Nonlinear Analysis: Real World Applications 13 (2012) 158–167
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Some properties of solutions to the weakly dissipative b-family equation Mingxuan Zhu, Zaihong Jiang ∗ Department of Mathematics, Zhejiang Normal University, Jinhua 321004, PR China
article
abstract
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Article history: Received 22 March 2011 Accepted 19 July 2011
In this paper, we investigate the b-family equation with a weakly dissipative term. First, we present a new criterion on the blow-up phenomenon of the solution. Then the global existence and the persistence property of the solution are also established. Finally, we discuss the infinite propagation speed for this equation. © 2011 Elsevier Ltd. All rights reserved.
Keywords: b-family equation Blow-up Persistence property Infinite propagation speed
1. Introduction Recently, Holm and Staley [1] studied the exchange of stability in the dynamics of solitary wave solutions under changes in the nonlinear balance in a 1 + 1 evolutionary partial differential equation related both to shallow water waves and to turbulence. They derived the following equations (the b-family equation): yt + uyx + bux y = 0,
t > 0, x ∈ R,
(1.1)
where u(x, t ) denotes the velocity field and y(x, t ) = u − uxx . A detailed description of the corresponding strong solutions to (1.1) with the initial data u0 was given by Zhou in [2]. In this work, a sufficient condition in the profile of the initial data for blow-up in finite time is established. The necessary and sufficient condition for blow-up is still a challenging problem for us at present. More importantly, Theorem 3.1 in [2] means that no matter what the profile of the compactly supported initial datum u0 (x) is (no matter whether it is positive or negative), for any t > 0 in its lifespan, the solution u(x, t ) is positive at infinity and negative at negative infinity. It is a very good property for the b-family equation. The famous Camassa–Holm equation [3] and Degasperis–Procesi equation [4] are the special cases with b = 2 and b = 3, respectively. There have been extensive studies on the two equations, cf. [5–11]. In this paper, we consider the following weakly dissipative b-family equation, yt + uyx + bux y + λy = 0,
t > 0, x ∈ R,
(1.2)
where y = u − uxx , λ > 0 and λy = λ(u − uxx ) is the weakly dissipative term. 1
Let Λ = (1 − ∂x2 ) 2 , then the operator Λ−2 can be expressed by its associated Green’s function G =
Λ−2 f (x) = G ∗ f (x) =
∗
1 2
∫
e−|x−y| f (y)dy. R
Corresponding author. E-mail addresses:
[email protected] (M. Zhu),
[email protected],
[email protected] (Z. Jiang).
1468-1218/$ – see front matter © 2011 Elsevier Ltd. All rights reserved. doi:10.1016/j.nonrwa.2011.07.020
1 −|x| e 2
as (1.3)
M. Zhu, Z. Jiang / Nonlinear Analysis: Real World Applications 13 (2012) 158–167
159
So system (1.2) is equivalent to the following system ut + uux + ∂x G ∗
b 2
u2 +
3−b 2
u2x
+ λu = 0.
(1.4)
In [12], Niu and Zhang established the following local well-posedness result for (1.2) by using Kato’s theory. Theorem 1.1 ([12]). Given u0 ∈ H s (R), s >
3 ; 2
then, there exists a T and a unique solution u to (1.2) such that
u(x, t ) ∈ C ([0, T ); H s (R)) ∩ C 1 ([0, T ); H s−1 (R)). Then they present the precise blow-up scenario for solutions to (1.2). Theorem 1.2 ([12]). Assume that u0 ∈ H s (R), s > 2. If b =
1 , 2
then the solution of (1.2) will exist globally in time. If b >
then the solution blows up if and only if ux becomes unbounded from below in finite time. If b < time if and only if ux becomes unbounded from the above in finite time.
1 , 2
1 , 2
the solution blows up in finite
The paper is organized as follows. In Section 2, we establish a new criterion on blow-up for (1.2). A condition for global existence is found in Section 3. Persistence property is considered in Section 4. In Section 5, the infinite propagation speed will be established analogous to the b-family equation. It is worth pointing out that, recently, many works have been done for similar equations which have a dissipative term, cf. [13–17]. 2. Blow-up Motivated by Mckean’s deep observation for the Camassa–Holm equation [7], we can do the similar particle trajectory as
qt = u(q, t ), q(x, 0) = x,
0 < t < T , x ∈ R, x ∈ R,
(2.1)
where T is the life span of the solution, then q is a diffeomorphism of the line. Differentiating the first equation in (2.1) with respect to x, one has dqt dx
= qxt = ux (q, t ),
t ∈ (0, T ).
Hence, qx (x, t ) = exp
t
∫
ux (q, s)ds ,
qx (x, 0) = 1.
0
Since d dt
(y(q)qbx ) = [yt (q) + u(q, t )yx (q) − bux (q, t )y(q)]qbx = −λyqbx ,
It follows that y(q)qbx = y0 (x)e−λt .
(2.2)
In [12], a blow-up result was proved for odd initial data. Here, we establish sufficient conditions on more general initial data to guarantee blow-up for Eq. (1.2). Theorem 2.1. Let b ≥ 2. Suppose that u0 ∈ H 2 (R) and there exists a x0 ∈ R such that y0 (x0 ) = (1 − ∂x2 )u0 (x0 ) = 0, y0 ≥ 0(̸≡ 0) e −x 0
∫
x0
for x ∈ (−∞, x0 ) and
eξ y0 (ξ )dξ > 2λ and
−∞
ex0
∫
y0 ≤ 0(̸≡ 0)
for x ∈ (x0 , ∞),
(2.3)
∞
e−ξ y0 (ξ )dξ < −2λ.
(2.4)
x0
Then the corresponding solution u(x, t ) to Eq. (1.2) with u0 as the initial datum blows up in finite time. Proof. Suppose that the solution exists globally. Due to Eq. (2.2) and the initial condition (2.3), we have y(q(x0 , t ), t ) = 0, and
y(q(x, t ), t ) ≥ 0(̸≡ 0), y(q(x, t ), t ) ≤ 0(̸≡ 0),
for x ∈ (−∞, (q(x0 , t ), t )), for x ∈ ((q(x0 , t ), t ), ∞),
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M. Zhu, Z. Jiang / Nonlinear Analysis: Real World Applications 13 (2012) 158–167
for all t ≥ 0. Since u(x, t ) = G ∗ y(x, t ), one can write u(x, t ) and ux (x, t ) as ∞ 1 1 −x x ξ e y(ξ , t )dξ + ex e−ξ y(ξ , t )dξ , e 2 2 −∞ x ∫ ∫ 1 −x x ξ 1 x ∞ −ξ ux (x, t ) = − e e y(ξ , t )dξ + e e y(ξ , t )dξ . 2 2 −∞ x
∫
u(x, t ) =
∫
Consequently, u2x (x, t ) − u2 (x, t ) = −
x
∫
∞
∫
eξ y(ξ , t )dξ
−∞
e−ξ y(ξ , t )dξ , x
for all t > 0. For any fixed t, if x ≤ q(x0 , t ), then u2x (x, t ) − u2 (x, t ) = −
q(x0 ,t )
∫
eξ y(ξ , t )dξ −
−∞ ∞
× q(x0 ,t )
=
eξ y(ξ , t )dξ
x
∫
u2x
q(x0 ,t )
∫
e−ξ y(ξ , t )dξ +
q(x0 ,t )
∫
e−ξ y(ξ , t )dξ
x
(q(x0 , t ), t ) − u (q(x0 , t ), t ) − 2
∫
x
ξ
e y(ξ , t )dξ −∞
q(x0 ,t )
∫ +
ξ
e y(ξ , t )dξ
e−ξ y(ξ , t )dξ
x
∞
∫
q(x0 ,t )
x
q(x0 ,t )
∫
e−ξ y(ξ , t )dξ
≤ u2x (q(x0 , t ), t ) − u2 (q(x0 , t ), t ).
(2.5)
Similarly, for x ≥ q(x0 , t ), we also have u2x (x, t ) − u2 (x, t ) ≤ u2x (q(x0 , t ), t ) − u2 (q(x0 , t ), t ).
(2.6)
Combining (2.5) and (2.6) together, we get that for any fixed t, u2x (x, t ) − u2 (x, t ) ≤ u2x (q(x0 , t ), t ) − u2 (q(x0 , t ), t ),
(2.7)
for all x ∈ R. Differentiating Eq. (1.4) with respect to x, we obtain utx + uuxx −
b 2
2
u −
1−b 2
u2x
b
+G∗
2
2
u +
3−b 2
u2x
+ λux = 0.
Differentiating ux (q(x0 , t ), t ) with respect to t, where q is the diffeomorphism defined in (2.1)
∂t ux (q(x0 , t ), t ) = uxt (q(x0 , t ), t ) + uxx (q(x0 , t ), t )qt (q(x0 , t ), t ) b 1−b 2 b 2 3−b 2 = u2 (q(x0 , t ), t ) + ux (q(x0 , t ), t ) − λux (q(x0 , t ), t ) − G ∗ u (x, t ) + ux (x, t ) 2 2 2 2 b 2 1−b 2 b 2 3−b 2 = G∗ u (q(x0 , t ), t ) + ux (q(x0 , t ), t ) − u (x, t ) − ux (x, t ) − λux (q(x0 , t ), t ) 2 2 2 2 b−2 2 = G∗ (u (q(x0 , t ), t ) − u2x (q(x0 , t ), t ) − u2 (x, t ) + u2x (x, t )) 2 1 1 + G ∗ u2 (q(x0 , t ), t ) − u2x (q(x0 , t ), t ) − u2 (x, t ) − u2x (x, t ) − λux (q(x0 , t ), t ) 2
≤
1 2
u2 (q(x0 , t ), t ) −
1 2
2
u2x (q(x0 , t ), t ) − λux (q(x0 , t ), t ),
where we have used (2.7) and the inequality G ∗ (u2 (x, t ) + 21 u2x (x, t )) ≥ By (2.4), we find that
(u0x (x0 ) + λ) − (u0 (x0 ) + λ) = −e 2
2
−x 0
∫
x0
−∞
ξ
e y0 (ξ )dξ ×
e
x0
∫
1 2 u . 2
∞
e x0
(2.8)
−ξ
y0 (ξ )dξ + 2λ
>0
M. Zhu, Z. Jiang / Nonlinear Analysis: Real World Applications 13 (2012) 158–167
161
and ∞
∫
(u0x (x0 ) + λ)2 − (u0 (x0 ) − λ)2 = −ex0
e−ξ y0 (ξ )dξ ×
x0
∫
e−x0
eξ y0 (ξ )dξ − 2λ
> 0.
−∞
x0
Claim. ux (q(x0 , t ), t ) < 0 is decreasing, (u(q(x0 , t ), t ) + λ)2 < (ux (q(x0 , t ), t ) + λ)2 and (u(q(x0 , t ), t ) − λ)2 < (ux (q (x0 , t ), t ) + λ)2 for all t ≥ 0. Suppose not, i.e. there exists a t0 such that (u(q(x0 , t ), t ) + λ)2 < (ux (q(x0 , t ), t ) + λ)2 and (u(q(x0 , t ), t ) − λ)2 < (ux (q(x0 , t ), t )+λ)2 on [0, t ), then (u(q(x0 , t ), t )+λ)2 = (ux (q(x0 , t ), t )+λ)2 or (u(q(x0 , t ), t )−λ)2 = (ux (q(x0 , t ), t )+λ)2 . Now, let 1 −q(x0 ,t ) q(x0 ,t ) ξ e y(ξ , t )dξ e 2 −∞
∫
I (t ) := and II (t ) :=
1 2
q(x0 ,t )
∫
∞
e
q(x0 ,t )
e−ξ y(ξ , t )dξ .
First, differentiating I (t ), we have dI (t ) dt
1
= − u(q(x0 , t ), t )e−q(x0 ,t )
q(x0 ,t )
∫
2
eξ y(ξ , t )dξ +
−∞
1 −q(x0 ,t ) q(x0 ,t ) ξ e e yt (ξ , t )dξ 2 −∞
∫
1 −q(x0 ,t ) q(x0 ,t ) ξ b−2 2 e e uyx + 2ux y + (u − u2x )x + λy dξ 2 2 2 −∞ 1 1 2 λ 2 ≥ u(ux − u)(q(x0 , t ), t ) + (u + ux − 2uux )(q(x0 , t ), t ) − (u − ux )(q(x0 , t ), t ) 2 4 2 1 2 λ 2 = (ux − u )(q(x0 , t ), t ) − (u − ux )(q(x0 , t ), t ) 4 2 1 1 2 = (ux + λ) (q(x0 , t ), t ) − (u + λ)2 (q(x0 , t ), t ) > 0, on [0, t0 ). 4 4
=
1
∫
u(ux − u)(q(x0 , t ), t ) −
(2.9)
Second, by the same argument, we get dII (t ) dt
= = ≤
1 2 1 2 1 2
u(q(x0 , t ), t )eq(x0 ,t )
∫
∞ q(x0 ,t )
u(ux + u)(q(x0 , t ), t ) −
1
u(ux + u)(q(x0 , t ), t ) −
1
2 4
e−ξ y(ξ , t )dξ + q(x0 ,t )
2
∞ −ξ
e
eq(x0 ,t )
∫
∞ q(x0 ,t )
e−ξ yt (ξ , t )dξ
e q(x0 ,t )
uyx + 2ux y +
(u2 + u2x + 2uux )(q(x0 , t ), t ) −
1
λ
4 1
2 1
4
4
= − (u2x − u2 )(q(x0 , t ), t ) −
∫
1
b−2
λ 2
2
(u − 2
) + λy dξ
u2x x
(ux + u)(q(x0 , t ), t )
(ux + u)(q(x0 , t ), t )
= − (ux (q(x0 , t ), t ) + λ)2 + (u(q(x0 , t ), t ) − λ)2 < 0,
on [0, t0 ).
(2.10)
Hence, it follows from (2.9), (2.10) and the continuity property of ODEs that
(ux (q(x0 , t ), t ) + λ)2 − (u(q(x0 , t ), t ) + λ)2 = −4I (t )(II (t ) + λ) > −4I (0)(II (0) + λ) > 0, and
(ux (q(x0 , t ), t ) + λ)2 − (u(q(x0 , t ), t ) − λ)2 = −4(I (t ) − λ)II (t ) > −4(I (0) − λ)II (0) > 0, for all t > 0, this implies that t0 can be extended to the infinity. Using (2.9) and (2.10) again, we have the following equation for [2(ux + λ)2 − (u + λ)2 − (u − λ)2 ](q(x0 , t ), t ): d dt
[2(ux + λ)2 − (u + λ)2 − (u − λ)2 ](q(x0 , t ), t ) = −4
d dt
[I (t )(II (t ) + λ)] − 4
d dt
[(I (t ) − λ)II (t )]
≥ −[(ux + λ)2 − (u + λ)2 ](q(x0 , t ), t )(II (t ) + λ) + [(ux + λ)2 − (u − λ)2 ](q(x0 , t ), t )I (t ) − [(ux + λ)2 − (u + λ)2 ](q(x0 , t ), t )II (t ) + [(ux + λ)2 − (u − λ)2 ](q(x0 , t ), t )(I (t ) − λ) = −λ[2(ux + λ)2 − (u + λ)2 − (u − λ)2 ](q(x0 , t ), t ) − ux (q(x0 , t ), t )(2(ux (q(x0 , t ), t ) + λ)2 ) + 2(u + λ)2 II (t ) − 2(u − λ)2 I (t )
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M. Zhu, Z. Jiang / Nonlinear Analysis: Real World Applications 13 (2012) 158–167
= −(ux (q(x0 , t ), t ) + λ)[2(ux + λ)2 − (u + λ)2 − (u − λ)2 ](q(x0 , t ), t ) − ux (q(x0 , t ), t )[(u + λ)2 + (u − λ)2 ](q(x0 , t ), t ) + 2(u + λ)2 II (t ) − 2(u − λ)2 I (t ) ≥ −(ux (q(x0 , t ), t ) + λ)[2(ux + λ)2 − (u + λ)2 − (u − λ)2 ](q(x0 , t ), t ),
(2.11)
where we use ux (q(x0 , t ), t ) = −I (t ) + II (t ). Now, recall (2.8), we get
∂t ux (q(x0 , t ), t )(q(x0 , t ), t ) ≤ =
1 2 1 4
u2 (q(x0 , t ), t ) −
1 2
u2x (q(x0 , t ), t ) − λux
[(u + λ)2 + (u − λ)2 − 2(ux + λ)2 ](q(x0 , t ), t ).
(2.12)
Substituting (2.12) into (2.11), it yields d dt
[2(ux + λ)2 − (u + λ)2 − (u − λ)2 ](q(x0 , t ), t ) 1
[2(ux + λ)2 − (u + λ)2 − (u − λ)2 ](q(x0 , t ), t ) ∫ t × [2(ux + λ)2 − (u + λ)2 − (u − λ)2 ](q(x0 , τ ), τ )dτ − 4u0x (x0 ) − 4λ . ≥
4
(2.13)
0
Before completing the proof, we need the following technical lemma. Lemma 2.2 ([2]). Suppose that Ψ (t ) is twice continuously differentiable satisfying
Ψ ′′ (t ) ≥ C0 Ψ ′ (t )Ψ (t ), Ψ (t ) > 0,
t > 0, C0 > 0, Ψ ′ (t ) > 0.
(2.14)
Then ψ(t ) blows up in finite time. Moreover, the blow up time can be estimated in terms of the initial datum as
T ≤ max Let Ψ (t ) = with C0 =
1 . 4
t 0
Ψ (0) . C0 Ψ (0) Ψ ′ (0) 2
,
[2(ux + λ)2 − (u + λ)2 − (u − λ)2 ](q(x0 , τ ), τ )dτ − 4u0x (x0 ) − 4λ, then (2.13) is an equation of type (2.14)
The proof is completed by applying Lemma 2.2.
Remark 2.1. Mckean got the necessary and sufficient condition for the Camassa–Holm equation in [7]. It is worth pointing out that Zhou and his collaborators [18] gave a new proof to Mckean’s theorem. However, the necessary and sufficient condition for (1.2) is still a challenging problem for us at present. Theorem 2.3. Let b = 2. Suppose that u0 ∈ H 2 (R) and there exists x0 ∈ R such that y0 (x0 ) = (1 − ∂x2 )u0 (x0 ) = 0, e−x0
∫
x0
eξ y0 (ξ )dξ > 2λ
ex0
and
∫
−∞
∞
e−ξ y0 (ξ )dξ < −2λ. x0
Then the corresponding solution u(x, t ) to Eq. (1.2) with u0 as the initial datum blows up in finite time. Proof. When b = 2, it is the famous Camassa–Holm equation with the weakly dissipative term. We can easily get 2
utx + uuxx − u +
1 2
u2x
2
+G∗ u +
1 2
u2x
+ λux = 0.
Differentiating ux at the point (q(x0 , t ), t ) with respect to t, we have d dt
ux (q(x0 , t ), t ) ≤
1 2
u2 (q(x0 , t ), t ) −
1 2
u2x (q(x0 , t ), t ) − λux (q(x0 , t ), t ) < 0.
The proof follows from Theorem 2.1 directly. So, to be concise, we omit the detailed proof. Remark 2.2. The condition in [13] is that u(0, t ) = 0 is odd,
∫
0
−∞
eξ y0 (ξ ) > 2λ and
∞
∫
e−ξ y0 (ξ ) < −2λ. 0
Theorem 2.3 is an improvement of that in [13].
M. Zhu, Z. Jiang / Nonlinear Analysis: Real World Applications 13 (2012) 158–167
163
3. Global existence Now, let us try to find a condition for global existence. Unfortunately, like the Degasperis–Procesi equation [11], only the following easy one can be proved at present. Theorem 3.1. Suppose that u0 ∈ H 3 (R), y0 = (1 − ∂x2 )u0 is have the same sign. Then the corresponding solution to (1.2) exists globally. Proof. Without loss of generality, we assume that y0 ≥ 0. It is sufficient to prove that ux (x, t ) has a lower and upper bound for all t. In fact, x 1 1 eξ y(ξ , t )dξ + ex ux (x, t ) = − e−x 2 2 −∞
∫
∞
∫
e−ξ y(ξ , t )dξ , x
so, x 1 x 1 ux (x, t ) ≥ − e−x eξ y(ξ , t )dξ ≥ − y(ξ , t )dξ 2 2 −∞ −∞ ∫ ∞ ∫ ∞ 1 1 y(ξ , t )dξ = − y0 (ξ , t )dξ ≥− 2 −∞ 2 −∞
∫
∫
and ux (x, t ) ≤
≤
1 2
x
∞
∫
e
1
e
−ξ
y(ξ , t )dξ ≤
x
∫
∞
2 −∞
y(ξ , t )dξ =
This completes the proof.
1
∫
1
∞
∫
2
y(ξ , t )dξ x
∞
2 −∞
y0 (ξ , t )dξ .
4. Persistence property Now, we shall investigate the following property for the strong solutions to (1.4) in L∞ -space with asymptotic exponential decay at infinity as their initial profiles. The main idea comes from a recent work of Zhou and his collaborators [6] for the standard Camassa–Holm equation (for slower decay rate, we refer to [19]). Theorem 4.1. Assume that for some T > 0 and s > satisfies that for some θ ∈ (0, 1),
5 , 2
u ∈ C ([0, T ]); H s (R) is a strong solution of (1.2) and u0 (x) = u(x, 0)
|u0 (x)|, |u0x (x)| ∼ O(e−θ x ). Then,
|u(x, t )|, |ux (x, t )| ∼ O(e−θ x ) uniformly in the time interval [0, T ]. Proof. First, we shall introduce the weight function to get the desired result. This function ϕN (x) with N ∈ Z+ is independent on t as follows:
ϕN (x) =
1,
eθ x , θN e ,
x ≤ 0, x ∈ (0, N ), x ≥ N,
which implies that 0 ≤ ϕN′ (x) ≤ ϕN (x). From Eq. (1.4), we can get
∂t (uϕN ) + (uϕN )ux + ϕN ∂x G ∗
b 2
2
u +
3−b 2
u2x
+ λϕN u = 0.
Multiplying (4.1) by (uϕN )2p−1 with p ∈ Z+ and integrating the result in the x-variable, we get
∫
+∞
∫ +∞ ∂t (uϕN )(uϕN )2p−1 dx + (uϕN )ux (uϕN )2p−1 dx −∞ −∞ ∫ ∫ +∞ b 2 3−b 2 + ϕN ∂x G ∗ u + ux (uϕN )2p−1 + −∞
2
2
+∞
λϕN u(uϕN )2p−1 dx = 0, −∞
(4.1)
164
M. Zhu, Z. Jiang / Nonlinear Analysis: Real World Applications 13 (2012) 158–167
from which we can deduce that d dt
‖uϕN ‖L2p ≤ (‖ ‖
+ λ)‖uϕN ‖L2p
ux L∞
3−b 2 b 2 + ϕN ∂x G ∗ u + ux 2
2
. L2p
Denoting M = supt ∈[0,T ] ‖u(t )‖H s and by Gronwall’s inequality, we obtain
‖uϕN ‖L2p ≤ ‖u0 ϕN ‖L2p
∫ t b 2 3−b 2 (M +λ)t + . ϕN ∂x G ∗ 2 u + 2 ux 2p dτ e 0 L
(4.2)
Taking the limits in (4.2), we get t
∫ ‖uϕN ‖L∞ ≤ ‖u0 ϕN ‖L∞ + 0
ϕN ∂x G ∗ b u2 + 3 − b u2 dτ e(M +λ)t . x 2 2 L∞
(4.3)
Next differentiating (1.4) in the x-variable produces the equation utx + uuxx +
u2x
+∂
2 xG
∗
b 2
2
u +
3−b 2
u2x
+ λux = 0.
(4.4)
Using the weight function, we can rewrite (4.4) as
∂x (ux ϕN ) + uuxx ϕN + (ux ϕN )ux + ϕN ∂x2 G ∗
b 2
3−b
u2 +
2
u2x
+ λϕN ux = 0.
(4.5)
Multiplying (4.5) by (ux ϕN )2p−1 with p ∈ Z+ and integrating the result in the x-variable, it follows that +∞
∫
∂t (ux ϕN )(ux ϕN )
2p−1
∫
+∞
uuxx ϕN (ux ϕN )
2p−1
dx +
−∞ +∞
∫
ϕN ∂x2 G ∗
b 2
−∞
u2 +
3−b 2
(ux ϕN )ux (ux ϕN )2p−1 dx
dx +
−∞
+
+∞
∫
−∞
u2x
(ux ϕN )2p−1 dx +
∫
+∞
λϕN ux (ux ϕN )2p−1 dx = 0.
(4.6)
−∞
For the second term on the right side of (4.6), we know that
∫
+∞
2p
uuxx ϕN (ux ϕN )2p−1 dx ≤ 2(‖u‖L∞ + ‖ux ‖L∞ )‖ux ϕN ‖L2p .
−∞
Using the above estimate and Hölder inequality, we deduce that d dt
‖ux ϕN ‖L2p ≤ (2M + λ)‖ux ϕN ‖L2p + ‖ϕN ∂x S ‖L2p .
Thanks to Gronwall’s inequality, it holds that
‖ux ϕN ‖L2p ≤ ‖u0x ϕN ‖L2p
∫ t b 2 3−b 2 2 (2M +λ)t + . ϕN ∂x G ∗ 2 u + 2 ux 2p dτ e 0 L
(4.7)
Taking the limits in (4.7), we have
∫ ‖ux ϕN ‖L∞ ≤ ‖u0x ϕN ‖L∞ + 0
t
ϕN ∂ 2 G ∗ b u2 + 3 − b u2 dτ e(2M +λ)t . x x 2 2 L∞
(4.8)
Combining (4.3) and (4.8) together, it follows that
‖uϕN ‖
L∞
+ ‖ux ϕN ‖
L∞
≤ (‖u0 ϕN ‖
L∞
+ ‖u0x ϕN ‖
L∞
)e
(2M +λ)t
+e
(2M +λ)t
∫ t ϕN ∂x G ∗ b u2 + 3 − b u2 x 2 2 0 L∞
b 2 3−b 2 2 + ϕN ∂x G ∗ u + ux dτ . 2 2 L∞ A simple calculation shows that there exists c0 > 0, depending only on θ ∈ (0, 1), such that for any N ∈ Z+ ,
ϕN (x)
∫
∞
e−|x−y| −∞
1
ϕN (y)
dy ≤ c0 =
4 1−θ
.
(4.9)
M. Zhu, Z. Jiang / Nonlinear Analysis: Real World Applications 13 (2012) 158–167
165
Thus, for any appropriate function f and g, one sees that
|ϕN G ∗ f (x)g (x)| = ≤ ≤ ≤
∫ ∞ 1 −|x−y| ϕN (x) e f (y)g (y)dy 2 −∞ ∫ ∞ 1 1 e−|x−y| ϕN (x) ϕN (y)f (y)g (y)dy 2 ϕ N (y) −∞ ∫ ∞ 1 1 e−|x−y| ϕN (x) dy ‖ϕN f ‖L∞ ‖g ‖L∞ 2 ϕN (y) −∞ c0 ‖ϕN f ‖L∞ ‖g ‖L∞ .
Similarly, we can get
|ϕN ∂x G ∗ f (x)g (x)| ≤ c0 ‖ϕN f ‖L∞ ‖g ‖L∞ , and
|ϕN ∂x2 G ∗ f (x)g (x)| ≤ c0 ‖ϕN f ‖L∞ ‖g ‖L∞ . Thus, inserting the above estimates into (4.9), there exists a constant c˜ = c˜ (M , T , λ) ≥ 0 such that
‖uϕN ‖L∞ + ‖ux ϕN ‖L∞ ≤ c˜ (‖u0 ϕN ‖L∞ + ‖u0x ϕN ‖L∞ ) + c˜
t
∫
(‖u‖L∞ + ‖ux ‖L∞ )(‖uϕN ‖L∞ + ‖ux ϕN ‖L∞ )dτ 0
≤ c˜ (‖u0 ϕN ‖L∞ + ‖u0x ϕN ‖L∞ ) + c˜
t
∫
(‖uϕN ‖L∞ + ‖ux ϕN ‖L∞ )dτ . 0
Hence, for any t ∈ Z+ and any t ∈ [0, T ], we have
‖uϕN ‖L∞ + ‖ux ϕN ‖L∞ ≤ c˜ (‖u0 ϕN ‖L∞ + ‖u0x ϕN ‖L∞ ) ≤ c˜ (‖u0 max(1, eθ x )‖L∞ + ‖u0x max(1, eθ x )‖L∞ ).
(4.10)
Finally, taking the limit as N goes to infinity in (4.10) we find that for any t ∈ [0, T ]
‖ueθ x ‖L∞ + ‖ux eθ x ‖L∞ ≤ c˜ (‖u0 max(1, eθ x )‖L∞ + ‖u0x max(1, eθ x )‖L∞ ), which completes the proof of the theorem.
5. Infinite propagation speed Recently, Zhou and his collaborators established the infinite propagation speed for the Camassa–Holm equation in [6]. Later, Guo [13,14] considered a similar problem on the weakly dissipative Camassa–Holm equation and the weakly dissipative Degasperis–Procesi equation. The purpose of this section is to give a more detailed description on the corresponding strong solution u(x, t ) to (1.2) in its life span with initial data u0 (x) being compactly supported. The main theorem reads as follows. Theorem 5.1. Let 0 ≤ b ≤ 3. Assume that for some T ≥ 0 and s ≥ 52 , u ∈ C ([0, T ]; H s (R)) is a strong solution of (1.2). If u0 (x) = u(x, 0) has compact support [a, c ], then for t ∈ (0, T ], we have u(x, t ) =
f+ (t )e−x , f− (t )e−x ,
for x > q(c , t ) for x < q(a, t ),
where f+ (t ) and f− (t ) denote continuous nonvanishing functions, with f+ (t ) > 0 and f− (t ) < 0 for t ∈ (0, T ]. Furthermore, f+ (t ) is a strictly increasing function, while f− (t ) is a strictly decreasing function. Proof. Since u0 has compact support in x in the interval [a, c ] from (2.6), so does y(, t ) in x in the interval [q(a, t ), q(c , t )] in its lifespan. Hence the following functions are well-defined. E (t ) =
∫
ex y(x, t )dx and
F (t ) =
∫
R
e−x y(x, t )dx, R
with
∫
ex y0 (x)dx = 0
E0 = R
∫ and
e−x y0 (x)dx = 0.
F0 = R
166
M. Zhu, Z. Jiang / Nonlinear Analysis: Real World Applications 13 (2012) 158–167
Then, for x > q(c , t ), we have 1 −|x| 1 e ∗ y(x, t ) = e−x 2 2
u(x, t ) =
q(b,t )
∫
q(a,t )
eτ y(τ , t )dτ =
1 −x e E (t ).
(5.1)
2
Similarly, when x < q(a, t ), we get 1 1 u(x, t ) = e−|x| ∗ y(x, t ) = ex 2 2
q(b,t )
∫
q(a,t )
e−τ y(τ , t )dτ =
1 2
ex F (t ).
(5.2)
Hence, as consequences of (5.1) and (5.2), we have 1 −x e E (t ), 2
u(x, t ) = −ux (x, t ) = uxx (x, t ) =
as x > q(c , t )
(5.3)
and u(x, t ) = ux (x, t ) = uxx (x, t ) =
1 2
ex F (t ),
as x < q(a, t ).
(5.4)
On the other hand, dE (t ) dt
∫
ex yt (x, t )dx.
= R
It is easy to get yt = −uux + (uux )xx − ∂x
b 2
Substituting the identity (5.5) into dE (t ) dt
u2 +
dE (t ) , dt
3−b 2
u2x
− λu + λuxx .
(5.5)
we obtain
∫ b 2 3−b 2 −uux + (uux )xx − ∂x u + ux dx + ex (−λu + λuxx )dx 2 2 R R ∫ 3−b 2 b 2 x u + ux dx, = e ∫
ex
=
2
R
2
where we use (5.3) and (5.4). Therefore, in the lifespan of the solution, we have E (t ) =
∫ t∫ 0
ex R
b 2
u2 +
3−b 2
u2x
(x, τ )dxdτ > 0.
By the same argument, one can check that the following identity for F (t ) is true F (t ) = −
∫ t∫ 0
e−x R
b 2
u2 +
3−b 2
u2x
(x, τ )dxdτ < 0.
In order to complete the proof, it is sufficient to let f+ (t ) =
1 E 2
(t ) and f− (t ) = 12 F (t ).
Remark 5.1. Theorem 4.1 means that no matter what the profile of the compactly supported initial datum u0 (x) is (no matter whether it is positive or negative), for any t > 0 in its lifespan, the solution u(x, t ) is positive at infinity and negative at negative infinity. Acknowledgments This work is partially supported by the Zhejiang Innovation Project (T200905) and the ZJNSF (Grant No. R6090109). References [1] D. Holm, M. Staley, Nonlinear balance and exchange of stability of dynamics of solitons, peakons, ramps/cliffs and leftons in a 1 + 1 nonlinear evolutionary PDE, Phys. Lett. A 308 (2003) 437–444. [2] Y. Zhou, On solutions to the Holm–Staley b-family of equations, Nonlinearity 23 (2010) 369–381. [3] R. Camassa, D. Holm, An integrable shallow water equation with peaked solitons, Phys. Rev. Lett. 71 (1993) 1661–1664. [4] A. Degasperis, M. Procesi, Asymptotic integrability, in: A. Degasperis, G. Gaeta (Eds.), Symmetry and Perturbation Theory, World Scientific, Singapore, 1999, pp. 23–37. [5] A. Constantin, J. Escher, Well-posedness, global existence and blow-up phenomena for a periodic quasilinear hyperbolic equation, Commun. Pure Appl. Math. 51 (1998) 475–504.
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