The modified Camassa-Holm equation in Lagrangian coordinates
Yu Gao, Jian-Guo Liu

TL;DR
This paper investigates the finite-time blow-up and solution behavior of the modified Camassa-Holm equation in Lagrangian coordinates, establishing lifespan, collision phenomena, and the formation of peakons.
Contribution
It provides a detailed analysis of solution lifespan, blow-up, and peakon formation for the modified Camassa-Holm equation in Lagrangian form, including regularization for global weak solutions.
Findings
Classical solutions blow up in finite time for certain initial data.
Lifespan of solutions is bounded below by inverse of initial data norms.
Peakons can form at the blow-up time.
Abstract
In this paper, we study the modified Camassa-Holm (mCH) equation in Lagrangian coordinates. For some initial data , we show that classical solutions to this equation blow up in finite time . Before , existence and uniqueness of classical solutions are established. Lifespan for classical solutions is obtained: And there is a unique solution to the Lagrange dynamics which is a strictly monotonic function of for any : . As approaching , we prove that classical solution in Eulerian coordinate has a unique limit in Radon measure space and there is a point such that which means is an onset time of collision of characteristics. We also show that in some cases peakons areβ¦
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Taxonomy
TopicsNonlinear Waves and Solitons Β· Algebraic structures and combinatorial models Β· Advanced Differential Equations and Dynamical Systems
The modified Camassa-Holm equation in Lagrangian coordinates
Yu Gao [email protected] Department of Mathematics, Harbin Institute of Technology, Harbin, 150001, P.R. China.
Department of Mathematics and Department of Physics, Duke University, Durham, NC 27708, USA.
Jian-Guo Liu [email protected] Department of Mathematics and Department of Physics, Duke University, Durham, NC 27708, USA.
Abstract
In this paper, we study the modified Camassa-Holm (mCH) equation in Lagrangian coordinates. For some initial data , we show that classical solutions to this equation blow up in finite time . Before , existence and uniqueness of classical solutions are established. Lifespan for classical solutions is obtained: And there is a unique solution to the Lagrange dynamics which is a strictly monotonic function of for any : . As approaching , we prove that classical solution in Eulerian coordinate has a unique limit in Radon measure space and there is a point such that which means is an onset time of collision of characteristics. We also show that in some cases peakons are formed at . After , we regularize the Lagrange dynamics to prove global existence of weak solutions in Radon measure space.
1 Introduction
In this work, we consider the following nonlinear partial differential equation in :
[TABLE]
subject to an initial condition
[TABLE]
This equation is referred to as the modified Camassa-Holm(mCH) eqaution with cubic nonlinearity, which was introduced as a new integrable system by several different researchers [14, 16, 24, 25]. It has a bi-Hamiltonian structure [18, 24] and a Lax-pair [25]. Equation (1.1) also has solitary wave solutions of the form [18]:
[TABLE]
where is a constant representing the amplitude of the soliton and is the fundamental solution for the Helmholtz operator . With this fundamental solution , we have the following relation between functions and :
[TABLE]
Moreover, global existence of -peakon weak solutions of the following form was obtained in [17]:
[TABLE]
In the present paper, we study local well-posedness for classical solutions and global weak solutions to (1.1) in Lagrangian coordinates. Below we introduce the Lagrange dynamics for the mCH equation. To this end, we first review the Lagrange dynamics for incompressible Euler equation:
[TABLE]
where the velocity is determined from the vorticity by the Biot-Savart law
[TABLE]
involving the kernel Assume is the flow map generated by the velocity field :
[TABLE]
By the incompressible property , we know
[TABLE]
The Euler equation can be rewritten in the Lagrange dynamics
[TABLE]
Comparing with the incompressible Euler equation, assume is the flow map for the mCH equation generated by the velocity field :
[TABLE]
In contrast with (1.3), we have the following property for the mCH equation:
[TABLE]
Combining the above two equalities, the mCH equation (1.1) can be rewritten in the Lagrange dynamics:
[TABLE]
Changing of variable gives
[TABLE]
Set
[TABLE]
Then, Equation (1.4) can be rewritten as
[TABLE]
When , the following useful properties can be easily obtained:
[TABLE]
In the rest of this paper, we assume the initial satisfying for some constant . Next, we summarize our main results in four theorems.
Theorem 1.1**.**
Suppose . Then, there exists a unique maximum existence time such that Lagrange dynamics (1.8) has a unique solution
[TABLE]
which satisfies
[TABLE]
(The solution space is defined by (2.1).) The mCH equation (1.1)-(1.2) has a unique classical solution
[TABLE]
which can be represented by as
[TABLE]
Moreover, satisfies:
[TABLE]
*If , then the following holds:
We have*
[TABLE]
* The following equivalent statements hold:*
(a)**
[TABLE]
(b)**
[TABLE]
(c)**
[TABLE]
(d)**
[TABLE]
(e)**
[TABLE]
(f)**
[TABLE]
* There exists a unique function such that*
[TABLE]
Moreover, for any we have
[TABLE]
and
[TABLE]
*Here, is the space of functions with bounded variation (see definition 5.1).
There exists a unique (Radon measure space on ) such that*
[TABLE]
(a) and (b) tells us that is an onset time of collisions of characteristics. (1.11) implies that the supports for classical solutions will not change.
Our another main theorem is about finite time blow-up behaviors and the lifespan of classical solutions. Let be the maximum existence time of the classical solution to the mCH equation subject to an initial condition . Then we have the following theorem about lifespan for classical solutions.
Theorem 1.2**.**
*Assume .
We have*
[TABLE]
* If there exists such that*
[TABLE]
then the classical solution to the mCH equation will blow up in finite time. Moreover, for any we have
[TABLE]
This theorem implies that there are smooth initial data with arbitrary small support and arbitrary small -norm, , for which the classical solution does not exist globally.
Next, we give a theorem to show the formation of peakons at finite blow-up time . From Theorem 1.1, we know there is a point such that . Set
[TABLE]
For any , because , we know that is either a single point or a closed interval. Denote
[TABLE]
The figure below describe these singular points.
For and , we show that will not change sign in (see Proposition 5.1). Hence, . We have the following theorem.
Theorem 1.3**.**
Assume and (). Let and for . Then
[TABLE]
where is given by (5.20).
At last, we give a theorem to show global existence of weak solutions (see Definition 6.2). Theorem 1.1 (iv) tells that classical solutions become Radon measures when blow-up happens. After the blow-up time , we can extend our solution globally in the Radon measure space. We have:
Theorem 1.4**.**
Let with compact support. Then there exists a global weak solution to the mCH equation satisfying:
[TABLE]
and
[TABLE]
Now, we compare the mCH equation with the Camassa-Holm (CH) equation:
[TABLE]
The CH equation was established by Camassa and Holm [6] to model the unidirectional propagation of waves at free surface of a shallow layer of water ( representing the height of waterβs free surface above a flat bottom). It is also a complete integrable system which has a bi-Hamiltonian structure and a Lax pair [6].
There are some different properties between the CH equation and the mCH equation.
Classical solutions and blow-up criteria. For a large class of initial data, classical solutions to the CH equation blow up in finite time (see [2] and references in it). Moreover, the only way that a classical solution of the CH equation fails to exist globally is that the wave breaks [10] in the sense that the solution remains bounded while the spatial derivative becomes unbounded. For the mCH equation, blow-up behaviors also happen for a large class of initial data (see [8, 18, 22]). However, (hence ) becomes unbounded when blow-up happens, while and remain bounded.
Lifespan for classical solutions. Comparing with (1.14), the lower bound for lifespan of strong solutions to the CH equation with initial data is given by [13, 23]:
[TABLE]
-peakon weak solutions. Trajectories for -peakon weak solutions to the CH equation never collide [7, 9] provided that the initial datum satisfies and for . However, the trajectories for -peakon solutions of the mCH equation may collide in finite time even if [17]. Moreover, for the CH equation, when blow-up happens at finite time , we have (see [10, 23]). Peakon solutions and its derivative are in BV space, which are bounded functions. Hence, peakon solutions can not be formed when blow-up happens (comparing with Theorem 1.3) for the CH equation.
General weak solutions. In [17], the authors proved nonuniqueness of weak solutions obtained by Theorem 1.4. Comparing with Theorem 1.4, there is a unique global weak solution and (see [9, 12]) to the CH equation when and . For general initial data , global existence of weak solutions to the CH equation was obtained by several different methods (see [4, 5, 19, 20, 27, 28]).
For more results about local well-posedness and blow up behavior of strong solutions to the Cauchy problem (1.1)-(1.2), one can refer to [8, 15, 18, 22]. For weak solutions, one can refer to [17, 29].
The rest of this article is organized as follows. In Section 2, we use contraction mapping theorem to prove local existence and uniqueness of solutions to the Lagrange dynamics (1.8). Then, we use to give and prove that it is a unique classical solution to the mCH equation (1.1)-(1.2). Besides, when is finite, we can extend this classical solution in time. In Section 3, we show some blow-up criteria for classical solutions. In Section 4, we prove that for some initial data classical solutions blow up in a finite time and the estimates for blow-up rates are given. For small initial data, almost global existence of classical solutions is obtained. In Section 5, we study classical solutions at blow-up time . and are BV functions while has a unique limit in Radon measure space as . Moreover, we prove that in some cases peakons are formed at . In the last section, we use regularized Lagrange dynamics to prove global existence of weak solutions in Radon measure space.
2 Lagrange dynamics and short time classical solutions
In this section, we study the existence and uniqueness of solutions to Lagrange dynamics (1.8). Then, we prove defined by (1.10) is a unique classical solution to (1.1)-(1.2).
First, letβs introduce the spaces for solutions. For nonnegative integers and real number , we denote
[TABLE]
and the function space
[TABLE]
Similarly, we can define .
We will present the results of this section in three subsections as follows.
In Subsection 2.1, when , we prove local existence and uniqueness of a solution to (1.8) such that
[TABLE] 2. 2.
In Subsection 2.2, we prove defined by (1.10) belongs to and () is a unique classical solution to the mCH equation. 3. 3.
In Subsection 2.3, we prove that whenever the classical solution satisfies
[TABLE]
we can extend the classical solution in time.
2.1 Local existence and uniqueness of solutions to Lagrange dynamics
In this subsection, we use the contraction mapping theorem to prove short time existence and uniqueness of solutions to the Lagrange dynamics (1.8), which is equivalent to the following integral equation:
[TABLE]
where is defined by (1). Set
[TABLE]
For constants and , we define
[TABLE]
Obviously, is a closed subset of . We will look for suitable constants and then use the contraction mapping theorem in the set .
Before presenting the existence and uniqueness theorem, we give two useful lemmas.
Lemma 2.1**.**
Assume and for some constants and . Let
[TABLE]
Then, we have
Proof.
According to (2.1), is monotonic about . For given , we separate the proof into three parts.
Step 1. Continuity at when .
For closed to and because is monotonic, we can assume for . A direct estimate gives
[TABLE]
Therefore, according to the uniform continuity of , is continuous at . The proof of the case is similar.
Step 2. Continuity at when for some .
Due to the continuity of , for closed to , there exists such that . Without lose of generality, we assume
[TABLE]
Then, the monotonicity of implies that
[TABLE]
From the definition of , we have
[TABLE]
Therefore, . Hence, is continuous at .
Step 3. Continuity at when . The case is similar.
For closed to , we have two cases. When , we can use Step 1. When there exists such that , we can use Step 2.
This is the end of the proof. β
Lemma 2.2**.**
Assume and for some constants and . Then, for , we have
[TABLE]
where and .
Proof.
Assume for some constants and . For , we have
[TABLE]
By (1.9), we obtain
[TABLE]
Because , we have
[TABLE]
Thus,
[TABLE]
Next, we estimate .
When , we have for . On the other hand, we know when . Therefore,
[TABLE]
Thus
[TABLE]
Combining and gives
[TABLE]
Together with (2.7), we obtain (2.2). β
We have the following existence and uniqueness theorem.
Theorem 2.1**.**
Assume . Let and . Then, for any with
[TABLE]
there exist constants satisfying
[TABLE]
and
[TABLE]
such that (2.2) has a unique solution satisfying
[TABLE]
for .
Moreover, for any , , there exists a constant (depending on , and ) such that
[TABLE]
Proof.
We separate this proof into two parts.
Part I.(Existence and Uniqueness) We use the contraction mapping theorem to prove the existence of a unique solution to (2.2).
Step 1. When , we prove there are constants such that when , we have , where is defined by (2.3).
When satisfies (2.8), we have
[TABLE]
A simple computation shows that
[TABLE]
Hence, there is a constant satisfying (2.9). Moreover, inequality (2.9) implies
[TABLE]
and
[TABLE]
Therefore, we can choose satisfying (2.10).
When , combining (2.2), (2.10) and (2.14) gives
[TABLE]
and Step 1 is completed.
Step 2. We prove is a contraction map on .
For , combining (1.9) we have
[TABLE]
For the first term , we estimate
[TABLE]
For the second term, due to , we obtain
[TABLE]
Combining (2.1), (2.1), and (2.1), we have
[TABLE]
which implies
[TABLE]
Inequality (2.13) shows that is a contraction map.
At last, by the contraction mapping theorem, the system (2.2) (or (1.8)) has a unique solution in .
On the other hand, using Lemma 2.1 we can see , which means
[TABLE]
Hence, and Part I is finished.
Part II. (Regularity) We show obtained in the first part belongs to
From the first part, we can see solution belongs to For this solution we have the following properties
[TABLE]
On the other hand, satisfies:
[TABLE]
We obtain
[TABLE]
Hence,
[TABLE]
We obtain
[TABLE]
Thus
[TABLE]
Because is monotonic about , its derivative exists for a.e. . Differentiating with respect to shows that for a.e. ,
[TABLE]
Due to (2.18) and (2.19), the sum of the last two terms in (2.22) is zero, which leads to
[TABLE]
Because , we have which means .
From (2.1), we have
[TABLE]
Differentiating (2.1) with respect to shows that
[TABLE]
Hence, we obtain and
[TABLE]
We have .
Similarly, taking derivative about for times on both sides of (2.1) gives that
[TABLE]
and (2.12) holds.
β
Remark 2.1*.*
Monotonicity of plays an important role in our proof. Without monotonicity, the vector field for the Lagrange dynamics may be not Lipschitz. From (2.1), we know . Hence, we can continuously extend globally as
[TABLE]
2.2 Classical solutions to the mCH equation
Next, we prove the short time existence and uniqueness of the classical solutions to (1.1)-(1.2).
The following lemma shows that we can construct classical solutions to the mCH equation (1.1)-(1.2) from the solutions to the Lagrange dynamics (1.8). Moreover, we show that the support of will not change.
Lemma 2.3**.**
Let for some interger . Assume that (for some ) is the solution of (1.8) and strictly monotonic about for any fixed time . , are defined by (1.10). And assume . Then, is a classical solution of (1.1)-(1.2).
Moreover, we have
[TABLE]
Proof.
We denote For any test function , we have
[TABLE]
[TABLE]
Since that is arbitrary, we have
[TABLE]
Next, we prove (2.26). Because is monotonic and for , we obtain
[TABLE]
Hence, we have
[TABLE]
which implies
[TABLE]
Similarly, we have
For any , gives
[TABLE]
Hence, (2.26) holds. β
Remark 2.2*.*
Consider the following general equation with ,
[TABLE]
When , the support of the classical solution to (2.27) is also contained in . Indeed, by scaling and , and satisfy
[TABLE]
Due to , by (2.26) we know . Hence, we have .
Next, we present a useful lemma which is similar to Lemma 2.1.
Lemma 2.4**.**
Assume and for any fixed time . Let satisfy (2.11) for some constants . Set
[TABLE]
Then, we have and
[TABLE]
Proof.
From the proof of Lemma 2.3, we know . However, in order to make no confusion, we still use in this proof.
By using the inverse function theorem, for any , there is a continuously differentiable function such that
[TABLE]
and
[TABLE]
Moreover, we have
[TABLE]
Changing variable and using the property of Dirac measure, we have
[TABLE]
Next, we separate the proof into three parts, which is similar to the proof of Lemma 2.1.
Step 1. Continuity at when . Then case for is similar.
In this case, we have . For any closed to and because , we can assume . Because , we have . Hence, is continuous at .
Step 2. Continuity at when for some . This means .
Due to the continuity of , for closed enough to , we can assume . In other words, there exists such that . Because
[TABLE]
we only have to prove and are continuous at . (2.1) shows that
[TABLE]
which means is continuous at .
Because and , we have
[TABLE]
From (2.31) we can see as . Together with implies the continuity of at .
Hence, is continuous at .
Step 3. . The case is similar.
For closed to , we have two cases. When , we can use Step 1. When there exists such that , we can use Step 2.
Put Step 1,2,3 together and we can see .
At last, because is fundamental solution for Helmholtz operator , we have
[TABLE]
Hence,
β
Now we prove that defined by (1.10) is a unique classical solution of (1.1)-(1.2).
Theorem 2.2**.**
Assuming . Then, for
[TABLE]
* given by (1.10) belongs to and belongs to . is a unique classical solution to (1.1)-(1.2).*
Proof.
Let and . For , by Theorem 2.1, we know there exist a solution to (1.8) satisfying (2.11) for given by (2.9) and (2.10).
Part I. Regularity.
Step 1. When , we have and we prove .
Taking derivative about for in (1.10) gives that
[TABLE]
Because and for any fix time , Lemma 2.4 shows that .
For the spatial variable , integration by parts leads to
[TABLE]
[TABLE]
and
[TABLE]
Set g(\theta,t):=\partial_{\theta}\bigg{(}\frac{m_{0}(\theta)}{X_{\theta}(\theta,t)}\bigg{)}. Then, satisfies the assumption of Lemma 2.4. Hence
[TABLE]
Step 2. When , we have . Integration by parts changes (2.32) into
[TABLE]
Hence
[TABLE]
And Lemma 2.4 shows that .
Step 3. If , we can keep using integration by parts and Lemma 2.4 and obtain
[TABLE]
Step 4. Because , from the above steps, we already know . In this step, we show Due to (2.26), we only have to show . From (2.2), for and , we have
[TABLE]
Taking derivative of both sides of (2.33), we have
[TABLE]
and
[TABLE]
Combining (2.33), (2.2) and (2.35), we obtain
[TABLE]
From the above proof (or Lemma 2.3), we can see that is a classical solution to (1.1)-(1.2).
Part II. Uniqueness of the classical solution to (1.1)-(1.2).
Assume there is another classical solution to (1.1)-(1.2). We prove that can also be defined by the solution to (1.8), which means
[TABLE]
To this end, define another characteristics by
[TABLE]
subject to
[TABLE]
By standard ODE theory, we can obtain a solution .
Step 1. We prove
[TABLE]
Taking derivative with respect to shows that
[TABLE]
Taking time derivative of gives that
[TABLE]
This implies
[TABLE]
Hence, we can see
[TABLE]
Step 2. We prove .
From (2.2), we obtain
[TABLE]
which means that is also a solution to (1.8).
From Theorem 2.1 we know that the strictly monotonic solution to (1.8) is unique. Therefore, to prove , we only have to prove is strictly monotonic for .
Combining (2.37) and (2.38) gives that
[TABLE]
Because , and , the minimum and maximum of can be obtained on . Hence
[TABLE]
where
[TABLE]
and
[TABLE]
Hence, is strictly monotonic for .
Combining Step 1 and Step 2, we obtain (2.36). β
Remark 2.3*.*
(2.38) also can be easily obtained by [26, Theorem 5.34]
The strictly monotonic property of plays an crucial role in the proof of the above Theorem. Whenever is strictly monotonic, we can use integration by parts to obtain the regularity of . Conversely, if is a classical solution, then the characteristics for the mCH equation is strictly monotonic.
For the convenience of the rest proof, we summarize the results in the proof of Part II of Theorem 2.2 and give a corollary.
Corollary 2.1**.**
Let and be the solution to (1.8). , is a classical solution to (1.1)-(1.2). Then, we have
[TABLE]
and
[TABLE]
where
[TABLE]
and
[TABLE]
Moreover, we have
[TABLE]
Proof.
The proof for (2.41) and (2.42) is the same as the proof for uniqueness in Theorem 2.2. β
Remark 2.4*.*
From (2.42), we know that does not change sign for any . We present a precise argument here.
Set
[TABLE]
and
[TABLE]
Hence,
[TABLE]
For , denote
[TABLE]
and
[TABLE]
Then, we have , and . Due to the monotonicity of , one can easily show that and are open sets while is a closed set for . Also we have
[TABLE]
and (by (2.42))
[TABLE]
Due to
[TABLE]
we obtain
[TABLE]
This can also be obtained by (2.1).
2.3 Solution extension
In this subsection, we will show that as long as classical solutions to (1.1)-(1.2) satisfying we can extend the solutions and in time.
Proposition 2.1**.**
Assume and is the solution to (1.8). Let be the corresponding solution to (1.1)-(1.2). If
[TABLE]
then there exists such that
[TABLE]
is a solution to (1.8), and
[TABLE]
Proof.
There exists a constant satisfies
[TABLE]
From Lemma 2.3, we know has a uniform (in ) support. Hence, there exists a constant such that
[TABLE]
Consider time . Our target is to prove that the classical solution can be extend to . We will show this in two steps.
Step 1. In this step we consider a dynamic system from time
From (2.26) we know . Set
[TABLE]
Consider dynamics for :
[TABLE]
Because , by Theorem 2.2, we know that for any
[TABLE]
there exists a solution to (2.46) and a classical solution () to (1.1) subject to initial condition
[TABLE]
Moreover,
[TABLE]
[TABLE]
Choose and set Thus .
Step 2. In this step we extend the solutions to .
Changing variable by , initial value \widetilde{X}\big{(}X(\xi,T_{1}),0\big{)}=X(\xi,T_{1}) allows us to define
[TABLE]
and we have
[TABLE]
Similarly, because , we can use to define
[TABLE]
and we have
[TABLE]
Moreover, we can see we defined is a classical solution to (1.1)-(1.2) in .
Next, we show satisfies (1.8) in .
Actually, changing variable by and combining (2.47) and (2.42) lead to
[TABLE]
Similarly,
[TABLE]
Therefore, (2.46) turns into
[TABLE]
for and .
Hence, is a solution to (1.8). Corollary 2.1 ensures the strictly monotonicity of for . Therefore, is the unique solution which extends the solution to
β
3 Blow-up criteria
In this section, we give some criteria on finite time blow-up of classical solutions to the mCH equation.
Let be the maximal existence time of classical solution to the mCH equation. In other words, satisfies
[TABLE]
Next lemma shows that the solution to Lagrange dynamics (1.8) can be extended to the blow-up time .
Lemma 3.1**.**
Let . Let be the maximal existence time for the classical solution to (1.1)-(1.2) and be the solution to (1.8). Then we have
[TABLE]
Proof.
Let go to in (2.21) and we obtain . Using (2.24) and Lipschitz property of , we can obtain that
[TABLE]
Let go to in (2.1) and (2.1). Similarly, combining (2.12) gives
[TABLE]
Keep doing like this and we can see
[TABLE]
At last, let go to in (2.1) and combining (1.8), we have .
β
We have the following blow up criteria.
Theorem 3.1**.**
*Let . is the solution to Lagrange dynamics (1.8). Assume is the maximum existence time for the classical solution to (1.1)-(1.2). Then, the following equivalent statements hold.
*
[TABLE]
**
[TABLE]
**
[TABLE]
**
[TABLE]
**
[TABLE]
**
[TABLE]
Proof.
We follow the following lines to prove this theorem,
[TABLE]
and
[TABLE]
Step 1. We prove .
Assume blows up in finite time . We prove (3.3) by contradiction. From Lemma 3.1, we know . If does not hold, then we have
[TABLE]
Combining (2.42) and (2.26), we have
[TABLE]
This is a contradiction to (3.2).
Step 2. We prove
From (3.3), we have
[TABLE]
Together with (2.40), we can see .
Step 3. We prove .
(3.4) implies that
[TABLE]
Because of (2.26), for any we have
[TABLE]
Hence, we can see that (3.8) and (3.5) are equivalent.
Step 4. We prove .
Assume (3.5) holds. We prove (3.6) by contradiction. For any , if
[TABLE]
then
[TABLE]
with continuous injection for all implies that
[TABLE]
On the other hand, we have
[TABLE]
Hence we obtain , which is a contradiction with (3.5). Therefore, (3.6) holds.
Step 5. We prove .
Assume (3.6) holds. If , by Proposition 2.1, there exists such that Because has uniform compact support for , we have
[TABLE]
which is a contradiction.
Step 6. At last, we prove
[TABLE]
When (3.7) holds, one can easily obtain (3.2). So, we only have to prove . (3.4) implies
[TABLE]
Due to (3.9), we obtain
[TABLE]
and this gives (3.7).
β
Remark 3.1*.*
(3.3) shows that there is a such that . This means is an onset time of collision of characteristics. Now, we can conclude that if blows up in finite time , then we have
[TABLE]
The blow-up criterion (3.5) can also be found in [18]. Besides, (3.7) is similar to the well known blow-up criterion for smooth solutions to Euler equation [1].
Remark 3.2* (Other equivalent criteria).*
Because has compact support for , by PoincarΓ© inequality, (3.6) is equivalent to (for any )
[TABLE]
Because and |u(x,t)|=\Big{|}\int_{-L}^{L}G(x-X(\theta,t))m_{0}(\theta)d\theta\Big{|}\leq\frac{1}{2}||m_{0}||_{L^{1}}, we know that (3.2) is equivalent to
[TABLE]
(3.9) tells us is bounded. Hence the blow up behavior is different with the Camassa-Holm equation, where becomes unbounded [10, 11].
When , equality (2.42) implies for any . Then, all the above blow-up criterions are equivalent to
[TABLE]
Next, when (), we give another proof for (3.7) based on (3.10)(p=2).
Another proof for (3.7).
By Theorem 2.1 and Theorem 2.2, we know . From (1.1), we obtain
[TABLE]
Multiplying both sides by and taking integral show that
[TABLE]
Integration by parts for the last term implies that
[TABLE]
On the other hand, we have
[TABLE]
Hence
[TABLE]
Inequality (3.9) gives
[TABLE]
By PoincarΓ© inequality, we have
[TABLE]
Hence
[TABLE]
Gronwallβs inequality shows that
[TABLE]
which implies .
β
4 Finite time blow up and almost global existence of classical solutions
In the rest of this paper, we assume .
In this section, we show that for some initial data solutions to the mCH equation blow up in finite time. Some blow-up rates are obtained. Moreover, for any and initial data , we prove that the lifespan of the classical solutions satisfies
[TABLE]
where is a constant depends on
Our finite time blow-up results are similar to the blow-up results in [8, 18, 22] but with some subtle differences. All these three papers apply the idea from transport equation and focus on the derivative of which is . Comparing with [18, Theorem 5.2,5.3], we show finite time blow-up for which can change its sign. Besides, our starting point do not have to be the maximum point of in contrast with [22, Theorem 1.3]. The main idea of our proof is similar to [8, Theorem 1.5] which shows blow-up for a sign-changing with the effect of the linear dispersion term ().
We have the following proposition.
Proposition 4.1**.**
*Suppose . Let be the maximal time of the existence of the corresponding classical solution to (1.1)-(1.2). is the solution to (1.8).
If satisfies , then we have*
[TABLE]
* We have the following lower bound for blow-up time*
[TABLE]
Proof.
(i) The mCH equation (1.1) can be rewritten as
[TABLE]
Therefore, we have
[TABLE]
By (2.42), when we know and it will keep sign (positive or negative) for . Hence
[TABLE]
This implies
[TABLE]
Integrating from [math] to leads to
[TABLE]
and combining (2.42) gives (4.1).
(ii) If , then (4.1) and (1.9) give that
[TABLE]
which is a contradiction with the assumption of blow-up at .
β
In view of equation (4.3), the most natural way to study blow-up behavior is following the characteristics. This method was used for the Burgers equation and the CH equation. Equality (4.5) reminds us the proof for finite time blow-up of Burgers equation:
[TABLE]
Consider its characteries and we have
[TABLE]
Taking derivative of (4.6) gives
[TABLE]
Then we have
[TABLE]
which implies
[TABLE]
Hence, if there exists such that , then goes to in finite time.
(4.5) is similar to (4.7). But we can not have direct estimate on the blow-up time like the Burgers equation. Hence we need to give some estimate about . We have the following lemma.
Lemma 4.1**.**
Suppose and . Let be the maximal time of existence of the corresponding classical solution to (1.1)-(1.2). is the solution to (1.8). Then we have
[TABLE]
Proof.
From (1.1), we obtain
[TABLE]
which implies
[TABLE]
Taking derivative to (4.9) with respect to yields
[TABLE]
Due to and , we have
[TABLE]
After some calculation we obtain
[TABLE]
For the last two terms on the right side, integration by parts shows that
[TABLE]
Hence
[TABLE]
Youngβs inequality and (1.9) give that
[TABLE]
which implies (4.8).
β
Next, we state and prove our main results in this section.
Theorem 4.1**.**
Suppose and . Let be the maximal time of existence of the classical solution to (1.1)-(1.2). is the solution to (1.8). If there is a such that and
[TABLE]
then defined by (1.10) blows up at a time
[TABLE]
Moreover, when , we have the following estimate of the blow-up rate for :
[TABLE]
and for we have
[TABLE]
Where
[TABLE]
Proof.
Step 1.
Assume . Combining (4.4) and (4.8) shows that
[TABLE]
Integrating (4.14) shows that
[TABLE]
where we used
[TABLE]
Integrating (4.15) gives
[TABLE]
If satisfies (4.10), then we have
[TABLE]
where
[TABLE]
and
[TABLE]
Hence
[TABLE]
This implies that there is a time such that
[TABLE]
which means blows up at the time
Step 2.
Assume From (4.16), we have
[TABLE]
Hence, we have (4.12).
From (2.42) and (4.16), we have
[TABLE]
Hence, (4.13) follows and this ends the proof.
β
Similarly, we have the following theorem.
Theorem 4.2**.**
Suppose and . Let be the maximal time of existence of the classical solution to (1.1)-(1.2). is the solution to (1.8). If there is a such that and
[TABLE]
then defined by (1.10) blows up at a time
[TABLE]
Moreover, when , we have the following estimate of the blow-up rate for :
[TABLE]
and for we have
[TABLE]
Where
[TABLE]
From conditions (4.10) and (4.17), if there exists such that (1.13) holds, then the classical solution will blow up in finite time.
Now we can prove Theorem 1.2.
Proof of Theorem 1.2.
(i) (1.12) follows from (4.2).
(ii) Let satisfies the assumptions in Theorem 4.1. Then, for any we know also satisfies the assumptions. Hence, from (4.11) we have
[TABLE]
where (1.9) was used. Together with (1.12) we can obtain (1.14). β
5 Solutions at blow-up time and formation of peakons
In this section, we study the behavior of classical solutions at blow-up time .
First, we show that and are uniformly BV function for (including the blow-up time ) and has a unique limit in Radon measure space as approaching .
Let us recall the concept of the space .
Definition 5.1**.**
* For dimention and an open set , a function belongs to if*
[TABLE]
* (Equivalent definition for one dimension case) A function belongs to if for any , , the following statement holds:*
[TABLE]
Remark 5.1*.*
Let for and . is the distributional gradient of . Then, is a vector Radon measure and the total variation of is equal to the total variation of : Here, is the total variation measure of the vector measure ([21, Definition (13.2)]).
If a function satisfies Definition 5.1 (ii), then satisfies Definition (i). On the contrary, if satisfies Definition 5.1 (i), then there exists a right continuous representative which satisfies Definition (ii). See [21, Theorem 7.2] for the proof.
We have the following theorem about and at .
Theorem 5.1**.**
*Let and . Let be the maximal existence time for the classical solution to (1.1)-(1.2) and be the solution to (1.8). Then, the following assertions hold:
There exists a function such that*
[TABLE]
* For any we have*
[TABLE]
and
[TABLE]
Proof.
We use three steps to prove (i) and (ii) together.
Step 1. We prove .
Due to (3.1) and for , let go to and we obtain
[TABLE]
Moreover, we have .
Step 2. For , we prove (5.2).
For , we know and the following holds
[TABLE]
When , for any , , we have
[TABLE]
which means Similarly, we can obtain for
Step 3. We prove (5.1) and show that satisfies (5.2).
The first part of (5.1) is deduced by . To prove the second part, we have to do a little more job.
Combining (1.9), step 2, and [3, Theorem 2.3], we know that there exists a consequence and two BV functions such that
[TABLE]
and
[TABLE]
Because
[TABLE]
we know
For any test function , we have
[TABLE]
which means is the derivative of in distribution sense. Define for every and we obtain
[TABLE]
Because is continuous in , we know
[TABLE]
This is the end of the proof.
β
Next we give a theorem to prove that has a unique limit in Radon measure space as approaching . Before this, letβs recall the definition and in Remark 2.4 and denote
[TABLE]
Because may not be strictly monotonic, it is not obvious to see that and are open sets. We give a lemma to show this.
Lemma 5.1**.**
* and are open sets.*
Proof.
We only deals with and the proof for is similar.
For , there exist such that and Set
[TABLE]
and
[TABLE]
By continuity of and , and can be obtained.
If , then there is only one point such that and In this case, set
[TABLE]
and
[TABLE]
Because , we know and for . Hence
[TABLE]
Because is nondecreasing, we obtain
[TABLE]
If , we have
[TABLE]
By definition we know for . When for or , from Remark 2.4 we know . This implies that is strictly monotonic in a neighborhood of which is a contradiction with (5.3). Hence, we have
[TABLE]
Hence, there exist and such that
[TABLE]
Therefore, we have
[TABLE]
and
[TABLE]
which imply
[TABLE]
β
For any Radon measure and measurable set , we use to stand for the restriction of on the set . We have the following Theorem.
Theorem 5.2**.**
Let the assumptions in Theorem 5.1 holds. Then there exists a unique Radon measure such that
[TABLE]
*Moreover, has the following properties:
Compact support:*
[TABLE]
* Denote*
[TABLE]
Then is a positive Radon measure and is a negative Radon measure. Besides, we have
[TABLE]
* The following equality holds:*
[TABLE]
Proof.
Step 1. Proof of (5.4).
Because is a BV function, its derivative is a Radon measure. We know
[TABLE]
is a Radon measure and for any test function , we have
[TABLE]
Then, we have
[TABLE]
This proves (5.4).
Step 2. Proof of (i).
For any test function , we have
[TABLE]
where (2.42) was used. Because and for , we have . Let test function satisfy Then we obtain
[TABLE]
which implies (5.5).
Step 3. Proof of (ii).
Due to (5), we know
[TABLE]
For and , by the definition of we have
[TABLE]
Hence, is a positive Radon measure. With the same argument, we can see that is a negative Radon measure.
On the other hand, by using (5), we have
[TABLE]
which implies (5.6).
Step 4. Proof of (iii).
From (2.42), we have
[TABLE]
which implies
[TABLE]
For any test function , we have
[TABLE]
Choose satisfying
[TABLE]
Hence, we have
[TABLE]
This ends the proof. β
Remark 5.2*.*
In Section 6, we will prove the global existence of weak solutions to the mCH equation when initial data belongs to . Hence, we can extend globally in time after blow up time. Similar results can be found in [17], where a sticky particle method was used.
Next, we introduce another two sets to study solutions at . Assume and is the solution to the Lagrange dynamics (1.8). Set
[TABLE]
and
[TABLE]
Then, is a closed set and is an open set. Moreover, we have
[TABLE]
Because the classical solution blows up in finite time , we know is not empty. On the other hand, due to , Remark 2.4 tells that which implies is not empty.
Set
[TABLE]
Then, we have
[TABLE]
is strictly monotonic in . Hence, is also an open set and is a closed set. Moreover, we claim that
[TABLE]
To show (5.11), we only have to prove . For any , there exists such that and . Let Then there is a small constant such that and for . Hence, for and which implies .
We have the following theorem.
Theorem 5.3**.**
Let assumptions in Theorem 5.1 hold. Then we have
[TABLE]
and
[TABLE]
Moreover, the following holds
[TABLE]
Proof.
Step 1. We first consider the cases when
Because , from Remark 2.4 we know , which means is strictly monotonic in a small neighborhood of . Hence,
[TABLE]
From this we know, if , we have for . From Theorem 5.1, we know
[TABLE]
Thus
[TABLE]
This shows
[TABLE]
Hence, .
Similarly, we can show .
Step 2. We only left the case for .
When , there exists a such that . Because we know is the unique point satisfying Rewrite as
[TABLE]
Using , we can obtain
[TABLE]
Hence,
[TABLE]
Taking derivative again shows that
[TABLE]
Because and , which implies
[TABLE]
Together with Step 1 and Step 2, we obtain
[TABLE]
Step 3. Because is an open set, for any we have
[TABLE]
where (5.8) was used. Because is arbitrary and , we obtain
[TABLE]
From Theorem 5.2, we know has compact support in . Hence,
[TABLE]
Because the Radon measure has finite total variation, we obtain
[TABLE]
From (5), we know
[TABLE]
where and This means (2.42) holds in the set :
[TABLE]
This finishes our proof.
β
Because and are BV functions, their discontinuous points are countable. We give a proposition to show discontinuous points of . First, let us introduce two subsets of .
[TABLE]
and
[TABLE]
Proposition 5.1**.**
Let the assumptions in Theorem 5.1 hold. Then, and is not continuous at .
Proof.
Step 1. Assume and we prove is continuous at .
By definition of , we know there is only one point , such that . Due to (5.11), there exist two sequence and such that the following hold:
[TABLE]
and
[TABLE]
Because , there is a unique such that . Similarly, we have a unique such that (Uniqueness is because is strictly monotonic in .) Moreover, we have
[TABLE]
and
[TABLE]
Because formula (5) holds for , we know
[TABLE]
Let goes to infinity and we obtain
[TABLE]
Similarly, we have
[TABLE]
and
[TABLE]
This implies . For any , define
[TABLE]
Then using similar argument for any sequence , we know
[TABLE]
Step 2. Assume and we prove is discontinuous at .
Set
[TABLE]
By definition of we know . Moreover, we know
[TABLE]
Claim: will not change sign in .
If this is not true, then we have such that . Remark 2.4 tells us that and we obtain a contradiction.
Similar to Step 1, we have four sequences , , and which satisfy
[TABLE]
[TABLE]
and
[TABLE]
From (5), we know
[TABLE]
Let go to and we obtain
[TABLE]
Similarly, we also have
[TABLE]
Hence, using the above claim, we have
[TABLE]
which shows that is not continuous at .
β
Next, we prove Theorem 1.3. Letβs give some notations first.
Assume and . Let (). From the proof (5), we know that for each there exist such that
[TABLE]
where
[TABLE]
Set
[TABLE]
Proof of Theorem 1.3.
For any text function , we have
[TABLE]
Because , integration by parts leads to
[TABLE]
Because is continuous at for , combining (5.14) and (5.17) gives that
[TABLE]
β
This theorem tells us that peakons are exactly the points in the set . Hence, a peakon is formulated when some Lagrangian labels in a interval aggregate into one point at and the weight of the peakon is the integration of on .
6 Solutions after blow-up.
At the blow up time, the solution to the mCH equation becomes a Radon measure. In this section, we assume initial data belongs to the Radon measure space and use the Lagrange dynamics to prove that weak solution to (1.1)-(1.2) exists globally in Radon measure space.
6.1 Regularized Lagrange dynamics and BV estimate.
Let satisfies
[TABLE]
is not continuous and may not be integrable with respect to Radon measure . (1.8) can not be used directly. Hence, a regularization is needed.
Letβs give the definition of mollifier.
Definition 6.1**.**
* Define the mollifier , satisfying*
[TABLE]
* For each , set*
[TABLE]
With this definition, we define
[TABLE]
Hence, for . By Youngβs inequality we have
[TABLE]
and
[TABLE]
Because when , we have
[TABLE]
On the other hand, because , there is a constant such that
[TABLE]
Hence, is a global Lipschitz function. For any measurable function , we define
[TABLE]
and
[TABLE]
The regularized Lagrange dynamics is given by
[TABLE]
Consider this equation in the Banach space with norm. One can easily show that the vector field is globally Lipschitz. Hence, by the Picard theorem for ODEs in a Banach space, we obtain a unique global solution
[TABLE]
Define
[TABLE]
and
[TABLE]
By the definition, we have
[TABLE]
Hence, we have the following relation between and
[TABLE]
In the following of this paper, we denote
[TABLE]
Hence, we have
[TABLE]
From Definition 5.1 we can easily obtain
[TABLE]
and
[TABLE]
We have the following Lemma about .
Lemma 6.1**.**
*Let satisfy (6.1). For , is defined by (6.3). Then, the following statements hold:
*
[TABLE]
**
[TABLE]
* For any , we have*
[TABLE]
Moreover, for any , there exist subsequences of , (also denoted as , ) and two functions such that
[TABLE]
and , satisfy all the properties in , and .
Proof.
(i) From (6.2) and the definition of , we can easily obtain (i).
(ii) For any , , (6.7) yields
[TABLE]
Hence, . Similarly, we can obtain .
(iii)
[TABLE]
By the definition of and (6.6), we know
[TABLE]
Hence,
[TABLE]
[3, Lemma 2.3] gives
[TABLE]
Hence
[TABLE]
Similarly, we can obtain
[TABLE]
The rest results can be obtained by using [3, Theorem 2.4,2.6].
β
6.2 Weak consistency and convergence theorem
In this subsection, we show that defined by (6.3) is weak consistent with the mCH equation (1.1)-(1.2).
We rewrite (1.1) as equation of ,
[TABLE]
Now, we introduce the definition of weak solution in terms of . To this end, for , we denote the functional
[TABLE]
Then, the definition of the weak solution to (1.1) in terms of is given as follows.
Definition 6.2**.**
For , a function
[TABLE]
is said to be a weak solution of (1.1)-(1.2) if
[TABLE]
holds for all . If , we call as a global weak solution of the mCH equation.
For simplicity in notations, we denote
[TABLE]
For any test function , we have
[TABLE]
On the other hand, combining the definition (6.3) and (6.2) gives
[TABLE]
Combining the last two equalities, we define
[TABLE]
We now state the main result of this section.
Proposition 6.1**.**
We have the following estimate
[TABLE]
The constant is independent of
Proof.
By the definition of and , the first term in (6.10) can be estimated as
[TABLE]
For the second term of (6.10), because is an even function, by the definition of we can obtain
[TABLE]
This ends the proof.
β
Next, we state our main theorem in this section, which contains Theorem 1.4.
Theorem 6.1**.**
Assume that initial data satisfies (6.1). and are defined by (6.3). Then, the limit function given by Lemma 6.1 is a global weak solution of the mCH equation (1.1)-(1.2) and
[TABLE]
Furthermore, for any , we have
[TABLE]
[TABLE]
and there exists subsequence of (also labelled as ) such that
[TABLE]
Proof.
Step 1. Global weak solution.
As it is shown in Lemma 6.1, we have such that
[TABLE]
Moreover, for any , the limit functions satisfy
[TABLE]
[TABLE]
and
[TABLE]
for . Hence,
[TABLE]
Similarly, we have
[TABLE]
These two inequalities imply
[TABLE]
Therefore
[TABLE]
For each , there exists such that We now consider convergence for each term of ,
[TABLE]
For the first term, because supp is compact, we can see
[TABLE]
The second term can be estimated as follows
[TABLE]
Similarly, we obtain
[TABLE]
and
[TABLE]
Combining the above estimates and Proposition 6.1 gives
[TABLE]
This proves that is a global weak solution to the mCH equation.
Step 2. Now we prove that
[TABLE]
For any test function , integrating by parts and using the relationship imply that
[TABLE]
Taking , the right hand side of the above equality converges to
[TABLE]
Hence, . This ends the proof.
β
Remark 6.1*.*
In [17], the authors also provee the total variation stability of . That is
[TABLE]
The weak solution is unique when Moreover, examples about nonuniqueness of peakon weak solutions can also be found in [17]. Notice that peakon solutions are not in the solution class .
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