Engineering Analysis with Boundary Elements 37 (2013) 805–811
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Engineering Analysis with Boundary Elements journal homepage: www.elsevier.com/locate/enganabound
Elastodynamic problems by meshless local integral method: Analytical formulation P.H. Wen a, M.H. Aliabadi b,n a b
School of Engineering and Materials Science, Queen Mary, University of London, London E1 4NS, UK Department of Aeronautics, Imperial College, London SW7 2BY, UK
a r t i c l e i n f o
abstract
Article history: Received 22 August 2012 Accepted 30 January 2013 Available online 27 March 2013
In this paper, analytical forms of integrals in the meshless local integral equation method in the Laplace space are derived and implemented for elastodynamic problems. The meshless approximation based on the radial basis function (RBF) is employed for implementation of displacements. A weak form of governing equations with a unit test function is transformed into local integral equations. A completed set of the local boundary integrals are obtained in closed form. As the closed form of the local boundary integrals are obtained, there are no domain or boundary integrals to be calculated numerically. Several examples including dynamic fracture mechanics problems are presented to demonstrate the accuracy of the proposed method in comparison with analytical solutions and the boundary element method. & 2013 Elsevier Ltd. All rights reserved.
Keywords: Meshless local integral equation method Radial basis function Dynamic fracture mechanics
1. Introduction The boundary element method (BEM) is a well-established technique for analysis of certain engineering problem such as fracture mechanics [1–4] and acoustics [5–8]. For certain nonlinear problems such as plasticity [9–11] and creep [12], BEM normally requires some internal discretization. In recent years, the computational mechanics community has turned its attention to so-called mesh reduction methods. These mesh reduction methods (commonly referred to as Meshless or Meshfree) have received much interest since Nayroles et al. [13] proposed the diffuse element method. Later, Belyschko et al. [14] and Liu et al. [15] proposed element-free Galerkin method and reproducing kernel particle methods, respectively. MLPG is reported to provide a rational basis for constructing meshless methods with a greater degree of flexibility. Local Boundary Integral Equation method (LBIE) with moving least square and polynomial radial basis function (RBF) has been developed by Sladek et al. [16]. However, Galerkin-base meshless methods, except MLGP presented by Atluri [17] still include several awkward implementation features such as numerical integrations in the local domain. Other recent developments can be found in Refs. [18–46]. Recently, Sladeks developed an analytical integration method using MLS interpolation (see [40,41]) for non-homogeneous 2D elasticity. However, the analytical solutions are complex. Wen and Aliabadi [42] presented the meshless local integral equation method for the functionally graded Reissner’s plate in analytical formulation.
More recently, Soares et al. [43,44] have presented a time domain method with MLS interpolation for elastodynamic and poroelastic problems. The application of mesh free method to linear elastostatic fracture mechanics, i.e. evaluation of stress intensity factors and analysis of crack growth, was demonstrated by Fleming et al. [45] and Rao et al. [46] using enriched basis function in the moving least square interpolation. However, their method is computationally time consuming because the coefficient matrix must be inverted at each Gauss integration point. To overcome this difficulty, Wen et al. [35] developed a mesh free Galerkin method using enriched radial basis functions. In this paper, a meshless local integral method is presented for two-dimensional dynamic problems. With the use of radial basis functions, analytical solutions for all domain integrals in the weak form are derived. The weak formulation for the governing equations with a unit test function is obtained exactly for the local domain integrals. As the closed form of the local boundary integrals are obtained, the computational time are reduced significantly. A numerical inversion technique, Durbin’s inversion method, is applied to determine each variable in the time domain. The accuracy of the proposed method is illustrated by comparing the numerical results with available analytical solution and boundary element method. 2. The meshless local integral method Consider a linear elastic body in three dimensional domain O with boundary G. The governing equations of motion can be written as
n
Corresponding author. E-mail address:
[email protected] (M.H. Aliabadi).
0955-7997/$ - see front matter & 2013 Elsevier Ltd. All rights reserved. http://dx.doi.org/10.1016/j.enganabound.2013.01.019
sij,j þf i ¼ ru€ i
ð1Þ
806
P.H. Wen, M.H. Aliabadi / Engineering Analysis with Boundary Elements 37 (2013) 805–811
where sij are stresses, f i is the body force, r is the density of material and u€ i is the acceleration ði ¼ 1, 2j ¼ 1, 2 for 2DÞ and ði ¼ 1, 2, 3 j ¼ 1, 2, 3 for 3DÞ. Recalling Hooke’s law for plane stress problem, one has E @u1 @u2 E @u2 @u1 s11 ¼ þ n s ¼ þ n , , 22 @x2 @x1 1n2 @x1 1n2 @x2 E @u1 @u2 s12 ¼ þ ð2Þ 2ð1 þ nÞ @x2 @x1
domain, the transform of a function f ðtÞ is defined as Z 1 f~ ðsÞ ¼ f ðtÞept dt
for two-dimensional problem, where E is Young’s modulus, n is Possion ratio and m ¼ E=2ð1 þ nÞ the shear modulus. The boundary conditions are given as
3. Radial basis function approximation
ui ¼ u0i
on
Gu
t i ¼ sij nj ¼ t 0i
on
Gt
ð3Þ
t 0i
u0i
and are the prescribed displacements and tractions, in which respectively on the displacement boundary GD and on the traction boundary GT , and ni is the unit normal outward to the boundary G. In the local boundary integral equation approach, the weak form of differential equation over a local integral domain Os can be written as Z ðsij,j þ f i ru€ i Þuni dO ¼ 0 ð4Þ Os
where uni is a test function. By use of divergence theorem, Eq. (4) can be rewritten in a symmetric weak form as Z Z sij nj uni dG ðsij uni,j f i uni þ ru€ i ÞdO ¼ 0 ð5Þ Gs
Os
If there is an intersection between the local boundary and the global boundary, a local symmetric weak form in linear elasticity may be written as, see [42] Z Z Z Z Z sij uni,j dO ti uni dG ti uni dG ¼ t0i uni dG þ ðf i ru€ i Þuni dO Ls
Os
GD
GT
Os
ð6Þ in which, Ls is the other part of the local boundary inside the local integral domain Os ; GD is the intersection between the local boundary Gs and the global displacement boundary; GT is a part of the traction boundary as shown in Fig. 1. The local weak forms in (5) and (6) are a starting point to derive local boundary integral equations if appropriate test functions are selected. A step function can be used as the test functions uni in each integral domain ( ji ðxÞ at x ðOs [ Gs Þ : ð7Þ uni ðxÞ ¼ 0 at x= 2Os
where p is a Laplace parameter. Eq. (6) can be rewritten as Z Z s~ ij nj uni dG ðs~ ij uni,j f~ i uni þp2 ru~ i ÞdO ¼ 0 Gs
Γ
node x
Local integral domain Ω s
Ω
Node in support domain ξk
ð9Þ
Os
A local domain Os shown in Fig. 1, which is the neighborhood of a point x ( ¼ fx1 ,x2 g) and is considered as the domain of definition of the RBF approximation for the trail function at x and also called as support domain to an arbitrary point x. To interpolate the function u over a number of randomly distributed nodes in the local support domain Os x½ ¼ fn1 , n2 ,. . ., nK g, nk ¼ ðxk1 , xk2 Þ, k ¼ 1,2,. . .,K, one has function u at the point x as ui ðxÞ ¼
K X
Rk ðx, nÞak þ
T X
P t ðxÞbt ¼ RðxÞa þ PðxÞb
ð10Þ
t¼1
k¼1
where RðxÞ ¼ fR1 ðx, nÞ,R2 ðx, nÞ,. . .,RK ðx, nÞg is a set of radial basis T functions centered around the point x, fak gKk ¼ 1 and fbt gt ¼ 1 are the unknown coefficients to be determined and fPt gTt ¼ 1 is a basis for PT1 , the set of d-variate polynomials of degree rT1. If the radial basis function is selected as multi-quadrics [48,50] qffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffi ð11Þ Rk ðx, nk Þ ¼ c2 þ ðx1 xk1 Þ2 þ ðx2 xk2 Þ2 where c is a free parameter and with the constraints and K X
1 rt r T
P t ðnk Þak ¼ 0,
ð12Þ
k¼1
Following polynomials are considered (T ¼ 6) P ¼ f1,x1 ,x2 ,x21 ,x1 x2 ,x22 g
ð13Þ
Then a set of linear equations can be written in a matrix form as R0 a þ P0 b ¼ u, where matrix 2 R ðn Þ
P0 a ¼ 0
ð14Þ 3
R2 ðn1 Þ R2 ðn2 Þ
... ...
:
:
...
: :
: :
... ...
: :
R1 ðnK Þ
R2 ðnK Þ
...
RK ðnK Þ
1
1
6 R1 ðn2 Þ
6 R0 ðnÞ ¼ 6 6 4
RK ðn1 Þ RK ðn2 Þ 7
7 7 7 5
:
ð15Þ KK
and 2P
where fi ðxÞ is arbitrary function. In the Laplace transform support domain of x
ð8Þ
0
3
1 ðn1 Þ
P 2 ðn1 Þ
...
P T ðn1 Þ
6 P1 ðn2 Þ 6 : P0 ðnÞ ¼ 6 6 : 4
P 2 ðn2 Þ
...
: :
... ...
P T ðn2 Þ 7
:
:
...
:
P 1 ðnK Þ
P2 ðnK Þ
...
P T ðnK Þ
7 7 7 5
: :
:
ð16Þ
KT
Solving equations in (14) gives b ¼ bu,
b
a ¼ au
1 ¼ ðPT0 R1 P0 T R1 0 P0 Þ 0 ,
T 1 1 a ¼ R1 P0 T R1 0 ½IP0 ðP0 R 0 P0 Þ 0
ð17Þ Ls
Γs=ΓD+ΓT Fig. 1. Arbitrary distributed node, support domain of x, local integral domain for weak formulation.
where I denotes the diagonal unit matrix, matrices a, b, a and b are scale ðK 1Þ, ðT 1Þ, ðK KÞ and ðT KÞ respectively. Substituting the coefficients a and b from (17) into (10), we obtain the approximation of u in terms of the nodal values: uðxÞ ¼ UðxÞu, UðxÞ ¼ RðxÞa þ PðxÞb:
ð18Þ
also UðxÞ is called as shape function, matrix RðxÞ and PðxÞ are scale
P.H. Wen, M.H. Aliabadi / Engineering Analysis with Boundary Elements 37 (2013) 805–811
ð1 KÞ and ð1 6Þ matrix respectively. It is worth noting that the shape function depends uniquely on the distribution of scattered nodes within the support domain and it has the Kronecker Delta property.
807
d2 ¼ ðxlb1 xi1 Þcosbl þ ðxlb2 xi2 Þsinbl þ r 2 If the area of local integral domain is small, the domain integral can be approximated as Ii ¼ p2 ru~ i Os
4. Analytical forms of domain integrals in Laplace space Consider a unit test function, i.e. ji ðxÞ ¼ 1 and the local domain is enclosed by several straight lines as shown in Fig. 2, therefore, the local boundary integral equation becomes: Z Z Z L X s~ ij nj dG ¼ nlj s~ ij dG þ ðf~ i p2 ru~ i ÞdO ¼ 0 ð19Þ Gs
Gl
l¼1
Os
where L is number of straight line. Suppose there are nodes both in the domain and on the boundary, M ¼ M O þ MT þ M D , where M O indicates the number of nodes collocated in domain, M T and MD are numbers of nodes on the traction/displacement boundaries and consider the radial basis function interpolation in (18) and relationship between stress and strain in (2), then (4) becomes, see [42]: " # K X L K T X X X E E l l l l ~ ðjÞ F n þ m F n a þ G n þ m G n ij 2il 2 2tl 2 btj u 1 þ 1n2 1il 1 1n2 1tl 1 t¼1 j¼1l¼1 i¼1 " # K X L K T X X X En En l l l l ~ ðjÞ F n þ m F n a þ G n þ m G n ij 1il 2 1tl 2 btj u 2 ¼ I1 1n2 2il 1 1n2 2tl 1 t¼1 j¼1l¼1 i¼1
ð20aÞ " # K X L K T X X X En En l l l l ~ ðjÞ F n þ m F n a þ G n þ m G n ij 2il 1 2tl 1 btj u 1 þ 1n2 1il 2 1n2 1tl 2 t¼1 j¼1l¼1 i¼1 "
#
K X L K T X X X E E F nl þ mF 1il nl1 aij þ G nl þ mG1tl nl1 btj u~ ðjÞ 2 ¼ I2 2 2il 2 2 2tl 2 n n 1 1 t¼1 j¼1l¼1 i¼1
ð20bÞ R
for xk , k ¼ 1,2,. . .M O , where the integral functions Ii ¼ Os ðf~ i þ 2 ~ p ru i ÞdO and Z sl Z sl @Ri @P t ds, Gjtl ¼ ds ð21Þ F jil ¼ 0 @xj 0 @xj Consider form
nl1
¼
sinbl , nl2
¼ cosbl , we have solutions in closed
h i d1 F 1il ¼ ðr 2 r 1 Þcosbl ðxla1 xi1 Þsinbl ðxla2 xi2 Þcosbl sinbl ln d2 h i d1 l l F 2il ¼ ðr 2 r 1 Þsinbl ðxa2 xi2 Þcosbl ðxa1 xi1 Þsinbl cosbl ln d2 qffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffi c2 þðxla1 xi1 Þ2 þ ðxla2 xi2 Þ2 qffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffi r 2 ¼ c2 þ ðxlb2 xi1 Þ2 þ ðxlb2 xi2 Þ2
r1 ¼
ð22Þ
ð23Þ
However, for a rectangular local integral domain as shown in Fig. 3, we have its analytical form as " # K K T X X X ðjÞ J i aij þ Ht btj ðf~ n þ u~ ðjÞ ð24Þ In ¼ n Þ j¼1
i¼1
t¼1
where qffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffi 1 2 c x2 ln x1 þ c2 þðx1 xi1 Þ2 þ ðx2 xi2 Þ2 Ji ¼ 2 qffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffi 1 þ c2 x1 ln x2 þ c2 þ ðx1 xi1 Þ2 þ ðx2 xi2 Þ2 2 qffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffi 1 þ x1 x2 c2 þ ðx1 xi1 Þ2 þðx2 xi2 Þ2 3 qffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffi 1 þ x32 ln x1 þ c2 þ ðx1 xi1 Þ2 þðx2 xi2 Þ2 6 qffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffi 1 þ x31 ln x2 þ c2 þ ðx1 xi1 Þ2 þðx2 xi2 Þ2 6 0
c3 B þ tan1 @ 3
1 + cx1 C x þ D =2 x þ D =2 qffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiA jx1 D 1=2 jx2 D 2=2 1 1 2 2 c2 þ x22 þ x2 c2 þ ðx1 xi1 Þ2 þ ðx2 xi2 Þ2
and x þ D =2 x þ D =2
H1 ¼ x1 x2 jx11 D11=2 jx22 D22=2 , x1 þ D1 =2 x þ D =2 1 x1 x22 x D =2 jx22 D22=2 , 1 1 2 x1 þ D1 =2 x þ D =2 1 H5 ¼ x21 x22 x D =2 jx22 D22=2 , 1 1 4 H3 ¼
1 2 x1 þ D1 =2 x2 þ D2 =2 x x2 j 2 1 x1 D1 =2 x2 D2 =2 1 3 x1 þ D1 =2 x2 þ D2 =2 H4 ¼ x1 x2 x D =2 jx2 D2 =2 1 1 3 x1 þ D1 =2 x þ D =2 1 H6 ¼ x1 x32 x D =2 jx22 D22=2 1 1 3
H2 ¼
For the nodes on the traction boundary, (9) should be introduced: Z Z 0 t~ i dG t~ i dG ¼ Ii for xk k ¼ 1,2,. . .,MT ð25Þ G GT
GT
For the displacement boundary nodes, we can introduce the displacement equation directly, i.e. u~ i ðnk Þ ¼ u~ 0i , k ¼ 1,2,. . .M D . Therefore, there are total 2 ðM O þ M T þM D Þ linear algebraic equations which are used to determine the same number unknowns of displacements either in the domain or on the traction boundary. For linear test function, the analytical formulations were given by Wen and Aliabadi [42]. In the Laplace transform domain, a total number of Lþ1 samples in the transformation space sk , k ¼ 1, 2,. . ., L, are selected. Physical values are calculated for these transform parameters and the real value at time t must be obtained by an inverse transform. Here, the method given by Durbin [49] is used. Demonstration of
d1 ¼ ðxla1 xi1 Þcosbl þðxla2 xi2 Þsinbl þ r 1
L
b (xlb1 , xlb2)
Ωs
1
sl
2
l x1
x2
(xl1 , xl2)
xk
x2
xk
Δ1
βl
a
nl
(xla1 , xla2)
Fig. 2. Local integral domain with straight boundary lines.
x1 Fig. 3. Rectangular local integral domain.
Δ2
808
P.H. Wen, M.H. Aliabadi / Engineering Analysis with Boundary Elements 37 (2013) 805–811
the Durbin’s inverse method was made by Wen et al. [50] for elastodynamic problems with elasticity wave propagation. The calculation formula used is shown below: f ðtÞ ¼
" # L X 2eZt 1 2kp 2kpt f~ ðZÞ þ i exp Re f~ Z þ 2 T T T k¼0
ð26Þ
where f ðpk Þ stands for the transformed variables in the Laplace pffiffiffiffiffiffiffi space for parameters pk ¼ Z þ 2kp i=T ð i ¼ 1Þ. The selection of parameters Z and T only slightly affects the accuracy of the numerical solution. In our computations, we have chosen Z ¼ 5=t0 and T=t 0 ¼ 20 in the following examples, where t 0 ¼ b=c1 is the unit of time, b is specified length and longitudinal pffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffi ffi wave speed c1 ð ¼ Eð1nÞ=½ð1 þ nÞð12nÞrÞ. In addition, the dynamic stress intensity factor is evaluated by crack opening displacement (COD) in the Laplace transform domain. For mode I fracture, the stress intensity factor for plan stress problem is related to crack opening displacement, in the transformed domain, as following [35]: K~ I ¼
E 8ð1n2 Þ
sffiffiffiffiffiffi 2p Du~ 2 , r0
Du~ 2 ¼ u~ 2þ u~ 2:
ð27Þ
where r 0 indicates the distance between the collocation point and crack tip, Du~ 2 is the Crack Opening Displacement (COD) in the Laplace transform domain.
5.1. Rectangular sheet under dynamic load A square plate of width a subjected to a Heaviside load s0 HðtÞ on the top edge with fixed edge on the bottom is considered, where HðtÞ is Heaviside function. The regular distribution of collocation point (11 11 points) is shown in Fig. 2(a and b) and the Poisson ratio is taken as zero to allow comparison with the exact solution. The sample number (L þ1) in the transformed domain is taken to be 51 in this example. Free parameters n and K are selected as 1 and 16, and the local integral size D1 ¼ D2 ¼ D as shown in Fig. 4(b). Analytical formulations in (20a and b) are used for the domain integral of the acceleration/force terms. The dynamic displacement on the top (A) and middle of plate (B) and the stresses on the bottom (C) and middle (B) of plate are plotted in the Figs. 5 and 6, respectively. Good agreement with analytical solution has been achieved particularly for the displacement. Similar results can be obtained for large number of collocation point in the support domain and high density of collocation point distribution, i.e. ð31 31Þ and ð41 41Þ. In addition, the approximation approach of domain integral in (23) is tested and the results are very close as well. Therefore, the approximation approach in (23) is used in the following example.
5.2. A single central crack in rectangular plate under tension Consider a rectangular plate of width 2b and length 2h with a centrally located crack of length 2a. It is loaded dynamically in the direction perpendicular to the crack by a uniform tension s0 HðtÞ on the top and the bottom. Due to symmetry, a quarter of plate is
5. Numerical examples 2.5 u2(A)
Exact (A)
u2(B)
1.5 1.0 0.5 c1t / b 0.0 0
2
4
6
8
10
12
B x2 x1
16
Fig. 5. Normalized displacement u2 =b on the top (A) and middle (B) of a square plate subjected to uniform tensile load on the top against the normalized time c1 t=b.
Δ
h
14
-0.5
σ 0 H(t)
A
Exact (B)
2.0
u2/b
In this section, the application of proposed meshless method for two-dimensional elasticity dynamic problems is demonstrated. Although the nodes can be arbitrary or uniformly distributed in the domain, in this paper, all collocation points are the uniformly distributed in the domain. Normalized free parameter in the radial basis function c=D ¼ 10n , where D indicates the minimum distance between the nodes in the local integral domain and n is free parameter (n is chosen as zero in general cases). The support domain is selected as a circle of radius R centered at field point x, which is determined such that the minimum number of nodes in the support domain K Z 16. The mode I stress intensity factor in the time domain is calculated using COD technique.
support domain (R)
local integral domain
C
Fig. 4. Square plate subjected to uniform tensile load on the top: (a) geometry and coordinate and (b) regular distribution of node.
P.H. Wen, M.H. Aliabadi / Engineering Analysis with Boundary Elements 37 (2013) 805–811
and 21 41 respectively. Figs. 10–12 show the normalized stress intensity factors various against the normalized time c1 t=b for different geometry of plate. In addition, the results given by Wen et al. [34] using the mesh free Perov–Galerkin method and the indirect boundary element method (fictitious load method [47]) are presented in the same figures for comparison. Apparently before the 1.6
2
1.2
3
1 K I / σ0√ π a
considered as shown in Fig. 7. Here Poisson’s ratio n ¼ 0:3 and Young’s modulus ¼1 unit. Firstly we observe the accuracy of stress intensity factor with the density of collocation point. Fig. 8 shows the normalized stress intensity factor obtained by the nodal values of COD near the crack tip for the free parameters c=D ¼ 1ðn ¼ 0Þ, the local integral size D1 ¼ D2 ¼ D and K ¼ 16. Obviously the nearest point (first) should not be considered as the singularity of stress at the crack tip and the points from the second to the sixth can be used to obtain high accuracy results. The analytical static solution for a square plate pffiffiffiffiffiffi b=h ¼ 1 containing a central crack, if a=b ¼ 0:5, is K I ¼ 1:325s0 pa [51] and the result by the second nodal value with 21 21 node pffiffiffiffiffiffi distribution is K I ¼ 1:331s0 pa. Therefore, the relative error can be expected to be less than 1% for elastostatic problems. Therefore, we use the second nodal value with 21 21 node distribution to evaluate stress intensity factor in the following examples. Secondly, we observe the sensitivity of the free parameter selection, i.e. factor c=D and K, if the local integral size D1 ¼ D2 ¼ D with 21 21 nodes. The contours of relative error in percentage are shown in Fig. 9. In the region of 0:5 on o 0:5 and K 410, we can obtain the numerical solution with degree of accuracy which is less than 5%. Three geometries of rectangular plate are considered in this example, i.e. b=h ¼ 0:5, b=h ¼ 1 and b=h ¼ 2 while a=b ¼ 0:5. The total numbers of nodes for each case are selected as 21 11, 21 21
809
Series1 21×21 0.8
Series2 3
2
31×31
1
Series3 41×41
0.4
Series4 r0 / b
0.0 0.00
0.05
0.10
0.15
0.20
0.25
0.30
Fig. 8. Stress intensity factor various with normalized distance r 0 =b between collocation point and crack tip.
3.0 u2(C)
2.5
u2(B)
Exact (B)
Exact (C)
%
1.0
σ 22/b
2.0 1.5
0.5
1.0 0.5 c1t / b 0
2
4
6
8
10
12
14
16
-0.5
Fig. 6. Normalized stress s22 =s0 on the middle (B) and bottom (C) of a square plate subjected to uniform tensile load on the top against the normalized time c1 t=b.
n
0.0
0.0
-0.5
σ0H (t) -1.0 10
15
20 K
25
30
Fig. 9. Contour of the relative error (%) various with free parameters: the number of point in support domain K and n, c=D ¼ 10n , in RBF.
5.0 This paper
h
4.0
MFPG [34] BEM [47]
x2 crack tip
a x1
KI/σ0√πa
3.0 2.0 1.0
c1t / b
0.0 0
b Fig. 7. Rectangular plate with a central crack of length 2a under tension s0 HðtÞ.
2
4
6
8
10
12
14
16
-1.0
pffiffiffiffiffiffi Fig. 10. Normalized stress intensity factor K I =s0 pa against the normalized time c1 t=b for b=h ¼ 0:5.
810
P.H. Wen, M.H. Aliabadi / Engineering Analysis with Boundary Elements 37 (2013) 805–811 3.5 This paper
3.0
MFPG [34]
2.5
BEM [47]
KI/σ0√πa
2.0 1.5 1.0 0.5
c1t / b
0.0 -0.5
0
2
4
6
8
10
12
14
16
-1.0
pffiffiffiffiffiffi Fig. 11. Normalized stress intensity factor K I =s0 pa against the normalized time c1 t=b for b=h ¼ 1:0. 3.0 2.5 This paper
K I / σ 0 √π a
2.0
MFPG [34] BEM [47]
1.5 1.0 0.5
c1t / b
0.0 0
2
4
6
8
10
12
14
16
-0.5 -1.0
pffiffiffiffiffiffi Fig. 12. Normalized stress intensity factor K I =s0 pa against the normalized time c1 t=b for b=h ¼ 0:5.
arrival time of dilatation wave traveling from the top of plate, the stress intensity factor should remain to be zero. The agreement between these solutions is considered to be good.
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