The generalized-strain mesh-free (GSMF) formulation is a local meshfree method in the field of numerical analysis, completely integration free, working as a weighted-residual weak-form collocation. This method was first presented by Oliveira and Portela (2016),[1] in order to further improve the computational efficiency of meshfree methods in numerical analysis. Local meshfree methods are derived through a weighted-residual formulation which leads to a local weak form that is the well known work theorem of the theory of structures. In an arbitrary local region, the work theorem establishes an energy relationship between a statically-admissible stress field and an independent kinematically-admissible strain field. Based on the independence of these two fields, this formulation results in a local form of the work theorem that is reduced to regular boundary terms only, integration-free and free of volumetric locking.
Advantages over finite element methods are that GSMF doesn't rely on a grid, and is more precise and faster when solving bi-dimensional problems. When compared to other meshless methods, such as rigid-body displacement mesh-free (RBDMF) formulation, the element-free Galerkin (EFG)[2] and the meshless local Petrov-Galerkin finite volume method (MLPG FVM);[3] GSMF proved to be superior not only regarding the computational efficiency, but also regarding the accuracy.[4]
The moving least squares (MLS) approximation of the elastic field is used on this local meshless formulation.
In the local form of the work theorem, equation:
\int | |
\GammaQ |
tTu*d\Gamma+
\int | |
\OmegaQ |
bTu*d\Omega=
\int | |
\OmegaQ |
\boldsymbol{\sigma}T\boldsymbol{\varepsilon}*d\Omega.
The displacement field
u*
\boldsymbol{\varepsilon}*
u*
\boldsymbol{\varepsilon}*
u*
\boldsymbol{\varepsilon}*
For the sake of the simplicity, in dealing with Heaviside and Dirac delta functions in a two-dimensional coordinate space, consider a scalar function
d
d=\lVert x-xQ\rVert
which represents the absolute-value function of the distance between a field point
x
xQ
\OmegaQ\cup\GammaQ
Q
d=d(x,xQ)\geq0
x
xQ
For a scalar coordinate
d\supsetd(x,xQ)
H(d)=1ifd\leq0(d=0forx\equivxQ)
H(d)=0ifd>0(x ≠ xQ)
in which the discontinuity is assumed at
xQ
\delta(d)=H'(d)=inftyifd=0thatisx\equivxQ
\delta(d)=H'(d)=0ifd ≠ 0(d>0forx ≠ xQ)
and
+infty | |
\int\limits | |
-infty |
\delta(d)dd=1
in which
H'(d)
H(d)
H(d)
xi
H(d),i=H'(d)d,i=\delta(d)d,i=\delta(d)ni
Since the result of this equation is not affected by any particular value of the constant
ni
Consider that
dl
dj
dk
d
xl
xj
xk
u*(x)
u*(x)=[
Li | |
ni |
ni | |
\sum | |
l=1 |
H(d | ||||
|
nt | |
\sum | |
j=1 |
H(dj)+
S | |
n\Omega |
n\Omega | |
\sum | |
k=1 |
H(dk)]e
in which
e=[11]T
ni
nt
n\Omega
\GammaQi=\GammaQ-\GammaQt-\GammaQu
Li
\GammaQt
Lt
\OmegaQ
S
u*(x)
\boldsymbol{\varepsilon}*(x)
\boldsymbol{\varepsilon}*(x)=Lu*(x)=[
Li | |
ni |
ni | |
\sum | |
l=1 |
LH(d | ||||
|
nt | |
\sum | |
j=1 |
LH(dj)+
S | |
n\Omega |
n\Omega | |
\sum | |
k=1 |
LH(dk)]e =[
Li | |
ni |
ni | |
\sum | |
l=1 |
T | ||
\delta(d | + | |
l)n |
Lt | |
nt |
nt | |
\sum | |
j=1 |
T | |
\delta(d | |
j)n |
+
S | |
n\Omega |
n\Omega | |
\sum | |
k=1 |
T | |
\delta(d | |
k)n |
]e
Having defined the displacement and the strain components of the kinematically-admissible field, the local work theorem can be written as
Li | |
ni |
ni | |
\sum | |
l=1 |
\int\limits | |
\GammaQ-\GammaQt |
tTH(dl)ed\Gamma+
Lt | |
nt |
nt | |
\sum | |
j=1 |
\int\limits | |
\GammaQt |
\overline{t
Taking into account the properties of the Heaviside step function and Dirac delta function, this equation simply leads to
Li | |
ni |
ni | |
\sum | |
l=1 |
t | |
xl |
=-
Lt | |
nt |
nt | |
\sum | |
j=1 |
\overline{t
Discretization of this equations can be carried out with the MLS approximation, for the local domain
\OmegaQ
\hat{u
Li | |
ni |
ni | |
\sum | |
l=1 |
n | |
xl |
DB | |
xl |
\hat{u
or simply
KQ\hat{u
This formulation states the equilibrium of tractions and body forces, pointwisely defined at collocation points, obviously, it is the pointwise version of the Euler-Cauchy stress principle. This is the equation used in the Generalized-Strain Mesh-Free (GSMF) formulation which, therefore, is free of integration. Since the work theorem is a weighted-residual weak form, it can be easily seen that this integration-free formulation is nothing else other than a weighted-residual weak-form collocation. The weighted-residual weak-form collocation readily overcomes the well-known difficulties posed by the weighted-residual strong-form collocation,[6] regarding accuracy and stability of the solution.