
where ∂4h/∂x4represents the elastic bending pressure due to long-wavelength sheet deformations, B>0
is a scaling parameter for the bending pressure, ∂2h/∂x2represents the surface tension between the elastic
sheet and liquid, and the disjoining pressure
Π(h) = A
hm,m>0,A=1
m>0 (2c)
characterizes the wetting property of the solid substrate, where A>0 is the Hamaker constant. For m=3,
Π(h) = A/h3corresponds to the van der Waals model [5] for the destabilizing intermolecular adhesion
pressure [1]. Other elastohydrodynamic lubrication models [4, 6] have also used the disjoining pressure
˜
Π(h) = A(h−3−σ6h−9)with σ>0, where the two terms in ˜
Π(h)represent the repulsive and attractive
intermolecular forces corresponding to the standard Lennard-Jones potential. A similar form of the disjoining
pressure ˜
Π(h) = Ah−3(1−εh−1)with ε>0 is often used in thin film models, setting a lower bound h=
O(ε)>0 for the film thickness hand preventing thin film rupture from happening [7–9].
Starting from positive and finite-mass initial data h0(x)>0 at time t=0, the dynamics of the model
(1) are governed by the interaction between the higher-order elastic bending pressure, the surface tension,
and the disjoining pressure. Following the work of Young and Stone [4], we consider the no-flux boundary
conditions at x=0 and x=L,
hx=hxxx =hxxxxx =0,at x=0,L.(3)
The dynamics of (1) can also be described by a monotone decreasing energy functional
E=ZL
0
B
2∂2h
∂x22
+1
2∂h
∂x2
+U(h)dx,with dE
dt =−ZL
0
hn∂p
∂x2
dx ≤0,(4)
where U(h)is the interaction potential that satisfies U0(h) = Π(h).
Thin film rupture is a type of nonlinear instability that leads to finite-time singularities as the film thick-
ness approaches zero at a point. That is, h→0 at an isolated point, x=xc, at a finite critical time t=tc. It
was shown in [10] that thin film equations can yield self-similar rupture singularities driven by van der Waals
forces. Different types of finite-time rupture dynamics have been investigated in a family of generalized lu-
brication equations parametrized by exponents in conservative and non-conservative loss terms, respectively
[7, 11]. In this work, we focus on the impact of the sixth-order bending pressure and the fourth-order surface
tension terms on the rupture dynamics of the generalized elastohydrodynamic lubrication equation (1).
Finite-time singularities in thin film equations can result from growth in spatial perturbations due to
strong instabilities. To perform a stability analysis of flat film solutions in (1), we perturb the spatially-
uniform base state h=¯
hby an infinitesimal Fourier mode h(x,t) = ¯
h+δeikπx/L+λt+O(δ2), where kis
the wave number, λis the growth rate of disturbances, and the initial amplitude δ1. Substituting the
expansion into model (1) and linearizing about h=¯
hyields the dispersion relation
λ=−¯
hnkπ
L2"Bkπ
L4
+kπ
L2
−1
¯
hm+1#.(5)
This relation indicates that the uniform film ¯
h<hcis long-wave unstable with respect to perturbations asso-
ciated with any wave number k∈Z+, where the critical film thickness hc=B(kπ/L)4+ (kπ/L)2−1/(m+1).
Moreover, the relation (5) also shows that the disjoining pressure Π(h) = 1/(mhm)is destabilizing, and both
the elastic bending pressure B∂4h/∂x4and the surface tension −∂2h/∂x2are stabilizing in the PDE (1).
The structure of the paper is as follows. In Section 2 we analyze the asymptotic self-similar rupture
solutions in (1), with a focus on the role of the bending pressure term. Numerical studies for the singularity
solutions are presented in Section 3, followed by concluding remarks in Section 4.
2