J. Korean Math. Soc. 45 (2008), No. 1, pp. 79–95
THE INITIAL-BOUNDARY-VALUE PROBLEM OF A GENERALIZED BOUSSINESQ EQUATION
ON THE HALF LINE
Ruying Xue
Reprinted from the
Journal of the Korean Mathematical Society Vol. 45, No. 1, January 2008
c
°2008 The Korean Mathematical Society
THE INITIAL-BOUNDARY-VALUE PROBLEM OF A GENERALIZED BOUSSINESQ EQUATION
ON THE HALF LINE
Ruying Xue
Abstract. The local existence of solutions for the initial-boundary value problem of a generalized Boussinesq equation on the half line is consid- ered. The approach consists of replacing the Fourier transform in the initial value problem by the Laplace transform and making use of mod- ern methods for the study of nonlinear dispersive wave equation
1. Introduction
We consider the initial-boundary value problem for the generalized Boussi- nesq equation on the half line
(1.1)
u tt − u xx + u xxxx + (|u| κ u) xx = 0, t > 0, x > 0, u(0, t) = h 1 (t), u x (0, t) = h 2 (t),
u(x, 0) = f (x), u t (x, 0) = ∂ x h(x),
where 0 < κ < 4, the velocity is an x-derivative function. Equations of type (1.1) are a class of essential model equations appearing in physics and fluid mechanics. It is derived by Boussinesq to describe two-dimensional irrotational flows of an inviscid liquid in a uniform rectangular channel. And it also arises in a large range of physical phenomena including the propagation of ion-sound waves in a plasma and nonlinear lattice wave.
The study of the initial-value problem for the Boussinesq-type equation has recently attracted considerable attention of many mathematicians and physi- cists ( See [1], [2] and references therein). For instance, Bona and Sachs in [2] proved that the initial-value problem of the Boussinesq equation is lo- cally well posed for smooth data by using Kato’s abstract theory of quasi- linear evolution equation. They proved that for any f (x) ∈ H s+2 (R) and h(x) ∈ H s+1 (R) with some s > 1/2, there exists a time T > 0 such that the initial-value problem of the Boussinesq equation has a unique solution u ∈ C([0, T ]; H s+2 (R)) ∩ C 1 ([0, T ]; H s (R)) ∩ C 2 ([0, T ]; H s−2 (R)). In the case
Received May 18, 2006; Revised September 26, 2006.
2000 Mathematics Subject Classification. 35Q35, 35G30.
Key words and phrases. Boussinesq equation, existence, initial-boundary-value problem.
Supported by NSFC (10571158) and Zhejiang Provincial NSF of China (Y605076).
c
°2008 The Korean Mathematical Society
79
1 < κ < 4, Linares in [8] established the local and global existence the- ory for the initial-value problem of the Boussinesq equation when (f, ∂ x h) ∈ L 2 (R)× ˙ H −1 (R) or (f, ∂ x h) ∈ H 1 (R)×L 2 (R), by the so-called L p −L q smooth- ing effect of the Strichartz type. In [12], Xue considered the case κ > 4 and proved some local and global existence results when the initial data belong to some suitable Besov spaces.
The practical, quantitative use of the Boussinesq equation and its rela- tives does not always involve the pure initial-value problem. Instead, initial- boundary value problems either on a finite domain or on the half line often come to the fore. The main difficulty in the study of initial-boundary-value problems is the evaluation of the contribution of the boundary data. In the literature, very few results are available. By using the finite element Galerkin method, Pani and Saranga in [10] got some local existence and uniqueness of the solu- tions of the initial-boundary-value problems of the Boussinesq equation on a finite domain with homogenous boundary conditions. In [11] Varlamov consid- ered the damped Boussinesq equation with the initial-boundary-value problem in a unit disk, and the global-in-time solvability was obtained by using the Fourier-Bessel series. As far as we know the existence of the initial-boundary- value problem of a generalized Boussinesq equation on the half line was not considered previously. In this paper we consider the local existence of the initial-boundary-value problem for the Boussinesq-type equations on the half line. The approach consists of replacing the Fourier transform in the initial- value problem by the Laplace transform and making use of modern methods for the study of nonlinear dispersive wave equation. The main result obtained in this paper is
Theorem 1.1. Assume that f (x)∈ L 2 (R + ), h(x)∈ H 0 −1 (R + ), h 1 (t)∈ H 014(R + ) and h 2 (t)∈ H − 012,−
14(R + ). Then there exists a positive constant T > 0, which depends only on
,−
14(R + ). Then there exists a positive constant T > 0, which depends only on
kf k L2(R
+) + khk H
−1(R
+) + kh 1 k
H
014(R
+) + kh 2 k
H
− 102,− 14(R
+) ,
such that the initial-boundary-value problem (1.1) possess a unique local solution u(t, x) satisfying
u ∈ C([0, T ]; L 2 x (R + )) ∩ L 4 t ([0, T ]; L ∞ x (R + )).
In the sequel, we denote by R + the open right half-line {x : x > 0} and
denote by C some large constant which may vary from line to line. The notation
A ∼ B means that there exist two harmless positive constants C 1 and C 2 such
that C 1 A ≤ B ≤ C 2 A. For a Banach space X, we denote by k · k X the norm
in X. We also denote by χ(x) the function satisfying χ(x) = 1 for x ∈ R + and
χ(x) = 0 for x 6∈ R + .
The rest of this paper is organized as follows. In section 2 we prove some smoothing effects for the linear Boussinesq equation with inhomogeneous initial- boundary data. The existence and the uniqueness of the solution is given in Section 3.
2. Linear estimates
In this section we give some smoothing effects for the linear equation asso- ciated to (1.1). These estimates will be the main ingredient in the proof of local existence of the initial-boundary-value problem (1.1). Consideration is first directed to the linear initial-boundary-value problem
(2.1)
u tt − u xx + u xxxx = 0, t > 0, x > 0, u(0, t) = h 1 (t), u x (0, t) = h 2 (t), u(x, 0) = 0, u t (x, 0) = 0.
Denote by
C 0 (R + ) = {u ∈ C(R) : u = 0 for x ≤ 0}.
Lemma 2.1. Assume that h 1 , h 2 ∈ C 0 (R + ). Then the solution, W b (t)(h 1 , h 2 ), of the linear problem (2.1) has an explicit formula
u(x, t) = W b (t)(h 1 , h 2 ) = U 1 (x, t) + U 2 (x, t) + U 1 (x, t) + U 2 (x, t), where
U 1 (x, t) = 1 2π
Z +∞
1
2µ 2 − 1 p µ 2 − 1(µ + i p
µ 2 − 1) e iµ
√ µ2−1t e −µx µZ +∞
0
³ i p
µ 2 − 1h 1 (ξ) − h 2 (ξ)
´ e −iµ
√ µ2−1ξ dξ
¶ dµ,
U 2 (x, t) = − 1 2π
Z +∞
1
2µ 2 − 1 p µ 2 − 1(µ + i p
µ 2 − 1) e iµ √
µ
2−1t e i √
µ
2−1x
µZ +∞
0
(µh 1 (ξ) + h 2 (ξ)) e −iµ √
µ
2−1ξ dξ
¶ dµ.
Proof. As a potential global solution of (2.1) is defined on a half-line R + in each of the two independent variables x and t, it is not unnatural to think of replacing the use of the Fourier transform with the Laplace transform. By taking the Laplace transform with respect to t of both sides of the equation in (2.1), the initial-boundary-value problem is converted to a one-parameter family of four-order, boundary-value problems
(2.2)
½ λ 2 u(x, λ) − ˆ ˆ u(x, λ) xx + ˆ u(x, λ) xxxx = 0, Re(λ) ≥ 0, x > 0, ˆ
u(0, λ) = ˆh 1 (λ), ˆ u x (0, λ) = ˆh 2 (λ), ˆ u(+∞, λ) = 0, ˆ u x (+∞, λ) = 0,
where λ is the dual variable, ˆ u(x, λ), ˆh 1 (λ) and ˆh 2 (λ) are the Laplace transform
of u(x, t), h 1 (t) and h 2 (t) with respect to t, respectively. Let γ 1A , γ 2A , γ 3A and
γ 4A be the four roots of the characteristic equation
γ 4 − γ 2 + λ 2 = 0, λ ∈ A = {λ : Re(λ) > 1/2},
ordered so that Re(γ 1A ) < 0, Re(γ 2A ) < 0, Re(γ 3A ) > 0 and Re(γ 4A ) > 0.
It is obvious that γ 1A , γ 2A , γ 3A and γ 4A are analytic for Re(λ) > 1/2 and continuous for Re(λ) ≥ 1/2 except at λ = 1/2. As both ˆ u(x, λ) and ˆ u x (x, λ) tend to zero as x → +∞, it is concluded that for any λ with Re(λ) > 1/2
ˆ
u(x, λ) = 1 γ 2A − γ 1A
h
(γ 2A ˆh 1 (λ) − ˆh 2 (λ))e γ1Ax − (γ 1A ˆh 1 (λ) − ˆh 2 (λ))e γ
2Ax i
. Thus, for any fixed p with Re(p) > 1/2, one has the representation for x > 0 and t > 0,
u(x, t) = 1 2πi
Z p+i∞
p−i∞
e λt u(x, λ)dλ ˆ
= 1
2πi Z p+i∞
p−i∞
e λt γ 2A − γ 1A
h
(γ 2A ˆh 1 (λ) − ˆh 2 (λ))e γ1Ax (2.3)
−(γ 1A ˆh 1 (λ) − ˆh 2 (λ))e γ2Ax i dλ.
A little analysis shows that
γ 1A (λ) = γ 2A (¯ λ), γ 3A (λ) = γ 4A (¯ λ) for Re(λ) ≥ 1/2, λ 6= 1/2, and
|γ 1A (λ) − γ 2A (λ)| = O(|λ − 1/2| 1/2 ) as λ → 1/2, Re(λ) ≥ 1/2.
As this singularity is integrable, we may let p → 1/2 in (2.3), thereby obtaining for x > 0 and t > 0,
u(x, t) = 1 2πi
Z
12
+i∞
12
−i∞
e λt γ 2A − γ 1A
h
(γ 2A ˆh 1 (λ) − ˆh 2 (λ))e γ1Ax (2.4)
−(γ 1A ˆh 1 (λ) − ˆh 2 (λ))e γ2Ax i dλ.
Let γ 1B , γ 2B , γ 3B and γ 4B be the four roots of the characteristic equation γ 4 − γ 2 + λ 2 = 0, λ ∈ B = {λ : 0 < Re(λ) < 1/2},
ordered so that Re(γ 1B ) < 0, Re(γ 2B ) < 0, Re(γ 3B ) > 0 and Re(γ 4B ) > 0. It is obvious that γ 1B , γ 2B , γ 3B and γ 4B are analytic for λ ∈ B and continuous for 0 ≤ Re(λ) ≤ 1/2 except at λ = 1/2 and λ = 0. By the uniqueness and the continuity of the root of the characteristic equation γ 4 − γ 2 +λ 2 = 0 on the half lines Γ + = {λ : Re(λ) = 1/2, Im(λ) > 0} and Γ − = {λ : Re(λ) = 1/2, Im(λ) <
0}, we assume, without loss of generality,
γ 1B = γ 1A , γ 2B = γ 2A , λ ∈ Γ + . Then we have
γ 1B = γ 1A , γ 2B = γ 2A , λ ∈ Γ − ,
or
γ 1B = γ 2A , γ 2B = γ 1A , λ ∈ Γ − . By symmetry we deduce from (2.4) that
u(x, t) = 1 2πi
Z
12
+i∞
1 2
−i∞
e λt γ 2B − γ 1B
h
(γ 2B ˆh 1 (λ) − ˆh 2 (λ))e γ1Bx (2.5)
−(γ 1B ˆh 1 (λ) − ˆh 2 (λ))e γ2Bx i
dλ.
A little analysis shows that
γ 1B (λ) = γ 1B (¯ λ), γ 2B (λ) = γ 2B (¯ λ) for 0 < Re(λ) < 1/2
|γ 1B (λ) − γ 2B (λ)| = O(|λ − 1/2| 1/2 ), as λ → 1/2, 0 < Re(λ) ≤ 1/2,
|γ 1B (λ) − γ 2B (λ)| = O(1), as λ → 0, 0 ≤ Re(λ) < 1/2, and for λ ∈ B, |λ| → +∞,
|γ 1B (λ)| ∼ |λ| 1/2 , |γ 2B (λ)| ∼ |λ| 1/2 , Re(γ 1B (λ)) ∼ −|λ| 1/2 , Re(γ 2B (λ)) ∼ −|λ| 1/2 .
Hence, we are allowed to change the contour on the basis of Cauchy’s Theorem and thereby determine from (2.5) that
u(x, t) = 1 2πi
Z 0+i∞
0−i∞
e λt γ 2B − γ 1B
h
(γ 2B ˆh 1 (λ) − ˆh 2 (λ))e γ1Bx (2.6)
−(γ 1B ˆh 1 (λ) − ˆh 2 (λ))e γ2Bx i dλ.
Denote by
U 1 (x, t) = 1 2πi
Z 0+i∞
0+i0
e λt
γ 2B − γ 1B (γ 2B ˆh 1 (λ) − ˆh 2 (λ))e γ1Bx dλ, U 2 (x, t) = − 1
2πi Z 0+i∞
0+i0
e λt
γ 2B − γ 1B (γ 1B ˆh 1 (λ) − ˆh 2 (λ))e γ2Bx dλ.
Note that
γ 1B (λ) = γ 1B (¯ λ), γ 2B (λ) = γ 2B (¯ λ) for 0 ≤ Re(λ) ≤ 1/2 with λ 6= 0, λ 6= 1 2 and
ˆh 1 (λ) = ˆh 1 (¯ λ), ˆh 2 (λ) = ˆh 2 (¯ λ) for 0 ≤ Re(λ) ≤ 1/2 with λ 6= 0, λ 6= 1 2 . By direct computation, it follows that for x > 0 and t > 0
1 2πi
Z 0+i0
0−i∞
e λt γ 2B − γ 1B
(γ 2B ˆh 1 (λ) − ˆh 2 (λ))e γ1Bx dλ = U 1 (x, t) and
− 1 2πi
Z 0+i0
0−i∞
e λt
γ 2B − γ 1B (γ 1B ˆh 1 (λ) − ˆh 2 (λ))e γ2Bx dλ = U 2 (x, t).
Then we get for x > 0 and t > 0
(2.7) u(x, t) = W b (t)(h 1 , h 2 ) = U 1 (x, t) + U 2 (x, t) + U 1 (x, t) + U 2 (x, t).
For λ ∈ {λ : Re(λ) = 0, Im(λ) > 0}, it is convenient to make the change of variables
λ = iµ p
µ 2 − 1 for µ ≥ 1
in the characteristic equation γ 4 − γ 2 + λ 2 = 0. In terms of µ, the four roots are
γ 1B = −µ, γ 2B = i p
µ 2 − 1, γ 3B = µ and γ 4B = −i p µ 2 − 1, and the integral U 1 (x, t) and U 2 (x, t) may be rewritten as
U 1 (x, t) = 1 2π
Z +∞
1
2µ 2 − 1 p µ 2 − 1(µ + i p
µ 2 − 1) e iµ √
µ
2−1t e −µx µZ +∞
0
³ i p
µ 2 − 1h 1 (ξ) − h 2 (ξ) ´ e −iµ √
µ
2−1ξ dξ
¶ dµ,
U 2 (x, t) = − 1 2π
Z +∞
1
2µ 2 − 1 p µ 2 − 1(µ + i p
µ 2 − 1) e iµ √
µ
2−1t e i √
µ
2−1x
µZ +∞
0
(µh 1 (ξ) + h 2 (ξ)) e −iµ √
µ
2−1ξ dξ
¶ dµ.
We complete the proof. ¤
For α, β ∈ R we define
H α,β (R) = {f : |ξ| α (1 + |ξ|) β−α f (ξ) ∈ L ˆ 2 (R)}
with
kf k Hα,β(R) =
° °
°|ξ| α (1 + |ξ|) β−α f (ξ) ˆ
° °
° L2(R) , where ˆ f is the Fourier transform in x of the function f (x). Let
H α,β 0 (R + ) = {f ∈ H α,β (R) : suppf ⊆ [0, ∞)}
with
kf k Hα,β
0
(R
+) = kf k H
α,β(R) , and let
H α,β (R + ) = {f = F | R+, F ∈ H α,β (R)}
with
kf k Hα,β(R
+) = inf{kF k H
α,β(R) , f = F | R
+}.
Denote by
H 0 β (R + ) = H 0,β 0 (R + ), H β (R + ) = H 0,β (R + ) and
H ˙ 0 α (R + ) = H 0 α,0 (R + ), ˙ H α (R + ) = H α,0 (R + ).
For any α and β with α ≤ 0 and α ≤ β, we have
(2.8) kf k Hα,β(R) ∼ kf k H ˙
α(R) + kf k H
β(R)
because of
|ξ| α (1 + |ξ|) β−α ∼ |ξ| α + (1 + |ξ|) β .
Lemma 2.2. Assume α, β and f satisfy one of the following conditions:
• α ∈ (− 1 2 , 0] and β ∈ (− 1 2 , 1 2 ) with α ≤ β, and f ∈ H α,β (R);
• α ∈ (− 1 2 , 0] and β ∈ ( 1 2 , 3 2 ), f ∈ H α,β (R) and f (0) = 0.
Then χ(x)f (x) ∈ H α,β 0 (R + ), and kχ(x)f (x)k Hα,β
0
(R
+) ≤ Ckf k H
α,β(R) .
Proof. For 0 ≤ β < 1 2 and f 1 (x) ∈ H β (R), or for 1 2 < β < 3 2 and f 1 (x) ∈ H β (R) with f (0) = 0, that χ(x)f 1 (x) ∈ H 0 β (R + ) and
(2.9) kχ(x)f 1 (x)k Hβ
0
(R
+) ≤ Ckf 1 (x)k H
β(R)
comes from Lemma 2.3 and Proposition 2.4 in [4].
Note that H 0 β (R + ) is the dual space of H −β (R + ) for β < 0 ( see Proposition 2.1 in [4]). For any g(x) ∈ H −β (R + ), we can choose F ∈ H −β (R) with g = F | R+ and kgk H−β(R
+) ∼ kF k H
−β(R) . Thus, for − 1 2 < β < 0 and f 1 (x) ∈ H β (R) we have the following chain of inequalities
(R
+) ∼ kF k H
−β(R) . Thus, for − 1 2 < β < 0 and f 1 (x) ∈ H β (R) we have the following chain of inequalities
|hχ(x)f 1 (x), g(x)i| ≤ |hf 1 (x), χ(x)F (x)i|
≤ kf 1 (x)k Hβ(R) kχ(x)F (x)k H
−β
0
(R) ≤ Ckf 1 (x)k H
β(R) kχ(x)F (x)k H
−β 0(R
+)
≤ Ckf 1 (x)k Hβ(R) kF (x)k H
−β(R) ≤ Ckf 1 (x)k H
β(R) kg(x)k H
−β(R
+) ,
the last two inequalities hold because of Lemma 2.3 in [4]. Then, χ(x)f 1 (x) ∈ H 0 β (R + ) and
(2.10) kχ(x)f 1 (x)k Hβ
0
(R
+) ≤ Ckf 1 (x)k H
β(R) . For − 1 2 < α ≤ 0 and f 2 ∈ ˙ H α (R), we have
kf 2 k Hα(R) = k(1 + |ξ|) α f ˆ 2 (ξ)k L
2
ξ
(R) ≤ k |ξ| α f ˆ 2 (ξ)k L
2ξ
(R) = kf 2 k H ˙
α(R) , where ˆ f 2 (ξ) is the Fourier transform with respective to x of the function f 2 (x).
The similar argument to that used in (2.10) yields χ(x)f 2 (x) ∈ H 0 α (R + ) and kχ(x)f 2 (x)k H0α(R
+) ≤ Ckf 2 k H
α(R) ≤ Ckf 2 k H ˙
α(R) ,
which, together with Proposition 2.8 in [4], implies χ(x)f 2 (x) ∈ ˙ H 0 α (R + ) and (2.11) kχ(x)f 2 (x)k H ˙α0(R
+) ≤ Ckχ(x)f 2 (x)k H
0α(R
+) ≤ Ckf 2 k H ˙
α(R) . Then the lemma follows from a combination of (2.9), (2.10) and (2.11) with
(2.8). The proof is completed. ¤
Lemma 2.3. There exists a positive constant C such that, for h 1 ∈ H 014(R + ) and h 2 ∈ H − 012,−
14(R + ),
,−
14(R + ),
sup
t≥0 kW b (t)(h 1 , h 2 )k L
2x(R
+) ≤ C µ
kh 1 k
H
014(R
+) + kh 2 k
H
− 102,− 14(R
+)
¶ .
Proof. It suffices to prove the lemma for h 1 , h 2 ∈ C 0 ∞ (R + ). It follows from Lemma 3.1 in [3] that
(2.12)
kU 1 (x, t)k L2x(R
+)
≤ C
° °
° °
° µ − i p
µ 2 − 1 p µ 2 − 1 e iµ
√ µ2−1t
×
µZ +∞
0
(i p
µ 2 − 1h 1 (ξ) − h 2 (ξ))e −iµ √
µ
2−1ξ dξ
¶° °
° °
L
2µ(1,+∞)
≤ C
° °
° °
p 2µ 2 − 1 Z +∞
0
h 1 (ξ)e −iµ
√ µ2−1ξ dξ
° °
° °
L
2µ(1,+∞)
+ C
° °
° °
°
p 2µ 2 − 1 p µ 2 − 1
Z +∞
0
h 2 (ξ)e −iµ √
µ
2−1ξ dξ
° °
° °
° L2µ(1,+∞)
≤ C
° °
° °(1 + η)
1 4
Z +∞
0
h 1 (ξ)e −iηξ dξ
° °
° °
L
2η(0,+∞)
+ C
° °
° °η −
1
2
(1 + η) −34
Z +∞
0
h 2 (ξ)e −iηξ dξ
° °
° °
L
2η(0,+∞)
≤ C µ
kh 1 k
H
014(R
+) + kh 2 k
H
− 102,− 14(R
+)
¶ .
Note that for U (x) =
Z ∞
1
g(µ)e i √
µ
2−1x dµ = Z ∞
0
g(µ(s)) s
µ(s) e isx ds where µ(s) ≥ 0 is the solution satisfying s = p
µ 2 − 1 for s ≥ 0, we have kU (x)k L2x(0,∞) = kg(µ(s)) s
µ(s) k L2s(0,∞) = kg(µ)(µ 2 − 1)
14µ −12k L2µ(1,∞) . Then we have
(1,∞) . Then we have
(2.13)
kU 2 (x, t)k L2x(R
+)
≤ C
° °
° °µ
12
p 2µ 2 − 1(µ 2 − 1) −14
Z +∞
0
h 1 (ξ)e −iµ √
µ
2−1ξ dξ
° °
° °
L
2µ(1,+∞)
+ C
° °
° °µ −
1 2
p 2µ 2 − 1(µ 2 − 1) −14
Z +∞
0
h 2 (ξ)e −iµ √
µ
2−1ξ dξ
° °
° °
L
2µ(1,+∞)
≤ C
° °
° °(1 + η)
1 4
Z +∞
0
h 1 (ξ)e −iηξ dξ
° °
° °
L
2η(0,+∞)
+ C
° °
° °(1 + η) −
1 4
Z +∞
0
h 2 (ξ)e −iηξ dξ
° °
° °
L
2η(0,+∞)
≤ Ckh 1 k
H
014(R
+) + Ckh 2 k
H
0− 14(R
+) .
The lemma now follows from (2.12) and (2.13) together with Lemma 2.1. We
complete the proof. ¤
Lemma 2.4. There exists a positive constant C such that, for h 1 ∈ H 014(R + ) and h 2 ∈ H 0 −14(R + ),
(R + ),
µZ ∞
0
kW b (t)(h 1 , h 2 )k 4 L∞
x(R
+) dt
¶
14
≤ C µ
kh 1 k
H
014(R
+) + kh 2 k
H
0− 14(R
+)
¶ . Proof. For given real functions K ∈ C(R) and h ∈ C 0 (R + ) satisfying K(−µ) = K(µ), we define
G(K, h) = Z +∞
1
K(µ)e −iµ
√ µ2−1t e −|µ|x
µZ +∞
0
h(ξ)e iµ
√ µ2−1ξ dξ
¶ dµ and
H(K, h) = Z +∞
1
K(µ)e −iµ
√ µ2−1t e iµ √
1−(1/µ)
2x
µZ +∞
0
h(ξ)e iµ
√ µ2−1ξ dξ
¶ dµ.
Then
G(K, h) + G(K, h)
= Z
|µ|>1
K(µ)e −iµ √
µ
2−1t e −|µ|x µZ +∞
0
h(ξ)e iµ √
µ
2−1ξ dξ
¶ dµ
=
Z +∞
−∞
K(ϕ −1 (η)) dϕ −1 (η)
dη e iηt e −|ϕ−1(η)|x
µZ +∞
0
h(ξ)e −iηξ dξ
¶ dη, and similarly,
H(K, h) + H(K, h)
= Z +∞
−∞
K(ϕ −1 (η)) dϕ −1 (η)
dη e iηt e −iϕ−1(η) √
1−(1/ϕ
−1(η))
2x
µZ +∞
0
h(ξ)e −iηξ dξ
¶ dη, where, µ = ϕ −1 (η) is the inverse function of η = ϕ(µ) = µ p
µ 2 − 1. For any g(x, t) ∈ L t43(R, L 1 x (R + )), denoting by
ˆ
g(x, −η) = 1 2π
Z +∞
−∞
g(x, t)e itη dt, ˆh(η) = Z +∞
0
h(ξ)e −iηξ dξ,
we deduce by H¨ older’s inequality and the Sobolev embedding theorem Z +∞
−∞
Z +∞
0
[G(K, h) + G(K, h)]g(x, t)dxdt
= 2π Z +∞
−∞
Z +∞
−∞
K(ϕ −1 (η)) dϕ −1 (η)
dη e −|ϕ−1(η)|x ˆ g(x, −η)ˆh(η)dηdx
≤ C Z +∞
−∞
¯ ¯
¯ ¯(1 + |η|)
1
4
K(ϕ −1 (η)) dϕ −1 (η) dη ˆh(η)
¯ ¯
¯ ¯
° °
° ° ˆ g(x, −η) (1 + |η|)
14° °
° °
L
1x(R)
dη
≤ C
° °
° °(1 + |η|)
1
4
K(ϕ −1 (η)) dϕ −1 (η) dη ˆh(η)
° °
° °
L
2η(R)
kg(x, t)k
H
− 14(R,L
1x(R
+))
≤ C
° °
° °(1 + |η|)
1
4
K(ϕ −1 (η)) dϕ −1 (η) dη ˆh(η)
° °
° °
L
2η(R)
kg(x, t)k
L
t43(R,L
1x(R
+)) , which implies that
kG(K, h) + G(K, h)k L4
t
(R
+,L
∞x(R
+))
≤ kG(K, h) + G(K, h)k L4
t
(R,L
∞x(R
+))
≤ C
° °
° °(1 + |η|)
14
K(ϕ −1 (η)) dϕ −1 (η) dη ˆh(η)
° °
° °
L
2η(R)
. (2.14)
Similarly,
(2.15)
kH(K, h) + H(K, h)k L4
t
(R
+,L
∞x(R
+))
≤ C
° °
° °(1 + |η|)
14
K(ϕ −1 (η)) dϕ −1 (η) dη ˆh(η)
° °
° °
L
2η(R)
.
Rewrite U 1 (x, t) and U 2 (x, t) as U 1 (x, t) = i
2π G(µ, h 1 )+ 1 2π G( p
µ 2 − 1, h 1 )− 1
2π G( µ
p µ 2 − 1 , h 2 )+ i
2π G(1, h 2 ), and
U 2 (x, t) = − 1
2π H( µ 2
p µ 2 − 1 , h 1 )+ i
2π H(µ, h 1 )− 1
2π H( µ
p µ 2 − 1 ,h 2 )+ i
2π H(1,h 2 ).
Then we get from (2.14) that kU 1 (x, t) + U 1 (x, t)k L4
t
(R
+,L
∞x(R
+))
≤ C ³
kη(1 + |η|) −34ˆh 1 (η)k L2η(R) + kη 2 (1 + |η|) −
74ˆh 1 (η)k L2η(R) ´ +C ³
(R) + kη 2 (1 + |η|) −
74ˆh 1 (η)k L2η(R) ´ +C ³
k(1 + |η|) −14ˆh 2 (η)k L2η(R) + kη(1 + |η|) −
54ˆh 2 (η)k L2η(R) ´
(R) + kη(1 + |η|) −
54ˆh 2 (η)k L2η(R) ´
≤ C µ
kh 1 k
H
014(R
+) + kh 2 k
H
0− 14(R
+)
¶
,
(2.16)
and from (2.15),
(2.17) kU 2 (x, t)+U 2 (x, t)k L4
t
(R
+,L
∞x(R
+)) ≤ C µ
kh 1 k
H
014(R
+) + kh 2 k
H
0− 14(R
+)
¶ . Then the lemma follows from (2.16) and (2.17) together with Lemma 2.1. We
complete the proof. ¤
Let φ(ξ) = ξ(1 + |ξ| 2 ) 1/2 . For f, h ∈ S 0 (R) define
(2.18) V (t)(f ) =
Z +∞
−∞
e itφ(ξ) e ixξ f (ξ)dξ. ˆ
(2.19) V 1 (t)(f )) = 1 2
Z +∞
−∞
[e itφ(ξ)+ixξ + e −itφ(ξ)+ixξ ] ˆ f (ξ)dξ and
(2.20) V 2 (t)(∂ x h) = Z +∞
−∞
h
A(ξ)e i(−tφ(ξ)+xξ) + B(ξ)e i(tφ(ξ)+xξ) i dξ, where A(ξ) = 2(1+ξ ˆ h(ξ)2)
1/2 and B(ξ) = − 2(1+ξ h(ξ) ˆ 2)
1/2, ˆ f and ˆh are the Fourier transform of f and h respectively. Denote by
)
1/2, ˆ f and ˆh are the Fourier transform of f and h respectively. Denote by
W R (t)(f, ∂ x h) = V 1 (t)(f ) + V 2 (t)(∂ x h).
Then u(x, t) = W R (t)(f, ∂ x h) is the formal solution to the initial-value problem (2.21)
½ u tt − u xx + u xxxx = 0, t > 0, x ∈ R, u(x, 0) = f (x), u t (x, 0) = ∂ x h.
Lemma 2.5. Let T > 0. There exists a positive constant C such that, for f ∈ L 2 (R) and h ∈ H 0 −1 (R) with h(x) = −h(−x),
kχ(t)W R (t)(f, ∂ x h)| x=0 k
H
014(R
+) ≤ C ³
kf k L2(R) + khk H
−1
0
(R)
´ , kχ(t)∂ x W R (t)(f, ∂ x h)| x=0 k
H
− 102,− 14(R
+) ≤ C ³
kf k L2(R) + khk H
−1
0
(R)
´
and ÃZ T
0
kW R (τ )(f, ∂ x h)k 4 L∞
x(R
+) dτ
!
14
≤ C(1 + T
14) ³
kf k L2(R) + khk H
−1
0 (R)
´ . Proof. It suffices to prove the lemma for f, h ∈ C 0 ∞ (R) with f (0) = 0 and h(x) = −h(−x). The results in [2] show that u(x, t) = W R (t)(f, ∂ x h) is the classical solution of the initial-value problem
½ ∂ tt u − ∂ xx u + ∂ xxxx u = 0, −∞ < x < +∞, t > 0 u(x, 0) = f (x), ∂ t u(x, 0) = ∂ x h(x), −∞ < x < +∞,
and W R (t)(f, ∂ x h) ∈ C 2 (R × R) with W R (t)(f, ∂ x h)| (x,t)=(0,0) = f (0) = 0.
For given α, β ∈ R, sup
x∈R kV (t)(f )k H
α,β(R)
= °
°|τ| α (1 + |τ |) β−α F t→τ (V (t)(f )) (τ ) °
° L2τ(R)
≤ C
° °
°|τ | α (1 + |τ |) β−α f (ξ) |φ ˆ 0 (ξ)| −1 | ξ=φ−1(τ )
° °
° L2τ(R)
≤ C
° °
°|φ(ξ)| α (1 + |φ(ξ)|) β−α f (ξ) |φ ˆ 0 (ξ)| −12
° °
° L2ξ(R)
≤ C
° °
°|ξ| α (1 + |ξ|) 2β−α−12f (ξ) ˆ
° °
° L2ξ(R) = C kf k
H
α,2β− 10 2(R) , which, together with (2.19) and (2.20), implies
sup
x∈R
kW R (t)(f, ∂ x h)k
H
14(R) ≤ C ³
kf k L2(R
+) + khk H
−1
0
(R
+)
´ .
Then, χ(t)W R (t)(f, ∂ x h)| x=0 ∈ H 014(R + ) because of Lemma 2.2, and the first inequality in the lemma holds. To prove the second inequality in the lemma, we define
v(x, t) = Z t
0
χ(τ )∂ x W R (τ )(f, ∂ x h)dτ, (x, t) ∈ R × R.
Obviously v(0, t) ∈ C 0 (R + ), dv(x,t) dt = χ(t)∂ x W R (t)(f, ∂ x h), and v(x, t) solves the initial-value problem
½ ∂ tt v − ∂ xx v + ∂ xxxx v = ∂ xx h(x), x ∈ R, t ∈ R + , v(x, 0) = 0, ∂ t v(x, 0) = ∂ x f (x).
By Duhamel’s principle we can rewrite v(x, t) as
v(x, t) = V 2 (t)(∂ x f (x)) + Z t
0
V 2 (t − τ )(∂ xx h(x))dτ, t > 0.
Thus, for t ≥ 0, v(0, t)
= V 2 (t)(∂ x f )| x=0 + Z t
0
V 2 (t − τ )(∂ xx h)| x=0 dτ
= V 2 (t)(∂ x f )| x=0 + Z t
0
Z +∞
−∞
iξsgn(ξ)ˆh(ξ) 2(1 + ξ 2 )
12×
³
e −itφ(ξ)+iτ φ(ξ) − e itφ(ξ)−iτ φ(ξ) ´
dξdτ
= V 2 (t)(∂ x f )| x=0 + Z +∞
−∞
ˆh(ξ) 2(1 + ξ 2 )
³
2 − e itφ(ξ) − e −itφ(ξ)
´ dξ
= V 2 (t)(∂ x f )| x=0 + Z +∞
−∞
ˆh(ξ)
1 + ξ 2 dξ − 1 2
Z +∞
−∞
ˆh(ξ) 1 + ξ 2
³
e itφ(ξ) + e −itφ(ξ)
´ dξ
= V 2 (t)(∂ x f )| x=0 − 1
2 V (t)(g)| x=0 − 1
2 V (−t)(g)| x=0 , with g(x) = R +∞
−∞
ˆ h(ξ)
1+ξ
2e ixξ dξ, the last inequality holds because of ˆh(−ξ) = ˆh(−ξ). Denote by
J(t) = V 2 (t)(∂ x f )| x=0 − 1
2 V (t)(g)| x=0 − 1
2 V (−t)(g)| x=0 .
It follows from the similar argument to that used in the proof of the first inequality in the lemma that J(t) ∈ H
34(R) and
kJ(t)k
H
34(R) ≤ C ³
kf k L2(R) + khk H
−1
0 (R)
´ .
Note that χ(t)J(t) = v(0, t) and J(0) = v(0, 0) = 0. Lemma 2.2 implies v(0, t) = χ(t)J(t) ∈ H 034(R + ) and
(2.22) kv(0, t)k
H
034(R
+) ≤ C ³
kf k L2(R) + khk H
−1
0 (R)
´ . Then
kχ(t)∂ x W R (t)(f, ∂ x h)| x=0 k
H
− 102,− 14(R
+) =
° °
° ° dv(0, t) dt
° °
° °
H
− 102,− 14(R
+)
≤ kv(0, t)k
H
034(R
+) ≤ C
³
kf k L2(R) + khk H
−1
0
(R)
´ .
The second inequality in the lemma is proved. The last inequality in the lemma comes from the results in [8], the proof is omitted. ¤ For any f ∈ L 2 (R + ) and h ∈ H 0 −1 (R + ) we define ( ˜ f (x), ˜h(x)) = (f (x), h(x)) for x ≥ 0 and ( ˜ f (x), ˜h(x)) = (0, −h(−x)) for x < 0, and define
W C (t)(f, ∂ x h) = W R (t)( ˜ f , ∂ x ˜h) − W b (χ(t)g 1 (t), χ(t)g 2 (t)), where
g 1 (t) = W R (t)( ˜ f , ∂ x ˜h)| x=0 , g 2 (t) = ∂ x W R (t)( ˜ f , ∂ x ˜h)| x=0
are the trace of W R (t)( ˜ f , ∂ x ˜h) and ∂ x W R (t)( ˜ f , ∂ x ˜h) at x = 0, respectively.
Lemma 2.3 and Lemma 2.5 mean W C (t)(f, ∂ x h) is well-defined and solves the initial-boundary-value problem
(2.23)
u tt − u xx + u xxxx = 0, t > 0, x > 0, u(0, t) = 0, u x (0, t) = 0,
u(x, 0) = f (x), u t (x, 0) = ∂ x h(x).
The following lemma comes from a combination of Lemma 2.3 and Lemma 2.4
with Lemma 2.5.
Lemma 2.6. There exists a positive constant C such that, for f ∈ L 2 (R + ) and h ∈ H 0 −1 (R + ),
sup
t≥0 kW C (t)(f, ∂ x h)k L
2x
(R
+) ≤ C
³
kf k L2(R
+) + khk H
−1
0
(R
+)
´ , ÃZ T
0
kW C (t)(f, ∂ x h)dtk 4 L∞
x(R
+)
!
14
≤ C(1 + T
14) ³
kf k L2(R
+) + khk H
−1
0
(R
+)
´ . Lemma 2.7. Let T > 0 and let g(x, t) ∈ L 1 ([0, T ], L 2 x (R + )). Then the linear initial-boundary-value problem
(2.24)
u tt − u xx + u xxxx = ∂ xx g, t > 0, x > 0, u(0, t) = 0, u x (0, t) = 0,
u(x, 0) = 0, u t (x, 0) = 0,
has a solution W I (t)(g) ∈ C([0, T ], L 2 x (R + )) ∩ L 4 t ([0, T ], L ∞ x (R + )) such that sup
0≤t≤T
kW I (t)(g)k L2
x
(R
+) ≤ Ckgk L
1t
([0,T ],L
2x(R
+))
and ÃZ T
0
kW I (t)(g)k 4 L∞
x(R
+) dt
!
14
≤ C(1 + T
14)kgk L1t([0,T ],L
2x(R
+)) .
Proof. Choose g n (x, t) ∈ C([0, T ], C 0 ∞ (R + )) such that g n → g in L 1 ([0, T ], L 2 x (R + )) as n → +∞. It follows from Duhamel’s principle that
u n (x, t) = Z t
0
W C (t − τ )(0, ∂ xx g n (x, τ ))dτ
is the solution to the initial-boundary-value problem (2.24) replacing g by g n . By Lemma 2.6,
(2.25) sup
0≤t≤T ku n k L
2x(R
+) ≤ Z T
0
kg n (x, τ )k L2x(R
+) dτ, and
(2.26)
ÃZ T
0
ku n k 4 L∞
x(R
+) dt
!
14
≤ C(1 + T
14)kgk L1
t
([0,T ],L
2x(R
+))
and
(2.27) sup
0≤t≤T
ku n − u m k L2x(R
+) + ÃZ T
0
ku n − u m k 4 L∞
x(R
+) dt
!
14
≤ C(1 + T
14)kg n − g m k L1
t
([0,T ],L
2x(R
+)) . Then u n (x, t) is a convergent sequence in
C([0, T ], L 2 x (R + )) ∩ L 4 t ([0, T ], L ∞ x (R + ))
because of (2.27). Let W I (t)(g) = lim n→+∞ u n (x, t). Obviously W I (t)(g) is a solution of (2.24). Taking n → +∞ in (2.25) and (2.26) we obtain W I (t)(g)
satisfies the estimates in the lemma. ¤
3. The local existence of solutions
In this section we give the proof of Theorem 1.1. To prove the local exis- tence we are going to use a contraction mapping argument. For some positive constant δ > 0 and T > 0 determined below, we define the set Z T δ by
Z T δ =
½ u ∈ C([0, T ]; L 2 x (R + )) ∩ L 4 t ([0, T ]; L ∞ x (R + )) with sup t∈[0,T ] ku(·, t)k L2(R
+) + kuk L
4
t
([0,T ];L
∞x(R
+)) ≤ δ
¾ .
Let X be the product space
L 2 (R + ) × H 0 −1 (R + ) × H 014(R + ) × H − 012,−
14(R + ) with the norm
,−
14(R + ) with the norm
k(f, h, h 1 , h 2 )k X
= kf (x)k L2(R
+) + kh(x)k H
−1
0
(R
+) + kh 1 (t)k
H
014(R
+) + kh 2 (t)k
H
− 102,− 14(R
+) . For (f, h, h 1 , h 2 ) ∈ X and u ∈ Z T δ we define a mapping Φ(u) by
Φ(u) = W C (t)(f, ∂ x h) + W b (t)(h 1 , h 2 ) − W I (t)((|u| κ u(τ )) xx )dτ.
We only need to prove that Φ(u) is a contraction mapping from Z T δ into Z T δ for suitable δ > 0 and T > 0. Denote by δ 0 = k(f, h, h 1 , h 2 )k X and denote by
k|u|k T = sup
0≤t≤T
kuk L2
x(R
+) +
ÃZ T
0
ku(x, t)k 4 L∞
x(R
+) dt
!
14
.
For u, v ∈ Z T δ , it follows from Lemma 2.3, Lemma 2.4, Lemma 2.6 and Lemma 2.7 that
k|Φ(u)|k T
≤ C(1 + T
14) Ã
δ 0 + Z T
0
° ° |u(τ)| κ+1 °
° L2x(R
+) dτ
!
≤ C(1 + T
14) Ã
δ 0 + T
4−κ4sup
t∈[0,T ]
kuk L2x(R
+) k|u|k κ T
! (3.1)
≤ C(1 + T
14)
³
δ 0 + T
4−κ4δ κ+1
´
,
and (3.2)
k|Φ(u) − Φ(v)|k T
≤ C(1 + T
14) Z T
0
k|u(τ )| κ u(τ ) − |v(τ )| κ v(τ )k L2
x(R
+) dτ
≤ C(1 + T
14) Z T
0
³
ku(τ )k κ L∞
x