In fracture mechanics, the energy release rate,
G
The energy release rate
G
\Pi
s
G\equiv-
\partial\Pi | |
\partials |
,
where the total potential energy is written in terms of the total strain energy
\Omega
t
u
b
\Pi=\Omega-\left\{\intl{St}t ⋅ udS+\intl{V}b ⋅ udV\right\} .
The first integral is over the surface
St
V
The figure on the right shows the plot of an external force
P
q
P
P(q)
In the case of prescribed displacement, the strain energy can be expressed in terms of the specified displacement and the crack surface
\Omega(q,s)
\delta\Omega=(\partial\Omega/\partials)\deltas
G=-\left.
\partial\Omega | |
\partials |
\right|q .
Here is where one can accurately refer to
G
When the load is prescribed instead of the displacement, the strain energy needs to be modified as
\Omega(q(P,s),s)
G=-\left.
\partial | |
\partials |
\right|P\left(\Omega-Pq\right) .
If the material is linearly-elastic, then
\Omega=Pq/2
G=\left.
\partial\Omega | |
\partials |
\right|P .
In the cases of two-dimensional problems, the change in crack growth area is simply the change in crack length times the thickness of the specimen. Namely,
\partials=B\partiala
G
G=-\left.
1 | |
B |
\partial\Omega | |
\partiala |
\right|q.
G=-\left.
1 | |
B |
\partial | |
\partiala |
\right|P\left(\Omega-Pq\right).
G=\left.
1 | |
B |
\partial\Omega | |
\partiala |
\right|P.
U=\Omega/B
G=-\left.
\partialU | |
\partiala |
\right|q.
G=-\left.
\partial | |
\partiala |
\right|P\left(U-
Pq | |
B |
\right).
G=\left.
\partialU | |
\partiala |
\right|P.
The energy release rate is directly related to the stress intensity factor associated with a given two-dimensional loading mode (Mode-I, Mode-II, or Mode-III) when the crack grows straight ahead.[3] This is applicable to cracks under plane stress, plane strain, and antiplane shear.
For Mode-I, the energy release rate
G
KI
G=
| |||||||
E' |
,
where
E'
E
\nu
E'=\begin{cases} E,&plane~stress,\\ \\ \dfrac{E}{1-\nu2},&plane~strain. \end{cases}
For Mode-II, the energy release rate is similarly written as
G=
| |||||||
E' |
.
\mu
G=
| |||||||
2\mu |
.
For an arbitrary combination of all loading modes, these linear elastic solutions may be superposed as
G=
| |||||||
E' |
+
| |||||||
E' |
+
| |||||||
2\mu |
.
Crack growth is initiated when the energy release rate overcomes a critical value
Gc
G\geqGc,
Under Mode-I loading, the critical energy release rate
Gc
KIC
Gc=
| |||||||
E' |
.
There are a variety of methods available for calculating the energy release rate given material properties, specimen geometry, and loading conditions. Some are dependent on certain criteria being satisfied, such as the material being entirely elastic or even linearly-elastic, and/or that the crack must grow straight ahead. The only method presented that works arbitrarily is that using the total potential energy. If two methods are both applicable, they should yield identical energy release rates.
The only method to calculate
G
all in terms of the crack surface area.
If the material is linearly elastic, the computation of its energy release rate can be much simplified. In this case, the Load vs. Load-point Displacement curve is linear with a positive slope, and the displacement per unit force applied is defined as the compliance,
C
C=
q | |
P |
.
\Omega
\Omega=
1 | |
2 |
Pq=
1 | |
2 |
q2 | |
C |
=
1 | |
2 |
P2C.
G=
1 | |
2 |
P2
\partialC | |
\partials |
.
In the case of prescribed displacement, holding the crack length fixed, the energy release rate can be computed by [3]
G=
q | |
-\int | |
0 |
\partialP | |
\partials |
dq,
while in the case of prescribed load,[3]
G=
P | |
\int | |
0 |
\partialq | |
\partials |
dP.
G
ds
Gds=-ds
q | |
\int | |
0 |
\partialP | |
\partials |
dq=ds
P | |
\int | |
0 |
\partialq | |
\partials |
dP.
Since the energy release rate is defined as the negative derivative of the total potential energy with respect to crack surface growth, the energy release rate may be written as the difference between the potential energy before and after the crack grows. After some careful derivation, this leads one to the crack closure integral [3]
G=\lim\Delta-
1 | |
\Deltas |
\int\Delta
1 | |
2 |
0\left(\Delta | |
t | |
i |
+ | |
u | |
i |
-\Delta
-\right)dS, | |
u | |
i |
where
\Deltas
0 | |
t | |
i |
\Delta
+ | |
u | |
i |
-\Delta
- | |
u | |
i |
S
The crack closure integral is valid only for elastic materials but is still valid for cracks that grow in any direction. Nevertheless, for a two-dimensional crack that does indeed grow straight ahead, the crack closure integral simplifies to [3]
G=\lim\Delta
1 | |
\Deltaa |
\Deltaa | |
\int | |
0 |
\sigmai2(x1,0)ui(\Deltaa-x1,\pi)dx1,
where
\Deltaa
r=\Deltaa-x1
\theta=\pi
In certain situations, the energy release rate
G
G=J
J=\int\Gamma\left(Wn1-
t | ||||
|
\right)d\Gamma,
where
W
n1
x1
\Gamma
ti
t=\boldsymbol{\sigma} ⋅ n
\boldsymbol{\sigma}
ui
This integral is zero over a simple closed path and is path independent, allowing any simple path starting and ending on the crack faces to be used to calculate
J
G=J
\Gamma
The J-integral may be calculated with these conditions violated, but then
G ≠ J
G=J=
| |||||||
E' |
+
| |||||||
E' |
+
| |||||||
2\mu |
.
A handful of methods exist for calculating
G
If the crack is growing straight, the energy release rate can be decomposed as a sum of 3 terms
Gi
Gi
\Deltaa
\Delta\vec{u}=\vec{u}(t+1)-\vec{u}(t)
\vec{F}
G
\Deltaa
G=\lim\DeltaGNR
If the energy release rate exceeds a critical value, the crack will grow. In this case, a new FEA simulation is performed (for the next time step) where the node at the crack tip is released. For a bounded substrate, we may simply stop enforcing fixed Dirichlet boundary conditions at the crack tip node of the previous time step (i.e. displacements are no longer restrained). For a symmetric crack, we would need to update the geometry of the domain with a longer crack opening (and therefore generate a new mesh[5]).
Similar to the Nodal Release Method, the Modified Crack Closure Integral (MCCI) is a method for calculating the energy release rate utilizing FEA nodal displacements
j | |
(u | |
i |
)
j | |
(F | |
i |
)
i
j
A necessary condition for the MCCI method is uniform element length
(\Deltaa)
x1-
K(a+\Deltaa) ≈ K(a)
The 4-node square linear elements seen in Figure 2 have a distance between nodes
j
j+1
\Deltaa.
j.
x1
\boldsymbol{uj}
(j+1)
\boldsymbolFj+1.
j
j-1
j+1
j.
Where}
MCCI G = 1
1 2\Deltaa
j F 2 {\Delta
j-1 u 2 }
MCCI G = 2
1 2\Deltaa
j F 1 {\Delta
j-1 u 1 }
MCCI G = 3
1 2\Deltaa
j F 3 {\Delta
j-1 u 3
\Delta
j-1 | |
u | |
i |
=
(+)j-1 | |
u | |
i |
(-)j-1 | |
-u | |
i |
(+)j-1 | |
u | |
i |
=
(-)j-1 | |
-u | |
i |
.
Thus,
\Delta
j-1 | |
u | |
i |
=
(+)j-1 | |
2u | |
i |
.
The 8-node rectangular elements seen in Figure 3 have quadratic basis functions. The process for calculating G is the same as the 4-node elements with the exception that
\Deltaa
j
j+2.
Like with the nodal release method the accuracy of MCCI is highly dependent on the level of discretization along the crack tip, i.e.} + F_2^\right)
MCCI G = 1
1 2\Deltaa
j \left(F 2 {\Delta
j-2 u 2 } + F_1^\right)
MCCI G = 2
1 2\Deltaa
j \left(F 1 {\Delta
j-2 u 1 } + F_3^\right)
MCCI G = 3
1 2\Deltaa
j \left(F 3 {\Delta
j-2 u 3
G=\lim\DeltaGMCCI.
The J-integral may be calculated directly using the finite element mesh and shape functions.[9] We consider a domain contour as shown in figure 4 and choose an arbitrary smooth function
\tilde{q}(x1,x2)=\sumiNi(x1,x2)\tilde{q}i
\tilde{q}=1
\Gamma
\tilde{q}=0
l{C}1
For linear elastic cracks growing straight ahead,
G=J
J=\intl{A}(\sigmaijui,1\tilde{q},j-W\tilde{q},1)dl{A}
The formula above may be applied to any annular area surrounding the crack tip (in particular, a set of neighboring elements can be used). This method is very accurate, even with a coarse mesh around the crack tip (one may choose an integration domain located far away, with stresses and displacement less sensitive to mesh refinement)
The above-mentioned methods for calculating energy release rate asymptotically approach the actual solution with increased discretization but fail to fully capture the crack tip singularity. More accurate simulations can be performed by utilizing quarter-point elements around the crack tip.[10] These elements have a built-in singularity which more accurately produces stress fields around the crack tip. The advantage of the quarter-point method is that it allows for coarser finite element meshes and greatly reduces computational cost. Furthermore, these elements are derived from small modifications to common finite elements without requiring special computational programs for analysis. For the purposes of this section elastic materials will be examined, although this method can be extended to elastic-plastic fracture mechanics.[11] [12] [13] Assuming perfect elasticity the stress fields will experience a
1 | |
\sqrtr |
The 8-node quadratic element is described by Figure 5 in both parent space with local coordinates
\xi
η,
x
y.
Ni(\xi,η)
(xi,yi).
\xi=-1,η=-1
x=0,y=0.
x(\xi,η)=
8 \sum i=1 Ni(\xi,η)xi
In a similar way, displacements (defined asy(\xi,η)=
8 \sum i=1 Ni(\xi,η)yi
u\equivu1,v\equivu2
u(\xi,η)=
8 \sum i=1 Ni(\xi,η)ui
A property of shape functions in the finite element method is compact support, specifically the Kronecker delta property (i.e.v(\xi,η)=
8 \sum i=1 Ni(\xi,η)vi
Ni=1
i
When considering a line in front of the crack that is co-linear with theN1=
-(\xi-1)(η-1)(1+η+\xi) 4 N2=
(\xi+1)(η-1)(1+η-\xi) 4 N3=
(\xi+1)(η+1)(-1+η+\xi) 4 N4=
-(\xi-1)(η+1)(-1+η-\xi) 4 N5=
(1-\xi2)(1-η) 2 N6=
(1+\xi)(1-η2) 2 N7=
(1-\xi2)(1+η) 2 N8=
(1-\xi)(1-η2) 2
x
Ni(\xi,η=-1)
N1,2,5.
Calculating the normal strain involves using the chain rule to take the derivative of displacement with respect toN1(\xi,-1)=-
\xi(1-\xi) 2 N2(\xi,-1)=
\xi(1+\xi) 2 N5(\xi,-1)=(1-\xi2)
x.
If the nodes are spaced evenly on the rectangular element then the strain will not contain the singularity. By moving nodes 5 and 8 position to a quarter of the length\gammaxx=
\partialu \partialx =\sumi
\partialNi \partial\xi
\partial\xi \partialx ui
(\tfrac{L}{4})
\xi → x
Solving forx(\xi)=
\xi(1+\xi) 2 L+
2) L 4 (1-\xi
\xi
\xi(x)=-1+2\sqrt
x L
Plugging this result into the equation for strain the final result is obtained:}
\partial\xi \partialx =
1 \sqrt{xL
By moving the mid-nodes to a quarter position results in the correct}\left(2u_5-\frac\right)\gammaxx=
4 \left( L
u2 2 -u5\right)+
1 \sqrt{xL
1 | |
\sqrtr |
The rectangular element method does not allow for singular elements to be easily meshed around the crack tip. This impedes the ability to capture the angular dependence of the stress fields which is critical in determining the crack path. Also, except along the element edges the
1 | |
\sqrt{r |
\xi=-1
η=\pm1
A better candidate for the quarter-point method is the natural triangle as seen in Figure 7. The element's geometry allows for the crack tip to be easily surrounded and meshing is simplified. Following the same procedure described above, the displacement and strain field for the triangular elements are:
}\left[4u_6-3u_3-u_1\right] + \frac\left[2u_1+2u_3-4u_6\right]u=
u
3+\sqrt{ x L
This method reproduces the first two terms of the Williams solutions[15] with a constant and singular term.}\left[-\frac{u_1}{2}-\frac{3u_3}{2}+2u_6\right]+ \frac\left[2u_1+2u_3-4u_6\right]\gammaxx=
\partialu \partialx =
1 \sqrt{xL
An advantage of the quarter-point method is that it can be easily generalized to 3-dimensional models. This can greatly reduce computation when compared to other 3-dimensional methods but can lead to errors if that crack tip propagates with a large degree of curvature.[16]