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Research Article

On properties of solutions to the improved modified Boussinesq equation

Yuzhu Wang, Yinxia Wang

School of Mathematics and Information Sciences, North China University of Water Resources and Electric Power, Zhengzhou 450011, China.

Communicated by X. Qin

Abstract

In this paper, we investigate the Cauchy problem for the generalized IBq equation with damping in one dimensional space. When σ = 1, the nonlinear approximation of the global solutions is established under small condition on the initial value. Moreover, we show that as time tends to infinity, the solution is asymptotic to the superposition of nonlinear diffusion waves which are given explicitly in terms of the self- similar solution of the viscous Burgers equation. Whenσ ≥2, we prove that our global solution converges to the superposition of diffusion waves which are given explicitly in terms of the solution of linear parabolic equation. c2016 all rights reserved.

Keywords: IMBq equation with damping, large time behavior, diffusion waves.

2010 MSC: 35L30, 35L75.

1. Introduction

We investigate the Cauchy problem for the following generalized improved modified Boussinesq (IBq) equation with damping in one space dimension

utt−uxxtt−uxx−νuxxt=φ(u)xx (1.1) with the initial value

t= 0 :u=f(x), ut=∂xg(x). (1.2)

Corresponding author

Email addresses: [email protected](Yuzhu Wang),[email protected](Yinxia Wang) Received 2016-03-07

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Hereu=u(x, t) is the unknown function ofx∈Rand t >0,ν >0 is a constant. The nonlinear term is as form ofφ(u) =O(|u|1+σ) (σ ≥1).

Boussinesq [2, 3] deduced an important model

utt−∆u−∆utt= ∆(u2), (1.3)

which approximately describes the propagation of long waves on shallow water. Equation (1.3) is called improved Boussinesq (IBq) equation by [11]. Equation (1.3) and its generalized form innspace dimensions

utt−∆u−∆utt = ∆φ(u) (1.4)

can also describe the dynamical and thermodynamical properties of an harmonic monatomic and diatomic chains (see [14, 15]). Existence and nonexistence of global solutions, the global existence of small amplitude solutions for the Cauchy problem for (1.4) were obtained by Wang et al. [13, 19, 20]. Cho and Ozawa [4]

studied the existence and scattering of global small amplitude solutions to (1.4).

To take into account internal friction (it is called this type of friction hydrodynamical), which is due to irreversible processes taking place within the system, the dissipation function depends on the time derivatives of the relative displacements, in [1] the authors obtained the following IBq equation with damping

utt−∆u−∆utt−ν∆ut= ∆(u2).

Equation (1.4) has the following generalized form

utt−∆u−∆utt−ν∆ut= ∆φ(u). (1.5)

Polat [13] established the global existence and blow-up of solutions to (1.5) with the initial data.

(u, ut)(x,0) = (u0, u1)(x). (1.6)

Under smallness condition on the initial data, Wang and Xu [23] obtained asymptotic behavior of global solutions to (1.5) and (1.6) by the contraction mapping principle. Later, global existence and asymptotic behavior of solutions were refined in [24]. More precisely, the decay estimate

k∂xku(t)kL2 ≤CE1(1 +t)n4k2 (1.7) is obtained, where nσ ≥ 1 and s≥[n/2] + 1, E1 =ku0kHs∩L1 +ku1kHsW˙−1,1 and 0 ≤k ≤ s. Moreover, when nσ≥2, the proof in [24] also implies

k∂xk(u−uL)(t)kL2 ≤CE11+σ(1 +t)n4k2η(t) (1.8) for 0≤k≤s, where uL(t) is the solution to (1.5) and (1.6) withφ(u)≡0 andη(t) is defined by

η(t) =





1, n= 1,

(1 +t)12log(2 +t), nσ= 2, (1 +t)12, nσ ≥3.

However, such a linear approximation does not hold for (1.1) with σ = 1. This comes from the slower decay of the solution for n = 1 and σ = 1. We note that, when n = 1, the decay estimate (1.7) for the problem (1.1), (1.2) is given by

k∂xku(t)kL2 ≤CE1(1 +t)14k2, (1.9) wheres≥0, 0≤k≤s, and E1 =kfkHs∩L1+kgkHs+1∩L1.

The first main purpose of this paper is to establish nonlinear approximation to global solutions to the problem (1.1), (1.2) withσ = 1. We state the result as follows.

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Theorem 1.1. Let σ = 1 and s ≥ 1. Assume that f ∈ HsT

L1 and g ∈ Hs+1T

L1, and put E1 = kfkHsT

L1 +kgkHs+1T

L1. Let u(x, t) be the global solution to the problem (1.1), (1.2), and let $ be the approximation function defined by (3.10). Then for any ε > 0 and 0 ≤ k ≤ s, there is a small positive constant δ2 such that if E1 ≤δ2, we have

k∂xk(u−$)(t)kL2 ≤CE1(1 +t)34k2.

Theorem 1.1 implies that the global solution u to the problem (1.1), (1.2) is well approximated by the solution $ to the simpler problem (3.10). In the following result, we give the further approximation, i.e., we show that as time tends to infinity, the solution is asymptotic to the superposition of nonlinear diffusion waves which are given explicitly in terms of the self-similar solution of the viscous Burgers equation. The result is as follows:

Theorem 1.2. Let σ = 1 and s ≥ 1. Assume that f, g ∈ Hs+1∩L11/2 and put E˜1 = k(f, g)kHs+1∩L1 and E2 =k(f, g)kHs+1∩L11/2. Letu be the global solution to the problem (1.1), (1.2), and let v± be the nonlinear diffusion waves defined by (4.9) with the parameters in (4.11). Then there is a small positive constant δ3 such that ifE˜1 ≤δ3, then we have

k∂xk(u−v+−v)(t)kL2 ≤CE2(1 +t)12k2, (1.10) where 0≤k≤s.

Whenσ ≥2, our global solution is approximated by the superposition of diffusion waves which are given explicitly in terms of the solution of linear parabolic equation. We state the results as follows:

Theorem 1.3. Let s ≥ 1 and σ = 2. Assume that f, g ∈ Hs+1T

L11. Put E1 = k(f, g)kHs+1T

L1 and E3 =k(f, g)kHs+1T

L11. Let u be the global solution to the problem (1.1), (1.2), and let v± be the diffusion waves defined by (5.2). There exists a small positive constant δ3 such that ifE1≤δ3, we have

k∂xk(u−v+−v)(t)kL2 ≤CE3(1 +t)34k2 log(2 +t) for 0≤k≤s.

Theorem 1.4. Let s ≥ 1 and σ ≥ 3. Assume that f, g ∈ Hs+1T

L11. Put E1 = k(f, g)kHs+1T

L1 and E3 =k(f, g)kHs+1T

L11. Let u be the global solution to the problem (1.1), (1.2), and let v± be the diffusion waves defined by (5.2). There exists a small positive constant δ3 such that ifE1 ≤δ3, we have

k∂xk(u−v+−v)(t)kL2 ≤CE3(1 +t)34k2 for 0≤k≤s.

The global existence and asymptotic behavior of solutions to high order wave equation have been inves- tigated by many authors. We may refer to [6, 8, 16–18, 21–24]. For quantum stochastic evolution inclusions and variational inclusions, some related results have been established in [12].

The paper is organized as follows. In Section 2 we review the previous results on the problem (1.1), (1.2). A nonlinear approximation of global solutions to (1.1), (1.2) withσ= 1 is established in Section 3. In Section 4, whenσ= 1, we prove that global solution is asymptotic to the superposition of nonlinear diffusion waves which are given explicitly in terms of the self-similar solution of the viscous Burgers equation. Finally, large time behavior of global solutions is obtained forσ≥2 in Section 5.

2. Decay property of solution operator

To prove our main results, we need to deduce the solution formula for the problem (1.1), (1.2), which will be used in the present paper (see also [24]). For this purpose, we first investigate the linear equation of (1.1):

utt−uxxtt−uxx−νuxxt= 0. (2.1)

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Taking the Fourier transform, we have

(1 +ξ2)ˆutt+νξ2t2uˆ= 0. (2.2) The corresponding initial values are given as

t= 0 : ˆu= ˆf(ξ),uˆt=iξˆg(ξ). (2.3) The characteristic equation of (2.2) is

(1 +ξ22+νξ2λ+ξ2= 0. (2.4)

Letλ=λ±(ξ) be the corresponding eigenvalues of (2.4), we obtain λ±(ξ) = −µξ2±iξp

(4−ν22−4 2(1 +ξ2) . The solution to the problem (2.2)-(2.3) is given in the form

ˆ

u(ξ, t) =iξG(ξ, t)ˆˆ g(ξ) + ˆH(ξ, t) ˆf(ξ), (2.5) where

G(ξ, t) =ˆ 1

λ+(ξ)−λ(ξ)(eλ+(ξ)t−eλ(ξ)t) (2.6) and

H(ξ, t) =ˆ 1

λ+(ξ)−λ(ξ)(λ+(ξ)eλ(ξ)t−λ(ξ)eλ+(ξ)t). (2.7) We defineG(x, t) andH(x, t) byG(x, t) =F−1[ ˆG(ξ, t)](x) andH(x, t) =F−1[ ˆH(ξ, t)](x), respectively, where F−1 denotes the inverse Fourier transform. Then, applying F−1 to (2.5), we obtain

u(t) =G(t)∗∂xg+H(t)∗f. (2.8)

By the Duhamel principle, we obtain the solution formula to (1.1), (1.2) u(t) =G(t)∗∂xg+H(t)∗f +

Z t 0

G(t−τ)∗(I −∂x2)−1x2φ(u)(τ)dτ. (2.9) Next, we state the decay estimates of the solution operatorsG(t) andH(t) appearing in the solution formula (2.8), which was established in [23] and [24].

Lemma 2.1. The solution of the problem (2.2), (2.3) satisfies

(1 +ξ2)|ˆut(ξ, t)|22|ˆu(ξ, t)|2 ≤Ce−cω(ξ)t((1 +ξ22|ˆg(ξ)|22|fˆ(ξ)|2) for ξ∈Rand t≥0, where ω(ξ) = 1+ξξ22.

Lemma 2.2. Let G(ξ, t)ˆ and H(ξ, t)ˆ be the fundamental solution of (2.1) in the Fourier space, which are given in (2.6)and (2.7), respectively. Then we have the estimates

|G(ξ, t)| ≤ˆ C|ξ|−1(1 +ξ2)12e−cω(ξ)t and

|H(ξ, t)| ≤ˆ Ce−cω(ξ)t for ξ∈R andt≥0, where ω(ξ) = 1+ξξ22.

Lemma 2.3. Let k≥0 and 1≤p≤2. Then we have

k∂xkG(t)∗∂xϕkL2 ≤C(1 +t)12(1p12)−k2kϕkLp+Ce−ctk∂xkϕkL2, k∂xkH(t)∗ϕkL2 ≤C(1 +t)12(1p12)−k2kϕkLp+Ce−ctk∂xkϕkL2, and

k∂xkG(t)∗(I−∂x2)−1x2ϕkL2 ≤C(1 +t)12(1p12)−k212kϕkLp+Ce−ctk∂xkϕkL2. (2.10)

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3. Approximate to solution to (1.1), (1.2) with σ = 1

In this section, our main aim is to obtain the nonlinear approximation to the global solutions. It follows from mean value theorem that





























e

ν|ξ|2t

2(1+|ξ|2) =eν2|ξ|2t+ ¯K1, sin

|ξ|q

1−4−ν|ξ|22|ξ|2t

1 +|ξ|2 = sin(|ξ|t) + ¯K2, cos

|ξ|q

1−4−ν|ξ|22|ξ|2t

1 +|ξ|2 = cos(|ξ|t) + ¯K3, 1

q

1−4−ν4 2|ξ|2

= 1 + ¯K4, where





































1= ν|ξ|4t 2(1 +|ξ|2)e

ν 2|ξ|2[ θ1

1+|ξ|2+(1−θ1)]t

,

2=− |ξ|3(|ξ|2+12−ν4 2)t (1 +|ξ|2)(

q

1−4−ν4 2|ξ|2+ 1 +|ξ|2) cos

h|ξ|

q

1−4−ν4 2|ξ|2t

1 +|ξ|2 θ2+ (1−θ2)|ξ|ti ,

3= |ξ|3(|ξ|2+12−ν4 2)t (1 +|ξ|2)(

q

1−4−ν42|ξ|2+ 1 +|ξ|2)

sinh|ξ|

q

1−4−ν42|ξ|2t

1 +|ξ|2 θ3+ (1−θ3)|ξ|ti ,

4= (4−ν2)|ξ|2 8(1−4−ν4 2|ξ|2θ4)32 withθi(i= 1,2,3,4)∈(0,1).

When |ξ| ≤δ, whereδ is a small positive constant, we obtain from the above four equalities G(ξ, t) =ˆ eλ+t−eλt

λ+−λ

= 1 +|ξ|2

|ξ|

q

1−4−ν42|ξ|2 e

ν|ξ|2t 2(1+|ξ|2)sin

|ξ|q

1−4−ν|ξ|22|ξ|2t 1 +|ξ|2

= 1

|ξ|eν2ξ2tsin|ξ|t+ ¯J1

and

H(ξ, t) =ˆ λ+eλt−λeλ+t λ+−λ

= v|ξ|

2 q

1−4−ν42|ξ|2 e

ν|ξ|2t 2(1+|ξ|2)sin

|ξ|q

1−4−ν|ξ|22|ξ|2t 1 +|ξ|2 +e

ν|ξ|2t 2(1+|ξ|2)cos

|ξ|q

1−4−ν|ξ|22|ξ|2t 1 +|ξ|2

=eν2ξ2tcos|ξ|t+ ¯J2.

(3.1)

When |ξ| ≤δ, ¯J1 and ¯J2 satisfy

|J¯1| ≤C(1 +|ξ|2t)e−c|ξ|2t and

|J¯2| ≤C(|ξ|+|ξ|3t)e−c|ξ|2t.

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Taking

0(ξ, t) = 1

|ξ|eν2|ξ|2tsin|ξ|t, Hˆ0(ξ, t) =eν2|ξ|2tcos|ξ|t.

Then

|( ˆG −Gˆ0)(ξ, t)| ≤Ce−c|ξ|2t, |( ˆH −Hˆ0)(ξ, t)| ≤C|ξ|e−c|ξ|2t (3.2) for|ξ| ≤δ.

Lemma 3.1. Let k≥0 and 1≤p≤2. Then we have

k∂xkG0(t)∗∂xϕkL2 ≤C(1 +t)12(1p12)−k2kϕkLp+Ce−ctk∂xkϕkL2, (3.3) k∂xkH0(t)∗ϕkL2 ≤C(1 +t)12(1p12)−k2kϕkLp+Ce−ctk∂xkϕkL2, (3.4) k∂xkG0(t)∗∂xϕkL2 ≤C(1 +t)12(1p12)−k2kϕkLp+Ce−cttk−l2 k∂xlϕkL2, (3.5) and

k∂xkG0(t)∗∂xϕkL2 ≤Ct12(1p12)−k2kϕkLp. (3.6) Proof. We only give the proof of (3.5). The Plancherel theorem entails that

k∂xkG0(t)∗∂xφk2L2 = Z

|ξ|≤1

|ξ|2k+2|Gˆ0(ξ, t)|2|ϕ(ξ)|ˆ 2dξ+ Z

|ξ|≥1

|ξ|2k+2|Gˆ0(ξ, t)|2|ϕ(ξ)|ˆ 2dξ=:I1+I2. (3.7) By (3.1), H¨older inequality and Hausdorff inequality, we have

I1 ≤C(1 +t)12(2p−1)−kkϕk2Lp. (3.8) Owing to (3.1),I2 can be estimated as

I2 ≤Ce−ct sup

|ξ|≥1

(|ξ|2(k−l)e−c|ξ|2t) Z

|ξ|≥1

|ξ|2l|ϕ|ˆ2dξ≤Ce−ctt−(k−l)k∂xlϕk2L2. (3.9) Inserting (3.8) and (3.9) into (3.7) yields (3.5). Thus we have completed the proof.

Let

$(t) =G0(t)∗∂xg+H0(t)∗f +φ00(0) 2

Z t 0

G0(t−τ)∗∂x2$2(τ)dτ. (3.10) In order to obtain nonlinear approximation of global solutions to the Cauchy problem (1.1), (1.2), we need the following lemma, which comes from [9] (see also [25]).

Lemma 3.2. Assume that φ = φ(v) is a smooth function. Suppose that φ(v) = O(|v|1+θ) (θ ≥ 1 is an integer) when |v| ≤ ν0. Then for integer m ≥ 0, if v ∈ Wm,q(Rn)T

Lp(Rn)T

L(Rn) and kvkL ≤ ν0, thenφ(v)∈Wm,r(Rn). Furthermore, the following inequality holds:

k∂xmφ(v)kLr ≤CkvkLpk∂xmvkLqkvkθ−1L, where 1≤p, q, r≤+∞ and 1r = 1p+ 1q.

Lemma 3.3. Let s≥1. Assume that f, g∈Hs(R)T

L1(R). Put E0:=kfkHsT

L1 +kgkHsT L1.

$(t) is defined by (3.10). IfE0 is suitably small, then

k∂xk$(t)kL2 ≤CE0(1 +t)14k2 (3.11) for 0≤k≤s.

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Remark 3.4. If “f, g∈Hs(R)T

L1(R)” is replaced by “f ∈Hs(R)T

L1(R) andg∈Hs+1(R)T

L1(R)”, put E1 :=kfkHsT

L1 +kgkHs+1T L1. IfE1 is suitably small, then

k∂xk$(t)kL2 ≤CE1(1 +t)14k2. (3.12) Proof. We only prove (3.11). Set

M(t) =

s

X

k=0

sup

0≤τ≤t

(1 +τ)14+k2k∂xk$(t)kL2.

By applying (3.10) and Minkowski inequality, we arrive at k∂xk$(t)kL2 ≤ k∂xkG0(t)∗∂xgkL2 +k∂xkH0(t)∗fkL2 +

Z 2t

0

k∂xkG0(t−τ)∗∂x200(0)

2 $2)kL2(τ)dτ +

Z t

t 2

k∂xkG0(t−τ)∗∂x200(0)

2 $2)kL2(τ)dτ ,I1+I2+I3+I4.

(3.13)

It follows from (3.3) withp= 1 that

I1≤C(1 +t)14k2kgkHsT

L1. (3.14)

Due to (3.4) withp= 1 to I2, it holds that

I2 ≤C(1 +t)14k2kfkHsT

L1. (3.15)

Equation (3.5), Lemma 3.2, and Gagliardo-Nirenberg inequality entail that I3 ≤C

Z t

2

0

(1 +t−τ)34k2k$2kL1dτ+C Z t

2

0

e−c(t−τ)(t−τ)12k∂xk$2kL2

≤CM2(t) Z t

2

0

(1 +t−τ)14k212(1 +τ)12dτ +CM2(t)

Z 2t

0

e−c(t−τ)(t−τ)12(1 +τ)12(1 +τ)14k2

≤CM2(t)(1 +t)14k2.

(3.16)

By exploiting (3.6), Lemma 3.2, and Gagliardo-Nirenberg inequality, we get I4 ≤C

Z t

t 2

(t−τ)12k∂xk$2kL2

≤CM2(t) Z t

t 2

(t−τ)12(1 +τ)12(1 +τ)14k2

≤CM2(t)(1 +t)14k2.

(3.17)

Combining (3.13)-(3.17) yields

M(t)≤CE0+CM2(t),

This inequality can be solved asM(t) ≤CE0 if E0 is sufficiently small. Thus we have completed the proof of lemma.

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Lemma 3.5. Let k≥0 and 1≤p≤2. Then we have

k∂xk(G − G0)(t)∗∂xϕkL2 ≤C(1 +t)12(1p12)−k212kϕkLp+Ce−ctk∂xk+1ϕkL2, (3.18) k∂xk(G − H0)(t)∗ϕkL2 ≤C(1 +t)12(1p12)−k212kϕkLp+Ce−ctk∂xkϕkL2, (3.19) k∂xkG0(t)∗ {(1−∂x2)−1−I}∂x2ϕkL2 ≤C(1 +t)12(1p12)−k232kϕkLp+Ce−cttk+1−l2 k∂xlϕkL2, (3.20) and

k∂xk(G − G0)(t)∗(1−∂x2)−1x2ϕkL2 ≤C(1 +t)12(1p12)−k2−1kϕkLp+Ce−ctk∂xk+lϕkL2.

Proof. We only give the proof of (3.18). By applying the Plancherel theorem, we deduce that k∂xk(G − G0)(t)∗∂xϕk2L2 =

Z

|ξ|≤δ

|ξ|2k+2|( ˆG −Gˆ0)(ξ, t)|2|ϕ(ξ)|ˆ 2dξ +

Z

|ξ|≥δ

|ξ|2k+2|( ˆG −Gˆ0)(ξ, t)|2|ϕ(ξ)|ˆ 2

=:I1+I2.

(3.21)

For the low frequency part I1, using (3.2), H¨older inequality and Hausdorff inequality, we estimate as I1 ≤C(

Z

|ξ|≤δ

|ξ|(2k+2)qe−cq|ξ|2tdξ)1qkϕkˆ 2

Lp0 ≤C(1 +t)12(2p−1)−k−1kϕk2Lp, (3.22) where 1q +p20 = 1 and 1p +1q = 1. Also, for the high frequency part I2, we have

I2≤C Z

|ξ|≥δ

|ξ|2k+2e−ct|ϕ|ˆ2dξ≤Ce−ctk∂xk+1ϕk2L2. (3.23)

Combining (3.21), (3.22) and (3.23) yields (3.18). Thus we have completed the proof of lemma.

In what follows, we prove Theorem 1.1.

Proof. We introduce the quantity X(t) =

s

X

k=0

sup

0≤τ≤t

(1 +τ)34+k2−εk∂kx(u−$)kL2,

whereε >0 is a fixed small constant. Due to (2.9) and (3.10), we arrive at (u−$)(t) = (G − G0)(t)∗∂xg+ (H − H0)(t)∗f

+ Z t

0

G(t−τ)∗(I −∂x2)−1x2(φ(u)−φ00(0)

2 u2)(τ)dτ +φ00(0)

2 Z t

0

G(t−τ)∗(I−∂x2)−1x2{(u+$)(u−$)}(τ)dτ +φ00(0)

2 Z t

0

(G − G0)(t−τ)∗(I−∂x2)−1x2($2)(τ)dτ +φ00(0)

2 Z t

0

G0(t−τ)∗ {(I −∂2x)−1−I}∂x2($2)(τ)dτ.

(3.24)

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Owing to (3.24) and Minkowski inequality, we get

k∂xk(u−$)(t)kL2 ≤ k∂kx(G − G0)(t)∗∂xgkL2 +k∂xk(H−H0)(t)∗fkL2

+ Z t

2

0

k∂xkG(t−τ)∗(I−∂x2)−1x2(φ(u)−φ00(0)

2 u2)(τ)kL2dτ +

Z t

t 2

k∂xkG(t−τ)∗(I−∂x2)−1x2(φ(u)−φ00(0)

2 u2))(τ)kL2dτ +|φ00(0)|

2 Z t

2

0

k∂xkG(t−τ)∗(I −∂x2)−1x2{(u+$)(u−$)}(τ)kL2dτ +|φ00(0)|

2 Z t

t 2

k∂xkG(t−τ)∗(I−∂x2)−1x2{(u+$)(u−$)}(τ)kL2dτ +|φ00(0)|

2 Z t

2

0

k∂xk(G − G0)(t−τ)∗(I−∂x2)−1x2($2)(τ)kL2dτ +|φ00(0)|

2 Z t

t 2

k∂xk(G − G0)(t−τ)∗(I−∂x2)−1x2($2)(τ)kL2dτ +|φ00(0)|

2 Z t

2

0

k∂xkG0(t−τ)∗ {(I−∂x2)−1−I}∂x2($2)(τ)kL2dτ +|φ00(0)|

2 Z t

t 2

k∂xkG0(t−τ)∗ {(I−∂x2)−1−I}∂x2($2)(τ)kL2dτ ,J1+J2+J31+J32+J41+J42+J51+J52+J61+J62.

(3.25)

By (3.18), we have

J1 ≤C(1 +t)34k2(kgkL1+kgkHs+1). (3.26) Making use of (3.19), we obtain

J2 ≤C(1 +t)34k2(kfkL1 +kfkHs). (3.27) Thanks to Lemma 3.2 and (1.9), we obtain

kφ(u)−φ00(0)

2 u2(τ)kL1 ≤Cku(τ)kLku(τ)k2L2 ≤CE13(1 +τ)−1 (3.28) and

k∂xk(φ(u)−φ00(0)

2 u2)(τ)kL2 ≤Cku(τ)k2Lk∂xku(τ)kL2 ≤CE13(1 +τ)54k2. (3.29) It follows from (2.10) and (3.28)-(3.29) that

J31≤C Z t

2

0

(1 +t−τ)34k2k(φ(u)− φ00(0)

2 u2)(τ)kL1dτ +

Z 2t

0

e−c(t−τ)k∂xk(φ(u)− φ00(0)

2 u2)(τ)kL2

≤CE13

Z t

2

0

(1 +t−τ)34k2(1 +τ)−1dτ+CE13

Z t

2

0

e−c(t−τ)(1 +τ)54k2

≤CE13(1 +t)34k2.

(3.30)

(10)

By using (2.10) withp= 2 and (3.29), it holds that J32≤C

Z t

t 2

(1 +t−τ)12k∂xk(φ(u)−φ00(0)

2 u2)(τ)kL2

≤CE13

Z t

t 2

(1 +t−τ)12(1 +τ)54k2

≤CE13(1 +t)34k2.

(3.31)

From Lemma 3.2, Gagliardo-Nirenberg inequality and (1.9), (3.12), we arrive at

k(u2−$2)(τ)kL1 ≤Cku+$kL2ku−$kL2 ≤CE1X(t)(1 +τ)−1+ε (3.32) and

k∂xk(u2−$2)(τ)kL2 ≤CE1X(t)(1 +τ)54k2. (3.33) For the term J41, applying (2.10) and (3.32), (3.33) yields

J41≤C Z 2t

0

(1 +t−τ)34k2ku2−$2(τ)kL1dτ+C Z 2t

0

e−c(t−τ)k∂xk(u2−$2)(τ)kL2

≤CE1X(t) Z t

2

0

(1 +t−τ)34k2(1 +t)−1+εdτ+CE1X(t) Z t

2

0

e−c(t−τ)(1 +t)54k2

≤CE1X(t)(1 +t)34k2

(3.34)

and

J42≤C Z t

t 2

(1 +t−τ)12k∂xk(u2−$2)(τ)kL2dτ+C Z t

t 2

e−c(t−τ)k∂xk(u2−$2)(τ)kL2

≤CE1X(t) Z t

t 2

(1 +t−τ)12(1 +τ)54k2dτ+CE1X(t) Z t

t 2

e−c(t−τ)(1 +t)54k2

≤CE1X(t)(1 +t)34k2.

(3.35)

Lemma 3.2, Gagliardo-Nirenberg inequality and (3.12) give the estimates

k$2(τ)kL1 ≤Ck$(τ)k2L2 ≤CE12(1 +τ)12 (3.36) and

k∂xk$2(τ)kL2 ≤Ck$(τ)kLk∂xk$(τ)kL2 ≤CE12(1 +τ)34k2. (3.37) Owing to (3.10) and (3.36), (3.37), we deduce that

J51≤C Z t

2

0

(1 +t−τ)54k2k$2(τ)kL1dτ+C Z t

2

0

e−c(t−τ)k∂xk$2(τ)kL2

≤CE12

Z t

2

0

(1 +t−τ)54k2(1 +τ)12dτ+CE12

Z t

2

0

e−c(t−τ)(1 +τ)34k2

≤CE12(1 +t)34k2.

(3.38)

Equations (3.10) and (3.37) give the estimates J52≤C

Z t

t 2

(1 +t−τ)−1k∂xk$2(τ)kL2dτ+C Z t

t 2

e−c(t−τ)k∂xk$2(τ)kL2

≤CE12

Z t

t 2

(1 +t−τ)−1(1 +τ)34k2dτ+CE12

Z t

t 2

e−c(t−τ)(1 +τ)34k2

≤CE12(1 +t)34k2.

(3.39)

(11)

Using (3.20), (3.36) and (3.37), we have J61≤C

Z t

2

0

(1 +t−τ)74k2k$2(τ)kL1dτ+C Z t

2

0

e−c(t−τ)(t−τ)12k∂kx$2(τ)kL2

≤CE12

Z t

2

0

(1 +t−τ)74k2(1 +τ)12dτ +CE12

Z t

2

0

e−c(t−τ)(t−τ)12(1 +τ)34k2

≤CE12(1 +t)54k2.

(3.40)

By (3.20) and (3.37), we may obtain J62≤C

Z t

t 2

(1 +t−τ)32k∂xk$2kL2dτ+C Z t

t 2

e−c(t−τ)(t−τ)12k∂xk$2kL2

≤CE12Z t

t 2

(1 +t−τ)32(1 +τ)34k2dτ +CE12Z t

t 2

e−c(t−τ)(t−τ)12(1 +τ)34k2

≤CE12(1 +t)34k2.

(3.41)

Combining (3.25)-(3.41) yields

X(t)≤CE1+CE1X(t) +CE12+CE13.

This inequality can be solved asX(t)≤CE1 ifE1 is sufficiently small. This completes the proof of Theorem 1.1.

4. Asymptotic profile of solution to (1.1), (1.2) with σ = 1 We may rewrite (3.10) as

$(t) =G1(t)∗$+0 + φ00(0) 4

Z t 0

G1(t−τ)∗∂x$2(τ)dτ+G2(t)∗$0 −φ00(0) 4

Z t 0

G2(t−τ)∗∂x$2(τ)dτ, (4.1) where





G1(t) =F−1{e(−ν2ξ2+iξ)t}= 1

√2πνte(x+1)22νt , G2(t) =F−1{e(−ν2ξ2−iξ)t}= 1

2πνte

(x−1)2 2νt ,

(4.2)

and

$0+= 1 2f+1

2g, $0= 1 2f−1

2g. (4.3)

We need the following decay properties forG1(t)∗and G2(t)∗.

Lemma 4.1 ([7]). Let 1≤q≤p≤ ∞ and 0≤j≤k. Then we have k∂xkG1(t)∗ϕkLp ≤Ct12(1q1p)−

k−j

2 k∂xjϕkLq (4.4)

and

k∂xkG2(t)∗ϕkLp ≤Ct12(1qp1)−

k−j

2 k∂xjϕkLq. (4.5)

Lemma 4.2 ([7]). Let 1≤p≤2, 0≤j≤k and 0≤l≤k. Then k∂xkG1(t)∗ϕkL2 ≤C(1 +t)12(p112)−

k−j

2 k∂xjϕkLp+Ce−cttk−l2 k∂xlϕkL2 (4.6) and

k∂xkG2(t)∗ϕkL2 ≤C(1 +t)12(1p12)−

k−j

2 k∂xjϕkLp+Ce−cttk−l2 k∂xlϕkL2.

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