Abstract
This paper describes a polynomial decay rate of the solution of the Kirchhoff type in viscoelasticity with logarithmic nonlinearity, where an asymptotically-stable result of the global solution is obtained taking into account that the kernel is not necessarily decreasing.
1. Introduction
Consider the quasilinear viscoelastic problem:
with:
where is a bounded domain with a sufficiently smooth boundary , and are positive constants, for and for , and h is a relaxation function, which will be specified later. From the physical point of view, the problem (1)–(3) is related to the spillover problem with memory and the panel flutter equation. Viscoelasticity has an important role in the study of biological phenomena, and it can have a strong effect on some factors that have a correlation with biological phenomenain general. A viscoelastic material will return back to its original size after an influential force has been detached, even though it will remain for a specific time in its original shape; see [1,2,3,4,5,6,7,8,9,10,11].
Recently, viscoelasticity problems have been handled carefully in several papers, and other results relating the global existence and decay of the global solution have been found (see [1,2,3,4,5,6,7,10,11,12,13,14,15,16,17,18,19,20,21,22,23]), where the function of the relaxation was supposed to be either exponential decay or polynomial decay. In [7], the mathematicians searched for a viscoelastic equation for more general decaying kernels and obtained some general decay results, from which the common exponential or polynomial rates were more specific samples of them. Later, many papers, using almost identical techniques, achieved analogous general decay outcomes. See [11,24]. Our decay rate obtained in the third section is less general than that obtained in [7,8], where a common decay rate outcome was established in order to let the functions of the relaxation satisfy:
a positive function , where H is either linear or a strictly-increasing and strictly-convex function on . In [7], the exponential decay for the viscoelastic wave equation of the solution with an unnecessarily decreasing kernel was handled. More specifically, the mathematicians had an exponential decay outcome as time tended to infinity for all provided that for some . Their proof depended on another technique, the so-called “Lyapunov functional”. In this present work, we follow up with the same steps of the previous result in [7,10] for a new class of Kirchhoff hyperbolic equations on bounded domain polynomial decay of the Kirchhoff type in viscoelasticity combined with the right-hand side defined as a logarithmic nonlinearity, and the kernel is not necessarily decreasing taking into account that the similar conditions in the last ones in ([7,10]) are considered. The logarithmic nonlinearity is of much use in physics, since it naturally appears in inflation cosmology and supersymmetric filed theories, quantum mechanics, and nuclear physics (see [5,14]). This kind of problem can be applied in many different areas of physics such as nuclear physics, optics, and geophysics (see [3,15]).
2. Preliminaries and Assumptions
We use the standard Lebesgue space and Sobolev space . For a Hilbert space X, we denote and , the inner product and norm of X, respectively. For simplicity, we denote and by and , respectively.
As in previous work in ([7,10]), we impose the following conditions on the relaxation function h. Namely, we suppose that the kernel is a function satisfying
for where
There exists a positive differentiable function such that:
and:
where and for and satisfies some positive constant
Furthermore, where for any there exists a positive constant depending only on such that:
Notation: We denote by and h the following expressions:
and we recall the binary notation:
Proof.
Multiplying (1) by and by integration over we have:
By using:
we get by direct calculation:
then:
By using integration by parts, we have:
Integrating by parts, we have:
Also integrating by parts, we get:
By using:
we get:
By replacing (12)–(16) in (11), we get:
then (17) is equivalent to:
and by using (9) in (18), we get (10).
The proof is complete. □
3. General Decay and Polynomial Decay
In the previous work, it was supposed that Therefore, from (20), we see that This implies that for all In our case, we are not assuming that In fact, we are allowing the function to oscillate.
To prove our result, we need to introduce the following auxiliary functional:
and:
where:
and:
is defined in (8). Further, we consider the functional:
where and for some positive constants , and to be determined later.
Proposition 1.
Let:
then there exist positive constants and such that:
Proof.
For the function definite in (27), by using Holder inequality , Young’s inequality embedding , and the Poincaré inequality, we get:
where comes from the embedding and the constant Poincaré inequality.
By multiplying (34) by and using we get:
By using Young’s inequality and using we get:
By using Young’s inequality and (28), we get:
Clearly, choosing:
Then, where:
The proof is complete. □
Lemma 3.
For and , we have:
for any
Proof.
It suffices to note that:
and applying Holder’s inequality for
The proof of the lemma is completed. □
Lemma 4.
Let be such that and h be a continuous function on and suppose that and Then, there exists a constant such that:
Proof.
By using Lemma 3 with we obtain:
It is easy to see that:
Lemma 5.
Let be such that and h be a continuous function on and suppose that . Then, there exists a constant such that:
Proof.
We use (45) for to arrive at:
It suffices to note that:
to obtain (47).
This completes the proof. □
Let:
and:
Now, we are in a position to state and prove our first result.
Theorem 1.
Assume that the hypotheses (A1)–(A3) hold, the initial data satisfy , and is as above.
Proof.
Now, a differentiation of definite in (31) with respect to time gives:
By a differentiation of (27), we have:
Integrating by parts, we get:
Also integrating by parts, we get:
By using integration by parts, we get:
By direct calculation, we get:
On the other hand, we have:
By using:
we get:
By direct calculation, we get:
By using direct calculation, we get:
By using direct calculation and , we get:
Next, we use the estimate (69).
By multiplying (34) by and we get:
By using Young’s inequality and , we get:
By using Young’s inequality and , we get:
Choosing hence and we get:
By using Young’s inequality and , we get:
Multiplying (73) by and using , we get:
Similarly, By using Young’s inequality we get:
Finally, we choose:
and:
Then, if we require from (76) that:
Case 1.
.
From (80), this is written in the form:
By virtue of Proposition 1 (the right-hand side inequality) in (81), we find for all :
By a simple integration in (82) over we find:
Notice that by our assumption in the theorem, we have . Again, by Proposition 1 (the left-hand side inequality), we conclude the assertion of our theorem:
Case 2.
Therefore, Lemma 4 and yield:
Similarly, using Lemma 4 and (30) yields:
for some and positive constants. Therefore, for any we arrive at:
By choosing and estimate (83) gives, for some
A simple integration of (85) over leads to:
Therefore,
Since and as , we get:
Therefore, we obtain:
Similarly, we get:
for some constant and
On the other hand, we can obtain:
for all and some constant Combining the last two inequalities and (33), we obtain:
for some constant A simple integration of (92) over gives:
Again by Proposition 1 (the left-hand side of the inequality), we conclude with the assertion of our theorem:
Therefore, (49) is obtained. This completes the proof. □
4. Conclusions
Our outcomes are natural extensions from the recent preceding ones in ( [7,8,24]), where the authors dealt with a viscoelastic equation and the system in more general decaying kernels and gave some common decay results, from which the usual exponential and polynomial rates are not only general cases. Our decay rate obtained in the third section is less general then that obtained in [7,8] with respect to the right-hand side defined as the logarithmic nonlinearity, which is familiar in physics, since it appears clearly natural in inflation cosmology and supersymmetric filed theories, quantum mechanics, and nuclear physics (see [5,14]). This sort of problem has many applications in several branches of physics such as nuclear physics, optics, and geophysics (see [3,15]). In future work, we will try to extend this study for the evolutionary case of the presented problem, but by using the semigroup theory.
Author Contributions
All authors contributed equally.
Acknowledgments
The first author gratefully acknowledges Qassim University, represented by the Deanship of Scientific Research, for the material support of this research under Number 3733-alrasscac-2018-1-14-S during the academic year 1439AH/2018.
Conflicts of Interest
The authors declare no conflict of interest.
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