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Semilinear parabolic equation in R N associated with critical Sobolev exponent

Ryo Ikehata

a,1

, Michinori Ishiwata

b,,2

, Takashi Suzuki

c,3

aDepartment of Mathematics, Faculty of Education, Hiroshima University, Higashi-Hiroshima 739-8524, Japan bDepartment of Mathematical Science, Common Subject Division, Muroran Institute of Technology, Muroran 050-8585, Japan

cDepartment of Mathematics, Graduate School of Science, Osaka University, Toyonaka 560-0043, Japan Received 27 February 2008; received in revised form 8 December 2009; accepted 15 December 2009

Available online 7 January 2010

Abstract

We consider the semilinear parabolic equationutu= |u|p1uon the whole spaceRN,N3, where the exponentp= (N+2)/(N−2)is associated with the Sobolev imbeddingH1(RN)Lp+1(RN). First, we study the decay and blow-up of the solution by means of the potential-well and forward self-similar transformation. Then, we discuss blow-up in infinite time and classify the orbit.

©2010 Elsevier Masson SAS. All rights reserved.

MSC:35K55

Keywords:Parabolic equation; Critical Sobolev exponent; Cauchy problem; Stable and unstable sets; Self-similarity

1. Introduction

The purpose of the present paper is to classify the asymptotic behavior of the solution to the semilinear parabolic equation

utu= |u|p1u inRN×(0, T ) (1)

with

u|t=0=u0 inRN, (2)

whereN3 andp=(N+2)/(N−2), the critical exponent associated with the Sobolev imbedding. In the previous work [9,8,11,23], we studied the long time behavior of the solution defined on the bounded domain in connection with

* Corresponding author.

E-mail addresses:ikehatar@hiroshima-u.ac.jp (R. Ikehata), ishiwata@mmm.muroran-it.ac.jp (M. Ishiwata), takashi@math.sci.osaka-u.ac.jp (T. Suzuki).

1 The author is partially supported by JSPS Grant-in-aid for Scientific Research (C) #19540184.

2 The author is partially supported by JSPS Grant-in-Aid for Young Scientists B #19740081.

3 The author is partially supported by JSPS Grant-in-aid for Scientific Research (B) #20340034.

0294-1449/$ – see front matter ©2010 Elsevier Masson SAS. All rights reserved.

doi:10.1016/j.anihpc.2010.01.002

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the stable and unstable sets introduced by [22,20]. We have shown that if the orbit enters in the stable set, then the solution exists globally in time [11]. If the orbit enters in the unstable set, then the solution blows up in finite time [9].

The other case is called “floating”. Thus, the orbit is floating, by definition, if it never enters in the stable set nor the unstable set. If the domain is star-shaped, then the orbit floating globally in time must blow up in infinite time, while the floating orbit blowing up in finite time never exists under the additional assumption of the domain and the initial value, that is, the convexity and symmetry [23].

In contrast with these cases on the bounded domain, there is a family of stationary solutions to (1)–(2) concerning the whole spaceRN. We have the lack of the Poincaré inequality also. These differences are made clear by the forward self-similar transformation and the non-existence of the self-similar solution [5,14]. Consequently, we can classify the rate ofu(t )ast↑ +∞for the solutionu=u(·, t )global in time.

More precisely, ifu=u(x, t )is the solution, then

v(y, s)=(1+t )1/(p1)u(x, t ), t=es−1, x=(1+t )1/2y (3) satisfies

vs+Lv= |v|p1v+ 1

p−1v inRN×(0, S) (4)

with

v|s=0=u0 inRN, (5)

whereS=log(1+T )and Lf = −f−1

2y· ∇f.

Since

Lf = −1

K∇ ·(Kf ) holds for

K(y)=e|y|2/4,

problem (4)–(5) is associated with the Hilbert spaceL2(K), the set of measurable functionsf =f (y)defined inRN such that

f2,K=

RN

f (y)2K(y) dy 1/2

<+∞.

We also take Hm(K)=

fL2(K)DαfL2(K)for any multi-indexαin|α|m , wherem=1,2, . . .. It is a Hilbert space provided with the norm

fHm(K)=

|α|m

Dαf 2

2,K

1/2

.

ThisLis realized as a self-adjoint operator inL2(K)associated with the bilinear form AK(u, v)=

RN

u(y)· ∇v(y)K(y) dy defined foru, vH1(K)through the relation

AK(u, v)=(Lu, v)K, uD(L)H1(K), vH1(K),

(3)

where

(u, v)K=

RN

u(y)v(y)K(y) dy,

see [13], for the general theory of the bilinear form. The domain D(L) of this operator is the set of vL2(K) satisfyingLvL2(K), and we haveD(L)=H2(K), see Lemma 2.1 of [14]. It holds also thatLis positive self- adjoint and has the compact inverse, and in particular, the set of normalized eigenfunctions ofL forms a complete ortho-normal system inL2(K). The first eigenvalueλ1ofLis given byλ1=N/2, and hence the Poincaré inequality

λ1v22,Kv22,K, vH1(K), (6)

is valid, see Proposition 2.3 of [5].

We have λ1=N

2 > λ≡ 1

p−1=N−2 4 and therefore, the operator

A=L− 1 p−1

inL2(K)is also positive self-adjoint with the domainD(A)=H2(K). The fractional powersAα and the semigroup {et A}t0 are thus defined inL2(K), where α∈ [0,1]. These structures guarantee the well-posedness of (4)–(5) locally in time. Later, we shall show the following fact.

Proposition 1.1.Eachu0H1(K) admitsT >0 such that (4)–(5) has a unique solution vC([0, T];H1(K)) satisfying the following:

1. vC((0, T];D(Aν)).

2. v(s)=esAu0+t

0e(sσ )A|v(σ )|p1v(σ ) dσ. 3. lims0sν12Aνv(s)2,K=0,

where

ν

⎧⎨

=N/(N+2) (N5),

(2/3,1) (N=4),

=4/5 (N=3).

We callv=v(·, s) theH1(K)-solution, or simply thesolutionto (4)–(5). Proposition 1.1 assures local in time unique existence of the solution u=u(·, t ) to (1)–(2) for u0H1(K). Also, this v=v(·, s) coincides with the solution discussed in [14]. Henceforth,Tm(K)(0,+∞]denotes the supremum ofT such that the solutionv=v(·, s) to (4)–(5) exists fors∈ [0, T]. The local existence timeT assured by Proposition 1.1, however, is not estimated from below byu0H1(K). Consequently, we cannot conclude

lim sup

sTm(K)

v(s)

H1(K)= +∞

fromTm(K) <+∞(cf. Theorem 1.10(ii) of [14]), similarly to the case of the bounded domain, see [9]. Henceforth, we putT =Tm(K)(0,+∞]for simplicity.

In this paper, we show that the orbit made from the above mentioned solution is classified in the following way.

We emphasize that the solutionu=u(·, t )may be sign-changing.

Theorem 1.Ifu=u(·, t )is the solution to(1)–(2)withu0H1(K)andp=NN+22,N3, then we have the following alternatives.

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1. T = +∞andlim supt↑+∞tN/2u(t )<+∞.

2. T = +∞andlimt↑+∞t(N2)/4u(t )= +∞.

3. T <+∞andlimtTu(t )= +∞.

Ifu0=u0(x)0,u0≡0, the first case is refined asT = +∞with u(t )

tN/2 ast↑ +∞. (7)

Here are some comments.

1. There is an analogous result concerning sub-critical nonlinearities [15]. Thus, ifu0=u0(x)0 and 1+N2 <

p <NN+22, then we have the following alternatives for the solutionu=u(·, t )to (1)–(2);

(a) T = +∞and (7).

(b) T = +∞andu(t )t1/(p1)ast↑ +∞. (c) T <+∞.

The second case of this result indicates the decay rate with that of the self-similar solution. Our Theorem 1 is, actually, associated with the non-existence of the self-similar solution for the critical Sobolev exponent [14], see Proposition 5.1 below. The second case of Theorem 1, thus, may be called “type II rate” att = +∞because 1/(p−1)=(N−2)/4 forp=NN+22.

2. The second case of Theorem 1 arises if the orbit is floating globally in time in the rescaled variables (3). Such a case occurs actually ifu0=u0(x)is a non-trivial stationary solution. In fact, in contrast with the case of the bounded star-shaped domain provided with the Dirichlet boundary condition, problem (1)–(2) admits a family of non-trivial stationary solutions, normalized by

U=Up, 0< U U (0)=1 inRN, (8)

see [1,3]. As for the solution converging uniformly to 0 in infinite time, however, there remains two possibilities – the first and the second cases of Theorem 1.

3. Positive radially symmetric solutions have been studied in detail. Particularly, analogous results to Theorem 1 are obtained [21], in accordance with the threshold of the modulus of the initial value for the blow-up of the solution. Its proof, however, uses the intersection comparison principle and is different from ours. The blow-up profile is also known by [12]. Thus,T = +∞implies the existence of limt↑+∞u(t )=α∈ [0,+∞]for a suitable family of radially symmetric positive initial values. Ifα=0, the second case of Theorem 1 arises. It holds, furthermore, that

u(t )= u(t )

U u(t ) N22

· +o(1) ast↑ +∞inH˙1(RN), where

H˙1 RN

=

vLN−22N

RNvL2 RNN

andU=U (y) >0 is the normalized non-trivial stationary solution defined by (8).

Our proof of Theorem 1 is involved by the imbedding theorem concerningH1(K). Henceforth,Lq(K)denotes the Banach space composed of measurable functionsf=f (y)defined inRNsuch that

fq,K=

RN

f (y)qK(y) dy 1/q

<+∞

forq∈ [1,∞)and f,K=ess sup

yRN

f (y)<+∞

forq= ∞. The spaceL(K)=L(RN)is thus compatible to the other spaces, i.e.,

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qlim↑∞fq,K= f,K, fL1(K)L RN

. (9)

Although the inclusion

Lp(K)Lq(K) (1q < p) fails, we have

H1(K)L2(K)

for 2=2N/(N−2)=p+1. More precisely, Corollary 4.20 of [5] guarantees the following fact, regarded as a Sobolev–Poincaré inequality.

Proposition 1.2.It holds that

S0v2p+1,K+λv22,Kv22,K, vH1(K), (10) whereλ=max(1, N/4)andS0stands for the Sobolev constant:

S0=inf

v22vC0 RN

, vp+1=1 .

We introduce the functionals JK(v)=1

2∇v22,Kλ

2v22,K− 1

p+1vpp++11,K and

IK(v)= ∇v22,Kλv22,Kvpp++11,K

defined forvH1(K), whereλ=1/(p−1). Then, the potential depth ofJKinH1(K)is defined by d0=inf

sup

μ>0

JK(μv)vH1(K)\ {0} ,

and it holds that d0=

1

2− 1

p+1

S(p0 +1)/(p1)= 1

NS0N/2>0. (11)

Here and henceforth, · q indicates the standardLq norm onRN. The stable and unstable sets to (4) are defined by

WK=

vH1(K)JK(v) < d0, IK(v) >0

∪ {0}

and

VK=

vH1(K)JK(v) < d0, IK(v) <0 , respectively.

Theorem 1 is proven by the study of the above defined stable and unstable sets. First, if the orbit enters in the stable set, thenv(·, s)converges to 0 in infinite time.

Proposition 1.3.Ifv=v(·, s)is the solution to(4)–(5)satisfyingv(s0)WK for somes0∈ [0, T ), then it holds that T = +∞and

v(s) 2

2,K=O eαs

(12) ass↑ +∞, whereα(0,1).

If the orbit enters in the unstable set, on the contrary, thenv(·, s)blows up in finite time; the following proposition implies Theorem 1.10(i) of [14].

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Proposition 1.4. If the solution v=v(·, s) to(4)–(5) satisfiesv(s0)VK for somes0∈ [0, T ), then it holds that T <+∞.

The orbit{v(s)}is, thus,floatingin the other case than the ones treated in Propositions 1.3–1.4, i.e.,v(s) /(WKVK)fors∈ [0, T ). In spite of the possibility of the floating orbit blowing up in finite time, the following proposition is sufficient to classify the orbit to (1)–(2) as in Theorem 1.

Proposition 1.5.If the orbit{v(s)}is floating globally in time, then it holds that

s↑+∞lim v(s)

,K= +∞. (13)

This paper is composed of six sections. Section 2 takes preliminaries. We confirm inequality (11) and Proposi- tion 1.1. In Section 3, we prove Propositions 1.3 and 1.4 by the study of stable and unstable sets. Section 4 describes theLq(K)-theory ofL. Using this, we study the floating orbit and show Proposition 1.5 in Section 5. The proof of Theorem 1 is completed in Section 6.

2. Preliminaries

This section is devoted to the preliminaries. First, we show (11), noting that sup

μ>0

JK(μv)=JK(μv)|μ=μ

holds for μ=

v22,Kλv22,K vpp++11,K

1/(p1)

and vH1(K)\ {0}. Then, it follows that

sup

μ>0

JK(μv)= p−1 2(p+1)

v22,Kλv22,K v2p+1,K

(p+1)/(p1)

and hence d0=

1

2− 1

p+1

Sλ(p+1)/(p1),

where Sλ=inf

v22,Kλv22,K v2p+1,K

vH1(K)

.

We have, however, λ= 1

p−1 =N−2 4 ,

and therefore,Sλ=S0by Theorem 4.10 and Lemma 4.11 of [5]. This means (11).

Next, we confirm the operator theoretical feature ofLinL2(K)described in the previous section. It is actually involved by the Schrödinger operator with harmonic oscillator;

K1/2LK1/2=H≡ −+V (y), where

V (y)=N 4 +|y|2

16 .

ThisHis associated with the bilinear form

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A(u, v)=

RN

u(y)· ∇v(y)+V (y)u(y)v(y) dy

defined foru, vH11(RN)through the relation A(u, v)=(H u, v)

foruD(H )H11(RN)andvH11(RN), where H11

RN

= vH1

RN |y|vL2 RN

and( , ) denotes theL2 inner product. It is realized as a positive self-adjoint operator inL2(RN)with the compact inverse, because the inclusionH11(RN)L2(RN)is compact. Now we show the following lemma.

Lemma 2.1.The domain ofH inL2(RN)is given by D(H )=H22

RN

vH2

RN |y|2vL2 RN

.

Proof. The inclusionH22(RN)D(H )is obvious. We show thatvH11(RN)with

v+V v=gL2 RN

(14) impliesvH2(RN). In fact, from the proof of Lemma 2.1 of [14] we have

RN

(v)2+V|∇v|2

dyCNg22 (15)

with a constant CN>0 determined by N. This implies vH2(RN), and then V vL2(RN)by (14). We obtain D(H )H22(RN)and the proof is complete. 2

For later arguments, we describe the proof of (15) in short. First, (14) implies, formally, that

RN

(v)2+V v·(v) dy=

RN

g(v) dy

and

RN

V v·(v) dy=

RN

V|∇v|2+1

2∇V · ∇v2

dy=

RN

V|∇v|2−1 2v2V

dy.

Then, (15) holds by

RN

(v)2+V|∇v|2 dy N

16v2+ g2· v2.

To justify these calculations, we note thatvHloc2 (RN)follows from (14). Next, takingϕC0(RN)such that 0ϕ1, suppϕ

|y|<2

, ϕ=1 for|y|1,

we multiply−v·ϕnby (15), whereϕn(y)=ϕ(y/n). Then, (14) is obtained by makingn→ +∞. Henceforth, such argument of justification will not be described explicitly.

Lemma 2.1 establishes the operator theoretical profiles ofLas is desired; it is realized as a positive self-adjoint operator inL2(K)with the compact inverse and the domainD(L)=H2(K). Here, we note the following lemma.

Lemma 2.2.The multiplicationK1/2induces the isomorphisms L2(K)∼=L2

RN

, H1(K)∼=H11 RN

, H2(K)∼=H22 RN

.

(8)

Proof. It is obvious thatK1/2:L2(K)L2(RN)is an isomorphism. To confirm thatK1/2:H1(K)H11(RN)is an isomorphism, we takev=K1/2uL2(RN), givenuH1(K). Since

v=K1/2u+y

4v, (16)

it holds that K|∇u|2=

vy 4v

2= |∇v|2y

2v· ∇v+|y|2

16 v2= |∇v|2−1

4y· ∇v2+|y|2 16 v2. Using

−1 4

RN

y· ∇v2dy=1 4

RN

(∇ ·y)v2dy=N 4

RN

v2dy,

we obtain

RN

|∇u|2K dy=

RN

|∇v|2+ N

4 + 1 16|y|2

v2

dy,

and therefore, yvL2(RN)N and∇vL2(RN)N. This meansv=K1/2uH11(RN). Given vH11(RN), con- versely, we takeu=K1/2vL2(K). Then,uL2(K)Nfollows from (16).

To show that K1/2:H2(K)H22(RN) is an isomorphism, first, we take uH2(K) and put v=K1/2uL2(RN). SinceuH1(K), it holds thatvH11(RN)and henceyvL2(RN)N. This means

yiuL2(K) (i=1,2, . . . , N ). (17)

It also holds that∇uH1(K)Nand hence yi ∂u

∂yjL2(K) (i, j=1,2, . . . , N ) (18)

follows similarly. The right-hand side of

∂yj

(yiu)=δiju+yi ∂u

∂yj

,

therefore, belongs toL2(K), and henceyuH1(K)N follows from (17). This implies

|y|2uL2(K) (19)

similarly to (17) again, which means|y|2vL2(RN). Finally, the right-hand side of

2v

∂yi∂yj =√ K 2u

∂yi∂yj +

K 4 yi ∂u

∂yj +

K

16 yiyju+

K 4 yj ∂u

∂yi

belongs toL2(RN)by (18) and (19). This meansvH2(RN)and hencev=K1/2uH22(RN).

GivenvH22(RN), conversely, we takeu=K1/2vL2(K). SincevH11(RN), it holds thatuH1(K). The right-hand side of

2u

∂yi∂yj =K1/2 2v

∂yi∂yjK1/2 4 yi ∂v

∂yj +K1/2

16 yiyjvK1/2 4 yj∂v

∂yi

,

on the other hand, belongs toL2(K)because ofvH22(RN)and the following lemma. Then, we obtainu=K1/2vH2(K)and the proof is complete. 2

Lemma 2.3.IfvH22(RN), then it holds that yi

∂v

∂yjL2 RN

(i, j=1, . . . , N ).

(9)

Proof. Henceforth,Cdenotes a generic large positive constant. It suffices to show y· ∇v2CvH2

2(RN) (20)

forvC0(RN), where vH2

2(RN)=

|α|2

Dαv 2

2+ yαv 2

2

1/2 .

This inequality is obtained by

RN

yi2 ∂v

∂yi 2

dy= −

RN

∂yj

yi2∂v

∂yj

v dy= −

RN

ijyi ∂v

∂yjv+yi22v

∂yj2v

dy

2yiv2· ∂v

∂yj

2

+ yi2v

2· 2v

∂yj2

2

,

and the proof is complete. 2

Lemma 2.4.The operatorA=Lp11 inL2(K), positive, self-adjoint, and with the compact inverse inL2(K), is provided with the following properties:

1. D(A) Lq(K)for

q

⎧⎨

=2∗∗ (N5),

∈ [2,∞) (N=4),

∈ [2,∞] (N=3), where2∗∗=2N/(N−4).

2. v2p,KCAN/(N+2)v2,K forvD(AN/(N+2)), whereC >0is a constant.

3. lims0sγAγesAv2,K=0, whereγ >0andvL2(K).

Proof. The last fact is a consequence of the general theory, becauseAis a positive self-adjoint operator inL2(K), see [9]. To show the first and the second facts, we use the relation derived from the interpolation theory, see [7], that is,

D Aθ

=

L2(K), H2(K)

θH(K), K1/2:H(K)

L2 RN

, H22 RN

θ is an isomorphism, whereθ(0,1).

In fact, we have H2N/(N+2)

RN

= L2

RN , H2

RN

N/(N+2)L2p RN

, Lp(K), Lq(K)

θ=

K1/pLp RN

, K1/qLq RN

θ=K1/rLr RN

=Lr(K), K1/(2p):H2p(K)L2p

RN

is an isomorphism, and therefore,

D

AN/(N+2)

= H2N/(N+2)(K)∼=K1/2 L2

RN , H22

RN

N/(N+2)

K1/2 L2

RN , H2

RN

N/(N+2)=K1/2H2N/(N+2) RN K1/2L2p

RN∼=K1/2+1/(2p)L2p(K) L2p(K).

This means the second case.

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The first case is proven as follows. IfN=3, we haveH2(RN) Lr(RN)for 2r∞. Then, it holds that D(A) = H2(K)∼=K1/2H22

RN

K1/2H2 RN K1/2Lr

RN

Lq(K) for 2< qr,r >2 andr=q=2, and therefore,

H2(K) Lq RN for any 2q∞.

IfN=4, we haveH2(RN)Lr(RN)for anyr∈ [2,∞). Then, it holds that D(A) = H2(K)∼=K1/2H22

RN

K1/2H2 RN K1/2Lr

RN

Lq(K) for 2< qr,r >2 andr=q=2, and therefore,

H2(K) Lq(K)

for any 2q <∞. Finally, ifN5, it holds that H2(K)=K1/2H22

RN

K1/2L2∗∗

RN

=K(1/2)+(1/2∗∗)L2∗∗(K) L2∗∗(K).

The proof is complete. 2

Once Lemma 2.4 is proven, Proposition 1.1 is shown similarly to [9]. It suffices to use f (u)−f (v)

2,KC

u2p,K+ v2p,K

p1

uv2p,K

forf (u)= |u|p1u. The following proposition is also proven similarly.

Proposition 2.1.Ifu0H1(K)andv=v(·, s)denotes the solution to(4)–(5), then we have the following properties:

1. t

svr(r)22,Kdr+JK(v(t ))=JK(v(s))fort, s∈ [0, S).

2. s∈ [0, S)→JK(v(s))is monotone decreasing.

3. v(s0)WK(resp.VK)v(s)WK (resp.VK)fors∈ [s0, S).

4. 12dsdv(s)22,K+IK(v(s))=0fors∈ [0, S).

The H1(K)-solutionv=v(·, s)to (4)–(5) is regarded as theH1(K)-solutionu=u(·, t )to (1)–(2) through the transformation (3). It is also theL1-mild solution of [16], and is provided with the following properties.

Proposition 2.2.Ifu0H1(K), we have d

dtJ u(t )

= − ut(t ) 2

2 and d

dt u(t ) 2

2=I u(t ) for the solutionu=u(·, t )to(1)–(2), where

J (u)=1

2∇u22− 1

p+1upp++11 and I (u)= ∇u22upp++11. 3. Stable and unstable sets

In this section we prove Propositions 1.3 and 1.4.

Lemma 3.1.Ifv=v(·, s)is the solution to(4)–(5)satisfyingv(s0)WKfor somes0∈ [0, T ), then it holds that v(s) p+1

p+1,K(1γ ) v(s) 2

2,Kλ v(s) 2

2,K

(21)

fors∈ [s0, T ), whereγ(0,1)andλ=p11.

(11)

Proof. First, Proposition 1.2 implies S0(p+1)/2vpp++11,K

v22,Kλv22,K

(p+1)/2

v22,Kλv22,K

v22,Kλv22,K(p1)/2

forvH1(K). Next, ifvWK it holds that JK(v)= p−1

2(p+1)

v22,Kλv22,K + 1

p+1IK(v)

p−1

2(p+1)

v22,Kλv22,K

p−1

2(p+1)

v22,Kλv22,K

0.

Letv=v(·, s)be the solution to (4)–(5) satisfyingv(s0)WK. Thenv(s)WK holds fors∈ [s0, T )by Proposi- tion 2.1. Using the above inequalities, we obtain

S02/2 v(s) p+1

p+1,K

2(p+1) p−1 JK

v(s)(p1)/2v(s) 2

2,Kλ v(s) 2

2,K

2(p+1) p−1 JK

v(s0)(p1)/2v(s) 2

2,Kλ v(s) 2

2,K

for 2=p+1. Since d0= p−1

2(p+1)S(p0 +1)/(p1)> JK v(s0)

,

it holds that

γ≡1−S02/2

2(p+1) p−1 JK

v(s0)(p1)/2

(0,1).

Then, inequality (21) follows. 2

Proof of Proposition 1.3. First, we showT = +∞, assumingv(s0)WK for somes0∈ [0, T ). In fact, ifvWKis the case, then

vpp++11<v22,Kλv22,K< 2

p+1vpp++11,K+2d0

and hence

vpp++11< S0n/2

byp=nn+22 andd0=1nSn/2. This implies

v22,Kλv22,K< 2

p+1vpp++11,K+2d0< S0n/2. Sincev(s0)WK, we obtain

lim sup

sT

v(s) 2

2,Kλ v(s) 2

2,K

< S0n/2, lim sup

sT

v(s) p+1

p+1< S0n/2 (22)

and hence lim sup

tT

v(s)

2,K<+∞ (23)

by Proposition 1.2.

(12)

Inequality (23) then implies S0 u(t ) 2

p+1u(t ) 2

2= ∇v(s) 2

2v(s) 2

2,KC

with a constantC >0 independent oft∈ [0, T0), whereT0=eT −1, and therefore,

tlimT0

J u(t )

>−∞

forJ (u)=12u22p+11upp++11. Then, the blow-up analysis guarantees lim sup

tT0

u(t ) p+1

p+1S0N/2

similarly to the bounded domain case, see [11], and therefore, lim sup

sT

v(s) p+1

p+1,Klim sup

sT

v(s) p+1

p+1=lim sup

tT0

u(t ) p+1

p+1S0N/2, a contradiction to (22). Thus,T = +∞follows.

The proof of (12) is similar to that of [9]. First,vWK implies JK(v) p−1

2(p+1)λ)v22,K (24)

with 0< λ=p11 < λ by (22) and Lemma 2.1. Ifv=v(·, s)is the solution satisfyingv(s0)WK for somes0∈ [0,+∞), then it holds that

s1

s

IK

v(r) dr=1

2 v(s) 2

2,Kv(s1) 2

2,K

1

2 v(s) 2

2,K p+1

(p−1)(λλ)JK v(s)

(25) by Proposition 2.1 and (24), wheres0ss1. Since Lemma 3.1 implies

γv(s) 2

2,Kλ v(s) 2

2,K

IK v(s) byv(s)WK, it follows that

JK

v(s)

= p−1

2(p+1) ∇v(s) 2

2,Kλ v(s) 2

2,K

+ 1 p+1IK

v(s)

p−1

2γ (p+1)+ 1 p+1

IK

v(s)

. (26)

Inequalities (25) and (26) imply +∞

s

JK

v(r)

drMJK

v(s)

with a constantM >0 independent ofs∈ [s0,+∞). Then, inequality (12) is obtained by Komornik’s method, see [17], and the proof is complete. 2

Lemma 3.2.Ifv=v(·, s)is anH1(K)-solution to(4)–(5), satisfyingv(s0)VK for somes0∈ [0, T ), then there is δ >0such that

v(s) p+1

p+1,K(1+δ) v(s) 2

2,Kλ v(s) 2

2,K

(27)

fors∈ [s0, T ).

(13)

Proof. IfvVK, we haveIK(v) <0, and therefore, 2(p+1)

p−1 d0{∇v22,Kλv22,K}(p+1)/(p1) {vp2+,K1}2/(p1)

{∇v22,Kλv22,K}(p+1)/(p1)

{∇v22,Kλv22,K}2/(p1) = ∇v22,Kλv22,K (28) by Lemma 1.2, (11), andλ> λ=1/(p−1). Proposition 2.1, on the other hand, implies

IK v(s)

=p−1

2 ∇v(s) 2

2,Kλ v(s) 2

2,K

(p+1)JK

v(s)

p−1

2 ∇v(s) 2

2,Kλ v(s) 2

2,K

(p+1)JK

v(s0)

=p−1

2 ∇v(s) 2

2,Kλ v(s) 2

2,K

(p+1)(1−0)d0 (29) forss0, where

0=1−JK(v(s0)) d0 >0.

We shall show p−1

2 ∇v(s) 2

2,Kλ v(s) 2

2,K

(p+1)(1−0)d0 δ v(s) 2

2,Kλ v(s) 2

2,K

(30)

forδ=(p−1)0/2>0. Then, (27) will follow from (29).

For this purpose, we use p−1

2 ∇v(s) 2

2,Kλ v(s) 2

2,K

(p+1)(1−0)d0δ v(s) 2

2,Kλ v(s) 2

2,K

= p−1

2 −δv(s) 2

2,Kλ v(s) 2

2,K

(p+1)(1−0)d0

=p−1 2 · 1

d0·JK

v(s0) v(s) 2

2,Kλ v(s) 2

2,K

(p+1)JK

v(s0)

=p−1 2 · 1

d0·JK

v(s0) v(s) 2

2,Kλ v(s) 2

2,K−2(p+1)d0

p−1

.

The right-hand side of the above inequality is non-negative by (28), and therefore, (30) follows. 2

Proof of Proposition 1.4. The argument of [9] for the case of the bounded domain is not valid here, because Lp+1(K)L2(K)does not arise. To avoid this difficulty, we suppose the contrary,T = +∞. It holds thatv(s)VK fors∈ [s0,+∞)by Proposition 2.1, and hence

IK v(s)

δ v(s) 2

2,Kλ v(s) 2

2,K

δ N

2 − 1

p−1 v(s) 2

2,K

by (6) and Lemma 3.2. This means 1

d

ds v(s) 2

2,Kδ1 v(s) 2

2,K

by Proposition 2.1, where δ1=δ

N

2 − 1

p−1

>0, and therefore,

Références

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