Chung-Yuen Hui*ab,
Xuemei Xiaoa and
Matteo Ciccotti
*c
aSibley School of Mechanical and Aerospace Engineering, Cornell University, Ithaca, NY 14853, USA. E-mail: ch45@cornell.edu
bGlobal Station for Soft Matter, GI-CoRE, Hokkaido University, Sapporo, Japan
cLaboratoire de Sciences et Ingénierie de la Matière Molle, ESPCI Paris, Université PSL, CNRS, Sorbonne Université, 75005 Paris, France. E-mail: matteo.ciccotti@espci.fr
First published on 19th May 2025
In stick-slip fracture, a crack stays still or only propagates a small amount until it reaches a critical energy release rate. Then, it suddenly grows rapidly, causing the energy release rate to drop and the crack to stop again. This behavior is common in many polymers, including glassy polymers and soft materials like adhesives. However, the theoretical understanding of this phenomenon is fragmented and incomplete. Here we propose a unified theory based on a rate-dependent cohesive model to explain these phenomena. Using this model, we demonstrate that an elastic backing layer in a zero-degree peel test can experience different types of stick-slip instability depending on the peeling rate. At slow peeling rates, the crack grows slowly until it reaches a maximum velocity, corresponding to a fixed maximum force, after which the growth becomes unstable. However, above a certain critical peeling rate, there is no slow crack growth: the crack enters the stick-slip regime once the critical energy release rate is reached for a reduced value of the applied force. Although our mathematical modeling is developed in a specific geometry that makes the computations easier, this behavior can be argued to be a more general feature of most materials and geometries presenting stick-slip fracture.
Stick-slip fracture is often modeled using a kinetic relationship between a velocity dependent fracture toughness (Γ) and the steady-state crack growth rate (v), as shown in Fig. 1. During crack growth, the velocity dependent fracture toughness equals the energy release rate G, which depends solely on specimen geometry and external loading. It is typically assumed that this relationship applies even during non-steady-state crack growth, motivating the development of differential equations to predict the dynamics and duration of stick-slip cycles.4–6
In the peeling of adhesive tapes, the fracture toughness Γ versus crack velocity v plot can be divided into three branches as shown in Fig. 1. On two of these branches (black solid lines), crack growth is stable, and the energy release rate required for crack growth increases with crack velocity. One branch corresponds to slow crack velocity (v < 10−2 m s−1 in general), while the other corresponds to fast or dynamic crack velocity (v > 1 m s−1). These two branches are connected by an unstable branch (dashed black line) where stick-slip occurs. Although the existence of a negative slope branch of the energy release rate is supposed to link the two stable branches, this cannot be directly measured in experiments since the steady-state solution would be unstable. Some papers report that, in this region, the maximum strain energy release rate (or the maximum force) experienced during stick-slip cycles-indicated by the red arrows in Fig. 1, decreases with increasing pulling velocity applied to the adhesive tape.4
In PMMA, the slow quasi-static crack growth regime typically spans several decades of crack velocities (from 10−9 m s−1 to 10−1 m s−1),7 while the range of dynamic crack growth is comparatively small (102 m s−1–103 m s−1). The maximum strain energy release rate experienced during the stick-slip regime does not depend on the sample loading velocity for PMMA.2 In epoxy polymers, the crack often remains static until it reaches a critical energy release rate. After this point, the crack grows intermittently in a stick-slip manner without experiencing a slow crack growth phase. However, Nziakou et al.8 have demonstrated that this slow branch is difficult to observe because the crack velocity on this branch is limited to less than 10−9 m s−1. Moreover, the critical energy release rate to initiate the dynamic crack propagation in the stick phase (or the maximum force during the stick-slip cycles), is found to decrease with the loading velocity of the sample.3
Fig. 1 illustrates the classical cyclic picture of stick-slip dynamics. Beginning with a slow loading rate (e.g., peeling velocity in a peel test), the crack velocity grows slowly until it reaches a critical velocity, vΓmax. At vΓmax, crack growth becomes unstable, and the propagation enters the dynamic crack propagation in the fast “slip” branch. During slip, the system unloads because the crack growth rate is much faster than the loading rate, causing the crack to slow down along the slip branch. When a second critical velocity vΓmin is reached, the crack velocity suddenly jumps back to the slow “stick” branch, and everything starts again leading to periodic stick-slip cycles as indicated by the red arrows in Fig. 1.
Although stick-slip occurs in both soft materials like adhesives and hard materials like polymer glasses, their fracture mechanics differ significantly. In polymer glasses, the fracture process zone (e.g., the size of the plastic zone) is much smaller than typical specimen dimensions, allowing the application of linear elastic fracture mechanics (LEFM). This means that there is a region near the crack tip where the singular fields generated by a sharp crack dominate. In contrast, the fracture of adhesives is dominated by large strain mechanics and non-linear rheology, as evident by cavitation and fibrillation of the adhesive layer during peeling.9 Specifically, the stress/strain singularity associated with a sharp crack is eliminated since the size of the fibrillated region is comparable to or larger than the thickness of the adhesive layer.
Until recently, no comprehensive theory has addressed all these features, especially as they occur in different material systems such as thermosets, thermoplastics, and adhesives. In a recent work, Nziakou et al.8 proposed a scaling theory to link these features into a unified model. Here, we propose a simple analytic model that captures the essence of their approach. Unlike scaling theory, our approach is quantitative, providing precise mathematical formulations and detailed analysis. While scaling theory often relies on order of magnitude estimates, our method employs a rate-dependent cohesive model to quantify the fracture process. This approach provides specific predictions and insights about the behavior of various material systems under different loading conditions.
In this paper, we use the zero-degree peel test (Fig. 2) to define the loading geometry of an adhesive tape, although most experiments typically employ the 90-degree peel configuration. For peel angles greater than or equal to 30 degrees, the toughening mechanism is known to involve the stretching of fibrils formed by cavitation in the highly constrained region ahead of the peel front or crack tip. The rate-dependent cohesive zone model described in the next section is motivated by the extension and rupture of these fibrils during peeling. However, it should be noted that cavitation is not observed at low peel angles, where shear dominates and failure is primarily due to frictional and adhesive slippage. We adopt the zero-degree geometry in this work to simplify the mechanics of load transfer between the adhesive and the extensible backing. Since our focus is on illustrating fundamental concepts rather than comparing theory with experimental data, the zero-degree peel test is chosen for its analytical simplicity and the availability of exact closed-form solutions.
Our model in a zero-degree peel test specifies a relation between the shear displacement jump or slip δ across the backing/substrate interface (indicated by yellow line in Fig. 2) and the interfacial shear stress τ by:
![]() | (1) |
We assume the simplest model: a rate dependent Dugdale–Barenblatt (DB) model, in which the interfacial shear stress maintains a constant value τ0 when the slip is less than a critical threshold denoted by δc. For δ > δc, the interface fails and offers no resistance to shear, i.e.,
![]() | (2a,2b) |
![]() | (3) |
![]() | (4) |
u(x,t) = δ(x,t), x ∈ (−l −c, −c) | (5) |
Ahead of the cohesive zone tip in x < −l −c, u = δ = 0. Combining (4)–(5) and (2a), (4) becomes
![]() | (6) |
In the elastic layer behind the crack tip, force balance implies that the force acting on the peel arm F is
![]() | (7a) |
The elastic backing is loaded by displacement control, and we denote
uA(t) ≡ u(x = 0,t) | (7b) |
δtip ≡ δ(x = −c,t) = u(x = −c,t) | (7c) |
![]() | (8) |
Using this normalization, eqn (6) simplifies to
![]() | (9) |
Δ(X,t = 0) = 0 | (10) |
The boundary conditions (BCs) are:
![]() | (11a-c) |
![]() | (12) |
![]() | (13) |
According to (12), the maximum slip occurs at the crack tip X = −C and is Δtip. The normalized length of the slip zone is .
![]() | (14) |
By continuity, (14) is also the tension strain at the crack tip, which is obtained using (12), i.e.,
![]() | (15) |
Equating (14) and (15) and using (13) and the normalization (8), the normalized applied displacement UA(t) ≡ uA(t)/δ0 and the normalized slip at the crack tip Δtip(t) are related to each other by
![]() | (16a) |
![]() | (16b) |
Note C is the normalized crack length, and β is directly proportional to it by the factor . From here on, we will refer to either C or β as the normalized crack length.
In the following, we introduce a normalized time T by
![]() | (17) |
We assume a constant displacement rate, , is applied to the peel arm at x = 0, where α is the normalized peel rate, i.e.,
![]() | (18) |
Using (18), the maximum normalized slip at the crack tip (16a) is
![]() | (19) |
Note that we have not restricted the crack length to be stationary, i.e., β can be a function of time.
![]() | (20a) |
The normalized form of (20a) (recall δ(x = −c,t) = δ0Δtip(T)) is
![]() | (20b) |
Here we note that in (20b) depends on both the crack motion and the loading rate. Specifically, using (12),
![]() | (20c) |
The physical interpretation of (20b) is as follows: the left-hand side (LHS) is the normalized energy release rate, while the right-hand side (RHS) represents the normalized intrinsic toughness, which depends on both the loading rate and the crack growth rate (for more details, see ESI†). These two (external loading rate and crack growth rate) compete. To see this and to unravel the features noted in the introduction, we consider two situations: crack initiation and the subsequent crack growth in a constant displacement rate test.
For crack initiation, the crack is stationary, so the normalized crack length C and are independent of time, the local slip rate is obtained by setting dC/dT = 0 in (20c) and evaluating
using (19), this results in
![]() | (21a) |
![]() | (21b) |
Note the effect of loading rate α and crack growth rate dβ/dT on the rate of energy flow to the crack tip is coupled since the crack growth rate and loading rate both appear in . Also, when crack growth rate is zero, (21b) reduces to (21a).
![]() | (22) |
We state a key result in this paper: for any arbitrary continuous ϕ(η) that has an ascending branch followed by a descending branch (with a maximum value ϕmax at η = ηmax), there exists a critical normalized loading rate α* given by
![]() | (23) |
the crack initiation time corresponding to α* is
![]() | (24) |
To illustrate these results, we use the special case of a piece-wise linear shear response function ϕ (illustrated in Fig. 3(b)) where
![]() | (25a-c) |
Fig. 4 plots the LHS of (22), i.e., as solid lines, and the RHS of (22), i.e.,
as dash-dot lines, both plotted against the normalized time T for different values of α. For each value of α, the RHS and LHS of (22) generate two curves. Note that the LHS of (22) is a monotonically increasing function of T with increasing slope whereas the RHS of (22) increases, reaches a maximum, and then decreases. As a result, the two curves intersect at a single point, which gives the initiation time TI. In Fig. 4, we use β = β0 = 1, ϕmax = 4, and ηmax = 1. The critical loading rate α* = 3/2 with
is used as a reference. An interesting result shown in Fig. 4 is that the initiation time decreases with increasing α.
![]() | ||
Fig. 4 Illustration of theory using (25a–c). The functions in (22), i.e., ![]() ![]() |
![]() | (26) |
Note that (9) is independent of rate, so the equation governing slip distribution is the same as (9) with x → ξ. Using the same normalization, the BCs are:
![]() | (27a-c) |
Following the same line of reasoning, the slip distribution inside the cohesive zone is:
![]() | (28) |
Next, we determine the steady-state crack velocity vss using the fracture condition (20a), i.e.,
![]() | (29a) |
![]() | (29b) |
To gain a deeper understanding of the requirement for steady-state, we apply energy balance analysis. Let Fss denote the constant peel force exerted at the end of the peel arm which is subjected to a constant strain εss, they are related by
Fss = E*hεss | (30) |
The strain in the peel arm is:
![]() | (31) |
![]() | (32) |
In steady-state, the rate of energy input must be constant and is given by
![]() | (33) |
![]() | (34a) |
After cancellation, (34a) is
![]() | (34b) |
![]() | (35) |
![]() | (36) |
Substituting (35) and (36) into the energy balance eqn (34b), we obtain
![]() | (37) |
We study stability of crack growth by imposing a small perturbation in the crack velocity and examining the change in the energy functional (see (29a))
![]() | (38) |
![]() | (39) |
![]() | (40) |
A simple example is when ϕ is given by (25a–c), SSCG is stable on the ascending branch since . Note when Δss = ϕmax, the maximum velocity for stable crack growth is reached, which is
![]() | (41) |
![]() | (42) |
During crack growth, the fracture criterion is determined using (19), (20b) and (21b), i.e.,
![]() | (43a) |
Eqn (43a) is a nonlinear ordinary differential equation for β with initial condition
β(T = TI) = β0 | (43b) |
Eqn (43a) is solved numerically using ode45 in Matlab using the initial condition (43b). In these calculations, we chose different values of α < α* so crack initiation occurs on the ascending branch at T = TI and is followed by stable growth. The initiation time is determined by solving (22). We stop the program if Δtip reaches its maximum value ϕmax, i.e., at T = Tmax. Fig. 5 below shows the result for α = 0.5 < α* = 1.7071, with β0 = 1, ηmax = 1 and ϕmax = 2. The blue line in this figure is the normalized crack length β versus time. It shows that the crack reaches a constant velocity shortly after initiation. For this value of α (fairly slow loading rate), the crack remains on the ascending branch for all times, that is, ϕmax is never reached (see the red line which plots Δtip versus time).
The numerical result in Fig. 5 shows that Δtip is practically constant for large T, and in this regime, β ≈ b + ωT where ω and b are constant. Since , it is possible for it to approach a constant at large T if β2 ≫ αT so that
![]() | (44) |
In Fig. 5, the fitted slope gives ω = 0.1879, and with α = 0.5, the asymptotic value of Δtip is predicted to be approximately 1.77, which is consistent with the numerical result of 1.75. As expected, crack growth remains on the ascending branch and reaches steady state as long as α < ηmax, which is consistent with our numerical results, shown in Fig. 5 and 6 (α = 0.9). Plots with other values of loading rates are similar and are given in ESI.†
The situation is different for α* > α > ηmax. For this case, our analysis (see Appendix) shows that Δtip will reach ϕmax, so it is possible for the crack to reach the descending branch. Fig. 7 and 8 show the simulation results with α = 1.1 and 1.2 respectively.
![]() | ||
Fig. 8 Normalized crack length β (blue line) and Δtip (red line) versus normalized time T for α = 1.2 < α* = 1.7071. Simulations used β0 = 1, ηmax = 1, ϕmax = 2. |
Note that the crack velocity starts at zero and keeps increasing until ϕ reaches its maximum value, which is 2 in our simulations. However, our attempt to solve the differential equation on the descending branch fails – we cannot find equilibrium solution for (43a) on the descending branch. Specifically, in the first step of the solution process with the initial condition obtained from the numerical solution on the ascending branch at Δtip = ϕmax, we find that the LHS of eqn (43a) is larger than ϕmax which is impossible. This indicates that the solution on this branch is unstable, and that it is necessary to include inertia effects to balance energy.
The classical understanding of crack propagation stability, which links structural characteristics such as (dG/dA < 0, A is the crack area) with material properties (dΓ/dv > 0), is overly simplistic as it only applies to steady-state conditions. It fails to explain phenomena like crack initiation and stick-slip dynamics. Key features, such as (1) whether slow fracture propagation occurs before rapid unstable crack growth (slip), (2) the dependence of the critical strain energy release rate for unstable rapid crack growth (slip) on the loading rate in elastic samples, and (3) delayed fracture initiation after static loading, cannot be fully captured or even qualitatively described by the classical approach.
The classical approach for predicting crack propagation under time-variable loading involves evaluating the strain energy release rate, G(c,uA) as a function of crack length and external loading, and using the steady-state toughness function, Γ(v), to predict the crack propagation rate. This yields a differential equation for quasi-static crack growth. While this method works when representing the crack front as a mathematical line with an energy sink Γ, it overlooks the finite length scale L of the cohesive zone at the crack front. This length scale introduces a characteristic timescale t* ≡ L/v which determines how long it takes to reach steady-state after changes in loading conditions. Thus, the classical approach is only valid if loading changes occur over timescales longer than t*. However, this is not the case during crack initiation under ramp loading or in stick-slip dynamics, where the loading time is comparable to or shorter than t*. The fracture energy function alone cannot capture these non-steady-state effects. Our work demonstrates that using a rate-dependent cohesive zone model provides a more accurate physical description of these effects. It also allows us to quantify critical loading rates where transitions between different phenomena occur, considering both crack propagation properties and the structural characteristics of the sample.
To provide a concise analytical description of the kinematics of crack propagation in a rate-dependent cohesive zone under time-dependent loading, we developed a model based on the zero-angle peeling of adhesive tape, also known as the shear lag test. We selected the simplest form of a rate-dependent cohesive zone to capture the general behavior of fracture energy: increasing with the local loading rate, reaching a maximum, and then decreasing. This was implemented using a Dugdale-like visco-plastic model with constant cohesive stress τ0 and rate-dependent maximum elongation δc.
The set of analytical expressions and differential equations, combined with numerical simulations, enabled us to describe different stability regimes of steady-state crack propagation and to illustrate the viscoelastic effects during non-steady-state loading. Specifically, we identified several regimes of crack propagation kinetics when a static crack is loaded at a constant velocity:
(1) At very low loading rates, crack propagation begins at a low velocity after a delay and gradually accelerates to reach steady-state conditions.
(2) At moderate loading rates, crack propagation starts slowly, similar to the low-rate case, but then the velocity continuously increases until a critical velocity is reached. Beyond this point, the strain energy release rate becomes critical, and the crack becomes unstable, rapidly accelerating to dynamic conditions. We remark that in these conditions, the critical strain energy release rate is independent of the sample loading rate.
(3) At high loading rates, no crack propagation occurs initially during loading. Once the unstable region is reached, sudden dynamic crack propagation occurs after the critical strain energy release rate is achieved, which decreases with increasing loading rate.
These different kinetic regimes demonstrate how the model captures the transition between stable and unstable crack propagation, driven by both loading rate and the viscoelastic response of the material. When applied to stick-slip dynamics, this model helps explain why, for some materials and geometries (such as PSA and epoxy resin), the amplitude of stick-slip oscillations depends on the loading rate, while for others (such as PMMA), it does not. The latter behavior is the only one predicted by classical models. Although the present simplified model cannot be directly applied to these experimental configurations, some quantitative links can be made with the fracture propagation regimes in previously published experimental data. Concerning PMMA, the characteristic velocity of the toughness peak is 1 cm s−1, the cohesive zone has typical length of 30 μm and the characteristic time to cross it is thus 3 ms.7 During any kind of macroscopic fracture tests leading to stick-slip the loading time for each stick-slip cycle is longer than 10 s, and is thus much larger than 3 ms.8 The loading rate is thus systematically slower than the critical value for unstable initiation, and the fracture will systematically reach steady-state (at low loading rate) or stick-slip with constant maximum toughness (at the highest achievable loading rates).2 Concerning epoxy resins, the characteristic velocity of the toughness peak is about 1 nm s−1, which is 7 orders of magnitude smaller than for PMMA.8 The typical length of the cohesive zone is 10 μm, and the characteristic time to cross it is thus several hours.8 During typical loading macroscopical fracture tests in epoxy the loading time before each stick-slip event ranges from seconds to minutes and is thus much shorter that hours. The loading rate is thus systematically faster than the critical value for unstable initiation, and the fracture will thus systematically start in an unstable condition, and thus present a toughness that decreases with the loading rate as observed in experiments.3 Concerning PSA, the characteristic velocity of the toughness peak is about 1 cm s−1, the cohesive zone has typical length of 100 μm and the characteristic time to cross it is thus 10 ms.14 During typical stick-slip crack propagation the order of magnitude of the frequency of stick-slip cycles is 100 Hz, so the typical duration of the reloading phases is 10 ms,6 which is comparable with the characteristic time to cross the process zone. This explains why typical experimental data present a transition from a constant maximum toughness at slow loading rates, to a decreasing toughness at higher loading rates, which is consistent with our modeling.1
There is one more stick-slip dynamics regime that escapes a sound interpretation using the classical approach. When the sample loading rate is so fast that the critical strain energy release rate for unstable crack initiation decreases close to the lower limit, the amplitude of the stick-slip cycles becomes very weak in experiments, and the crack length increment in each cycle can decrease to less than the cohesive zone length. Under these circumstances the entire slip phase occurs under non-steady-state conditions and its dynamics can no longer be described by Fig. 1, as is generally the case for large amplitude stick-slip. Although this regime is frequently reported as stable crack propagation,3 since the force fluctuations are very weak, and the crack increments are barely noticeable, the propagation is strictly unstable as long as the slope of the curve is weak but still negative and should be properly described by an extension of the present model to account for dynamic effects. For example, in the present shear loading configuration, the elasto-dynamic equation of the tight backing could be implemented in order to describe the generation of propagating elastic waves due to sharp variations of the crack propagation velocity during stick-slip or even the excitation of global vibrational modes of the backing when the stick-slip frequency matches the resonance frequency of the tight backing.
Finally, although our mathematical derivations are based on simplified assumptions, the model incorporates all fundamental aspects of rate-dependent crack propagation. We believe our model is broadly applicable across various materials and scenarios, even if more complex mathematical expressions may be needed in specific cases. These findings highlight the critical role of rate-dependent crack propagation, and they should be considered by researchers modeling crack propagation kinetics under non-steady-state conditions.
Next, we consider the RHS of (22). There are two cases: α ≤ ηmax and α > ηmax.
For the case of α ≤ ηmax, since
![]() | (A1.1) |
![]() | ||
Fig. 9 Schematic illustration of case 1 where α ≤ ηmax for fracture initiation. (a) Blue curve is the RHS of (22), i.e., ϕ while red curve is the LHS, i.e., Δtip, the intersection gives the initiation time. (b) Schematic plot of the shear response function ϕ showing relation between α, ηmax and α*. Plots not to scale. |
Next, consider the 2nd case where α > ηmax. For this case, the RHS of (22), when plotted against T, reaches ϕmax at some time Tmax(α), i.e., this occurs when
![]() | (A1.2) |
In the first scenario: Δtip(T = Tmax) < ϕmax, because of α > ηmax, the RHS of (22) takes value on the descending branch of for T > Tmax(α). On the other hand, the curve associated with the LHS increases monotonically from 0 to ∞, the two curves must intersect and since Δtip(T = Tmax) < ϕmax, this intersection must takes place on the descending branch of ϕ to the right of Tmax(α), i.e., TI > Tmax(α). This situation is shown schematically in Fig. 10(e) and (f).
![]() | ||
Fig. 10 Schematic illustration of case 2 where α > ηmax for fracture initiation. In (a), (c) and (e) blue curve is the RHS of (22), i.e., ϕ, and red curve is the LHS, i.e., Δtip, the intersection gives the initiation time. (b), (d) and (f) Plot the shear response function ϕ showing relation between α, ηmax, and α*. (a) and (b) ηmax < a < a*; (c) and (d) α = α*; (e) and (f) α > α* plots not to scale. |
The condition Δtip(T = Tmax) < ϕmax can be written as (using (A1.2) and the definition of Δtip)
![]() | (A1.3) |
![]() | (A1.4) |
This shows that for α* < α, initiation must take place on the descending branch.
For the 2nd scenario where Δtip(T = Tmax) > ϕmax, the LHS of (22) must intersect the ascending branch of to the left of Tmax(α), i.e., Tmax(α) > TI. Using the same idea, it is easy to show that Δtip(T = Tmax) > ϕmax is equivalent to α* > α. This situation is shown schematically in Fig. 10(a) and (b).
Finally, the third case corresponds to α = α*, the intersection occurs at ϕ = ϕmax and as shown in Fig. 10(c) and (d). Note that
![]() | (A1.5a,A1.5b) |
Eqn (A1.5a, b) are equivalent to (23) and (24).
To summarize: if α < α*, then initiation occurs on the ascending branch. If α > α*, then initiation occurs on the descending branch. If α = α*, the initiation occurs at the peak with initiation time given by (24).
Finally, we note
![]() | (A1.6a,A1.6b) |
The validity of (A1.6a, b) can be established by substituting (A1.6a, b) into the RHS of (22) and noting that this side goes to 1 as α → 0+, ∞. It is then straightforward to show that LHS of (22) is consistent with these expressions.
Next, we show that TI(α) is a strictly monotonically decreasing function of α for α > α*. Since we already proof that a unique root of exist, we compute
using implicit differentiation, i.e.,
![]() | (A1.7a) |
![]() | (A1.7b) |
![]() | (A1.7c) |
c | Length of interface crack or the length of the peel arm, see in Fig. 2 |
c0 | Crack length set at t = 0 for steady state |
C | ![]() |
Css | Steady-state normalized crack length |
Ċss | Steady-state normalized crack velocity |
E* | Plane strain modulus of the elastic backing layer |
F | Force applied to the peel arm |
Fss | Constant peel force at the end of peel arm for steady-state crack growth |
G | Strain energy release rate |
h | Elastic backing layer thickness, see in Fig. 2 |
l | Cohesive zone length, see in Fig. 2 |
L | ![]() |
Lss | Steady-state normalized cohesive zone length |
s | ≡ (ϕmax − 1)/ηmax positive slope of ϕ(η) used in piece-wise linear shear response function, eqn (25) |
t | Time |
T | ![]() |
TI | Normalized crack initiation time, eqn (22) |
![]() | Critical initiation time corresponding to critical normalized velocity, ![]() |
u | Displacement of the elastic backing layer |
uA | ≡ u(x = 0)) horizontal displacement applied to the end of elastic layer, see in Fig. 2 |
UA | ≡ uA/δ0 normalized applied displacement to the peel arm |
v | Crack velocity |
vss | Constant peel velocity, or crack growth rate in steady-state crack growth |
Vss | Normalized steady-state crack velocity, see in eqn (29b) |
x | Horizontal coordinate, with x = 0 located at right end of the elastic layer where displacement is applied to, Fig. 2 |
X | ![]() |
α | Normalized constant peeling (loading) velocity, eqn (18) |
α* | Critical normalized loading velocity determining whether fracture initiation occurs on the ascending or descending branch, eqn (23) |
β | ![]() |
β0 | ≡ β(T = TI), initial normalized crack length |
Γ | Velocity dependent fracture toughness |
Γ0 | = τ0δ0, interfacial toughness at zero slip rate of Dugdale–Barenblatt (DB) model |
Γc | = τ0δc, interfacial toughness of DB model |
δ | Shear displacement jump or slip across the backing/substrate interface |
δ0 | Critical slip at zero slip rate in DB model, see eqn (2) |
δc | Rate dependent critical slip above which the interface fails, see eqn (2) |
δtip | ≡ δ(x = −c) slip at the tip of crack |
![]() | Slip rate |
![]() | Characteristic slip rate in DB model, eqn (2) |
Δ | ≡ δ/δ0 normalized slip displacement |
Δss | Δtip for steady-state crack growth |
Δtip | ≡ Δ(X = −C) = δtip/δ0 normalized slip at the tip of crack |
![]() | ![]() |
![]() | ![]() |
εA | Tensile strain in the peel arm |
η | ![]() |
ηmax | ϕ(ηmax) = ϕmax |
Λ | Difference between normalized energy release rate and normalized intrinsic toughness, eqn (38) |
ξ | ≡ c0 + x + vsst coordinate with origin located at moving crack tip |
Ξ | ![]() |
σ | Uniaxial tension in elastic layer |
τ | Interfacial shear stress |
τ0 | Constant shear stress value used in DB model, eqn (2) |
ϕ | Shear response function used in this work, depends only on ![]() |
ϕmax | Maximum value of ϕ |
Φ | General form of shear response function which depends on both δ and ![]() |
ω | Normalized crack length β growth rate, i.e., ![]() |
Footnote |
† Electronic supplementary information (ESI) available. See DOI: https://doi.org/10.1039/d4sm01433b |
This journal is © The Royal Society of Chemistry 2025 |