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Article

Local and Global Existence of Solution for Love Type Waves with Past History

1
Department of Mathematics, College of Sciences and Arts, Qassim University, Ar-Rass 51921, Saudi Arabia
2
Department of Mathematics and Computer Science, Faculty of Science, Port Said University, Port Said 42511, Egypt
3
Laboratoire de Mathématiques Appliquées et de Modélisation, Université 8 Mai 1945 Guelma. B.P. 401, Guelma 24000, Algerie
*
Author to whom correspondence should be addressed.
Mathematics 2020, 8(11), 1998; https://doi.org/10.3390/math8111998
Submission received: 18 September 2020 / Revised: 18 October 2020 / Accepted: 28 October 2020 / Published: 9 November 2020

Abstract

:
In this paper, we consider an initial boundary value problem for nonlinear Love equation with infinite memory. By combining the linearization method, the Faedo–Galerkin method, and the weak compactness method, the local existence and uniqueness of weak solution is proved. Using the potential well method, it is shown that the solution for a class of Love-equation exists globally under some conditions on the initial datum and kernel function.

1. Introduction

Love equation is a one-dimensional mathematical model that is used to determine a many physical phenomenon. This theory is a continuation of the Euler–Bernoulli beam theory and was developed in 1888 by Love. This kind of system appears in the models of nonlinear Love waves or Love type waves. It is a generalization of a model introduced by [1,2,3].
In order to completely study an evolutionary mathematical equation, a quantitative and qualitative study must be approached. An initial boundary value problem for a nonlinear Love equation with infinite memory has been considered by Zennir and et al. in [4] and the finite time blow up of weak solution has been shown under a relationship between the relaxation function g and nonlinear sources, i.e., u when t T ( T is a finite time). Next, a very general decay rate for solution of the same problem, by certain properties of convex functions combined with some estimates, has been obtained in [5]. These two last results are considered as a qualitative studies. Obviously, in order to complete the study, we have to address the problem in quantitative terms. This is the subject of our present article, from a different angle, where we proved in detail, with the use of the most modern methods, the local existence (on small temporal period [ 0 , T m a x ] ) and global existence of solution on ( 0 , ) .
Investigations on the propagation of surface waves of Love-type are made by many authors in different models and many attempts to solve Love’s equation have been performed, in view of its wide applicability. To our knowledge, there are few results for damped equations of Love waves or Love type waves. However, the existence of solutions or blow up results, with different boundary conditions, have been extensively studied by many authors.
To begin with, one must goes to the origins of Love’s equation. It is derived in [6,7] by the energy method. Under the assumptions that the Kinetic energy per unit of length is
e 1 = 1 2 F ρ [ t u 2 + κ 2 w 2 t u x 2 ] ,
and the potential energy per unite of length is
e 2 = 1 2 E F ( u x 2 ) ,
where F is an area of cross-section, w is a cross-section radius of gyration about the central line.
Using in (2) the corrected form of tension, we have
e 2 = 1 2 F u x ( E u x + ρ κ 2 w 2 t t u x ) .
Then, the variational equation of motion is given by
δ t 1 t 2 d s 0 L ( e 1 e 2 ) d x = 0 ,
and we then obtain the equation of extensional vibrations of rods as
t t u E ρ u x x 2 κ 2 w 2 t t u x x = 0 .
The parameters in (5) have the following meaning: u is the displacement, κ is a coefficient, E is the Young modulus of the material and ρ is the mass density.
This type of problem describes the vertical oscillations of a rod and was established from Euler’s variational equation of an energy functional associated with (5). A classical solution of problem (5), with null boundary conditions and asymptotic behavior, is obtained by using the Fourier method and method of small parameter.
In this article, Love-equation is considered as follows
t t y λ 0 y x + λ 1 t y x + λ 2 t t y x x + λ t μ ( t s ) y x x ( s ) d s = F [ y ] F [ y ] x + f ( t , x ) , 0 < t < T , x Ω = ( 0 , L ) ,
subject to the homogeneous Dirichlet boundary conditions
y ( t , 0 ) = y ( t , L ) = 0 , t ( 0 , T ) ,
and the following initial conditions
y ( 0 , x ) = y ˜ 0 ( x ) , t y ( 0 , x ) = y ˜ 1 ( x ) , x Ω ,
where
F [ y ] = F t , x , y , y x , t y , t y x C 1 R + × [ 0 , L ] × R 4 ,
y = y ( t , x ) , y x = y x ( t , x ) , y x x = 2 y x 2 ( t , x ) , λ , λ 0 , λ 1 , λ 2 , L > 0 are constants. The past history in (6) is t μ ( t s ) y x x ( s ) d s , which is considered as a damping term. It is well known that the damping terms play an important role in the studying the propagation mechanism of wave. It shows a behavior which is something between that of elastic solids and Newtonian fluids. Indeed, the stresses in these media depend on the entire history of their deformation, not only on their current state of deformation or their current state of motion.
Equation (6) is a generalization of a class of symmetric regularized long wave equations, known in abbreviation as (SRLWEs), given by
t t y y x x t t y x x = y t y x u x t u .
Equation (10) was proposed as a model for propagation of weakly nonlinear ion acoustic and space charge waves, it is explicitly symmetric in the x and t derivatives and is very similar to the regularized long wave equation which describes shallow water waves and plasma drift waves. The SRLWE and its symmetric version also arises in many other areas of mathematical physics.
The functions μ and f satisfy
Hypothesis 1.
μ C 1 ( R + , R + ) is a nonincreasing function such that:
λ 0 λ 0 μ ( s ) d s = l > 0 , μ ( 0 ) > 0 , lim s μ ( s ) = 0 ;
Hypothesis 2.
y ˜ 0 , y ˜ 1 H 0 1 ( Ω ) H 2 ( Ω ) ;
Hypothesis 3.
f H 1 ( ( 0 , T ) × Ω ) ;
Hypothesis 4.
F C 1 [ 0 , T ] × [ 0 , L ] × R 4 , F ( t , 0 , 0 , y 2 , 0 , y 4 ) = F ( t , L , 0 , y 2 , 0 , y 4 ) = 0 for all t [ 0 , T ] , y 2 , y 4 R .
Below, for F = F ( t , x , y 1 , , y 4 ) , we denote D 1 F = F t , D 2 F = F x , D i + 2 F = F y i , with i = 1 , , 4 . Our interest in this paper arose in the first place in consequence of a query for existence of unique solution.
Equations of Love waves or Love-type waves have been studied by many authors, we refer to [8,9,10,11,12,13], and references therein. In [8] a higher order iterative scheme is established for a Dirichlet problem for a class nonlinear Love-type equations
t t y y x x t t y x x = f ( x , t , y ) ,
and the authors get a recurrence sequence that converges at a rate 1 to a local unique weak solution of the above mentioned equation. In [8] is considered the following nonlinear Love equation
t t y y x x t t y x x λ 1 t y x x + λ t y = F ( x , t , y , y x , t y , t y x ) G ( x , t , y , y x , t y , t y x ) x + f ( x , t ) ,
with initial conditions and homogeneous Dirichlet boundary conditions and the authors established the existence of a unique local weak solution, a blow-up result for solutions with negative initial energy, the global existence and exponential decay of weak solution. In [9] is investigated the following Love equation
t t y μ ( x , t ) y x x + f ( y , t y ) = F ( x , t ) ,
with initial conditions and boundary conditions of two-point type and the authors proved existence of a weak solution, uniqueness, regularity, and decay properties of solution. In [13] is investigated the following nonlinear Love equation
t t y B x , t , y , y 2 , y x 2 , t y 2 , t y x 2 y x + λ 1 t y x + t t y x x + λ t y       =   F x , t , y , y x , t y , t y x , y ( t ) 2 , y x ( t ) 2 , t y ( t ) 2 , t y x ( t ) 2             G x , t , y , y x , t y , t y x , y ( t ) 2 , y x ( t ) 2 , t y ( t ) 2 , t y x ( t ) 2 x             + f ( x , t ) ,
with initial conditions and homogeneous Dirichlet boundary conditions and the authors proved existence and uniqueness of a solution, a blow-up of the solution with a negative initial energy and the exponential decay of weak solution.
The existence/nonexistence, exponential decay of solutions, and blow-up results for viscoelastic wave equations, have been extensively studied and many results have been obtained by many authors (see [14,15,16]).
In this paper, the attention is focused on the local and global existence of weak solution of the problem (6)–(8). In Section 2, combining the linearization method, the Faedo–Galerkin method, and the weak compactness method, the local existence and uniqueness of the weak solution of the problem (6)–(8) is proved. In Section 3, using the potential well method, it is shown that the solution for class of Love-equation exists globally under some conditions on the initial datum.

2. Existence and Uniqueness of Local Weak Solution

Definition 1.
A function y is said to be a weak solution of (6)–(8) if
y , t y , t t y L ( ( 0 , T ) , H 0 1 ( Ω ) H 2 ( Ω ) )
and y satisfies the variational equation
0 L t t y w d x + 0 L ( λ 0 y x + λ 1 t y x + λ 2 t t y x ) w x d x λ 0 L 0 μ ( s ) y x ( t s ) d s w x d x = 0 L f w d x + 0 L F [ y ] w d x + 0 L F [ y ] w x d x ,
for all test functions w H 0 1 ( Ω ) and for almost all t ( 0 , T ) .
The following technical result will play an important role in the sequel. [4] For any v C 1 0 , T , H 0 1 ( Ω ) we have
Ω 0 μ ( s ) v x x ( t s ) t v ( t ) d s d x = 1 2 t 0 μ ( s ) Ω | v x ( t s ) v x ( t ) | 2 d x d s 1 2 t 0 μ ( s ) d s Ω v x ( t ) 2 d x 1 2 0 t μ ( s ) Ω | v x ( t s ) v x ( t ) | 2 d x d s + 1 2 μ ( t ) Ω v x ( t ) 2 d x .
Now, we will prove the existence of a unique local solution for (6)–(8). Our main result is as follows.
Theorem 1.
Let y 0 , y 1 H 0 1 ( Ω ) H 2 ( Ω ) be given. Assume that (Hypothesis 1) –(Hypothesis 4) hold. Then there exists a T ( 0 , T ] such that the problem (6)–(8) has a unique local solution y for which
y , t y , t t y L ( ( 0 , T ) ; H 0 1 ( Ω ) H 2 ( Ω ) ) .
Proof of Theorem 1.
Firstly, we will construct a sequence { y m } m N . Then, the Faedo–Galerkin method combined with the weak compactness method shows that { y m } m N converges to y which is exactly a unique local solution of (6)–(8).
Step 1. Let T > 0 be fixed and M > 0 be arbitrarily chosen. We set
K M ( f ) = f L 2 ( ( 0 , 1 ) × ( 0 , T ) ) 2 + t f L 2 ( ( 0 , 1 ) × ( 0 , T ) ) 2 + f x L 2 ( ( 0 , 1 ) × ( 0 , T ) ) 2 .
Let
F C 0 ( [ 0 , 1 ] × [ 0 , T ] × [ M , M ] 4 ) = sup ( x , t , y 1 , , y 4 ) [ 0 , 1 ] × [ 0 , T ] × [ M , M ] 4 | F ( x , t , y 1 , , y 4 ) | ,
and
F ¯ M = F C 1 ( [ 0 , 1 ] × [ 0 , T ] × [ M , M ] 4 ) = F C 0 ( [ 0 , 1 ] × [ 0 , T ] × [ M , M ] 4 ) + i = 1 6 D i F C 0 ( [ 0 , 1 ] × [ 0 , T ] × [ M , M ] 4 ) .
For some T ( 0 , T ] and M > 0 , we put
W ( M , T ) = { v , t v L ( 0 , T ; H 0 1 H 2 ) : t t v L ( 0 , T ; H 0 1 ) , with v L ( 0 , T ; H 0 1 H 2 ) , t v L ( 0 , T ; H 0 1 H 2 ) , t t v L ( 0 , T ; H 0 1 ) M } , W 1 ( M , T ) = { v W ( M , T ) : t t v L ( 0 , T ; H 0 1 H 2 ) } .
Take y 0 0 and define the sequence { y m } m N as follows
0 L t t y m w d x + 0 L λ 0 y x m + λ 1 t y x m + λ 2 t t y x m w x d x λ 0 μ ( s ) d s 0 L y x m w x d x λ 0 μ ( s ) 0 L ( y x m ( t s ) y x m ) w x d x d s = 0 L f w d x + 0 L F m 1 [ y ] w d x + 0 L F m 1 [ y ] w x d x , t [ 0 , T ] , w H 0 1 ( Ω ) , y m ( 0 ) = y ˜ 0 , t y m ( 0 ) = y ˜ 1 on Ω , m N ,
where
F m 1 [ y ] = F [ y m 1 ] = F x , t , y m 1 , y x m 1 , t y m 1 , t y x m 1 .
Let { w j } j = 1 be an orthonormal basis of H 0 1 ( Ω ) , formed by the eigenfunctions of the operator 2 x 2 . Let also, V k = s p a n { w 1 , w 2 , , w k } . We have
y ˜ 0 k = j = 1 k α j ( k ) w j , y ˜ 1 k = j = 1 k β j ( k ) w j ,
for
α j ( k ) = 0 L y ˜ 0 w j d x ,
β j ( k ) = 0 L y ˜ 1 w j d x .
Note that
y ˜ 0 k y ˜ 0 strongly in H 0 1 ( Ω ) H 2 ( Ω ) , y ˜ 1 k = y ˜ 1 strongly in H 0 1 ( Ω ) H 2 ( Ω ) .
We seek k functions φ m j ( k ) ( t ) C 2 [ 0 , T ] , 1 j k , such that the expression in the form
y m ( k ) = j = 1 k φ m j ( k ) w j ,
solves the problem
0 L t t y m ( k ) w j d x + 0 L λ 0 y x m ( k ) + λ 1 t y x m ( k ) + λ 2 t t y x m ( k ) w j x d x λ 0 μ ( s ) d s 0 L y x m ( k ) w j x d x λ 0 μ ( s ) 0 L ( y x m ( k ) ( t s ) y x m ( k ) ( s ) ) w j x d x d s = 0 L f w j d x + 0 L F m w j d x + 0 L F m w j x d x , 1 j k , y m ( k ) ( 0 ) = y ˜ 0 k ( t ) , t y m ( k ) ( 0 ) = y ˜ 1 k ,
This leads to a system of ODE’s for unknown functions φ m i ( k ) . Based on standard existence theory for ODE, the system (22) admits a unique solution φ m j ( k ) , 1 j k on the interval [ 0 , T ] .
Step 2. Now we will prove that there exist constants M > 0 and T [ 0 , T ) such that y m ( k ) W ( M , T ) , for all m, k N . We partially estimate the terms of the associated energy. We replace y m and w with y m ( k ) in (17) and we get
0 L t t y m ( k ) t y m ( k ) d x + 0 L λ 0 y x m ( k ) + λ 1 t y x m ( k ) + λ 2 t t y x m ( k ) t y x m ( k ) d x + λ 0 L 0 μ ( s ) y x m ( k ) ( t s ) t y x m ( k ) d s d x = 0 L F [ y m ( k ) ] t y m ( k ) d x + 0 L F [ y m ( k ) ] t y x m ( k ) d x + 0 L f t y m ( k ) d x .
Using (13), we obtain
1 2 t [ 0 L | t y m ( k ) | 2 + λ 0 + λ 0 μ ( s ) | y x m ( k ) | 2 + λ 2 | t y x m ( k ) | 2 d x d x λ 0 μ ( s ) 0 L | y x m ( k ) ( t s ) y x m ( k ) ( t ) | 2 d x d s ] + λ 1 0 L | t y x m ( k ) | 2 d x + λ 0 t μ ( s ) 0 L | y x m ( k ) ( t s ) y x m ( k ) ( t ) | 2 d x d s = 0 L F [ y m ( k ) ] t y m ( k ) d x + 0 L F [ y m ( k ) ] t y x m ( k ) d x + 0 L f m t y m ( k ) d x .
Let us denote the left hand side of (23) as
e ( k ) ( y m ) = 0 L | t y m ( k ) | 2 + λ 0 + λ 0 μ ( s ) d s | y x m ( k ) | 2 + λ 2 | t y x m ( k ) | 2 d x λ 0 μ ( s ) 0 L | y x m ( k ) ( t s ) y x m ( k ) ( t ) | 2 d x d s + 2 λ 1 0 t 0 L | t y x m ( k ) | 2 d x d s + 2 λ 0 t 0 t μ ( s ) 0 L | y x m ( k ) ( t s ) y x m ( k ) ( t ) | 2 d x d s d τ ,
and
e ( k ) ( y x m ) = 0 L | t y x m ( k ) | 2 + λ 0 + λ 0 μ ( s ) d s | y x x m ( k ) | 2 + λ 2 | t y x x m ( k ) | 2 d x λ 0 μ ( s ) 0 L | y x x m ( k ) ( t s ) y x x m ( k ) ( t ) | 2 d x d s + 2 λ 1 0 t 0 L | t y x x m ( k ) | 2 d x d s + 2 λ 0 t 0 t μ ( s ) 0 L | y x x m ( k ) ( t s ) y x x m ( k ) ( t ) | 2 d x d s τ ,
and
e ( k ) ( t y m ) = 0 L | t t y m ( k ) | 2 + λ 0 + λ 0 μ ( s ) d s | t y x m ( k ) | 2 + λ 2 | t t y x m ( k ) | 2 d x λ 0 μ ( s ) 0 L | t y x m ( k ) ( t s ) t y x m ( k ) ( t ) | 2 d x d s + 2 λ 1 0 t 0 L | t t y x m ( k ) | 2 d x d s + 2 λ 0 t 0 t μ ( s ) 0 L | t y x m ( k ) ( t s ) t y x m ( k ) ( t ) | 2 d x d s d τ .
Put
E m ( k ) ( t ) = e ( k ) ( y m ) + e ( k ) ( y x m ) + e ( k ) ( t y m ) .
Then
E m ( k ) ( t ) = E m ( k ) ( 0 ) + 2 0 t 0 L f ( s ) t y m ( k ) ( s ) d x d s + 2 0 t 0 L f x ( s ) t y x m ( k ) ( s ) d x d s + 2 0 t 0 L t f ( s ) t t y m ( k ) ( s ) d x d s + 2 0 t 0 L F m ( s ) t y x m ( k ) ( s ) d x d s + 2 0 t 0 L F m ( s ) t y m ( k ) ( s ) d x d s + 2 0 t 0 L F x m ( s ) t y x x m ( k ) ( s ) d x d s + 2 0 t 0 L t F m ( s ) t t y m ( k ) ( s ) d x d s + 2 0 t 0 L t F m ( s ) t t y x m ( k ) ( s ) d x d s + 2 0 t 0 L F x m ( s ) t y x m ( k ) ( s ) d x d s .
Now we will estimate
A m ( k ) = 0 L | t t y m ( k ) ( 0 ) | 2 d x + λ 2 0 1 | t t y x m ( k ) ( 0 ) | 2 d x .
Let w j = t t y m ( k ) in (22). Then we take t 0 + in the first term and we obtain
0 L | t t y m ( k ) ( 0 ) | 2 d x + λ 2 0 L | t t y x m ( k ) ( 0 ) | 2 d x + 0 L λ 0 λ 0 μ ( s ) d s y ˜ 0 k x + λ 1 y ˜ 1 k x t t y x m ( k ) ( 0 ) d x + λ 0 μ ( s ) 0 L ( y ˜ 0 k x ( 0 ) y ˜ 0 k x ( s ) ) t t y m ( k ) ( 0 ) d x d s = 0 L f ( 0 ) t t y m ( k ) ( 0 ) d x + 0 L F m ( 0 ) t t y m ( k ) ( 0 ) d x + 0 L F m ( 0 ) t t y x m ( k ) ( 0 ) d x .
Then
A m ( k ) 0 L λ 0 λ 0 μ ( s ) d s y ˜ 0 k x + λ 1 y ˜ 1 k x + F m ( 0 ) t t y x m ( k ) ( 0 ) d x + λ 0 μ ( s ) 0 L ( y ˜ 0 k x ( 0 ) y ˜ 0 k x ( s ) ) t t y m ( k ) ( 0 ) d x d s + 0 L f ( 0 ) t t y m ( k ) ( 0 ) d x + 0 L F m ( 0 ) t t y m ( k ) ( 0 ) d x , 0 L [ λ 0 λ 0 μ ( s ) d s y ˜ 0 k x + λ 1 y ˜ 1 k x + 2 F m ( 0 ) + f ( 0 ) + λ 0 μ ( s ) ( y 0 k x ( 0 ) y 0 k x ( s ) ) ] d x ξ , for all m , k N .
In the last inequality we have used that 0 L | F m ( 0 ) | d x is a constant independent of m. Note that ξ is a constant depending only on f, y ˜ 0 , y ˜ 1 , F, λ 0 , λ , λ 1 , λ 2 and 0 μ ( s ) d s . Equations (20), (24) and (26) imply that
E m ( k ) ( 0 ) = 0 L | y ˜ 1 k | 2 + λ 0 λ 0 μ ( s ) d s | y ˜ 0 k x | 2 + | y ˜ 1 k x | 2 d x d x + λ 0 μ ( s ) 0 L | y ˜ 0 k x ( s ) y ˜ 0 k x ( 0 ) | 2 d x d s + 0 L | y ˜ 1 k x | 2 + λ 0 λ 0 μ ( s ) d s | y ˜ 0 k x x | 2 + | y ˜ 1 k x x | 2 d x d x + λ 0 μ ( s ) 0 L | y ˜ 0 k x x ( s ) y ˜ 0 k x x ( 0 ) | 2 d x d s + A m ( k ) + 0 L λ 0 λ 0 μ ( s ) d s | y ˜ 1 k x | 2 d x + λ 0 μ ( s ) 0 L | y ˜ 1 k x y ˜ 1 k x | 2 d x d s , ξ 0 for all m , k N ,
where ξ 0 is a constant depending only on f, y ˜ 0 , y ˜ 1 , F, λ 0 , λ , λ 1 , λ 2 and 0 μ ( s ) d s .
Now we estimate the other terms of (25). By the Cauchy—Schwartz’s inequality, we obtain
E m ( k ) ( t ) ξ 0 + f L 2 ( Ω × ( 0 , T ) ) 2 + 0 t 0 L | t y m ( k ) | 2 d s d x ; + f x L 2 ( Ω × ( 0 , T ) ) 2 + 0 t 0 L | t y x m ( k ) | 2 d x d s ; + t f L 2 ( Ω × ( 0 , T ) ) 2 + 0 t 0 L | t t y m ( k ) | 2 d x d s ; + 2 0 t 0 L F m ( s ) t y x m ( k ) ( s ) d x d s + 2 0 t 0 L F m ( s ) t y m ( k ) ( s ) d x d s + 2 0 t 0 L F x m ( s ) t y x x m ( k ) ( s ) d x d s + 2 0 t 0 L t F m ( s ) t t y m ( k ) ( s ) d x d s + 2 0 t 0 L t F m ( s ) t t y x m ( k ) ( s ) d x d s + 2 0 t 0 L F x m ( s ) t y x m ( k ) ( s ) d x d s .
By (Hypothesis 1) and (24), we have
E m ( k ) ( t ) ξ 0 + f H 1 ( Ω × ( 0 , T ) ) 2 + c 0 t E m ( k ) ( s ) d s + 2 0 t 0 L F m ( s ) t y x m ( k ) ( s ) d x d s + 2 0 t 0 L F m ( s ) t y m ( k ) ( s ) d x d s + 2 0 t 0 L F x m ( s ) t y x x m ( k ) ( s ) d x d s + 2 0 t 0 L t F m ( s ) t t y m ( k ) ( s ) d x d s + 2 0 t 0 L t F m ( s ) t t y x m ( k ) ( s ) d x d s + 2 0 t 0 L F x m ( s ) t y x m ( k ) ( s ) d x d s .
We have
E m ( k ) ( t ) ξ 0 + f H 1 ( Ω × ( 0 , T ) ) 2 + c 0 t E m ( k ) ( s ) d s + T F ¯ M 2 + 0 t 0 L | t y x m ( k ) ( s ) | 2 d x d s + T F ¯ M 2 + 0 t 0 L | t y m ( k ) | 2 d x d s + 2 0 t 0 L F x m ( s ) t y x x m ( k ) ( s ) d x d s + T F ¯ M 2 + 0 t 0 L | t y x m ( k ) ( s ) | 2 d x d s + 2 0 t 0 L t F m ( s ) t t y m ( k ) ( s ) d x d s + 2 0 t 0 L t F m ( s ) t t y x m ( k ) ( s ) d x d s .
By (Hypothesis 1), (9) and (24), we arrive to
t F x m ( t ) = D 1 F [ y m 1 ] + D 3 F [ y m 1 ] t y x m 1 + D 4 F [ y m 1 ] t y x x m 1 + D 5 F [ y m 1 ] t y x m 1 + D 6 F [ y m 1 ] t y x x m 1 .
Then
E m ( k ) ( t ) ξ 0 + f H 1 ( Ω × ( 0 , T ) ) 2 + 2 T 1 + 2 ( 1 + 4 M ) 2 F ¯ M 2 + c 0 t E m ( k ) ( s ) d s .
We choose M > 0 sufficiently large such that
ξ 0 + f H 1 ( Ω × ( 0 , T ) ) 2 1 2 M 2 ,
and then choose T ( 0 , T ] small enough such that
1 2 M 2 + T 1 + 2 ( 1 + 4 M ) 2 F ¯ M 2 exp [ 2 T ] M 2 ,
and
k T = 2 F ¯ M 2 T exp [ T ] < 1 .
Then
y m ( k ) W ( M , T ) , for all m and k .
By (33), there exists a subsequence of { y m ( k ) } , such that
y m ( k ) y m in L ( 0 , T ; H 0 1 H 2 ) weakly , t y m ( k ) t y m in L ( 0 , T ; H 0 1 H 2 ) weakly , t t y m ( k ) t t y m in L ( 0 , T ; H 0 1 ) weakly , y m W ( M , T ) .
Passing to limit in (22) we see that y m satisfies (17), (18) in L 2 ( 0 , T ) . Furthermore, (17) 1 and (36) 4 give
λ 0 y m + λ 1 t y m + λ 2 t t y m + λ 0 μ ( s ) y m ( t s ) d s = t t y m F [ y m ] F [ y m ] x f ψ m L ( ( 0 , T ) ; H 0 1 ( Ω ) H 2 ( Ω ) ) .
We deduce that, if
y m L ( ( 0 , T ) ; H 0 1 ( Ω ) H 2 ( Ω ) ) ,
then
t y m , t t y m L ( ( 0 , T ) ; H 0 1 ( Ω ) H 2 ( Ω ) ) .
So, we obtain y m W 1 ( M , T ) .
Step 3. Consider the Banach space
W 1 ( T ) = { v L ( 0 , T ; H 0 1 ) : t v L ( 0 , T ; H 0 1 ) } ,
endowed with the norm
v W 1 ( T ) = v L ( 0 , T ; H 0 1 ) + t v L ( 0 , T ; H 0 1 ) .
We will show the convergence of { y m } m N to the solution of our problem. Let w m = y m + 1 y m . Then w m satisfies
0 L t t w m w d x + 0 L ( λ 0 w x m + λ 1 t w x m + λ 2 t t w x m ) w x d x λ 0 L 0 μ ( s ) w x m ( t s ) d s w x d x = 0 L F [ w m + 1 ] F [ w m ] w d x + 0 L F [ w m + 1 ] F [ w m ] w x d x , w m ( 0 ) = t w m ( 0 ) = 0 .
Consider (39) with w = t w m . Then, integrating in t, we obtain
0 L | t w m | 2 + λ 0 λ 0 μ ( s ) d s | w x m | 2 + λ 2 | t w x m | 2 d x + λ 0 μ ( s ) 0 L | w x m ( t s ) w x m ( t ) | 2 d x d s + 2 λ 1 0 t 0 L | t w x m | 2 d x d s λ 0 t 0 t μ ( s ) 0 L | w x m ( t s ) w x m ( t ) | 2 d x d s d τ = 2 0 t 0 L F m + 1 ( s ) F m ( s ) t w m ( s ) d x d s + 2 0 t 0 L F m + 1 ( s ) F m ( s ) t w x m ( s ) d x d s .
By (Hypothesis 2)–(Hypothesis 4), (15) and (36), we have
0 L | F m + 1 ( s ) F m ( s ) | 2 d x 2 F ¯ M 0 L | w m 1 | 2 d x .
Then
E m ( t ) 2 F ¯ M 0 L | w m 1 | 2 d x + 0 t 0 L | t w m | 2 d x d s + 2 F ¯ M 0 L | w m 1 | 2 d x + 0 t 0 L | t w x m | 2 d x d s 4 F ¯ M 0 L | w m 1 | 2 d x T + 0 t E m ( s ) d s ,
where
E m ( t ) = 0 L | t w m | 2 + λ 0 λ 0 μ ( s ) d s | w x m | 2 + λ 2 | t w x m | 2 d x + λ 0 μ ( s ) 0 L | w x m ( t s ) w x m ( t ) | 2 d x d s + 2 λ 1 0 t 0 L | t w x m | 2 d x d s λ 0 t 0 t μ ( s ) 0 L | w x m ( t s ) w x m ( t ) | 2 d x d s d τ .
By (41), using Gronwall’s Lemma, we get
0 L | w m | d x k T 0 L | w m 1 | d x m N .
So,
0 L | y m y m + p | d x M ( 1 k T ) 1 k T m , m , p N .
From here, it follows that { y m } m N is a Cauchy sequence in W 1 ( T ) . Therefore there exists y W 1 ( T ) such that
y m y strongly in W 1 ( T ) .
Note that y m W 1 ( M , T ) . Hence, there exists a subsequence { y m j } j N of { y m } m N such that
y m j y in L ( ( 0 , T ) ; H 0 1 ( Ω ) H 2 ( Ω ) ) weakly , t y m j t y in L ( ( 0 , T ) ; H 0 1 ( Ω ) H 2 ( Ω ) ) weakly , t t y m j t t y in L ( ( 0 , T ) ; H 0 1 ( Ω ) ) weakly , y W ( M , T ) .
By (15), (18) and (45) 4 , we obtain
0 L | F m ( t ) F [ y ] ( t ) | d x 2 ( 1 + 2 M ) F ¯ M 0 L | y m 1 y | d x .
Then (44) and (46) imply
F m F [ y ] strongly in L ( ( 0 , T ) ; L 2 ( Ω ) ) ,
Passing to limit in (17) and (18), as m = m j . By (44), (45) and (47), it follows that there exists y W ( M , T ) satisfying
0 L t t y w d x + 0 L ( λ 0 y x + λ 1 t y x + λ 2 t t y x ) w x d x λ 0 L 0 μ ( s ) y x ( t s ) d s w x d x = 0 L f w d x + 0 L F [ y ] w d x + 0 L F [ y ] w x d x ,
for all test function w H 0 1 ( Ω ) , for almost all t ( 0 , T ) , and satisfying the initial conditions. Let y 1 , y 2 be two weak solutions of (6)–(8), such that
y 1 , y 2 W 1 ( M , T ) .
Then v = y 1 y 2 satisfies
0 L t t v w d x + 0 L ( λ 0 v x + λ 1 t v x + λ 2 t t v x ) w x d x λ 0 L 0 μ ( s ) v x ( t s ) d s w x d x = 0 L F [ y 1 ] F [ y 2 ] w d x + 0 L F [ y 1 ] F [ y 2 ] w x d x ,
for all test function w H 0 1 ( Ω ) and for almost all t [ 0 , T ] . Taking t v = w in (50) 1 and integrating with respect to t, for
e ( t ) = 0 L | t w | 2 + λ 0 λ 0 μ ( s ) d s | w x | 2 + λ 2 | t w x | 2 d x + λ 0 μ ( s ) 0 L | w x ( t s ) w x ( t ) | 2 d x d s + 2 λ 1 0 t 0 L | t w x | 2 d x d s λ 0 t 0 t μ ( s ) 0 L | w x ( t s ) w x ( t ) | 2 d x d s d τ ,
we obtain
e ( t ) = 0 L F [ u 1 ] F [ y 2 ] t v d x + 0 L F [ y 1 ] F [ u 2 ] t v x d x .
On the other hand, by (Hypothesis 2)–(Hypothesis 4), we deduce from (15), that
0 1 | F [ u 1 ] F [ u 2 ] | d x 2 c ( 1 + 2 M ) F ¯ M e 1 / 2 ( s ) .
Then
e ( t ) 4 c ( 1 + 2 M ) F ¯ M 0 t e ( s ) d s .
Thanks again to Gronwall’s Lemma, we have e 0 , i.e., y 1 y 2 . This completes the proof. □

3. Global Solution

In this section, we consider the equation
t t y λ 0 y x + λ 1 t y x + λ 2 t t y x x + λ t μ ( t s ) y x x ( s ) d s = | y | p 2 y ( | y x | p 2 y x ) x + f ( t , x ) x Ω , 0 < t < T ,
subject to the boundary conditions (7) and to the initial conditions (8). Here p > 2 . We use methods introduced in [17,18,19,20,21,22,23,24].
Assume that f L 2 ( Ω × R + ) . We introduce the energy functional E ( t ) associated with Equation (53)
E ( t ) = 1 2 0 L | t y | 2 d x + 1 2 λ 2 0 L | t y x | 2 d x + J ( t ) ,
where
J ( t ) = 1 2 0 L λ 0 λ 0 μ ( s ) d s | y x | 2 d x + 1 2 λ 0 L 0 μ ( s ) | y x ( t ) y x ( t s ) | 2 d s d x + 1 p 0 L | y x | p d x 1 p 0 L | y | p d x .
Now, we introduce the stable set as follows
W = { y H 0 1 ( Ω ) H 2 ( Ω ) : I ( t ) > 0 , J ( t ) < d } { 0 } ,
where
I ( t ) = 0 L λ 0 λ 0 μ ( s ) d s | y x | 2 d x + λ 0 L 0 μ ( s ) | y x ( t ) y x ( t s ) | 2 d s d x + 0 L | y x | p d x 0 L | y | p d x ,
and
d = inf { sup y H 0 1 H 2 \ { 0 } , ν 0 J ν y } .
In addition, we introduce the “Nehari manifold
N = y H 0 1 ( Ω ) H 2 ( Ω ) \ 0 : I t = 0 .
It is readily seen that the potential depth d is also characterized by
d = inf y N J ( t ) .
This characterization of d shows that
d i s t 0 , N = min ( y N y H 0 1 ( Ω ) H 2 ( Ω ) .
Suppose that (Hypothesis 1) holds. Let y be a solution of Equation (53). Then the energy functional (54) is a nonincreasing function and for all t 0 , ϵ > 0 , we have
t E ( t ) λ 1 ϵ 2 0 L | t y x | 2 d x + 1 2 λ 0 1 0 t μ ( s ) | y x ( t ) y x ( t s ) | 2 d s d x + 1 2 ϵ 0 L | f | 2 d x .
Proof. 
Multiplying (53) by t y ( x , t ) and integrating over [ 0 , L ] , we obtain
t E ( t ) = λ 1 0 L | t y | 2 d x + 0 L f t y d x λ 1 0 L | t y | 2 d x + 1 2 ϵ 0 L | f | 2 d x + ϵ 2 0 L | t y | 2 d x ,
which completes the proof. □
We will prove the invariance of the set W . That is, if for some t 0 > 0 and y ( t 0 ) W , then y ( t ) W , t t 0 . d is a positive constant.
Proof. 
We have
J ( ν t ) = ν 2 2 0 L λ 0 λ 0 μ ( s ) d s | y x | 2 d x + ν 2 2 λ 0 L 0 μ ( s ) | y x ( t ) y x ( t s ) | 2 d s d x + ν p p 0 L | y x | p d x ν p p 0 L | y | p d x .
Using (Hypothesis 1), we get
J ( ν y ) K ( ν ) ,
where
K ( ν ) = ν 2 2 l 0 L | y x | 2 d x ν p p 0 L | y | p d x .
By differentiating the second term in the last equality with respect to ν , we obtain
d d ν K ( ν ) = ν l 0 L | y x | 2 d x ν p 1 0 L | y | p d x .
For ν 1 = 0 and
ν 2 = l 0 L | y x | 2 d x 0 L | y | p d x ( p 2 ) ,
we have
d d ν K ( ν 2 ) = 0 , K ( ν 1 ) = 0 .
Since
d 2 d ν 2 K ( ν ) | ν = ν 2 < 0 ,
we arrive to
sup ν 0 J ( ν ) sup ν 0 K ( ν ) = K ( ν 2 ) = 1 2 l 0 L | y x | 2 d x 0 L | y | p d x 2 p 2 × l 0 L | y x | 2 d x 1 p l 0 L | y x | 2 d x 0 L | y | p d x p p 2 × 0 L | y | p d x = 1 2 l p p 2 0 L | y | p d x 2 p 2 0 L | y x | 2 d x p p 2 1 p l p p 2 0 L | y | p d x 2 p 2 0 L | y x | 2 d x p p 2 = l p p 2 1 2 1 p 0 L | y | p d x 2 p 2 0 L | y x | 2 d x p p 2 .
By Sobolev-Poincare’s inequality, we deduce that K ( ν 2 ) > 0 . Then
sup ν 0 j ( ν ) d > 0 .
Then, by the definition of d , we conclude that d > 0 . This completes the proof. □
W is a bounded neighborhood of 0 in H 0 1 ( Ω ) H 2 ( Ω ) .
Proof. 
For y W and y 0 , we have
J ( t ) = 1 2 0 L λ 0 λ 0 μ ( s ) d s | y x | 2 d x + 1 2 λ 0 L 0 μ ( s ) | y x ( t ) y x ( t s ) | 2 d s d x + 1 p 0 L | y x | p d x 1 p 0 L | y | p d x = p 2 2 p [ 0 L λ 0 λ 0 μ ( s ) d s | y x | 2 d x + λ 0 L 0 μ ( s ) | y x ( t ) y x ( t s ) | 2 d s d x ] + I ( t ) p 2 2 p [ 0 L λ 0 λ 0 μ ( s ) d s | y x | 2 d x + λ 0 L 0 μ ( s ) | y x ( t ) y x ( t s ) | 2 d s d x ] .
By (Hypothesis 1), we get
J ( t ) p 2 2 p l 0 L | y x | 2 d x + λ 0 L 0 μ ( s ) | y x ( t ) y x ( t s ) | 2 d s d x p 2 2 p l 0 L | y x | 2 d x ,
and
0 L | y x | 2 d x 1 l 2 p p 2 J ( t ) < 1 l 2 p p 2 d = R .
Consequently, for any y W , we have y B , where
B = y H 0 1 ( Ω ) H 2 ( Ω ) : 0 L | y x | 2 d x < R .
This completes the proof. □
Now, we will show that our local solution y is global in time. For this purpose it suffices to prove that the norm of the solution is bounded, independently of t. This is equivalent to prove the following theorem.
Theorem 2.
Suppose that (Hypothesis 1) and
C p l ( 1 p ) 2 p p 2 E ( 0 ) ( p 2 ) < 1 ,
hold, where C is the best Poincaré’s constant. If y ˜ 0 W , y ˜ 1 H 0 1 ( Ω ) , then the solution y W , t 0 .
Proof. 
Since y 0 ( 0 ) W , then
I ( 0 ) = 0 L λ 0 λ 0 μ ( s ) d s | y x x ( 0 ) | 2 d x + λ 0 L 0 μ ( s ) | y 0 x ( 0 ) y x ( s ) | 2 d s d x + 0 L | y 0 x ( 0 ) | p d x 0 L | y 0 ( 0 ) | p d x > 0 .
Consequently, by continuity, there exists T m T such that
I ( t ) = 0 L λ 0 λ 0 μ ( s ) d s | y x | 2 d x + λ 0 L 0 μ ( s ) | y x ( t ) y x ( t s ) | 2 d s d x + 0 L | y x | p d x 0 L | y | p d x 0 , t 0 , T m .
This gives
J ( t ) = 1 2 0 L λ 0 λ 0 μ ( s ) d s | y x | 2 d x + 1 2 λ 0 L 0 μ ( s ) | y x ( t ) y x ( t s ) | 2 d s d x + 1 p 0 L | y x | p d x 1 p 0 L | y | p d x = p 2 2 p [ 0 L λ 0 λ 0 μ ( s ) d s | y x | 2 d x + λ 0 L 0 μ ( s ) | y x ( t ) y x ( t s ) | 2 d s d x ] + 1 p I ( t ) p 2 2 p [ 0 L λ 0 λ 0 μ ( s ) d s | y x | 2 d x + λ 0 L 0 μ ( s ) | y x ( t ) y x ( t s ) | 2 d s d x ] .
By (Hypothesis 1), we easily see that
0 L | y x | 2 d x 1 l 2 p p 2 J ( t ) 1 l 2 p p 2 E ( t ) 1 l 2 p p 2 E ( 0 ) , t 0 , T m .
We then exploit (Hypothesis 1), p > 2 and the embedding H 0 1 L p
0 L | y | p d x 1 / p C 0 L | y x | 2 d x 1 / 2 ,
for some C = C ( p , Ω ) > 0 , we get
0 L | y | p d x C p 0 L | y x | 2 d x p / 2 C p 0 L | y x | 2 d x ( p 2 ) / 2 0 L | y x | 2 d x C p l 1 2 p p 2 ( p 2 ) E ( 0 ) ( p 2 ) l 0 L | y x | 2 d x β l 0 L | y x | 2 d x ,
where β = C p l ( 1 p ) 2 p p 2 E ( 0 ) ( p 2 ) . This means, by the definition of l,
0 L | y | p d x β 0 L | y x | 2 d x λ 0 λ 0 μ ( s ) d s 0 L | y x | 2 d x λ 0 λ 0 μ ( s ) d s 0 L | y x | 2 d x + λ 0 L 0 μ ( s ) | y x ( t ) y x ( t s ) | 2 d s d x .
Therefore I ( t ) > 0 for all t 0 , T m , in view of the following relation
lim t T m C p l 1 p 2 p p 2 E ( 0 ) ( p 2 ) β < 1 .
This shows that the solution y W , for all t 0 , T m . By repeating this procedure we extend T m to T . This completes the proof. □
The next Theorem shows that the local solution is global in time.
Theorem 3.
Suppose that (Hypothesis 1), p > 2 and (65) hold. If y ˜ 0 W , y ˜ 1 H 0 1 ( Ω ) . Then the local solution y is global in time such that y G T , where
G T = y : y L R + ; H 0 1 ( Ω ) H 2 ( Ω ) , t y L R + ; H 0 1 ( Ω ) .
Proof. 
Now, it is enough to show that the following norm
0 L | t y | 2 d x + 0 L | y x | 2 d x
is bounded independently of t. To achieve this, we use (54), (55) and (61). We get
E ( 0 ) E ( t ) = J ( t ) + 1 2 0 L | t y | 2 d x p 2 2 p [ 0 L λ 0 λ 0 μ ( s ) d s | y x | 2 d x + λ 0 L 0 μ ( s ) | y x ( t ) y x ( t s ) | 2 d s d x ] + 1 2 0 L | t y | 2 d x + 1 p I ( t ) p 2 2 p l 0 L | y x | 2 d x + λ 0 L 0 μ ( s ) | y x ( t ) y x ( t s ) | 2 d s d x + 1 2 0 L | t y | 2 d x + 1 p I ( t ) l ( p 2 ) 2 p 0 L | y x | 2 d x + 1 2 0 L | t y | 2 d x .
Since I ( t ) and λ 0 L 0 μ ( s ) | y x ( t ) y x ( t s ) | 2 d s d x are positive, we conclude that
l ( p 2 ) 2 p 0 L | y x | 2 d x + 1 2 0 L | t y | 2 d x C E ( 0 ) ,
where C is a positive constant depending only on p and l. This completes the proof. □

4. Conclusions

By imposing less conditions with the help of some special results, we obtained local and global existence results extending some earlier results known in the existing literature. The main results in this manuscript are the following. Theorem 1 for local existence of solution and Theorem 3 for the global existence in time based on the potential depth.
This article is considered as an essential link in a series of articles by the same authors in the same type of equations. Our research falls within the scope of interests of many researchers in the modern era, according to the general objectives and broad scope of its application areas.
The importance of this research, although it is theoretical, lies in the following:
  • We proved our results without need of how to decrease for the kernel function.
  • In our previous work, we restricted on the case where f 0 , which is not the case in these studies.
  • There are several generalizations and contributions that are very important in terms of the system itself. We proposed a damped system related to a large number (infinite) of sources, each one has functionality and physical properties, and we look at the overlapping of these terms. Which makes the problem have very wide applications and important in terms of applications in modern science, especially when it comes in bounded domain.
  • Quantitatively, we used and developed the stable set method named potential well method, with details to study the global existence of solution commensurate with the bounded domain after proving the local existence of solution using a usual method, Faedo–Galerkin method.

Author Contributions

Supervision, M.B.; Writing—original draft, K.Z.; Writing—review & editing, A.H. All authors have read and agreed to the published version of the manuscript.

Funding

This research received no external funding.

Acknowledgments

The authors would like to thank the anonymous referees and the handling editor for their careful reading and for relevant remarks/suggestions to improve the paper.

Conflicts of Interest

The authors declare no conflict of interest.

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Biomy, M.; Zennir, K.; Himadan, A. Local and Global Existence of Solution for Love Type Waves with Past History. Mathematics 2020, 8, 1998. https://doi.org/10.3390/math8111998

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Biomy M, Zennir K, Himadan A. Local and Global Existence of Solution for Love Type Waves with Past History. Mathematics. 2020; 8(11):1998. https://doi.org/10.3390/math8111998

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Biomy, Mohamed, Khaled Zennir, and Ahmed Himadan. 2020. "Local and Global Existence of Solution for Love Type Waves with Past History" Mathematics 8, no. 11: 1998. https://doi.org/10.3390/math8111998

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