Abstract
In this paper, we consider the initial-boundary value problem for the two-dimensional primitive equations of the large-scale oceanic dynamics. These models are often used to predict weather and climate change. Using the differential inequality technique, rigorous a priori bounds of solutions and the continuous dependence on the heat source are established. We show the application of symmetry in mathematical inequalities in practice.
1. Introduction
Primitive equations are very useful models which are often used to study the climate and weather prediction. It was Lions, Teman and Wang (see [1,2,3,4]) who first started the mathematical study of the primitive equations of the atmosphere, the ocean and the coupled atmosphere–ocean. Assuming that all unknown functions are independent of the latitude y, Petcu et al. [5] obtained the two-dimensional primitive equations of the ocean from the three-dimensional primitive equations. The existence and uniqueness of strong solutions of the primitive equations were derived. In a following paper, Huang and Guo [6] considered the two-dimensional primitive equations of large-scale oceanic motion. They obtained the the existence and uniqueness of global strong solutions. Huang et al. [7] studied the two-dimensional primitive equations of large-scale ocean in geophysics driven by degenerate noise. They proved the asymptotically strong Feller property of the probability transition semigroups. Due to the importance of primitive equations, there are many papers to study the problems (see, e.g., [8,9,10,11,12,13,14]).
Recently, many authors began to study the structural stability of large-scale primitive equations. Li [15] obtained the continuous dependence on the viscosity coefficient of primitive equations of the atmosphere with vapor saturation. By using the energy analysis methods, Li [16] proved that the primitive equations of the coupled atmosphere-ocean depended continuously on the boundary parameters. The inspiration of the study came from the fluid equations. There have been a lot of articles in the literature to study the stability of fluid equations (for interest, see [17,18,19,20,21,22,23,24,25,26,27,28,29]).
In this paper, we also assume that all the unknown functions are independent of the latitude y as in [5,6]. We consider the following two-dimensional large-scale primitive equations with heat source:
The domain is defined as
where h is the depth of the oceanic which is always assumed to be a positive constant in this paper. In (1) the unknown functions , w, are the horizontal velocity field, the vertical velocity, the density, the pressure, the temperature, respectively. Q is the heat source function which is given. f is a function of the Earth’s rotation which is taken to be constant here, and are the viscosity coefficients. are the reference values of the density and the temperature. is the expansion coefficient (constants), . We observe that, in the case of ocean dynamics, one has to add the diffusion-transport equation of the salinity to the system (1). The salinity equation is not present in (1), but this would raise little additional difficulty to take into account the salinity.
The boundary of is denoted by which can be partitioned into
The system (1) also has the following boundary conditions:
where is a positive constant. In addition, the initial conditions can be written as
The aim of this paper is to prove the continuous dependence on the heat source of problem (1)–(3) by using the energy methods. This type of study is devoted to know whether a small change in the equation can cause a large change in the solutions. While we take advantage of the mathematical analysis and the symmetry in mathematical inequalities to study these equations, it is helpful for us to know their applicability in physics. Since there will appear some inevitable errors in reality, the study of continuous dependence or convergence results becomes more and more significant. At present, most articles in the literature mainly focused on the existence and long-time behavior of the solutions of the primitive equations. Obviously, the structural stability of the primitive equations has not been paid enough attentions. The research of this paper will bring reference to the study of structural stability of other types of primitive equations.
The present paper is organized as follows. In next section we give some preliminaries of the problem and some well-known inequalities which will be used in the whole paper. We establish rigorous a priori bounds of the solutions in Section 2. In Section 3 we want to prove that the energy is exponential decay with time. Finally, we show how to derive a continuous dependence on the the heat source of our problem in Section 4.
2. Preliminaries of the Problem
In view of
This means that is a constant for arbitrary . Realizing the boundary conditions (2)3 we deduce that
By integrating (1)3 and using (1)6 we have
where is the pressure on the surface of the ocean which is unknown and a function of the horizontal variable only, and . Inserting (4)–(6) into (1)–(3), our problem can be rewritten as
with the following boundary conditions
and the initial conditions
In this paper, we also use some well-known inequalities. We list them here.
Lemma 1.
If and , then
For proof of Lemma 2.1 one can see Refs. [30,31].
Lemma 2.
Ifis a sufficiently smooth function inand, then
or
where, C is a positive computable constant and δ is a positive arbitrary constant.
Proof.
By the Hölder inequality, we then write
Since , we have
Therefore
Then we have
Obviously, we have
so,
To bound the last term of (18), we define a new known function, , satisfying
where are positive constants. For example, satisfies all the conditions in (19). Using the above estimates and employing the divergence theorem allow us to write
Therefore
We have after simplification
□
3. A priori Estimates
3.1. Estimates for and
Integrating by parts we have
By the Cauchy–Schwarz inequality and the Hölder inequality we deduce
By the Gronwall inequality, we have
An integration leads to
Integrating by parts and using (7)4 we get
By the Cauchy–Schwarz inequality we have
Similarly, we can have from (7)2
3.2. Estimate for
We multiply (7)3 by , and integrate by parts to find
After integrating by parts on the third term of (39) and realizing the boundary condition (8) we get
By the Hölder inequality and the Cauchy–Schwarz inequality we have
Therefore,
By the Gronwall inequality we have
Therefore
Letting now in (43) we can obtain
where
3.3. Estimate for
Using (7)1 we start with
Integrating by parts we have
Upon integrating by parts we get
Inserting the above bounds into (46) we write
We now carry out a similar procedure starting from (7)2 to obtain
Upon integrating by parts we get
Upon using the Cauchy–Schwarz inequality, (11), (38)
where are positive constants which will be given later.
Using (11) with then we have
4. Exponential Decay Estimates with Time When
In this section we want to prove the following theorem basis on Section 3.
Theorem 1.
5. Continuous Dependence on the Heat Source
Supposing also be the solutions of (7)–(9) with the same initial-boundary conditions as , but with different heat source . Let
then satisfies the following initial-boundary problem
We have the following theorem:
Theorem 2.
Proof.
Now taking the inner product of the first equation of (63) with , in , we have
An integration by parts leads to
By the Hölder inequality, Lemma 2.2, (38), Lemma 2.1, (56) and the AG mean inequality, we have
for computable and positive arbitrary constant .
Applying the Cauchy–Schwarz inequality again we have
Now, taking the inner product of Equation (63)3 with , we have
Computing as previous we arrive at
for computable positive function . A combination of (74) and (78) leads to
We take the inner product of Equation (63)3 with , we have
On integrating by parts we have
Integrating by parts and using the Hölder inequality, (44), Lemma 3.2, the AG mean inequality we get
where is a positive constant.
By the Hölder inequality and the AG mean inequality it follows that
Therefore
An integration of (83) yields that
Then returning to (81), we obtain
6. Conclusions
In this paper, we obtain the continuous dependence of the two-dimensional large-scale primitive equations in oceanic dynamics, where the depth of the ocean is assumed to be a positive constant. When the depth of the ocean is positive but not always a constant, Huang and Guo [32] have obtained the existence and uniqueness of a global strong solution for the problem. The study of the continuous dependence of the primitive equations in this case may be more interesting.
Author Contributions
Conceptualization, and validation, Y.L.; formal analysis and investigation, P.Z. All authors have read and agreed to the published version of the manuscript.
Funding
This research was funded by Key projects of universities in Guangdong Province (NATURAL SCIENCE) (2019KZDXM042) and the Research team project of Guangzhou Huashang College(2021HSKT01).
Institutional Review Board Statement
Not applicable.
Informed Consent Statement
Not applicable.
Data Availability Statement
Not applicable.
Acknowledgments
The authors would like to deeply thank all the reviewers for their insightful and constructive comments.
Conflicts of Interest
The authors declare no conflict of interest.
Sample Availability
Sharing is not applicable to this article, as no new data were created or analyzed in this study.
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