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SOME ELASTIC MULTI-CRACK AND MULTI-PUNCH PROBLEMS
Qiang Lan
M.Sc., Simon Eraser University, Canada, 1991
M.Sc., Eudan University, Shanghai, China, 1987
A THESIS SUBMITTED IN PARTIAL FULFILLMENT
O F THE REQUIREMENTS FOR T H E DEGREE O F
DOCTOR OF PHILOSOPHY
in the Department of Mathematics & Statistics
@ Qiang Lan 1994
SIMON FRASER UNIVERSITY
June 1994
All rights reserved. This work may not be
reproduced in whole or in part, by photocopy
or other means, without the permission of the author.
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APPROVAL
Name: Qiang Ilan
Dcgrce: Doctor of I'l~ilosopl~y
Title of thesis: Sornc Elas tic Multi-Crack a.rld Multi-Purlcli
I'rohlclns
Examining Committee:
Chairman: Dr. S.K. 'I'honzcnson
Date Approved:
--
Dr. G.A.C. Gmhum
Dr. A. P.S. Selvudulni
I3xtcrna.l Esamincr Professor and Chair, Dcpartmcnt of Civil
Er~ginccring and Applied M d i ~ n i c s McGill University,
Montrcal
June 13, 1994
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PARTIAL COPYRIGHT LICENSE
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h t t o lend
my t h e s i s , p r o j e c t o r extended essay ( t h e t i t
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T i t l e o f Thes is /Pro ject /Extended Essay
Author:
(s igna tu re )
(name)
(date)
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Abstract
In this thesis, two types of problems involving a homogeneous
isotropic linear elastic medium
are studied. The first problem is that of an elastic body, which
could be an infinite solid or a
semi-infinite solid or a layer, containing two or more pardel
penny-shaped cracks whose upper
and lower surfaces are loaded by equal and opposite arbitrary
tractions. The second problem
is concerned with two or more circular punches, whose faces are
of arbitrary shape, indenting
the surface of an elastic layer which rests on a rigid
foundation. Both normal indentation and
tangential indentation are examined.
The method used in this thesis is based on a formulation, which
is very similar to that given
by Muki[24], for general three-dimensional asymmetric elasticity
problems and the superposition
principle of linear elasticity. For example, the solution to the
problem of an elastic layer con-
taining two penny-shaped cracks under arbitrary loadings can be
considered as a superposition
of the solutions to two layer problems, each containing one
penny-shaped crack. Furthermore,
the solution to the problem of a layer weakened by one
penny-shaped crack can be decomposed
into the sum of solutions to two basic problems, namely problem
of an infinite solid containing
one crack and problem of a layer without any crack. With the aid
of the solutions to the basic
problems and the addition formula for Bessel functions, we can
superpose solutions in different
cylindrical co-ordinates and then reduce the original problem to
a system of Redholm integral
equations of the second kind, which can be solved by iteration
for some special cases.
All the solutions given in this thesis can be extended to the
case where the elastic solid
is transversely isotropic. More important, the method used in
this thesis applies to any other
problem if the problem can be decomposed into several basic
problems and analytic solutions to
the basic problems in terms of some potential functions are
available.
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Acknowledgements
This work was initiated and completed under the supervision of
Professor Cecil Graham. The
author wishes to express his deepest gratitude to Dr. Graham for
his guidance, support and
encouragement.
The author would also like to thank Mrs. S. Holmes and Mrs. M.
Fankboner for their help,
and Simon Fraser University for financial support during part of
the writing of this thesis.
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Dedication
To my wife and our parents
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Contents
Abstract . . . . . . . . . . . . . . . . . . . . . . . . . . . .
. . . . . . . . . . . . . . . . iii . . . . . . . . . . . . . . . .
. . . . . . . . . . . . . . . . . . . . . . Acknowledgements iv
. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .
. . . . . . . . . . . Dedication v . . . . . . . . . . . . . . . .
. . . . . . . . . . . . . . . . . . . . . . . 1 Introduction 1
2 Some Three-Dimensional Elastic Problems . . . . . . . . . . .
. . . . . . . . . . . 5 . . . . . . . . . . . . . . . . . . . . . .
. . . . . . . . 2.1 Half-Space Problems 11
. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .
. 2.2 Crack problem 14 . . . . . . . . . . . . . . . . . . . . . .
. . . . . . . . . . 2.3 Contact Problem 18
. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .
. 2.4 Layer Problem 23 . . . . . . . . . . . . . . . 3 Interaction
of Penny-Shaped Cracks in an Elastic Solid 27
3.1 Penny-shaped cracks in an infinite solid . . . . . . . . . .
. . . . . . . . . 27 3.1.1 Derivation of the integral Equations . .
. . . . . . . . . . . . . . 29 3.1.2 Some Asymptotic Solutions . .
. . . . . . . . . . . . . . . . . . . 33
. . . . . . . . . . . . . . . . . . . . . . . . . . . . . .
3.1.3 Discussion 46 . . . . . . . . . . . . . . . . 3.2
Penny-Shaped Cracks in a Semi-Infinite Solid 48
3.2.1 Derivation of integral equations . . . . . . . . . . . . .
. . . . . 48 3.2.2 Some Asymptotic Solutions . . . . . . . . . . .
. . . . . . . . . . 55
. . . . . . . . . . . . . . . . . . . . . . . 3.3 Penny-Shaped
Cracks in a Layer 69 . . . . . . . . . . . . . . . . 3.3.1
Derivation of the integral equations 70
3.3.2 Some asymptotic solutions . . . . . . . . . . . . . . . .
. . . . . 75 . . . . . . . . . . . . . . . . . 4 Interaction of
Circular Punches on an Elastic Layer 84
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. . . . . . . . . . . . . . . . . . . . . . . . . 4.1 Normal
Indentation Problem 85 . . . . . . . . . . . . . . . . 4.1.1
Derivation of the integral equations 86
. . . . . . . . . . . . . . . . . . . . . 4.1.2 Some asymptotic
solutions 87 . . . . . . . . . . . . . . . . . . . . . . . . 4.2
Tangential indentation Problem 90
. . . . . . . . . . . . . . . . 4.2.1 Derivation of the integral
equations 91 . . . . . . . . . . . . . . . . . . . . . 4.2.2 Some
asymptotic solutions 94
. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .
. . . . . . Appendix: Kernels 99 . . . . . . . . . . . . . . . . .
. . . . . . . . . . . . . . . . . . . . . . . . Bibliography
109
vii
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List of Figures
Two parallel penny-shaped cracks in an infinite solid. . . . . .
. . . . . . . . . . . Equal uniform normal loadings: variation of
stress intensity factor 2 with angle B for c j = 0.2 and various f
when a = ii
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3.12 Two parallel penny-shaped cracks in a semi-infinite solid.
. . . . . . . . . . . . . 3.13 Two co-axial cracks with equal
uniform normal loadings: variation of the stress
- intensity factor & and & with respect to f for various
€h. . . . . . . . . . . .
3.14 Two co-axial cracks with equal uniform normal loadings:
variation of the stress -
intensity factor 2 and 2 with respect to 4 for various s. . . .
. . . . . . . 3.15 Two co-axial cracks with equal uniform normal
loadings: variation of the stress
- intensity factor & and 2 with respect to ch for various f
. . . . . . . . . . .
3.16 Two co-axial cracks with equal uniform shear loadings:
variation of the stress -
intensity factor & and $ with respect to f for various Q. .
. . . . . . . . . . 3.17 Two co-axial cracks with equal uniform
shear loadings: variation of the stress
- intensity factor 2 and $ with respect to 4 for various 4. . .
. . . . . . . . .
3.18 Two co-planar cracks with equal uniform normal loadings:
variation of the stress
intensity factor & with respect to : for various y. . . . .
. . . . . . . . . 3.19 Two co-planar cracks with equal uniform
normal loadings: variation of the stress
intensity factor & with respect to f; for various q. . . . .
. . . . . . . . . . . . 3.20 Two co-planar cracks with equal
uniform shear loadings: variation of the stress
intensity factor 2 with respect to : for various y. . . . . . .
. . . . . . . . . . 3.21 Two co-planar cracks with equal uniform
shear loadings: variation of the stress
intensity factor & with respect to f; for various U. . . . .
. . . . . . . . . . . . 3.22 Two co-planar penny-shaped cracks in
the mid-plane of an elastic layer. . . . . . 3.23 Normal loading:
variation of the stress intensity factor &- with respect to 3
at
8 = 0 for various ~f when the boundaries are stress free. . . .
. . . . . . . . . . . 3.24 Normal loading: variation of the stress
intensity factor 2 with respect to f; at
8 = 0 for various ~h when the boundaries are stress free. . . .
. . . . . . . . . . . 3.25 Normal loading: variation of the stress
intensity factor 2 with respect to €1 at
8 = 0 for various 9 when the boundaries are stress free. . . . .
. . . . . . . . . . 3.26 Shear loading: variation of the stress
intensity factor $ with respect t o 9 at
8 = 0 for various ~f when the boundaries are stress free. . . .
. . . . . . . . . . .
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3.27 Shear loading: variation of the stress intensity factor 2
with respect to i at 8 = 0 for various rh when the boundaries are
stress free. . . . . . . . . . . . . . . 81
3.28 Shear loading: variation of the stress intensity factor $
with respect to s j at 8 = 0 for various when the boundaries are
stress free. . . . . . . . . . . . . . . 82
3.29 Normal loading: variation of the stress intensity factor 3
with respect to $ at 8 = 0 for various sf when the layer has fixed
boundaries. . . . . . . . . . . . . . . 82
3.30 Normal loading: variation of the stress intensity factor
& with respect to i at 8 = 0 for various rh when the layer has
fixed boundaries. . . . . . . . . . . . . . . Normal loading:
variation of the stress intensity factor & with respect to s j
at 8 = 0 for various 4 when the layer has fixed boundaries. . . . .
. . . . . . . . . . Variation of the nondimensional resultant force
P, with respect t o $ for various s f . Variation of the
nondimensional resultant moment M, with respect to 4 for var- ious
r j in the case where two punches undergo equal rotational
displacements (in
. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .
. . . . . same direction). Variation of the nondimensional
resultant moment M, with respect to 4 for var- ious sf in the case
where two punches undergo equal rotational displacements (in
. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .
. . opposite directions). Variation of the nondimensional resultant
force P, with respect to 9 for various tzj in the case where two
punches undergo same x-direction displacemets. . . . . Variation of
the nondimensional resultant force P, with respect to $ for various
r j in the case where two punches undergo equal x-direction
displacemets (in opposite
. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .
. . . . . . . directions). Variation of the nondimensional
resultant force P, with respect to $ for various €1 in the case
where two punches undergo same y-direction displacemets. . . . .
Variation of the nondimensional resultant force P, with respect to
3 for various r j in the case where two punches undergo equal
y-direction displacemets (in opposite
. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .
. . . . . . . directions).
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Chapter 1
Introduction
In this thesis, two types of problems involving a homogeneous
isotropic linear elastic medium
are studied. The first problem is that of an elastic body, which
could be an infinite solid or a
semi-infinite solid or a layer, containing two or more parallel
penny-shaped cracks whose upper
and lower surfaces are loaded by equal and opposite arbitrary
tractions. We shall find the stress
intensity factors at the edge of each crack. The second problem
deals with two or more circular
punches, whose faces are of arbitrary shape, indenting the
surface of an elastic layer which rests
on a rigid foundation. We shall find how the existence of the
other punches and the thickness of
the layer affect the total force applied on the punch if the
indentations (normal or tangential)
are given.
Three-dimensional crack problems have received a great deal of
attention in the literature.
A review with a comprehensive list of reference can be found in
Panasyuk et al [25]. In most
of these works, there is only one crack involved. Problems of an
elastic solid containing more
than one crack have received much less attention. Collins[4]
considered the problem of an
infinite elastic solid containing two coplanar cracks which are
subjected to normal loading only.
By equivalenting the problem t o a Neumann problem in potential
theory, he showed that this
problem is governed by an infinite set of Fredholrn integral
equations, which can be solved
approximately by iteration when the spacing between the circular
regions is sufficiently large
compared with their radii. By using Westmann's[34] technique for
solving simultaneous pair
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CHAPTER 1 . INTRODUCTION 2
of dual integral equations, Fu and Keer[ll] extended Collins'
solutions to the case in which
arbitrary shear loadings are applied on the crack faces. As
pointed out by Fabrikant[8], some of
the formulas and results in [ l l ] are incorrect. Based on his
earlier results in potential theory,
Fabrikant [7,8] studied these two loading cases by a different
method. Instead of ending up with
an infinite set of integral equations, he reduced the problem to
a finite set of integral equations
with the number of equations equal to the number of cracks. His
method enables us to obtain
practically exact numerical solutions to the problem, since the
integral equations involved are
non-singular and the iteration procedure is rapidly convergent.
Recently, Xiao, Lin and Liew[35]
presented solutions to the problem of two coplanar penny-shaped
cracks under uniaxial tension
by using the superposition principle of elasticity theory and
Eshelby's [5] equivalent inclusion
method. All these methods fail to deal with off-set cracks,
which will be considered in this
thesis. The only paper we find in the literature dealing with
arbitrarily located penny-shaped
cracks was by Kachanov and Laures[20]. The problems are
dramatically simplified in [20] by
the assumption that the non-uniformities of the traction(with
zero average) on a crack have no
impact on the other cracks. This assumption can be considered as
an instance of Saint-Venant's
principle and allows the authors to find only approximate
solutions even for weak interactions.
The first solution to the problem involving two or more punches
was given by Collins[4]
for the case where the frictionless punches are normally
indenting an elastic half space. It is
shown that this contact problem is equivalent to a Dirichelet
problem in potential theory and
the Dirichelet problem is governed by an infinite set of
integral equations, which can be solved
approximately by iteration when the punches are far away. By
using Galin's[l2] expression for
pressure under the punch caused by a concentrated load at
another point of the half-space,
Gladwell and Fabrikant[l4] derived very simple approximate
relationships among the forces,
moments, and indentations for a system of punches on the elastic
half-space. Later Fabrikant[S]
extended this to elliptic punches. A similar problem (tangential
indentation problem), in which
uniform tangential displacements instead of normal displacement
are prescribed on several elliptic
domains, was solved by Fabrikant[G] using a method based on his
previous result in potential
theory. By employing the mean value theorem, he related the
resulting tangential forces acting
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CHAPTER 1 . INTRODUCTION 3
on each domain to the given displacements through a system of
linear algebraic equations.
Again Collins' and Fabrikant's methods fail when the half-space
is an elastic layer, which will
be considered in this thesis.
The method used in this thesis is based on a formulation, which
is very similar to that given
by Muki[24], for general three-dimensional asymmetric elasticity
problems and the superposition
principle of linear elasticity. For example, the solution to the
problem of an elastic layer con-
taining two penny-shaped cracks under arbitrary loadings can be
considered as a superposition
of the solutions to two layer problems, each containing one
penny-shaped crack. Furthermore,
the solution to the problem of a layer weakened by one
penny-shaped crack can be decomposed
into the sum of solutions to two basic problems, which are
problem of an infinite solid containing
one crack and problem of a layer without any crack. With the aid
of the solutions to the basic
problems and the addition formula for Bessel functions, we can
superpose solutions in different
cylindrical co-ordinates and then reduce the original problem to
a system of Fredholm integral
equations of the second kind, which can be solved by iteration
for some special cases.
All the solutions given in this thesis can be extended to the
case where the elastic solid
is transversely isotropic. More important, the method used in
this thesis applies to any other
problem if the problem can be decomposed into several basic
problems and analytic solutions
to the basic problems in terms of some potential functions are
available. We believe that this is
the first attempt to apply this method in three-dimensional
crack and contact problems, even
though the very same idea has been used by Chen[2] and many
others in two-dimensional fracture
mechanics.
This thesis contains four chapters. In chapter 2 a general
formulation for three-dimensional
linear elasticity is presented. Unlike Muki's formulation, three
harmonic functions instead of
one harmonic function and one biharmonic function are employed.
The advantage of using three
harmonic functions is that the expressions of these functions in
terms of the other cylindrical co-
ordinates can be obtained in a fairly easy way. Several basic
problems involving three-dimensional
elastic solids are then solved by using this general
formulation. These basic solutions will be
used later in chapter 3 and chapter 4.
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CHAPTER 1. INTRODUCTION 4
In chapter 3 interaction of penny-shaped cracks in an elastic
solid is examined. The elastic
solid involved can be an infinite elastic solid, or a
semi-infinite elastic solid, or an elastic layer.
By using the basic solutions given in chapter 2 and the
superposition principle, we reduce the
problem to an infinite set of Fredholm integral equations, which
are then solved for some special
cases. Solutions of the problem for an infinite solid containing
two parallel penny-shaped cracks
are presented in section 3.1, solutions for the semi-infinite
solid case are given in section 3.2
while section 3.3 deals with the layer case. For all three
cases, asymptotic solutions for stress
intensity factors in terms of some small parameters are
obtained. Comparisons are made with
previous results whenever possible.
Chapter 4 is concerned with the interaction of circular punches
on an elastic layer. Both nor-
mal indentation (normal displacement in the contact areas is
prescribed) problem and tangential
indentation ( tangential displacements are given in the contact
areas) problem are considered.
Again it is shown that this indentation problem is governed by
an infinite set of Fredholm in-
tegral equations, which can be solved by iteration for some
special cases. Asymptotic solutions
for resultant forces and moments are also presented in terms of
some small parameters.
-
Chapter 2
Some Three-Dimensional Elastic
Problems
In this chapter a general formulation for three-dimensional
linear elasticity is presented and then
solutions to several three-dimensional elastic problems are
given. These basic solutions will be
used later in chapter 3 when we investigate interaction between
penny-shaped cracks in an elastic
solid and in chapter 4 when interaction between circular punches
on an elastic layer is examined.
General asymmetric three-dimensional linear elastic problems for
a homogeneous, isotropic
half-space or elastic layer were first considered systematically
and solved by Muki [24] using
Hankel transforms. Muki's solution like the symmetrical one, by
Harding and Sneddon[l8], of
which it is a generalization, is based on the expression of the
displacement field in terms of a
harmonic function and a biharmonic function. The simple partial
differential equations for these
two functions are solved by the use of Hankel transforms. Muki's
method applies to any three-
dimensional elastic problem involving an infinite solid, a
semi-infinite solid or a layer. By using
Muki's formulation, the problem can be reduced to the
determination of six functions, which are
to be found by the given boundary conditions of the problem. As
pointed out by Sneddon[31]
that due to some reasons Muki's work does not seem to have
attracted the attention it deserves.
In our formulation, the elastic field of the problem is
expressed in terms of three harmonic
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CHAPTER 2. SOME THREE-DIMENSIONAL ELASTIC PROBLEMS 6
functions instead of one harmonic function and one biharmonic
function. Otherwise the formu-
lation is very much like that given by Muki. The advantage of
using three harmonic functions
becomes clear later when expressions of these functions in terms
of the other cylindrical co-
ordinates are needed.
Problems in the theory of classical elasticity are governed by
Navier equations. If we em-
ploy cylindrical co-ordinates (r, 8, a), the Navier equations in
terms of displacements u, (r, 8, z ) ,
uB(r, 8, z), u,(T, 8, z) in the r, 8, z directions are
where v is Poisson's ratio, e stands for the dilatation
and V2, the Laplacian operator, takes the form
in the cylindrical co-ordinates. It may be verified[21] by
direct substitution that
is a special solution for the Navier equations (2.1)-(2.3), if
4(r, 8, z), +(r, 0, z) and ~ ( r , 8, z)
are harmonic functions. Stress field {a,(r, 8, z), U@(T, 8, z),
az(r, 8, a), T,,(T, 8, z), rgz(r, 8, z),
rre(r, 8, z) ) corresponding to the above displacement field can
then be found. Among these
stresses, the ones of interest are
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CHAPTER 2. SOME THREE-DIMENSIONAL ELASTIC PROBLEMS
where p is the shear modulus of the elastic solid. We may write
the harmonic functions in the
Fourier series of 8 as follows
00
s( r , 8, Z) = C [ d n ( r , z) cos n8 - &(r, Z) sin no],
n=O
00
~ ( r , 8, Z) = C [xn(r7 z) cos n8 - xn(r, z) sin no], n=O
00
$(T, 8, Z) = x [$n(r, z) sin n8 + ( r , Z) cos no]. n=O
Here &(T, z) is the Fourier cosine coefficient of c$(r, 8,
z) and so on. Without loss of generality, - -
we assume &(T, z) = $ n ( ~ , z) = j&(r, z) = 0. The
formulation hereafter remain valid if we write
cos(n8 + $K) = - sin(n8) and sin(n8 + $a) = cos n8 instead of
cos no and sin no. Therefore the solutions corresponding to &,
4, and may be obtained by making the following replacements
cos n8 - sin no; sin n8 a cos no,
Substitution of (2.10)-(2.12) into the displacement field
(2.4)-(2.6) gives the displacements in
00
ur (r, 8 , ~ ) = C U: (r, Z) C O S ( ~ ~ ) , n=O
where the Fourier coefficients ur(r, z), u;(r, Z) and u ~ ( T ,
Z) of the displacement components are
given by
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CHAPTER 2. SOME THREE-DIMENSIONAL ELASTIC PROBLEMS 8
Here, of course, we have used the assumption that &(r, z ) =
'$n(T, Z ) = f n ( r , Z ) = 0. In terms
of & ( T , z ) , $ n ( ~ , Z ) and xn(r , z ) , the
corresponding stresses of interest can be written as
by using equations (2.7)-(2.9). Here the Fourier coefficients
r:(r, z ) , T&(T, Z ) and o;(r, Z ) of the
stress components are given by
The requirements of $(r, 8, z ) to be harmonic function gives us
the following partial differential
equation for c$,(T, z )
which can be solved by Hankel transforms. The kth order Hankel
transform of a function f ( r )
is defined to be
P ( s ) = im 7 - f ( r ) J+)dr, where Jk(rs ) is the kth order
Bessel function of the first kind. Taking the nth order Hankel
transform of the above partial differential equation for
&(r, z ) , we obtain
which is an ordinary differential equation with parameter s and
the general solution for this
equation is
K n ( s , I) = An(s)e-" + &(s)esz.
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CHAPTER 2. SOME THREE-DIMENSIONAL ELASTIC PROBLEMS
Similarly we obtain the general forms for K n ( s , Z ) and z n
( s 7 z ) ,
Here the arbitrary functions An(s) , A , ( s ) , Bn(s ) , B n (
s ) , Cn ( s ) and C n ( s ) are to be determined
from the given boundary conditions of the problem. Once these
six functions have been found, -n
G n ( s , z ) , $Jn ( s , z ) and Z n ( s , z ) are known
functions of z and s and expressions of &(T,z ) ,
& ( T , Z ) and xn(r7 Z ) can be obtained by Hankel inverse
transforms,
and so on. Substituting this into the displacement equations
(2.16)-(2.18), we can rewrite the
displacements in terms of Z n ( s , z) , G n ( s , z ) and Z n (
s , z ) ,
00 azn -n azn up + US = - 1 [ ( I - 2v)+n + Z- - 2JIn + 2(1-
v)zn + z - ] ~ ~ ~ ~ + ~ ( r s ) d s , a2 8~
Here we have used the following properties of Bessel
functions
d n - [ J ~ ( s x ) ] - - J ~ ( s x ) = - S J ~ + ~ ( S X ) , dx
x d n
- [ J ~ ( s x ) ] + - J ~ ( s x ) = s J ~ - ~ ( s x ) . dx x
Similarly we find that the stresses of interest take the
form
agn ax';;" a2zn re", + rz = -2rl~[zg - - 8% +- dz + zT]s2
Jn+l(rs)ds, a2
-', = -2pJ00[ 2-+- a2En 8 K n +- ax';;" + z - ] s ~ J ~ - ~ ( T
s ) ~ s , a2Zn (, a 2 2 az az a z 2
= 1 a2Ln a3Zn assn 1- a,a + z- a23 + z- 8 , IsJn (rs)ds,
from equations (2.19)-(2.21). In terms of An(s), Bn(s ) , Cn(s )
, &(s ) , &(s) and C n ( s ) , the
displacement field becomes
-
CHAPTER 2. SOME THREE-DIMENSIONAL ELASTIC PROBLEMS 10
+ lw [ ( I - 2u + S I ) & ( s ) + (2 - 2u + sr)& ( s ) +
2~ (s) ]s2 Jn- 1 (rs)e"dr, (2.26) 00
U: ( r , I ) = 1 [(2 - 2~ + sr)An ( s ) + ( 1 - 2~ + S Z ) B ~ (
s ) ]s2 Jn (rs)e-.'ds
and the stress field takes the form
It is essential for the method used in this thesis to find the
displacement and stress expressions
in terms of another cylindrical co-ordinate system ( f , 8 , z )
. Let the origin 0 of co-ordinates
( T , 8, Z ) be point ( f , T , 0 ) in co-ordinate system ( f ,
8, z ) and origin 0 of ( f , 8, z ) be point ( f , 0,O) in
co-ordinates ( T , 0, z), where f is the distance between 0 and d.
Let {u i ( f , 8, z ) , uB(f ,8 , z ) ,
placement and stress fields in terms of the new co-ordinates and
{ (u:(f , z ) , u$ ( f , z ) , ug( f , 2 ) ) )
and { @ ( f , I ) , o ; ( f , z ) , u:(f, z ) , T$(T, z ) ,
rFZ(F, z ) , rFB(f, z ) ) be the corresponding Fourier coef-
ficients. With the aid of the addition formula for Bessel
functions as given in Watson[33],
we can express the three harmonic functions in terms of
co-ordinates ( f , 8, z ) as follows:
-
CHAPTER 2. SOME THREE-DIMENSIONAL ELASTIC PROBLEMS
with
Here the prime on the summation sign implies that the
(-l)nJ,,+n(ds) terms do not appear
when n = 0. This shows that the potential functions take the
same form in the two systems
of cylindrical co-ordinates ( T , 8 , z ) and ( F , 8 , z ) .
Therefore it is clear that the displacement and stress components
in terms of co-ordinates ( F , 8, z ) also take the same form as
those in terms of
( ~ 7 '37 z ) as 10% as we replace An(s), Bn(s), Cn(s), An(s)7
Bn(s), Cn( s ) by A:(s)7 B:(s)7 C;t(s)7
En($), g n ( s ) , c n ( s ) and replace T by F . This argument
will be used repeatly in later chapters.
2.1 Half-Space Problems
Problem of an elastic half-space was first considered by
Boussinesq[l] and due to that reason the
half-space problem is sometimes referred to as Boussinesq
problem. If the half-space is taken to
be z 2 0 and the boundary conditions are given on the plane z =
0, then all the displacement
and stress components approach zero as z + oo. Therefore An(s),
&(s) and c n ( s ) have to be
-
CHAPTER 2. SOME THREE-DIMENSIONAL ELASTIC PROBLEMS
zero and the potential functions $(T, 8, z), $(r, 8, z) and X (
T , 0, z) can be written as
The corresponding displacement and stress fields in the
half-space can then be obtained
03
u:(r, Z ) - U; ( r , Z ) = 1 [ ( I - 2. - SZ)A. ( s ) + (2 - 2v
- sz)Bn ( s ) + 2G'.(s)]s2 ~ ~ - ~ ( ~ s ) e - ' " d s , ( 2 . 4 4
)
and
roo
Now we have reduced the half-space problem to the determination
of three functions A,(s),
B,(s) and C,(s), which will be found by the given boundary
conditions of the problem. In this
section, we consider two different boundary conditions.
Half-space problem 1 (Problem HI)
Problem H1 is that of an elastic half-space with tractions
applied on the surface of the
half-space. Boundary conditions of this problem can be written
as
where F,(r), G,(r) and H,(r) are some given functions. Imposing
these boundary conditions
on the stresses (2.46)-(2.48) and using the definitions of
Hankel transform and its inverse, we
-
CHAPTER 2. SOME THREE-DIMENSIONAL ELASTIC PROBLEMS
obtain three linear equations for An(s) , Bn ( s ) and Cn(s) .
Solutions for these equations are
This enables us to obtain, from (2.46)-(2.48), the stresses in
the half-space W n n -n+l n n - l
( T , Z ) = sJn (TS)e-" [(2 + 281) Fn ( s ) - szGn ( s ) - s1Hn
( s ) ] ~ s ,
which can be rewritten in a little shorter form
1 n n n n + l n n - 1 *"(s, Z ) = -e-" [(2 + 2sz)Fn ( s ) - S Z
G ~ ( s ) - szHn ( s ) ] , (2.52)
2 n n + l n n + l 1 n+l n-1 T ( s , ) + r Z ( s , z ) = - ~ - "
[ ~ s z ~ ~ ( s ) + ( ~ - s z ) G ~ ( s ) - s r H n ( s ) ] ,
(2.53)
2 n n - 1 n n - l 1 n n n n + l -n-1 re", ( s , z ) - T & (
s , z ) = - ~ - ~ ~ [ ~ s z F ~ ( s ) - s z G ~ ( ~ ) + ( 2 - S Z )
H ~ (s)]. (2.54)
2
These solutions will be used later in section 3.2 when we study
interaction of penny-shaped
cracks in a semi-infinite elastic solid with stress free
surface.
Half-space problem 2 (Problem H2)
Problem H2 is that of an elastic half-space with displacements
given on the surface of the
half-space. Boundary conditions of this problem can be written
as
where Un(r) , Vn ( r ) and W n ( r ) are some given functions.
Similarly we can express An(s) , B,(s)
and Cn(s ) in terms of these functions and then obtain the
stresses of interest in the half-space
-n n n + l u: ( s , z ) = -- ps e- lZ[(1 - 2v - sz )un ( s ) 3 -
4v
-n -n-l +(4 - 4 v + 2sz)Wn (s) - ( 1 - 2v - sz)Vn ( s ) ] ,
n n + l -n+l -n " e-Sz[(2sz + 2 - 4 v ) w n ( s ) T&
(s,z)+r,", ( s , z ) = - - 3 - 4v
-
CHAPTER 2. SOME THREE-DIMENSIONAL ELASTIC PROBLEMS
2.2 Crack problem
Now let us consider a problem, which will be referred to as
problem C later on, of an infinite
elastic solid containing a penny-shaped crack C whose upper and
lower surfaces are loaded by
equal and opposite arbitrary tractions. We choose a cylindrical
co-ordinates (r, 8, z) such that
this crack is taken to occupy
Z = O , r < a , o < o < ~ T .
In order to have a stress field which is consistent with the
symmetry of the potentials (2.40)-
(2.42), we assume that the arbitrary tractions on the crack face
take the form CO
g.z ( r7 47 0) = C an ( r ) cos(n6) 7 (2.55) n=O
00
~ r r ( ~ 7 87 0) = C bn(r) cos(n8) (2.56) n=O 03
roz(r7 8,O) = C cn(r) sin(n8). (2.57) n=O
This crack problem has been studied by many researchers. Among
them are Sneddon [30] for
the axisymmetric loading, Kassir and Sih[2l] and Guidera and
Lardner[lS] for general loadings.
Kassir and Sih7s solutions are quoted here. Without loss in
generality the arbitrary loadings
(2.55)-(2.57) applied on the crack surfaces may be resolved into
symmetrical (corresponding to
normal loading) and skew-symmetrical (corresponding to shear
loadings) parts with respect to
the crack plane. For clarity, these two parts are treated
separately.
Normal Loadings If the crack faces are subject to normal loading
only, then the crack problem
is symmetric with respect to the crack plane z = 0 and we need
only to find the displacement
and stress distributions in the upper half-space z 2 0.
Therefore formulas (2.43)-(2.48) for the
-
CHAPTER 2. SOME THREE-DIMENSIONAL ELASTIC PROBLEMS 15
half-space problem can be used to solve this crack problem. The
boundary conditions of the
problem can be written as
The first boundary condition gives us Bn( s ) = Cn(s ) = 0 , and
the remaining boundary conditions
lead us to the following dual integral equations for An(s )
,
If we assume that An( s ) is given by the following integral
where a l ( t ) is a function to be determined on interval 0
< t 5 a, then it is shown that integral equation (2.59) is
automatically satisfied with the aid of identity
Substituting (2.60) into equation (2.58), we end up with an
integral equation for @l(t)
after changing the order of integration. Solution of this
integral equation is
Here we have used the following two formulas for the Bessel
functions
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CHAPTER 2. SOME THREE-DIMENSIONAL ELASTIC PROBLEMS
Solution for a l ( t ) and the assumption (2.60) enable us to
obtain
Therefore we can find the three harmonic functions and determine
the displacement and stress
fields in the upper half-space of this problem by equations
(2.43)-(2.48).
Shear loadings If the crack faces are subjected to shear
loadings only, then the crack problem
is skew-symmetric with respect to the crack plane z = 0 . Again
we only need to find the stress
and displacement field in the upper half-space z > 0 . In
this case equations (2.43)-(2.48) are still valid. The boundary
conditions of this problem can be written as
The first boundary condition gives us An(s ) = 0 and the
remaining boundary conditions lead us
to Co(s) = 0 and the following dual integral equations for Bo(s
)
when n = 0 and simultaneous pairs of dual integral equations for
B n ( s ) and C n ( s )
when n > 1. Dual integral equations (2.64)-(2.65) can be
solved by using the same technique as for the normal loading. It is
seen, by comparing these equations with equations (2.58) and
-
CHAPTER 2. SOME THREE-DIMENSIONAL ELASTIC PROBLEMS
(2.59), that Bo(s) is the same as Al (s) with al(x) replaced by
-bl(x), and therefore
Solutions for the simultaneous pairs of dual integral equations
(2.66)-(2.69) can be obtained by
using Westmann7s[34] technique. They are
with
Bn(s) and Cn(s) together with An(s) = 0 enable us to find the
potential functions and then the
displacement and stress field in the upper half-space.
Superposing the solutions for the normal loading and shear
loadings results the solutions
for the crack problem (Problem C ) under arbitrary loading
(2.55)-(2.57). The displacements
and stresses of interest for the upper half-space(z 2 0) are
given by (2.43)-(2.48) with An(s)
given by (2.63), Co(s) = 0, Bo(s) given by (2.70), and Bn(s) and
Cn(s) given by (2.71) and
(2.72) respectively. By using the symmetry of the normal loading
crack problem and the skew-
symmetry of the crack problem under shear loading, the
displacements and stresses of interest
in the lower half-space ( z < 0) can also be found. In terms
of the very same An(s), Bn(s) and Cn(s) (rather than An(s),
&(s) and Cn(s)),
the elastic field in the lower half-space takes the following
form
u:(r, Z ) + u ~ ( T , Z ) = [ ( 2 ~ - 1 - S Z ) A ~ ( S ) + ( 2
- 2~ + S Z ) Bn ( s ) - 2Cn(s)] Jn+l (rs)eSzds, (2.75) 1" u:(r, z )
- u;f(r, z ) = [ ( I - 2v + sz)An ( s ) + (2v - 2 - sz) Bn ( s ) -
2Cn(s)] J n - l ( ~ ~ ) e " d ~ s , (2.76) 1"
-
CHAPTER 2. SOME THREE-DIMENSIONAL ELASTIC PROBLEMS 18
This solution together with the elastic field (2.43)-(2.48) in
the upper half-space will be used
repeatly in chapter 3 when we examine the multi-crack problems.
In deriving the integral
equations for the multi-crack problems, expressions for the
elastic field in terms of another
cylindrical co-ordinates ( f , 8, z) are also required. This
task can be accomplished by using the
arguments right before section 2.1.
In linear elasticity fracture mechanics, stresses have
singularities of the form ( r - a)-'I2 along
edge of the crack. Stress singularity factors are the most
important parameters and concepts in
linear fracture mechanics. If the stress intensity factors are
defined by
kl = lim \/2(r - a) cz(r, 8, O), r+a
k2 = lim 4 2 ( r - a) r,,(r, 8, O), ?-+a
k3 = lirn 4 2 ( r - a) ss,(r, 8, O), r+a
then in terms of the given loadings applied on the crack faces
they are
00
2~ 2 112 k3 = - -(-) [(1 - u)@2(a) f %(a)] sin(n8). a n=1
It is clear that the intensity factor kl of stress u,(r, 8, z)
is dependent on an(x) only and that k2
and k3 have nothing to do with a,(x) due to the geometric
symmetry of the problem.
2.3 Contact Problem
Contact problems or indentation problems are related to the name
of Hertz, who first in 1882
successfully treated a static contact problem. This section is
concerned with two indentation
-
CHAPTER 2. SOME THREE-DIMENSIONAL ELASTIC PROBLEMS 19
problems, namely normal indentation problem and tangential
indentation problem for an elastic
half-space. The normal indentation problem can be described as
an rigid punch of arbitrary
shape indenting a lubricated elastic half-space z 2 0. The shear
stresses on the contact plane
z = 0 are zero and the normal displacement in the contact region
is prescribed. The tangential
indentation problem can be interpreted either as that of two
elastic half-space interconnected
by the contact region and subjected to remote shear loadings, or
as a contact problem with a
flexible punch connected to the half-space such that there is no
normal stress on the contact
surface and the tangential displacements in the contact region
are given.
Normal indentation problem (Problem 11)
Problem I1 is that of a half-space z > 0 indented by a
circular cylinder punch with arbitrary preface. If the radius of
the punch is a and the shape of its preface can be expressed by a
function
with Fourier cosine coefficients fn(r), then boundary conditions
for this problem can be written
as
This contact problem has been studied by many researchers, for
example, Sneddon[BO] for the
axisymmetric case and Muki[24] for the asymmetric case. It can
also be treated by formulas
(2.43)-(2.48). The shear stress boundary conditions give us
Bn(s) = Cn(s) = 0 and the remaining
boundary conditions lead us to a dual integral equation for
An(s)
If we assume that
Pl (t) Jn-1/2(~t)dt,
then integral equation (2.84) can be rewritten as
-
CHAPTER 2. SOME THREE-DIMENSIONAL ELASTIC PROBLEMS
after using the following property for Bessel function
Now we can see, from identity (2.61), that integral equation (2
.84) is automatically satisfied and
equation (2.85) becomes to an Abel's integral equation for !PJ(
t )
after changing the order of integration. Solution for this
Abel's integral equation is
which enables us to find A n ( s ) from (2 .86) and then the
displacement and stress fields from
equations (2.43)-(2.48).
Tangential indentation problem (Problem 12)
Problem I2 is that of a half-space z 1 0 indented by a flexible
circular punch so that the
normal stress is zero on the whole contact surface z = 0 and the
tangential displacements are
given in the contact region. If the radius of the punch is a and
the tangential displacements can
be expanded as Fourier series, then boundary conditions for this
problem can be written as
where gn(r) and h n ( r ) are given functions determined by the
Fourier coefficients of the prescribed
displacements. Unlike the bonded punch problem considered by
Gladwell[l3], the tangential
indentation problem defined here is very similar to that studied
by Fabrikant[lO]. This problem
can be reduced to a system of a pair of integral equations by
using formulas (2.43)-(2.48) for the
half-space problem. The normal stress free boundary condition
gives us A n ( s ) = 0 and aJl the
other boundary conditions lead us to Co(s) = 0, a dual integral
equations for Bo(s )
-
CHAPTER 2. SOME THREE-DIMENSIONAL ELASTIC PROBLEMS
when n = 0 and a pair of simultaneous integral equations for
Bn(s) and Cn(s)
when n 2 1. By comparing the dual integral equation for Bo(s)
with the one for An(s) in
the normal indentation case, we find that Bo(s) is the same as
Al(s) with fl(r) replaced by
-go(r). As for the simultaneous pair dual integral equations for
Bn(s) and C,,,(s), again we use
Westmann's[34] method. If we assume that
then we can show that equation (2.90) is automatically satisfied
with the aid of identity (2.61).
Replacing Jn-3/2(~t) and Jn+llz(st) in equation (2.91) by
and applying indentity (2.61) again, it is shown that integral
equation (2.91) is also satisfied.
Substituting equations (2.92) and (2.93) into (2.89) and
changing the order of integration lead
to a Abel's integral equation for Q2(t) with solution
Now it remains to satisfy equation (2.88), which can be
rewritten as
la Q(t)dt J m Jn+l (rs) Jn-1/2(st)ds = gn(r> 0 2
-
CHAPTER 2. SOME THREE-DIMENSIONAL ELASTIC PROBLEMS
by using the same technique applied for (2.91). Here
Making use of identity (2.61), we can rewrite (2.95) as an Abel
integral equation for Q(t).
Solutions of this Abel equation for Q(t) in terms of gn(x)
result
after some integrations. The result as well as the solution
procedure presented here will be
used later in chapter 4 when we study the two punch tangential
indentation for an elastic
layer. Reference for tangential indentation problem of an
elastic half-space can also be made to
Fabrikant[lO] where a different method is used.
As an example, we consider the case where the flexible punch
undergoes a unidirectional
displacement u,(T, 8,O) = A and U ~ ( T , 8,O) = 0. Therefore
the displacement components in
the cylindrical co-ordinates are u,(T, 8,O) = A cos 8 and u ~ (
T , 8,O) = -A sin 8 and all gn(r) and
hn(r) are zero except hl(r) = 2A. Then it is not hard to
find
Substituting these two fuctions into (2.92) and (2.93) and then
using the stress field expressions
(2.46)-(2.48), we obtain
In terms of Cartesian co-ordintaes (x, y, z), the stresses
are
Like the bonded punch problem[l3] and the rigid disk inclusion
probelm[27], the stress has
singularity of the form (T - at the boundary of the contact
region.
-
CHAPTER 2. SOME THREE-DIMENSIONAL ELASTIC PROBLEMS
2.4 Layer Problem
In this section, several layer problems are examined by using
the general formulation for three-
dimensional asymmetric elastic problems given in the first part
of this chapter. Generally, in
this case, none of An(s), Bn(s), Cn(s) and &(s), Bn(s),
C,(s) in equations (2.25)-(2.30) is zero.
Layer problems have been studied by many researches and
references can be made to Lur7e[23]
and also to Muki[24].
Layer Problem l(Prob1em L1)
Problem L1 is that of an elastic layer - h < z < h with
tractions prescribed on the layer surfaces. Boundary conditions for
this problem can be written as
where the upper signs correspond to the upper layer surface z =
h and the lower signs correspond
to z = -h and F,~(T), G,f(r) and H,~(T) are given functions
determined by the stress boundary
conditions. By using equations (2.25)-(2.30), these six boundary
conditions lead us to six linear
algebraic equations for An(s), Bn(s), Cn(s) and An(s), B,(s),
Cn(s). Solutions for these six
equations enable us to find the stresses in the layer. In this
thesis, it is only required the stresses
in the mid-plane of the layer. The Hankel transforms of these
stresses take the form
-n sh sinh(sh) -n+l -n+l -n-1 e n - 1 "' O ) = 2[2sh + sinh
(2sh)l x [G,f ( s ) - G; (a) + Hz ( s ) - HG ( s ) ] sh cosh (sh) +
sinh (sh) -n
+ 2sh + sinh (2sh) x [F$ ( s ) + F: ( s ) ] , (2.101) n n + l n
n + l -sh sinh(sh) -n -n .a", ( s , + = -2.h + sinh(2sh) x [F$ ( s
) - FL ( s ) ]
-sh C O S ~ ( S ~ ) + sinh(sh) -n+l -n-1 -n-1 + 2[-2sh +
sinh(2sh)l x b,f ( s ) + G; ( s ) + Hz (4 + HG ( s ) ]
1 -n+l -n+l -n-1 -n-1
'4 cosh(sh) x [c,f ( s ) + G; ( 6 ) - Hz ( 6 ) - HL ( s ) ] ,
(2.102) -n-1 -n-1 -sh sinh(sh) -n -n re", (s,O) - T,", ( s , 0 ) =
-2sh + sinh(2sh) x [FZ ( s ) - F; ( a ) ]
-sh cosh(sh) + sinh(sh) -n+l -n-1 -n-1 + 2[-2sh + sinh(2sh)l x
b,f ( 8 ) + GZ ( s ) + Hz (8) + HG ( s ) ]
-
CHAPTER 2. SOME THREE-DIMENSIONAL ELASTIC PROBLEMS 24
1 -n+l -n+l -n-1 -n-1 - 4 cosh(sh) X [ct (s) + C; (s) - HZ (s) -
Xi (s)] . (2.103)
This solution will be used later in section 3.3 when we
investigate interaction of penny-shaped
cracks in the mid-plane of a layer with stress free
surfaces.
Layer Problem 2 (problem L2)
Problem L2 is that of a layer -h < z 5 h with displacements
given on the two surfaces of the layer. Therefore the boundary
conditions take the form
In the same way as for problem L1, the stresses in the mid-plane
of the layer can be found
+ -n+l n n + l re", +T& (s,O) =
+
+ -n-1 -n-1 r& - T:~ (s, 0) =
+
- ps[(l - 2p) sinh(sh) - sh cosh(sh)] -2sh + (3 - 4v)
sinh(2sh)
-n+l -n+l -n-1 -n-1 x [v.+ (s) - u (s) + v2 (s) - v; (s)] ps[2sh
sinh (sh) + 4(1- v) cosh(sh)] -n
-2sh + (3 - 4p) sinh (2sh) ps[(-2 + 4v) sinh(sh) - 2sh cosh(sh)]
-n
2sh + (3 - 4v) sinh(2sh) x [w.+ (s) + wi- (s)]
-n+l -n+l -n-1 -n-1 's X [.,+ (6) + u; (s) - v (6) - v; is)] , 2
sinh(sh)
p[(-2 + 4v) sinh(sh) - 2sh cosh(sh)] -n 2sh + (3 - 4v) sinh(2sh)
x [w,+ (8) + w; (s)]
-n+l -n+l -n-1 -fa-1 x [u.f (s) - u; (8) + v2 (s) - v (s)]
We will need this solution later in section 3.3 when we examine
interaction of cracks in the
mid-plane of a layer with fixed surfaces.
-
CHAPTER 2. SOME THREE-DIMENSIONAL ELASTIC PROBLEMS
Layer Problem 3 (Problem L3)
Problem L3 is that of an elastic layer 0 5 z < h with given
normal stress applied on the top surface z = 0 and the layer rests
on a frictionless rigid foundation. Therefore boundary
conditions for the problem can be written as
on the top surface and
u:(r,h) = 0, r&(r,h) = r&(r,h) = 0,
on the bottom surface, where Pn(r) is the Fourier coefficients
of the given normal stress. In
chapter 4 of this thesis, we are only interested in the
relationship between the normal indentation
on surface z = 0 and the applied stress. In terms of An(s),
B,(s) and &(s), Bn(s), this
relationship takes the form
Imposing the mixed boundary conditions on the elastic field
equations (2.25)-(2.30), we again
get six linear algebraic equations for An(s), Bn(s), Cn(s) and
&(s), B,(s), Cn(s). From these
equations, we find
where A,(s) is the nth order Hankel transform of the pressure
Fourier coefficients P,(T) and
function Kl(x) is given by 1 + x - e-"
K1(x) = x + sinh(x) ' Therefore the relationship between the
normal displacement on surface z = 0 and the applied
stress can be rewritten as
-
CHAPTER 2. SOME THREE-DIMENSIONAL ELASTIC PROBLEMS 26
Considering that An(s) is determined by An(s) and &(s) only,
the above expression in terms of
co-ordinates ( T , 8, Z) can also be written in terms of
co-ordinates (F, 8,z) by using the arguments
right before section 2.1. It becomes to
where A*,(s) is determined by An(s) in the same way as A:(s) by
An(s).
Layer Problem 4 (Problem L4)
Problem L4 can be described as: an elastic layer 0 5 z < h
with given shear stresses applied on the top surface z = 0 and the
layer is bonded with a rigid foundation on the bottom surface
z = h. Therefore boundary conditions of this problem are
Again we are only interested in the relationships between the
resulting tangential displacements
on the surface z = 0 and the applied shear forces. In the same
way as for the normal indentation
problem, we find
with
and functions K2(x) and K3(x) given by
In the same way as for equation (2.107), expressions for the
above relationships in terms of
co-ordinates ( f , g, z ) can also be found. Solutions for
problem L3 and problem L4 will be
used in chapter 4 when we investigate interaction of circular
punches on an elastic layer.
-
Chapter 3
Interaction of Penny-Shaped Cracks
in an Elastic Solid
In this chapter, we shall study the problem of an elastic solid
containing one or more parallel
circular cracks. The elastic solid involved can be an infinite
elastic solid, or a semi-infinite elastic
solid, or an elastic layer and its boundary surfaces, if any,
are parallel to the crack faces. It is
shown that the problem of an elastic solid containing two
penny-shaped cracks can be reduced to
a system of Fredholm integral equations of the second kind by
using some of the basic solutions
given in chapter 2 together with the superposition principle of
the linear elasticity and the
addition formula for Bessel functions.
3.1 Penny-shaped cracks in an infinite solid
Problems concerning interaction between penny-shaped cracks in
an infinite solid have only been
studied for the cases in which the cracks are either co-axial
[3, 261 or co-planar [4, 7, 8, 111 with
only one exception by Kachanov and Laures[20] in which
interaction of arbitrarily located penny-
shaped cracks is investigated. The problem is dramatically
simplified in [20] by assuming that
the non-uniformities of the traction(with zero average) on a
crack have no impact on the other
cracks. This assumption can be considered as an instance of
Saint-Venant's principle and allows
-
CHAPTER 3. INTERACTION OF PENNY-SHAPED CRACKS ...
the authors to find only approximate solutions even for weak
interactions.
I . this section we shall study the interaction of two
arbitrarily located parallel cracks C and
C in an infinite solid. It is assumed that radii of the two
cracks involved are a and ii respectively. We choose two similarly
oriented cylindrical co-ordinate systems ( r , 8, z ) and (F, 8, Z
) such that
cracks C and are taken to occupy
respectively. The origins 0 and 0 of these two coordinate
systems are the points (f, 0 , g ) and (f, R, -g) in these
respective sets of co-ordinates. Here f and g are the horizontal
and vertical
distances between the centers of the cracks as shown in figure
3.1.
Figure 3.1: Two parallel penny-shaped cracks in an infinite
solid.
On the crack faces tractions are prescribed and can be expanded
in Fourier series. To be
compatible to the displacements given by (2.13)-(2.15), the
tractions are assumed to take the
-
CHAPTER 3. INTERACTION OF PENNY-SHAPED CRACKS ...
form
on crack face C and take the form
on crack face c. Here Rn(r) is the Fourier cosine coefficient of
stress r,,(r, 8,O) on the crack face C and so on. We shall find the
stress intensity factors at the perimeter of these two cracks.
3.1.1 Derivation of the integral Equations
Instead of solving this problem directly, we consider two easier
problems: one is problem C
of an infinite solid containing just one crack C with arbitrary
tractions (2.55)-(2.57) (they are
unknown at this time) loaded on the crack faces and the other is
problem c of an infinite solid containing crack 6 with unknown
tractions
applied on the crack faces 6. It is clear that solutions to the
original problem can be represented as a superposition of the
solutions for these two easier problems as long a s this
superposition
-
CHAPTER 3. INTERACTION OF PENNY-SHAPED CRACKS.. . 30
satisfies the given boundary conditions on the two crack faces.
It will be shown that the original
problem can be reduced to a system of Fredholm integral
equations for these Fourier coefficients
an(z), bn(z), cn(z) and Cn(z), L(x ) , En(z).
In deriving the integral equations, we require not only the
expressions for the stress field
of problem C in terms of co-ordinates (r, 8, z) but also the
expressions in terms of (F, 8 , ~ ) .
In order t o do this, we introduce an auxiliary co-ordinates
system (F, 8, z). Let {u,(r, 8, z ) ,
U O ( ~ , 4 4, uz ( r , 8 , ~ ) ~ rrz(r, 8 , ~ ) ~ 7ez(r19,z), m
( r , 9 , ~ ) ) and {+, 8, z ) , u#(T, 8 , z ) , g Z ( ~ , g , ~ )
, T F ~ ( T , 8, z ) , r,-,(i;, 8, z ) , ri-,-(F, 8, a ) ) be the
stress field of the problem C in terms of (T , 8, z) and (F, 8, z)
re-
spectively and {u,"(r, z ) , u$(r, z ) , u,"(r, z ) , r,", ( r ,
z ) , r,",(r, z ) , r,",(r, z ) ) and {u;(F, z ) , g ; ( ~ , z ) ,
g , " ( ~ , z ) ,
r,?Z(F, z ) , rE(i;, z ) , rig(?, z ) ) be the corresponding
coefficients. Furthermore, expressions for the
stress field of problem c in terms of (F, 8, t) and (r, 8, z)
are also required. Introduce another auxiliary co-ordinates system
(r, 8 , t ) and let { Z i , n ( ~ , z ) , ~ ; ( t , z ) , a ; ( ~ ,
z ) , ?$(F, Z ) , . f&(F, Z ) , ? i B ( F , 5) ) and {8F(r, Z )
, ar (r , z ) , Fg(r, Z ) , ?:Z(r, z ) , ?Fz(r, z ) , ~-2 ( r , 2))
be the corresponding stress coeffi- cients in terms of (F7 8 , t )
and (r, 8 , t ) respectively. Then the stress boundary conditions
can be
rewritten as
on crack C and
on crack face C. The expressions of the stresses of problem C in
terms of (r, 9, z ) are given by (2.46)-(2.48)
in the upper half-space z > 0 and (2.78)-(2.80) in the lower
half-space z 5 0. By using the arguments given in chapter 2 and the
basic solutions (2.46)-(2.48), we find that the stress field
-
CHAPTER 3. INTERACTION OF PENNY-SHAPED CRACKS.. .
in terms of ( f , 8, z ) takes the form
in the upper half-space z 2 0 . Similarly the expressions of the
stress field of problem c in terms of both co-ordinates
( f , 8 , ~ ) and ( T , 8,Z) can be found. In terms of ( f , 8,
E), the stresses are given again by (2.46)- (2.48) in the upper
half-space E 2 0 and (2.78)-(2.80) in the lower half-space E 5 0
with T , 8 , z , An(s) , Bn(s ) , Cn( s ) replaced by f , 8, E,
&(s ) , Bn(s ) , Cn( s ) . From (2.78)-(2.80), we obtain
the
stress field in terms of co-ordinates (T , 8,Z)
Ttt(r , f ) + TFt(~ , f ) = 2p [ - s f $ , ( s ) + ( 1 + s f ) B
; ( S ) - C ; ( S ) ] S J ~ + ~ (r s )es zds , (3.19) 1" 03
( T , 2) = 2 1 [ ( I - s i ) A ; ( s ) + s ~ B ; ( s ) ] s J ~
(rs)es"ds, (3.21) in the lower half-space 5 0. Here r?;(s), B:(s)
and R ( s ) are given by
and An(s) , Bn( s ) and Cn(s ) are determined by ~i , ( z ) ,
6,(z) and Zn(x) in the same way as those
of An(s), Bn(s) and Cn(s) by an(z ) , bn(z), cn(z)-
Substituting of the above stress expressions into equations
(3.10)-(3.15) and changing the
order of integrations lead us to a system of six integral
equations, three on each crack. On the
face of crack C , they are
-
CHAPTER 3.
+ -
b o ( ~ ) -
+ +
~ o ( f ) =
if n = 0 and
INTERACTION OF PENNY-SHAPED CRACKS.. . 32
if n > 1. On the crack face C?, the same integral equations
are found with a n ( x ) , b n ( x ) , c n ( x ) and i in(x) ,
&, (x) , En(x) interchanged, a and ii switched and (-1)"
replaced by ( - l ) n . Kernels
of these integral equations are given in the Appendix. Now we
have reduced the problem to a
system of six integral equations for a n ( x ) , bn(x) , c n ( x
) and i in (x) , 6 , (x ) , G ( x ) , the coefficients
of the stresses on the faces of the isolated crack in an
infinite solid. Since the stress singularities
-
CHAPTER 3. INTERACTION OF PENNY-SHAPED CRACKS ... 33
for crack C are only dependent on the tractions applied on the
faces of the isolated crack C in
an infinite solid, therefore these tractions will be called
effective stresses and their coefficients
an(x), bn(x), cn(x), will be referred to as coefficients of the
effective stresses for crack C from
now on and 7in(x), 6,(x), Zn(x) will be referred to as the
effective stresses for crack c. The above integral equations,
though formidable looking, can be solved by iteration for some
special cases.
3.1.2 Some Asymptotic Solutions
In this subsection, we shall solve the above integral equations
for some special cases. Without
loss of generality, we assume the two cracks have equal radii a
and we will only consider two
cases. In the first, the horizontal distance f between these
cracks is large compared with their
radii a while in the second the horizontal distance is zero and
the vertical distance g is large
compared with a. In each case two different loadings, namely
equal uniform normal loadings and
equal(in the same direction or the opposite direction) uniform
shear loadings are considered.
CASEONEa=Si
-
CHAPTER 3. INTERACTION OF PENNY-SHAPED CRACKS.. .
for n 2 1.
Considering that the above integral equations (except equation
(3.34)) are infinitely long for
each given n, and also that there are infinitely many these
integral equations (n = 0,1,2, ...),
generally these integral equations cannot be solved by using
numerical methods before some
significant simplifications.
From the kernels given in the Appendix, we can see that all the
kernels can be expanded as
power series of e j = 4 , the ratio of the crack radii to the
horizontal distance. It is also seen
-
CHAPTER 3. INTERACTION OF PENNY-SHAPED CRACKS ... 35
that Knm33 is of order 0 ( € 7 m + n ) 7 Knmls and Knmll are of
order O(rFm+"), Knml17 Knmz3
and Knm32 are of order o ( c ; + ~ + ~ ) , Knm12 and Knmzl are
of order O ( C ? + ~ + "), and Knm22 is
of order 0 ( r 7 ~ + ~ ) when n 2 1. By using this observation,
we obtain the following: to get
solutions correct to order O(ry), we can truncate all the terms
with m 2 N - 1 to make each
equation finitely long, and neglect all the integral equations
if n 2 N - 2. The resulting finite
set of Fredholrn integral equations, each of which are finitely
long now, can be solved iteratively
by expanding all the kernels involved in terms of power series
of ef and neglecting all the terms
with order higher than N.
In order to obtain the solutions correct to order 0($), we can
neglect such terms that m 2 5
and only solve the first five equations. The non-zero terms of
the solutions are
bo(xa) =
al(xa) =
c1 (xu) + b i (xu) = cl (xu) - b l (xu) =
-
CHAPTER 3. INTERACTION OF PENNY-SHAPED CRACKS ...
which involve integrals 03
C = 1 y m ~ n ( y ) e - ~ d y . These integrals can be expressed
in terms of Gamma functions and the hypergeometric function
as given in [29]
The integrals IF can be evaluated numerically either using the
Gauss-Laguerre formula or using
the above formula and truncating the Hypergeometric function.
The stress intensity factors can
then be found from (2.81)-(2.83)
-
CHAPTER 3. INTERACTION OF PENNY-SHAPED CRACKS ...
The numerical results for these stress intensity factors are
shown graphically in figures 3.2-3.8.
There klo is the intensity factor for stress o,, due to a single
isolated crack subject to the uniform
normal loading P in an infinite solid. Later we will use k20 to
express the stress intensity factor
for a penny-shaped crack in an infinite solid under uniform
radial shear loading.
From figure 3.2 we can see that the effect of the angle 8 on the
stress intensity factor kl is
fairly small when cf is s m d , say no larger than 0.25. Figure
3.3 (cf = 0.45) does indicate that
the angle 8 has a significant effect on the stress intensity
factor when €3 is large.
Figure 3.2: Equal uniform normal loadings: variation of stress
intensity factor & with angle 0 for cf = 0.2 and various f when
a = ii
-
CHAPTER 3. INTERACTION OF PENNY-SHAPED CRACKS ...
Figure 3.3: Equal uniform normal loadings: variation of stress
intensity factor % with angle 9 for ef = 0.45 and various 7 when a
= ii < f.
Figure 3.4: Equal uniform normal loadings: variation of the
stress intensity factor with respect to c j at 9 = 0 for various 7
when a = ii < f .
Figure 3.4 shows the variation of the stress intensity factor kl
with respect to the normalized
-
CHAPTER 3. INTERACTION OF PENNY-SHAPED CRACKS. .. 39
crack size c j at 0 = 0 for some given values of 7. From this
picture we can see that kl increases with c f for some values of f
, say 0 or 0.25, and decreases for some other values of f , say 1.
This
implies that increasing the size of the crack sometimes reduces
the stress intensity factor kl and
sometimes increases it if the horizontal and vertical distances
f and g are fixed.
Figure 3.5: Equal uniform normal loadings: variation of the
stress intensity factor 5 with respect to f at 0 = 0 for various c
f when a = 3 6 , the stress intensity factor is very close t o that
for a single crack no matter what value of ~f is.
-
CHAPTER 3. INTERACTION OF PENNY-SHAPED CRACKS ...
respect to f at 0 = 0 for various cf when a = ii.
-
CHAPTER 3. INTERACTION OF PENNY-SHAPED CRACKS ... 4 1
From the above formulas, it is seen that the non-dimensional
stress intensity factors 2 and are dependent on v while & are
not. Figures 3.6 and 3.7 show the behaviors of 2 at 8 = 0
kl0
and 2 at 8 = n/2. In these figures, v = 0.3. It is interesting
to see that the behaviors of $ at 8 = 0 and -& at 8 = n/2 are
very similar. They are heavily depend on 8, though they are very
small (of the order O(E3f)). Also we note from figure 3.6 and
figure 3.7 that they change signs
when f is about 0.3 and reach maximum absolute value around 1.
Furthermore they reduce to
zero fairly quickly when f increases. Figure 3.8 shows that the
variations of 2 with respect to the Poison's ratio v for some given
values of €1 and they are very close to straight lines with
very
s m d slopes. This implies that the effects of the Poison's
ratio v on the stress intensity factor
& is not significant.
Figure 3.8: Equal uniform normal loadings: variation of the
stress intensity factor with respect to v at 0 = 0 for 7 = 0.3 and
various e j when a = Zi
-
CHAPTER 3. INTERACTION OF PENNY-SHAPED CRACKS.. .
B. Uniform shear loadings
In this case, the following unidirectional shears are applied on
the crack faces
-@1(x) = R I ( x ) = S = f & ( x ) = T R ~ ( Z ) ,
& ( x ) = Z l ( x ) = O , (3.41)
On(.) = Rn(x) = On(. ) = R , ( x ) = Z n ( t ) = Z n ( x ) = 0,
for n # 1,
where the upper signs correspond to the case in which shear
loadings on both cracks are in
opposite directions and the lower signs correspond to loadings
in the same direction. We can see
from (3.25) -(3.30) and their analogues on crack that
In the same way as for normal loading, we reduce the system of
six integral equations to a system
of three integral equations and then solutions can found by
iteration for the case when ef is very
small. By using these solutions, the stress intensity factors
correct to order O(E6f) are found
-
CHAPTER 3. INTERACTION OF PENNY-SHAPED CRACKS ...
2 * -[vI," 315n - 9c - (2 - V)I: + f&? cos(40)) , f k3 =
4S&(1- V) {U r 2 n(2 - v) 3n(2 - v)
1 9 5 5 *-[-(a + 3v)I; - 391: + (3v - 8)1: + 3-Io]rj
45n f f 8 3 2 6 4
(-I1 ) 'f + gr2(2 - v)2 + 9 r y 2 - u) f [UI; - 91; - (2 - U)I~
+ ~ I ~ ] ~ c ~ } sin 6 f
2 9 Q 4 4 *{- gn(2 - u)
[VI; - -1: - (2 - U)I? + 711]rf f
2 + 3157r(2 - u)
[-7(2 - U)I: + 6 9 ~ + (7v - 2)1: - 69g] r?} sin(20) f f
2 9 5 5 - (2 - U)I; + -12]ef sin(38) r K[vI: - ?I4 f 2 r -[uI; -
9c - (2 - v)~: + p&F sin(46)) .
315n f
Figure 3.9: Equal uniform shear loadings: variation of the
stress intensity factor f& with respect to €3 a t 0 = 0 for
various 7 when a = ii
-
CHAPTER 3. INTERACTION OF PENNY-SHAPED CRACKS ...
Figure 3.10: Equz d uniform shear loadings: variation of the
stress intensity factor & a respect to f at B = 0 for various
ef when a = ii < f.
Figure 3.11: Equal uniform shear loadings: variation of the
stress intensity factor 2 with respect to f at B = 0 for various cf
when a = ii < f.
AU -h and & are dependent on u when the cracks are subject
to shear loadings and u k2o ' k2o
-
CHAPTER 3. INTERACTION OF PENNY-SHAPED CRACKS ...
is taken to be 0.3 in all these figures.
Figure 3.9 shows that the presence of the second crack sometimes
( f = 0 or 0.25) reduces
the value of stress intensity and sometimes (f = 1) increases
it. From figure 3.10 we can see
that 8 reaches the maximum value when f is around 0.6. Figure
3.11 shows that the behavior of 2 is very similar to those of &
and 2 in the case of uniform normal loadings. CASETWO f =O; a = i i
< < g
Since f = 0, all the kernels Kijn, equal to zero unless n = m
and the infinite system of integral
equations decouple, which means that the nth Fourier coefficient
is only related to other nth
terms. The integral equations (3.25)-(3.30), resulted from the
boundary conditions on the crack
C, now become
if n = 0 and
for n 2 1. Similar integral equations can be obtained from the
boundary conditions on c. Due to the geometric symmetry of the
problem, each integral equation is finitely long, though there
are still infinitely many such kind of integral equations. For
some special loadings, which can
be expressed by finite Fourier series, this infinite set of
integral equations can be reduced to a
finite set and then can be solved by numerical methods.
Asymptotic solutions are also available
when cg = :, the ratio of the radius to the vertical distance,
is very s m d . Several asymptotic solutions are presented
below.
A. Equal uniform normal loadings
-
CHAPTER 3. INTERACTION OF PENNY-SHAPED CRACKS ... 46
If the cracks are opened by the equal uniform pressures (3 .31)
, the only non-zero terms
of a n ( x ) , b n ( x ) , c n ( x ) and % ( x ) , b n ( x ) , E
~ ( x ) are a o ( x ) , bo(x) , and a o ( x ) , bo(x ) . Note
that
a o ( x ) = go(,) and bo(x) = -bo(x) and therefore in this case
we end up with just two integral
equations
Solutions to these equations accurate to order 0 ( e t ) are
Hence the stress intensity factors are
B. Uniform shear loadings
If the cracks are under equal uniform shear loadings (3 .41) ,
the only nono-zero terms are
a l ( x ) = k a l ( x ) , & ( x ) = r f b l ( x ) , el(%) =
7 c l ( x ) . In the same way as for the normal loading, we reduce
the number of integral equations from six to three and obtain the
stress intensity factors
3.1.3 Discussion
It is of interest to compare our results with some previous
solutions for some particular cases.
Coplanar cracks
-
CHAPTER 3. INTERACTION OF PENNY-SHAPED CRACKS.. . 4 7
Coplanar cracks opened by uniform pressures have been studied by
Collins[4] and Fabrikant[7]
and expressions for the energy of each crack were given. In our
notation, it is
which takes the following form
after substituting the solutions we obtained in last section.
This agrees with that given by
Collins[4]. The series expansion of Fabrikant7s solution,
obtained by using the mean value theo-
rem, in our notation is
which is slightly lower than ours. His method can be used to
handle very close interactions but
failed in the non-coplanar case.
Coplanar cracks subjected t o uniform shear stresses have been
studied by Fu and Keer[ll]
and Fabrikant[8]. As mentioned in 181, some formulas and results
in [ll] are incorrect. In the
same way as for normal loadings we obtain the energy increase
per crack under shear loadings
This corrects the results in [ l l ] and also confirms that
(3.58) should be same as (3.56) when
v = 0, which had been observed by Fabrikant[8].
Co-axial cracks
If the cracks are opened by uniform pressures, the crack energy
is
which confirms the result given by Collins [3]. For the case of
shear loadings the results seem to
be new even for co-axial cracks.
A research paper1151 based on the work of this section is to be
published in the Theoretical
and Applied fracture Mechanics.
-
CHAPTER 3. INTERACTION OF PENNY-SHAPED CRACKS. ..
3.2 Penny-Shaped Cracks in a Semi-Infinite Solid
An elastic half-space containing one penny-shaped crack under
uniform normal loading has been
studied by Srivastava and Singh[32]. The problem of a half-space
containing one crack loaded
with arbitrary tractions and the problem of a half-space
containing more than one are the
subjects of this section.
The problem to be considered in this section involves a
semi-infinite elastic solid, with stress
free boundary, containing two arbitrarily located penny-shaped
cracks C and c, which are parallel to the half-space surface. Like
the infinite solid case, two local cylindrical co-ordinate
systems (r, 8, z) and ( F , 8 , ~ ) are employed such that
cracks C and are taken to occupy
respectively and the stress free boundary is taken to be z = -h
in the first co-ordinate and
5 = -6 in the second. The origins 0 and 0 of these two
coordinate systems are points (f, 0, g) and (f,n, -g) in these
respective sets of co-ordinates. Here f and g are the horizontal
and
vertical distances between the centers of these cracks,
respectively. The distances from the free
boundary to these two cracks are denoted by h and h respectively
and therefore 6 - h = g, which is non-negative (figure 3.12).
Tractions on the crack faces are prescribed and can be expanded
in Fourier series (3.1)-
(3.6). Besides these boundary conditions on the crack faces,
stress free boundary conditions
are imposed on the surface z = - h of the half-space. In terms
of co-ordinates ( r , 8 , z), these
boundary conditions can be written as
We s h d find the stress intensity factors for these two
cracks.
3.2.1 Derivation of integral equations
The problem of an elastic half-space weakened by two parallel
penny-shaped cracks can be de-
composed into two easier problems: problem a of a half-space
containing crack C and problem
-
CHAPTER 3. INTERACTION OF PENNY-SHAPED CRACKS ...
I I I I I I I
I
I I I I I
I I I I 2a - . I ,--Q--' ----,--- ,-,-,,, b' ------------ J
------- \
\ Stress free surface
Figure 3.12: Two parallel penny-shaped cracks in a semi-infinite
solid.
b of a half-space containing c. Furthermore problem a can be
decomposed into problem C of an infinite solid containing one crack
with effective stresses an(x), bn(x) and cn(x) applied
on the crack face C and problem H1 of a half-space with properly
chosen stresses applied on
the surface such that the sum of the solutions to these two
problems satisfies the stress free
boundary conditions at z = -h. Solutions to problem b can be
decomposed into two parts in
a similar fashion.
It will be shown that the original problem can be reduced to a
system of Fredholm integral
equations for an(x), bn(x), cn(x) and &(z), Zn(x), En(x),
where a,(x), bn(x), 4 ( x ) are the
corresponding effective stresses for crack c. The procedure of
deriving these integral equations involves finding the stress
fields of problem a and problem b in terms of the corresponding
effective stresses.
As mentioned before, the stress field of problem a can be
considered as the sum of the
-
CHAPTER 3. INTERACTION OF PENNY-SHAPED CRACKS ... 50
stress field of problem C and the stress field of problem HI. In
order to satisfy the stress
free boundary conditions of problem a , the boundary conditions
for problem H1 are chosen
so that
11 Fn ( s ) = 2p[An(s) ( l+ sh) - ~ ~ ( s ) s h ] e - " ~ ,
(3.61)
+I ( s ) = 2p[-shAn(s) - ( 1 - sh)Bn(s) + ~ n ( s ) ] e - " ~ ,
(3.62) -1 ( s ) = 2p[-shAn(s) - (1 - sh)Bn(s) - ~ , ( s ) ] e - " ~
. (3.63)
Here the basic solutions to problem C have been used. With those
stresses applied on the
half-space surface of problem HI, we can find the stresses in
the half-space by using the basic
solutions for problem H1. Adding these two stress fields results
the stress field of problem a.
In terms of the effective stress coefficients a,(x), b,(x) and
c,(x), the stresses on the crack C of
problem a can be written as
~,h, ( r , 0 ) = an ( T ) + 2p [ ( I + 2sh + 2s2h2)An(s) 1" - ~
s ~ ~ ~ B ~ ( s ) ] s ~ - ~ " ~ ~ ~ ( s r ) d s , (3.64)
Considering A, ( s ) , Bn ( s ) and Cn(s) are integrals of the
effective stress coefficients a, ( x ) , cn(x) + bn(x) and cn(x) -
bn(x), we now have expressed the stresses on the crack face by
these stress coefficients. With the aid of the arguments given in
chapter 2, expression of this stress field in
terms of ( F , # , z) can also mbe found. On the position where
crack shall be, the stresses are
given by
-
CHAPTER 3. INTERACTION OF PENNY-SHAPED CRACKS ...
+ 2p lm { ( sg + 2 s 2 h 6 ) ~ ; ( s ) - [ I - s(h + 6 ) + 2 s 2
h 4 ~ ; ( s ) - c;(s)} s~ , -1 (Fs )e - ' (~+~)ds .
Similarly we obtain the stress field of problem b in terms of
both co-ordinate systems ( f , e , E )
and (r7 8,E).
Now return to the original problem. It is clear that the
superposition of the above two
solutions automaticdy satisfies the stress free boundary
conditions (3.60). Superposing these
two stress fields and substituting them into the crack face
boundary conditions lead us to system
of Fredholm integral equations for the six effective stress
coefficients after changing the order of
integration. On crack face C , the integral equations are
-
CHAPTER 3. INTERACTION OF PENNY-SHAPED CRACKS.. . 52
co(r) = 0
if n = 0 and
an(^) t
t
+ + -
+ +
+ cn (r ) + bn(r) +
+ -
+ +
-
CHAPTER 3. INTERACTION OF PENNY-SHAPED CRACKS ...
when n 2 1. On crack c, they are
-
CHAPTER 3. INTERACTION OF PENNY-SHAPED CRACKS ...
+ + + + +
+ e ( f ) =
if n = 0 and
a n ( f ) + + + +
+ + +
+ G ( f ) + in (? ) +
+ + +
1' ~ a n m l 3 ( ~ 7 X ) [ c m ( ~ ) - b m ( x ) ] d x ) = i n (
f ) 7 ( 3 . 7 6 )
-
CHAPTER 3. INTERACTION OF PENNY-SHAPED CRACKS ...
when n 2 1. Kernels of these integral equations are given in the
Appendix. Now we have reduced
the problem to a system of six integral equations for an($),
bn(x), cn(x) and an(x), bn(x), z,(x).
These integral equations can be solved by iteration for some
special cases. Once these effective
stress coefficients are known, stress intensity factors can be
determined.
3.2.2 Some Asymptotic Solutions
In this subsection we shall solve the integral equations for
three special cases, the single crack
case, the two co-axial crack case and two coplanar crack case.
As for the infinite solid case, we
assume that the two cracks have equal radii a for the latter two
cases. In the second and third
cases, we will consider two different loadings which are the
equal uniform normal loadings and
equal uniform shear loadings.
-
CHAPTER 3. INTERACTION OF PENNY-SHAPED CRACKS.. .
CASE I SINGLE CRACK
If there is only one crack, the system of six integral equations
becomes to a system of three
integral equations because of the absence of the second crack.
Since all the kernels involving
parameters or g vanish, the system of integral equations
decouple. This implies that the nth
coefficients of the effective stresses are only related to the
other nth terms.
A. uniform normal loading
If the crack is under uniform normal loading P, all Zk(r), Rk(r)
and Ok(r) equal to zero except
Zo(r). Therefore all ak(x), bk(x) and ck(x) vanish except ao(x)
and bo(x). Hence the system of
integral equations becomes just two Fredholm integral equations
for ao(x) and bo(x),
These integral equations can be solved for the case when r h = f
, the ratio of the crack radius to
the distance between the crack and half-space surface, is very
small, considering Kbnij(r, x) can
expanded as power series of r h . Solutions correct to O ( 4 )
are
Therefore the stress intensity factors are
These recover the results given by Srivastava and Singh[32]
using a different method, noting that
the definitions of k2 differ by a constant.
-
CHAPTER 3. INTERACTION OF PENNY-SHAPED CRACKS.. .
B. unidirectional shear loading
If the crack is under uniform shear loading in the x
direction,
then Z k ( r ) , R k ( r ) and O k ( r ) are all zero except - O
1 ( r ) = R l ( r ) = S and therefore all a k ( x ) ,
b k ( x ) and c k ( x ) are zero except a l ( x ) , b l ( x )
and c l ( x ) , which satisfy the following integral
equations
In the same way as for the normal loading, we obtain solutions
correct to order O ( E ; )
these give us the stress intensity factors
kl = 10&S cos 8 21 3 r 2 ( 2 - v ) (4 + 3 3 7
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CHAPTER 3. INTERACTION OF PENNY-SHAPED CRACKS.. .
CASE I1 TWO CO-AXIAL CRACKS
If the cracks share the same axis, then the system of six
integral equations decouples too. Also
it is seen from the definitions of the kernels that K b n m i j
( y , x ) and Kbnmij(y, x ) can be expanded as power series in ~ h
, K c n m i j ( y , x ) and K m m i j ( y , x ) can be expanded as
power series in cg and
K a n m i j ( y , x ) and ~ a n m ; j ( ~ , x ) can either be
expanded as power series in ~h or as power series
in cg = 5 Therefore different forms of solutions can be sought
depending on which expressions 9 '
of K a n m i j ( ~ , x ) and K a n m ; j ( y , x ) we use. I f
the ch power series of K a n m i j ( y , x ) and ~ , , , ; ~ ( y ,
x )
are employed, solutions take the following form
where a i k ( r ) itself is a power series of cg and so on.
Examples given below show how this idea
works.
A. Equal normal loadings
When the cracks are opened by equal uniform pressure P as given
by ( 3 . 3 1 ) , the only non-
zero terms are a o ( x ) , b o ( x ) and i i o (x ) , 6 0 ( x )
, which satisfy the following four Fredholm integral
equations,
a o ( r ) + + +
b o ( r ) + -
+ no(.) +
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CHAPTER 3. INTERACTION OF PENNY-SHAPED CRACKS ...
Substituting (3.86)-(3.88) into the above integral equations, we
end up with system of integral
equations for a&, bkk and z$, 6kk by equaling the
coefficients of 6; for k = 0,1,2, .... For each given k, the
integral equations resulted can be solved by iteration when eg is
small.
The integral equations for k = 0 are
which agree with the equations in the last section for two
co-axial cracks in an infinite solid.
Solutions accurate to order 0($) are
It is not hard to find the solutions for the integral equations
for k = 1 and k = 2
The integral equations for k = 3 are
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CHAPTER 3. INTERACTION OF PENNY-SHAPED CRACKS ...
where cl and c2 are constants given by
which involving integrals
The non-zero terms of the solutions of ab3(ax), bb3(az), ~ i b ~
( a x ) , 6k3(ax) correct to order O ( { )
are
The stress intensity factors follow
It is worth mentioning that k2 and i2 are of order O ( $ ) +
0(&. From equation (3.50) in section 3.1 we know that the
presence of the second co-axial crack
under the same uniform pressure as the first one reduces the
stress intensity factor kl. Equation
(3.81) shows that the stress free boundary increases the value
of kl when there is only one crack.
The variations of nondimensional kl and il with respect to f,
and sh are shown in figures 3.13-3.15, respectively. From these
figures we can see how the stress free boundary and the two
cracks effect each other.
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CHAPTER 3. INTERACTION OF PENNY-SHAPED CRACKS.. .
1 .04 I 1 I I I
1.03 -
1.02 - -
1-01 - - -
rh = 0.15 -
-
0.98 I I I I I
1 2 3 4 5 6 7 9 h
Figure 3.13: Two co-axial cracks with equal uniform normal
loadings: variation intensity factor & and 2 with respect to f
for various Q.
of the stress
Figure 3.14: Two co-axial cracks with equal uniform normal
loadings: variation of the stress intensity factor & and 2 with
respect to a for various q.
Not surprisingly, we note from figure 3.13 that kl > El
whatever rh is when f > 4, since
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CHAPTER 3. INTERACTION OF PENNY-SHAPED CRACKS.. . 62
in this case the boundary plays the most important role. It is
interesting to note that kl < i1 when < 3, even though C is
the crack closer to the boundary. Figure 3.14 shows that kl and
El are monotonicdy decreasing with increasing for given E, and
the effect of the boundary is ignorable when > 6 . Figure 3.15
tells us that increasing the size of the cracks sometimes
increases the stress intensity factor kl and sometimes reduces
it when g and h are given.
Figure 3.15: Two co-axial cracks with equal uniform normal
loadings: variation of the stress intensity factor & and &
with respect to rh for various 9 .
B. Equal uniform shear loadings
When equal unidirectional shears are applied on the crack faces,
the boundary conditions are
- & ( x ) = - R 1 ( x ) = -S = & ( x ) = - R 1 ( x )
,
& ( x ) = Z l ( x ) = 0 , (3.91)
O ~ ( X ) = R n ( x ) = O ~ ( X ) = R n ( x ) = Zn(x) = Zn(x) =
0, for n # 1,
and the only non-zero solutions are a l ( x ) , b l ( x ) , c l
( x ) and i i l (x) , & ( x ) , El(x). The non-zero
terms of the solutions in the form of (3.86)-(3.88) accurate to
O($)+O({ ) produce the following
stress intensity factors
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CHAPTER 3. INTERACTION OF PENNY-SHAPED CRACKS.. . 63
and
Here cg and c4 are functions of R given by
Also it is worth mentioning that kl and i1 are of O(cj) + O ( E
~ ) .
Figure 3.16: Two co-axial cracks with equal uniform shear
loadings: variation of the stress intensity factor 2 and $ with
respect to f for various 4 .
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CHAPTER 3. INTERACTION OF PENNY-SHAPED CRACKS.. .
Figure 3.17: Two co-axial cracks with equal uniform shear
loadings: variation of the stress intensity factor 2 and & with
respect to a for various cg.
From these formulas we can see that k2 and k2 are cosine
functions of 8 and k3 and i3 are
sine functions of 8. Also we know that behaviors of kz at 0 = 0
and k3 at 8 = are the same
(correct to order O ( 4 ) + 0(
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CHAPTER 3. INTERACTION OF PENNY-SHAPED CRACKS.. . 65
as power series of cf or power series of ch, we can find two
different solutions depending on which
the expressions used. As an example, we use the ~f power series
expression and seek solutions
of the following form
f where cnk(x) itself is a power series of ch and so on.
A. Equal normal loadings
If the cracks are opened by the equal uniform pressures we
have
and thus the system of six integral equations can be reduced to
a system of three integral
equations, which can be solved by the same procedure used for
the co-axial case. Solutions
correct to O($) + O(4) lead to the following stress intensity
factors
where c5 and c6 are functions of 3 given by
which involve the following integrals