Abstract and Applied Analysis

Volume 2011 (2011), Article ID 647368, 15 pages

http://dx.doi.org/10.1155/2011/647368

## Wave Breaking and Propagation Speed for a Class of One-Dimensional Shallow Water Equations

^{1}Department of Mathematics, Zhejiang Normal University, Jinhua 321004, China^{2}Faculty of Mathematics and Informatics, Shumen University, 9712 Shumen, Bulgaria

Received 24 June 2011; Revised 1 September 2011; Accepted 13 September 2011

Academic Editor: P. J. Y. Wong

Copyright © 2011 Zaihong Jiang and Sevdzhan Hakkaev. This is an open access article distributed under the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.

#### Abstract

We investigate a more general family of one-dimensional shallow water equations. Analogous to the Camassa-Holm equation, these new equations admit blow-up phenomenon and infinite propagation speed. First, we establish blow-up results for this family of equations under various classes of initial data. It turns out that it is the shape instead of the size and smoothness of the initial data which influences breakdown in finite time. Then, infinite propagation speed for the shallow water equations is proved in the following sense: the corresponding solution with compactly supported initial datum does not have compact -support any longer in its lifespan.

#### 1. Introduction

In this paper we consider the equation where and are real constants.

Set , then we can rewrite (1.1) as Let , then (1.1) can be reformulated in terms of :

By comparison with the Camassa-Holm equation [1], the Degasperis-Procesi equation, [2] and the Holm-Staley -family of equations [3], it is easy to find that (1.1) is more general. The Camassa-Holm equation, the Degasperis-Procesi equation, and the Holm-Staley b-family of equations are the special cases with ; , and , respectively. The equation of type (1.1) arises in the modeling of shallow water waves; compare with the discussion in the papers [4, 5].

When , use the scaling , then (1.1) can be reformulated into which is the well-known Camassa-Holm equation. The Camassa-Holm equation was first written explicitly and derived physically as a water wave equation by Camassa and Holm [1], who also studied its solutions. It has infinitely many conserved integrals including the -norm, but wave breaking also happens in finite time, which coincides with physical phenomenon. Some satisfactory results have been obtained recently [6–8] for strong solutions. Moreover, wave breaking for a large class of initial data has been established in [9–11], and recently, a new and direct proof for McKean's theorem is given in [12]. In [13] some new criterion on blowup is established for the Camassa-Holm equation with weakly dissipative term. In [14] (see also [15]), Xin and Zhang showed global existence and uniqueness for weak solutions with . The solitary waves of the Camassa-Holm equation are peaked solitons and are orbitally stable [16] (see also [17, 18]). It is worthwhile to point out that the peakons replicate a feature that is characteristic for the waves of great height waves of largest amplitude that are exact solutions of the governing equations for water waves; compare with the papers [19–21]. Similarly, if , use the some scaling, then (1.1) can be reformulated into the Degasperis-Procesi equation, the existence of global solutions, persistence properties and propagation speed of Degasperis-Procesi equation is given in [22] and the references therein. For the the weakly dissipative Degasperis-Procesi equation, [23] is concerned with some aspects of existence of global solutions, persistence properties, and propagation speed. So, in our following discussion, we will always exclude these two cases.

In general, the family of equations are not always completely integrable systems. However, one can find the following conservation laws:

which are quite different from the invariants of the Camassa-Holm equation

Due to the similarity of (1.2) and the Camassa-Holm equation, just by following the argument for the Camassa-Holm equation, it is easy to establish the following well-posedness theorem for (1.2).

Theorem 1.1. *Given , , then there exist a and a unique solution to (1.1) such that
*

To make the paper concise we would like to omit the detailed proof, since one can find similar ones for these types of equations in [7, 24].

When we study the Camassa-Holm equation, the most frequently (crucially) used conservation law is that of the -norm of the solution. However, if is a strong solution (decays rapidly at infinity) to (1.1), direct computation yields Hence, the -norm of the solution is not conserved at all except for . However, we also have a clear blow-up scenario as follows: the solution blows up if and only if the first-order derivative blows up that is, wave breaking occurs. More precisely, assume that is the lifespan of the corresponding solution, then

Before giving our main results, we list some notations that will be used in our paper. denotes the inner product in the Hilbert space , ; use for the corresponding norm and to denote the corresponding norm.

The remainder of the paper will be organized as follows. In the next section, we establish blow-up results for this family of equations under various classes of initial data. In the last section, infinite propagation speed for the shallow water equations is proved.

#### 2. Blow-Up Phenomenon

After local well posedness of strong solutions is established, the next question is whether this local solution can exist globally. If the solution exists only for a finite time, how about the behavior of the solution when it blows up? What induces the blowup? On the other hand, to find sufficient conditions to guarantee the finite time blowup or global existence is of great interest, particularly for sufficient conditions added on the initial data.

Set as the characteristic evolved by the solution; that is, it satisfies Taking derivative with respect to in (2.1), we obtain

Hence

which is always positive before the blow-up time. Therefore, the function is an increasing diffeomorphism of the line before blowup. In addition, from (1.1), the following identity is proved:

The following theorem is proved in [25] it is one of sufficient conditions to guarantee the finite time blowup added on the initial data.

Theorem 2.1. *Let , with being odd and . Then the corresponding solution of (1.1) blows up in finite time.*

From the above blow-up result we can obtain the following.

Theorem 2.2. *Let , . Suppose that is odd and . Then the corresponding solution of (1.1) blows up in finite time.*

*Proof. *If is odd, then is also odd. In fact
On the other hand
So Theorem 2.2, follows from Theorem 2.1.

Before giving our main result, we first recall the following three lemmas that will be used in our proof.

Lemma 2.3. *If , then is algebra. Moreover
*

Lemma 2.4. *If , then
**
Here denotes the commutator of the linear operators and .*

Lemma 2.5 (see [26]). *Suppose that is twice continuously differentiable satisfying
**
Then blows up in finite time. Moreover the blow-up time can be estimated in terms of the initial datum as
*

Now, we are ready to give our main results. Firstly, we present the result which improves Theorem 2.1.

Theorem 2.6. *Let with , and assume that is the existence time of the corresponding solution with the initial data . If there exists such that
**
then the norm of does not blow up on .*

*Proof. *Let be the solution to (1.1) with initial data and let be the maximal existence time of the solution . Applying the operator to (1.2), multiplying by , and integrating, we obtain
where and . We have
where we applied Lemma 2.4 with . Again applying Lemma 2.4 with , we obtain
and, from Lemma 2.3, we have
Combining the above estimates, we obtain
From Gronwall inequality, we obtain
This completes the proof of the theorem.

In order to help the readers to understand the following theorem, we would like to give an intuitive explanation for this result. Neglecting lower-order source terms, (1.2) reduces to the generalized Hunter-Saxton equation: Differentiating with respect to , one obtains By looking at the evolution of along characteristics, it is clear that one can have or depending on the sign of .

Theorem 2.7. *Let with . If , then every solution will exist globally in time. If , then the solution blows up in finite time if and only if the slope of the solution becomes unbounded from below in finite time. If , then the solution blows up in finite time if and only if the slope of the solution becomes unbounded from above in finite time.*

*Proof. *It suffices to consider the case . Let be the maximal time of existence of the solution of (1.1). From [25] we know that . Multiplying (1.2) by and integrating by parts, we get
Note that
From (2.20), for , we have
From Theorem 2.6, for the solution exists globally in time. If and the slope of the solution is bounded from below or if and the slope of the solution is bounded from above on , then there exists such that
By Gronwall inequality, we have

There is no doubt that it is the shape of the initial data but not their smoothness or size that influences the lifespan. However, we try to understand what induces wave breaking. Another sufficient condition is given in the following theorem. The approach used to prove the following theorem is rooted in the considerations made in the paper [27].

Theorem 2.8. *Let , . Suppose that and there exists such that , and
**
Then the corresponding solution of (1.1) blows up in finite time with the lifespan
*

*Proof. *Suppose that the solution exists globally. Due to (2.4) and the initial condition, we have , and
for all .

Since , one can write and as

Consequently,

From the expression of in terms of ,

Rewrite (1.1) as
Using this identity, we can obtain

By direct calculation, we have
Using the inequality (see [26]), we obtain
Similarly, we have
Now using the inequality (see [26])
we obtain
Similarly, we have
Combining all the above terms together, we have
*Claim. * is decreasing and for all .

Suppose not that there exists a such that on and . Now, let
Firstly, by the same trick as above, we obtain
This implies that can be extended to infinity.

Moreover, due to the above inequality, we have
Now substituting (2.39) in (2.42), we get
Now the theorem follows from Lemma 2.5 with and . Then, we complete our proof.

The final goal for us is to establish a necessary and sufficient condition for guaranteeing singularity formation in finite time, which is in the opposite direction to global existence. So if the necessary and sufficient condition can be found, then the problem can be solved completely.

Now, let us try to find a condition for global existence. Unfortunately, when like the Degasperis-Procesi equation [22] and the Holm-Staley -family of equations [26], only the following easy form can be proved at present.

Theorem 2.9. *Suppose that , does not change sign. Then the corresponding solution to (1.1) exists globally.*

*Proof. *Without loss of generality we assume . It is sufficient to prove that is bounded for all .

In fact,
while we can also obtain
Combining the above terms together, we have
Then, we complete our proof.

#### 3. Propagation Speed

The purpose of this section is to give a detailed description of the corresponding strong solution in its lifespan with being compactly supported. The analogous results were obtained in [6] for the Camassa-Holm equation and in the papers [28, 29] for the Degasperis-Procesi equation. The main theorem reads as follows.

Theorem 3.1. *Let and . Assume that the initial datum is compactly supported in . Then, the corresponding solution of (1.1) has the following property: for **
with and , respectively, where is defined by (2.1) and is its lifespan. Furthermore, and denote continuous nonvanishing functions, with and for . And is a strictly increasing function, while is a strictly decreasing function.*

*Proof. *Since has a compact support, also does. From (2.4), it follows that is compactly supported in in its lifespan. Hence the following functions are well defined:
with . For , we have
and, for , we have
Hence, as consequence of (3.3) and (3.4), we have
On the other hand,
Differentiating (1.1) twice, we get
Combining (1.1) and (3.7), we obtain

Substituting the identity (3.8) into and using (3.5), we obtain
Therefore, in the lifespan of the solution, we have
By the same argument, one can check that the following identity for is true:
In order to complete the proof, it is sufficient to let and , respectively.

#### Acknowledgments

This work is partially supported by Zhejiang Innovation Project (Grant no. T200905) and NSFC (Grant no. 11101376). S. Hakkaev is also partially supported by Research Grant DVU_10_0338.

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