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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 OF THE REQUIREMENTS FOR THE DEGREE OF 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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  • 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.

  • 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

  • PARTIAL COPYRIGHT LICENSE

    I hereby g ran t t o Simon Fraser U n i v e r s i t y t he r i g 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 l e o f which i s shown below)

    t o users o f t he Simon Fraser U n i v e r s i t y L i b r a r y , and t o make p a r t i a l o r

    s i n g l e copies o n l y f o r such users o r i n response t o a request f rom the

    l i b r a r y o f any o t h e r u n i v e r s i t y , o r o t h e r educa t iona l i n s t i t u t i o n , on

    i t s own beha l f o r f o r one o f i t s users . I f u r t h e r agree t h a t permiss ion

    f o r m u l t i p l e copy ing o f t h i s work f o r s c h o l a r l y purposes may be g ran ted

    by me o r the Dean o f Graduate Stud ies. I t i s understood t h a t copy ing

    o r p u b l i c a t i o n o f t h i s work f o r f i n a n c i a l ga in s h a l l n o t be a l lowed

    w i t h o u t my w r i t t e n permiss ion.

    T i t l e o f Thes is /Pro ject /Extended Essay

    Author:

    (s igna tu re )

    (name)

    (date)

  • 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.

  • 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.

  • Dedication

    To my wife and our parents

  • 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

  • . . . . . . . . . . . . . . . . . . . . . . . . . 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

  • 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

  • 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. . . . . . . . . . . . . . .

  • 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).

  • 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

  • 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

  • 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.

  • 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

  • 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

  • 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

  • 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.

  • 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

  • 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

  • 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(.) +

  • 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

  • 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.

  • 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

  • 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

  • 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 .

  • 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(

  • 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