. The Fourier transformation can be
applied to the displacement functions obtained in the frequency domain to compute the
response in the time domain. It is obtained step by step by: (1) formulating the equations
of motion in the frequency-wave-number domain; (2) solving a complex-valued quadratic
eigen-value problem in the wave-numbers; (3) integrating analytically the displacement
functions over wave-numbers; (4) integrating numerically the displacement functions
over frequencies by means of the Fast Fourier transform (Kausel, 1992). In the following
the literature for the thin layer method is briefly reviewed.
Waas (1972) extended the method to in-plane motion of layered soils. Kausel et al.
(1975) and Kausel and Roesset (1977) generalized the method to axisymmetric problems.
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Kausel and Peek (1982) applied the method to obtain Green’s functions for point forces
acting within (or on) a layered medium. These Green’s functions were later extended by
Seale and Kausel (1989) for the modeling of layered media over elastic half-spaces. The
thin layer method was extended to poroelastic unbounded domains by Bougacha et al.
(1993). Kausel (1992) extended the thin layer method to the time-domain formulation.
The extension is restricted to a class of anisotropic materials for which the required linear
eigen-value problem involves only real, narrowly banded symmetric matrices. In this
approach the time-domain formulation is obtained by: (1) expressing the governing
equations in the frequency-wave-number domain; (2) solving a linear real-valued eigen-
value problem in the frequency variable; (3) performing an analytical integration of the
displacement functions over frequencies; and finally (4) performing a numerical
transformation of the displacement functions over wave-numbers. This formulation
avoids using the complex variables, involves only a real, linear eigen-value problem and
allows obtaining the Green’s functions directly in the time domain. This strategy is
particularly appealing for the problems when the response is required at only a few
receivers, when the dynamic loads do not vary sharply in space, when the loads are
applied impulsively, and when the system has little or no damping (Kausel, 1992). Kausel
(1999) presented Green’s functions for the solution of various types of point sources
acting within (or on) horizontally layered media: point forces, force dipoles, blast loads,
seismic double couples with no net resultant and moment dipoles. He modeled the full-
space in the examples with a homogeneous finite layer of unit depth (horizontal
layer) to which paraxial boundaries were added to simulate the infinite medium. Park and
Tassoulas (2002) extended the thin layer method into inclined boundaries with the so-
called zigzag shape for both anti-plane motion and plane-strain problems. In the thin
layer method, since it is necessary to consider a rigid rock under the layered media, the
formulation ignores any possible vertical radiation. The assumption of rigid bases and
horizontally layered media are not always close to reality. There are cases in practical
geotechnical problems where the soil deposit is not very rigid or the soil geometry is far
from being horizontally layered.
2.3 The Scaled boundary finite-element method
The scaled boundary finite-element method, a fundamental-solution-less boundary
element method, is an attractive alternative to the numerical schemes in computational
mechanics. It not only combines some important advantages of the finite-element and
boundary element methods but also has its own salient features. This method, which is
semi-analytical, is based on the finite-element technology so that it does not require
fundamental solutions. The radiation condition at infinity is satisfied rigorously. Like the
boundary element method only the boundary is discretized reducing the spatial
discretization by one and leading to the increase of computational efficiency. Problems
involving stress singularities and discontinuities can be modeled accurately. Anisotropic
media can be handled without additional computational efforts.
In the scaled boundary finite-element method, a so-called scaling center O is chosen in a
zone from which the total boundary, other than the straight surfaces passing through the
scaling center must be visible (Figure 2.4a). Only the boundary S directly visible from the
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scaling center O is discretized as shown in Figure 2.4a. One-dimensional line element is
used (Figure 2.4b). The straight surfaces passing through the scaling center (side faces)
and the interfaces between different materials are not discretized (Figure 2.4a). The
geometry of an element on the boundary is interpolated using the shape functions
formulated in the local coordinate η in the same way as in the finite-element method. The
geometry of the Side faces
Figure 2.4: (a) Spatial discretization for an unbounded domain in scaled boundary finite-
element method; (b) three-node line element on boundary domain V is described by
scaling the boundary with the dimensionless radial coordinate ξ pointing from the scaling
center to a point on the boundary (Figure 2.4a).
The radial and circumferential coordinates ξ and η form the scaled boundary coordinates.
Along the radial lines passing through the scaling center and a node on the boundary, the
nodal displacement functions are introduced. The shape functions are employed in the
circumferential direction to interpolate the displacement functions piece wisely. Having
expressed the governing differential equations in the scaled boundary coordinates,
Galerkin’s weighted residual method or the principle of virtual work is applied in the
circumferential direction transforming the governing partial differential equations to the
ordinary differential equations with the radial coordinate ξ as an independent variable.
This set of Euler-Cauchy ordinary differential equations is called the scaled boundary
finite-element equation in displacement. The coefficient matrices of this scaled boundary
finite-element equation are calculated and assembled in the same way as the static-
stiffness and mass matrices in the finite-element method. For static analysis, the scaled
boundary finite-element equation can be transformed into a system of first-order ordinary
differential equations. An eigen value problem can be used to solve this system of first-
order ordinary differential equations. Thus, the displacement and stress fields are
described by semi-analytical solutions permitting the boundary condition at infinity to be
satisfied rigorously. Obtaining the nodal forces on the boundary, introducing the
definition of the dynamic-stiffness matrix of an unbounded domain on the boundary and
making use of the scaled boundary finite-element equation in displacement, the scaled
boundary finite-element equation in dynamic stiffness with the frequency as the
independent variable is derived. It is a system of non-linear first-order ordinary
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differential equations to be solved numerically for the dynamic-stiffness matrix. The
radiation condition at infinity is satisfied using an asymptotic expansion of the dynamic-
stiffness matrix for high frequency. Applying the inverse Fourier transformation to the
scaled boundary finite-element equation in dynamic stiffness leads to the scaled boundary
finite-element equation in time domain involving the convolution integrals. The time-
discretization method is used to solve the scaled boundary finite-element equation in the
time domain.
A literature review on the evolution of the method from the first inspiration until March
2006 is presented by Vu (2006) in her PhD thesis. A brief summary with emphasis on the
application to the dynamic soil-structure interaction analysis is provided here.
3. Local procedures
To avoid the expensive computational problems associated with the global procedures,
various local procedures have been proposed over the last four decades. As was explained
in Section 1.4.2 local procedures are approximate. In them the response at a specified
location and time depends to the response at its immediate neighbors (spatially local) and
at a few previous times (temporally local). Most of them are constructed based on the
theory of wave propagation and using differential operators to enforce outgoing plane
waves (Wolf and Song, 1996). They can be constructed by enforcing artificial damping
to a finite layer to absorb the outgoing waves too. On the surface, the local procedures
appear to be vastly different from each other from the mathematical formulation,
conceptual basis and implementation point of views. However, many of them are
mathematically related and comparable in energy-absorbing performance (Kausel, 1988).
Generally speaking, local procedures are algorithmically simple so that most of them can
be easily implemented into the finite-difference or the finite-element methods. The
approximations in the local procedures lead to spurious reflections from the artificial
boundary. In order to obtain results of an acceptable level of accuracy a local procedure
has to be applied at a so-called artificial boundary sufficiently far away from the
structure-media interface. It increases the number of degrees of freedom in the
computational domain. Most of the local procedures have been developed for scalar wave
equations in unbounded domains of simple geometry and material property. However, a
reliable local procedure for modeling vector wave equations in unbounded domains of
arbitrary geometry and material property does not exist at present.
3.1 Transmitting boundary conditions
Transmitting boundary conditions have been introduced since the late 1960s. Most of
them are based on the mathematical representation of plane wave propagation to
eliminate the incident waves at special angle of incident. Lysmer and Kuhlemeyer (1969)
proposed the first transmitting boundary for elastodynamics often referred to as the
classical viscous boundary condition. It absorbs plane waves propagating perpendicularly
to the artificial boundary. For two-dimensional cases the viscous boundary condition is
formulated as ∂u
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σ = a ρ Cp
τ = b ρ Cs
where,
σ and τ are the normal and shear stresses on the boundary, respectively;
ρ is the mass density;
Cp and Cs are the longitudinal and shear wave velocities, respectively and
u and v are the normal and tangential displacements on the boundary, respectively.
Dimensionless parameters a and b are chosen to minimize the reflected energy for an
incident plane wave impinging at a given angle of incidence. Lysmer and Kuhlemeyer
(1969) found that the choice of a = b = 1 leads to good absorptions. The viscous
boundary condition can easily be implemented in finite-element codes for both
frequency-domain and transient analyses. It is algorithmically simple, geometrically
universal and frequency independent. As dashpots have no static stiffness, the viscous
boundary condition is not able to model a static problem as the limiting case of a dynamic
problem at low frequency. White et al. (1977) proposed the unified boundary condition
which is a viscous boundary condition applicable to anisotropic media with a certain
choice of the parameters a and b. By discretizing the domain using the finite elements,
and then determining the linear relationship between stresses and velocities on the
boundary, they obtained the parameters a and b. They presented formulations for both
plane-strain and Axisymmetric conditions. Akiyoshi (1978) presented a viscous boundary
for shear waves called compatible viscous boundary. It is actually a correction to the
viscous boundary to account for the discretization scheme used for the domain. This
approach has the disadvantage of involving a convolution integral in its formulation. It
loses the local character of the boundary condition. Smith (1974) proposed the
superposition boundary condition to solve both the scalar and elastic wave propagation
problems. The superposition boundary averages the solutions from two sets of boundary
conditions corresponding to symmetry and anti-symmetry, which eliminates the reflected
waves for a single boundary. The formulation is independent of both frequency and angle
of incidence. This boundary condition is not able to eliminate multiple reflections. The
superposition boundary condition was later modified to overcome multiple reflections by
introducing two overlapping narrow boundary neighborhoods in which the reflected
waves are canceled as they occur (Cundall et al., 1978; Kunar and Marti, 1981).
Underwood and Geers (1981) introduced the doubly-asymptotic boundary condition for
dynamic soil-structure interaction. In this boundary, dashpots and coupled static springs
are used which are asymptotically exact at high and low frequencies for plane waves
propagating perpendicularly to the boundary, respectively. They used the boundary
element method to determine the static-stiffness matrix for the medium leading to fully
coupled and non-symmetric coefficients. The doubly-asymptotic boundary results in
errors for modeling the intermediate frequencies. The approach is temporally local but
spatially global. The low accuracy is the most important concern associated with the
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above mentioned transmitting boundary conditions named as Sommerfeld-like
transmitting boundary conditions (Givoli, 2004). Since late 1970s, high-order
transmitting boundary conditions have been proposed for modeling unbounded domains.
They have the potential of leading to accurate results with increasing orders of
approximation. At the same time, they are computationally efficient owing to the local
formulation. Lindman (1975) proposed a very general set of transmitting boundary
conditions using projection operators leading to a high degree of effectiveness for the
time-dependent scalar wave equations. He determined coefficients for the high-order
boundary conditions to minimize reflections over a broad range of angle of incidence for
both traveling and evanescent waves. Engquist and Majda (1977) and Clayton and
Engquist (1977) proposed the so-called paraxial boundary conditions, which are closely
related to the boundary conditions proposed by Lindman (1975), using rational
approximations (Padé) to pseudo-differential equations for scalar and elastic wave
equations. This paraxial boundary constructs a differential equation which favors
outgoing waves by splitting the differential operator of the wave equation for plane
waves. It was the first time that the method of rational approximation appeared as a tool
to derive local absorbing boundary conditions. The paraxial boundary condition is exact
for plane waves propagating perpendicularly to the boundary and any wave with oblique
incidence will necessarily cause some reflections. The paraxial boundary condition leads
to a formulation with high-order derivatives. The first and second-order paraxial
boundary conditions for scalar wave equations in rectangular coordinates are formulated
as
u = 0
u = 0
The first-order boundary condition (Eq. (2.8)) is identical to the viscous boundary
condition. They showed that for any given angle of incidence other than right angle, the
second-order boundary condition (Eq. (2.9)) generates less reflections than the first-order
one (Eq. (2.8)). The Engquist-Majda boundary conditions are easily implemented in a
finite-difference scheme. There are instability problems associated with higher order
boundaries and for inclined body waves (Wolf, 1988). Bayliss and Turkel (1980)
proposed a sequence of transmitting boundary conditions based on an asymptotic
expansion of an exact solution at large distances for time-dependent wave-like equations
in polar coordinate systems. They constructed a set of special local differential relations
that identically eliminates a prescribed number of leading terms in the corresponding
series. For three-dimensional scalar wave equation in spherical coordinates, the mth
Bayliss and Turkel boundary condition is formulated as
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The high-order formulations lead to higher derivatives. The first order Bayliss and Turkel
boundary coincides with the first-order Engquist and Majda boundary. Bayliss et al.
(1982) extended the approach to Helmholtz and Laplace equations and implemented
them into finite elements. Utilizing the idea of factorizing the high-order operators,
Higdon (1986) constructed multi-directional boundary conditions for the scalar and
elastic wave equations at preselected angles of incidence. He demonstrated that all
transmitting boundary conditions based on a rational approximation of a pseudo-
differential operator can be cast in this form so that they are special cases of his multi-
directional boundary condition. Higdon’s boundary condition is expressed as
where,
α is the angle of incidence.
The multi-directional boundary condition which is exact for plane waves propagating at
preselected angle of incidence, can be regarded as the general case of the viscous and
paraxial boundaries. The higher the number of orders, the higher the accuracy is. In his
numerical studies, Higdon found instabilities for third-orders of these boundary
conditions. Same as in the paraxial boundary, number of orders higher than two is not
practical. Higdon later extended this idea to stratified media (Higdon, 1992) and
dispersive systems (Higdon, 1994). Liao and Wong (1984) proposed the extrapolation
boundary condition in elastodynamics which calculates the displacements at the artificial
boundary by extrapolating the data in the interior nodes at earlier times requiring an
estimate of the propagation velocity. Using higher order extrapolation or smaller distance
between the data points, can lead to more accurate results. For frequencies less than the
cut-off frequency, increasing the order of extrapolation does not improve accuracy.
Extrapolation boundary condition is more convenient to be implemented into finite
elements. Later Liao (1996) generalized the original extrapolation boundary condition by
coupling a space extrapolation to the space-time extrapolation and by introducing
multiple artificial wave speeds. Explicit time-integration schemes can only be used to
perform a time-domain analysis. The so-called doubly asymptotic multi directional
transmitting boundary (Wolf and Song, 1995b) combines the advantages of the doubly-
asymptotic and multi-directional boundary conditions. Wolf and Song (1995b) used the
interaction forces rather than displacements in the doubly asymptotic operators and
discretized the boundary condition with a forward difference formula. The static or low-
frequency behavior is modeled using a doubly asymptotic boundary implemented
implicitly. This boundary condition is temporally local but spatially global due to fully
coupled static-stiffness matrix in doubly asymptotic formulation. They used an
approximate banded static-stiffness matrix to construct a spatially local boundary
condition. Kellezi (2000) developed the so called linear cone and cone boundary
conditions for 2D and 3D transient models, respectively, which can be considered as
doubly asymptotic ones and a generalization of the viscous boundary. In constructing
these boundary conditions, it is assumed that the body waves in plane-strain analysis
should propagate radially outward along a cylindrical and hemispherical wave front for
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two- and three-dimensional cases, respectively. In the original high-order transmitting
boundary conditions the order of derivatives in the formulations increases with the order
of the transmitting boundary so that beyond the second order, the implementation in a
finite-element computer program becomes complex and instability may occur. Their
second-order terms are still widely used. (Givoli, 2004) considers these original ones as
low-order transmitting boundary conditions. Introducing auxiliary variables to high-order
transmitting boundary conditions to eliminate higher-order derivatives has recently
attracted interest of many researchers. Most of them have been developed for scalar wave
equations with simple geometry and isotropic and homogeneous materials. For certain
types of waves and geometries of unbounded domains, a two-and three-dimensional
problem can be decomposed into a series of one-dimensional problems. The method of
separation of variables is applicable to the Helmholtz equation in cylindrical and
spherical unbounded domains. Starting from one-dimensional wave equations,
approximate procedures can be constructed. They lead to a system of linear first-order
ordinary differential equations in the time domain. These high-order transmitting
boundary conditions are increasingly recognized as a potential technique for modeling
unbounded domains. They have the potential of leading to accurate results with
increasing orders of approximation. The order of boundary condition can be easily
increased to a desired level. They are local in time but non-local in space. They not only
can produce numerical results of high accuracy but also can be straightforwardly
implemented into finite elements. However, the application of current methods for
constructing high-order transmitting boundary conditions is usually limited to unbounded
domains of simple geometry. The extension to elastic wave propagation in unbounded
domains of arbitrary geometry and material property is not a straightforward task. Here
the literature of the existing high-order transmitting boundary conditions is briefly
reviewed. Grote and Keller (1995a) developed high-order local boundary conditions for
three-dimensional time-dependent scalar wave equations based on spherical harmonic
transformations. These boundary conditions are constructed for three-dimensional
problems as they are based on special properties of the spherical harmonics. Grote and
Keller (1996) implemented the boundary condition developed in Grote and Keller
(1995a) within finite difference and finite-element methods and proved the uniqueness of
the solution and discussed the stability issues associated with their boundary condition.
They later extended the high-order boundary condition to three-dimensional
elastodynamics (Grote and Keller, 2000) and Maxwell equations (Grote and Keller,
1998). Thompson and Huan (2000) rederived the high-order boundary conditions
presented in Grote and Keller (1995a, 1996) to improve the scaling of the related first-
order system of equations. They (Thompson and Huan, 1999, 2000) implemented the
local high-order boundary condition into the standard finite-element method with several
alternative implicit and explicit time integrators. Most recently, Grote (2006) derived a
spatially local formulation for the boundary condition proposed in Grote and Keller
(1998) for three-dimensional time-dependent Maxwell equations. It only involves first
time derivatives and second tangential derivatives of the electromagnetic field and is of
certain auxiliary functions. This new boundary condition does not need any vector
spherical harmonics or inner products with them. It leads to a somewhat easier and
cheaper implementation. Hagstrom and Hariharan (1998) derived local high-order
boundary conditions for two- and three-dimensional time-dependent scalar and Maxwell
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wave equations based on Bayliss and Turkel (1980) operators representing outgoing
solution of the equations. Two-dimensional boundary conditions are asymptotic while the
three-dimensional ones are exact. Huan and Thompson (2000) rederived the sequence of
boundary conditions formulated in Hagstrom and Hariharan (1998) based on the
hierarchy of local boundary operators used by Bayliss and Turkel (1980) and a recursion
relation for the expansion coefficients appearing in a radial asymptotic expansion. They
later in Thompson et al. (2001) extended this idea into two-dimensional scalar wave
equations on a circle. Zhao and Liu (2002) rederived the local high-order boundary
conditions proposed in Hagstrom and Hariharan (1998) for two-dimensional scalar
problems using the operator splitting method. They later in Zhao and Liu (2003) used the
splitting operator method to derive a high-order local boundary condition for a two-
dimensional infinite horizontal layer. Ruge et al. (2001) used a mixed-variable
formulation to transfer the solution of an unbounded domain approximated by a Padé
series in the frequency domain, into a high-order local boundary condition used for the
solution directly in the time domain. The mixed-variable formulation possesses a
continued-fraction form. The technique is applicable to scalar and vector wave equations,
arbitrary geometries and anisotropic and non-homogeneous materials. However, the
dynamic-stiffness matrix has to be specified at discrete frequencies using the global
procedures, for instance boundary element method or the scaled boundary finite-element
method, resulting in a high computational cost. Krenk (2002) derived a high-order
transmitting boundary condition from a rational function approximation of the plane
wave representation for scalar waves. This boundary condition is a modified form of that
proposed by Lindman (1975). It is suitable for the finite-element formulation. Guddati
and Tassoulas (2000) developed a high-order local boundary condition based on
recursive continued fraction of the dispersion relation for scalar wave equations in
Cartesian coordinates. This continued-fraction boundary was limited to straight
computational boundaries. Most recently, Guddati and Lim (2006) extended the
continued-fraction absorbing boundary condition to polygonal computational domains. In
their new derivations, the infinite domain is replaced by a computationally tractable
finite-element mesh to absorb the propagating waves. The infinite domain is recursively
split to an infinite number of finite element layers. Length of each layer is frequency
dependent and determined by choosing reference phase velocities. They found a link
between the continued fraction and the complex coordinate stretching of perfectly
matched layers. Zahid and Guddati (2006) modified the continued-fraction absorbing
boundary condition with adding padding elements to model dispersive waves. Special
techniques were used to discretize the resulting system of evolution equations which are
different form the conventional second-order systems in dynamic problems.
Givoli and Patlashenko (2002) proposed a frequency-domain high-order local boundary
condition for two-dimensional Helmholtz equation based on the localization of the non-
local DtN map in the frequency domain. The boundary geometry is of 2D cylindrical and
2D wave-guide configurations. Givoli and Neta (2003) developed high-order boundary
conditions based on Higdon (1986) boundary condition for both dispersive and non-
dispersive linear time-dependent scalar waves. It was limited to a geometry with a single
plane boundary (wave guide). In his review paper, Givoli (2004) summarizes the key
aspects of different high-order local boundary conditions developed by that time.
Hagstrom and Warburton (2004) generalized Givoli and Neta (2003) boundary condition
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to a full-space configuration and enhanced its stability by deriving corner compatibility
conditions for the auxiliary variable equations. van Joolen et al. (2005) extended the
high-order boundary condition proposed in Givoli and Neta (2003) in unbounded
domains with a rectangular boundary. Kechroud et al. (2005) proposed a high-order
Padé-type non-reflecting boundary condition for two-dimensional acoustic scattering
problems. The boundary condition can be applied on any convex fictitious boundary.
Givoli et al. (2006) incorporated the boundary condition developed in Hagstrom and
Warburton (2004) in a finite-element scheme and compared its performance with the
boundary condition developed in Givoli and Neta (2003).
3.2 Infinite Elements
In the standard finite-element method, it is only possible to discretize a finite part of the
domain. To overcome the difficulty in satisfying the radiation condition at the infinity for
modeling unbounded domains, infinite elements (Bettess, 1992; Astley, 2000) have been
developed. The infinite elements use decay functions representing the wave propagation
toward infinity as the shape functions of the displacements. The decay rate and the phase
velocity must be specified. The form of the shape functions in the unbounded direction is
usually derived from exact solutions of associated one-dimensional wave propagation
problems. Infinite elements can capture only a few propagation modes so that they are
generally not accurate even if the finite-element mesh is very fine. The sequence of
decaying functions may be expressed as reciprocal (1/rn), exponential (1/enr ) or
logarithmic (1/ln r)n types, in the radial coordinate r. The formulation of infinite elements
is spatially local. In this section a summary of the literature for this method is provided.
Bettess and Zienkiewicz (1977) proposed the original unconjugated infinite elements
using the exponential decay functions for radial distance. These infinite elements led to
symmetric discrete problems but were unable to simulate the correct asymptotic decay.
Astley (1983) introduced the so-called wave envelope elements using the complex
conjugate weighting functions in a Petrov-Galerkin scheme, along with mapping for the
exterior problems in acoustics. These infinite elements represent the correct asymptotic
behavior. This technique led to remarkable simplifications in the problem due to
cancellation of the oscillatory terms within integrands but results in local non-symmetric
matrices which destroy the symmetric structure of the semi-discretization of the interior
domains. Zienkiewicz et al. (1983) developed the mapped infinite elements. This
approach incorporates an amplitude decay which is asymptotically correct. The original
infinite elements use cylindrical or spherical boundaries to truncate the exterior domains.
For slender bodies like submarines, truncating the exterior domains using a spherical
boundary leads to a large computational bounded domains to be processed. To tackle this
problem for long and thin bodies, Burnett (1994) developed a novel unconjugated
spheroidal infinite elements in terms of prolate spheroidal coordinates for Helmholtz
equations. In addition to choose of spheroidal coordinate system, separate shape
functions in the radial and transverse directions are used. It leads to analytical radial
integrals. Later Burnett and Holford (1998a,b) extended this approach to ellipsoidal and
oblate acoustic infinite elements. The convergence of the ellipsoidal multiple expansions
is proved. As three axes of an ellipsoid can be chosen independently, an ellipsoid
boundary leads to a small number of meshes in the computational domains. It results in a
greater computational speed than those derived for the spheroidal elements. Shirron and
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Babuska (1998) formulated a conjugated spheroidal infinite element based on the Burnett
formulation and compared various local boundary conditions with infinite elements. They
mentioned that the rate of convergence for the conjugated infinite elements was slower
than the unconjugated ones. Once the domain tends to infinity, the unconjugated infinite
elements diverge from the exact solutions whereas the conjugated ones converge. The
instability of the unconjugated infinite elements is due to the bilinear form on which they
are based.
Astley (1998a) formulated conjugated infinite elements with geometric weight factor 1/r2
and based on Burnett’s spheroidal trial solutions (Burnett, 1994). Astley (2000)
summarized the developments of the infinite elements during 1980s and 1990s and
discussed their merits and drawbacks. Comparing different convergence studies, he
mentions that the unconjugated formulations lead to the most accurate results in the near
field but is limited by ill-conditioning as the radial orders increase. The conjugated
elements, on the other hand, are stable and less accurate in the near fiel dbut converge to
the exact solution in the far field. Astley and Coyette (2001) studied the performance of
the prolate spheroidal infinite elements. They investigated the convergence of these
infinite elements for conjugated and unconjugated test functions. They analyzed
examples for high and low frequencies and also low- and high-aspect ratios. Most of the
developments for the infinite elements have been performed for time harmonic analyses.
They tend to not performing well in a transient analysis since the wave shapes are not
constant and changing with time. Only low radial orders (up to order three) have been
implemented. Astley (1996) extended the conjugated infinite elements into a time-
domain analysis of acoustic problems by taking an inverse Fourier transform of the
discrete infinite element equation in the frequency domain. For conjugated elements, the
coefficient matrices can be written in terms of frequency-independent mass, stiffness and
damping matrices. However, for unconjugated elements this is not the case so that it leads
to convolution integrals. Later Astley (1998b) implemented the transient formulation in
spheroidal coordinate systems. He analyzed several examples to investigate the required
element orders, effect of temporal step size and the performance of the iterative solutions.
Astley and Hamilton (2006) studied the stability of infinite elements for transient acoustic
problems. Numerically mapped elements and analytically formulated spheroidal elements
were considered. In both cases the form of the interface between the finite and infinite
element meshes was shown to be critical in determining whether the transient equations
yield stable solutions.
In summary, the infinite elements use decay displacement shape functions to represent
the wave propagation toward infinity. The decay rate and phase velocity must be
specified. It overcomes the problem of satisfying the radiation condition at the infinity in
the standard finite-element method. However, instability and ill-conditioning problems
are associated with high-order elements. The low-order ones suffer from low accuracy.
The infinite elements do not perform well in a transient analysis.
3.3 Absorbing layers
The absorbing layers are alternatives to local boundary conditions discussed in the
previous sections. They are constructed by replacing the unbounded domain by an
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absorbing layer of finite thickness with the properties that appreciably reduces the wave
reflection into computational domain. Israeli and Orszag (1981) developed the sponge
layers in which artificial material damping is introduced to absorb waves propagating
through the layer. In the damping solvent extraction method (Song and Wolf, 1994), the
effect of the artificial damping on the outgoing waves is extracted leading to higher
accuracy.
Figure 2.5: Perfectly matched layer technique
The perfectly matched layers are the most developed absorbing layers. The theory and
concept of perfectly matched layers (PMLs), was initially introduced by Berenger (1994)
for electromagnetic waves (Maxwell equation). In this technique as shown in Figure 2.5,
the computational domain is surrounded by a finite-thickness layer in which artificial
attenuation of wave propagation in a pre-selected direction pointing to infinity is
introduced to the governing equations for the unbounded domain. As the wave
propagation in the other independent directions is not attenuated, the transmission of
plane waves from the domain of interest to the surrounding absorbing layer is improved.
Propagating waves of all non-tangential angles-of-incidence and of all non-zero
frequencies can be absorbed (Basu and Chopra, 2003). The perfectly matched medium
may be equivalently interpreted as an non-homogeneous viscoelastic medium as material
damping is introduced through the governing equations. Computational domain perfectly
matched layers in the pioneering paper; Berenger (1994) presented a finite-difference
time-domain formulation (FDTD) for 2D electromagnetic split fields.
Later Berenger (1996) extended the perfectly matched layers to three-dimensional
electromagnetic waves. Beranger’s computational domains are Cartesian rectangle and
parallelepiped in two and three dimensions, respectively. It has been demonstrated that
the Beranger’s original split-field formulation is weakly ill-posed (Tsynkov, 1998).
Abarbanel and Gottlieb (1998) used the non-split field components to obtain well-posed
formulations. Perfectly matched layers have been extended to various linear wave
equations: the Helmholtz equation (Qi and Geers, 1998; Harari et al., 2000), the
linearized Euler equations (Hu, 1998) and the wave equation for poroelastic media (Zeng
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et al., 2001). A literature review of perfectly matched layers applied to fields other than
elastodynamics is not covered in this paper.
4. Conclusions
This paper has described in brief, different methods for dynamic analysis of unbounded
domains. Various global and local procedures with particular emphasis on those
developed for elastodynamics are covered. Their mathematical backgrounds, potentials
and limitations are stated. In spite of existence of different techniques for treating
unbounded domains, a reliable and efficient technique applicable to vector wave
equations in unbounded domains of arbitrary geometry and material property does not
exist at present.
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