Home Solutions with Prescribed Local Blow-up Surface for the Nonlinear Wave Equation
Article Open Access

Solutions with Prescribed Local Blow-up Surface for the Nonlinear Wave Equation

  • Thierry Cazenave EMAIL logo , Yvan Martel and Lifeng Zhao
Published/Copyright: September 18, 2019

Abstract

We prove that any sufficiently differentiable space-like hypersurface of 1+N coincides locally around any of its points with the blow-up surface of a finite-energy solution of the focusing nonlinear wave equation ttu-Δu=|u|p-1u on ×N, for any 1N4 and 1<pN+2N-2. We follow the strategy developed in our previous work (2018) on the construction of solutions of the nonlinear wave equation blowing up at any prescribed compact set. Here to prove blow-up on a local space-like hypersurface, we first apply a change of variable to reduce the problem to blowup on a small ball at t=0 for a transformed equation. The construction of an appropriate approximate solution is then combined with an energy method for the existence of a solution of the transformed problem that blows up at t=0. To obtain a finite-energy solution of the original problem from trace arguments, we need to work with H2×H1 solutions for the transformed problem.

MSC 2010: 35L05; 35B44; 35B40

1 Introduction

1.1 Main Result

We consider the nonlinear energy-subcritical or -critical wave equation

(1.1) t t u - Δ u = | u | p - 1 u , ( t , x ) × N ,

for N1 and 1<pN+2N-2 (1<p< if N=1,2). For simplicity, we restrict ourselves to space dimensions 1N4. In this case, it is well known that the Cauchy problem for (1.1) is locally well posed in the energy space H1(N)×L2(N). (See Remark B.1.)

When a solution u with initial data at t=t0 is not globally defined ([14, 23, 1]), we introduce its maximal influence domain whose upper boundary is a 1-Lipschitz graph. See [1, Section III.2] and, for the present setting, Section 1.2.

We prove that any sufficiently differentiable space-like hypersurface of 1+N coincides locally around any of its points with the blow-up surface of a finite-energy solution of the focusing nonlinear wave equation (1.1). More precisely, our main result is the following.

Theorem 1.1.

Let 1N4 and 1<pN+2N-2. Let

(1.2) q 0 = 2 2 p + 2 p - 1 + 3 .

Let φ:RNR be a function of class Cq0 such that

(1.3) φ ( 0 ) = 0    𝑎𝑛𝑑    | φ ( x ) | < 1 for all  x N .

There exist ε>0, τ0>0 and (u0,u1)H1(RN)×L2(RN) such that the upper boundary of the maximal influence domain of the solution u of (1.1) with initial data (u,tu)(0)=(u0,u1) contains the local hypersurface {(t,x):t=τ0+φ(x) and |x|<ε}. Moreover, u blows up on this local hypersurface in the sense that if |x0|<ε and σ(|φ(0)|,1), then

(1.4) lim inf t τ 0 + φ ( x 0 ) 1 τ 0 + φ ( x 0 ) - t t τ 0 + φ ( x 0 ) 𝑑 t { | x - x 0 | < σ ( τ 0 + φ ( x 0 ) - t ) } | t u | 2 𝑑 x > 0 .

It follows from (1.4) that tu concentrates on the local hypersurface {(t,x):t=τ0+φ(x) and |x|<ε} in the sense of L2. In particular, this local hypersurface is a blow-up surface for the solution u.

Compared to previous results (see Section 1.3), Theorem 1.1 applies to any space dimension N4 and any subcritical or critical p. Moreover, our strategy is different. It mainly relies on the construction of an ansatz by elementary ODE arguments. (See Section 1.4.)

Remark 1.2.

In the definition of q0 above, we use the notation yy for the floor function which maps y to the greatest integer less than or equal to y. Note that q0=7 for p>5 and q0 as p1+. See Remark 2.3 for comments on this condition.

1.2 Definition of the Maximal Influence Domain

We adapt the presentation of [1, Chapter III] (see also [24]) to the framework of H1×L2 solutions for the energy subcritical or critical wave equation in space dimension N1. Let

+ 1 + N = [ 0 , + ) × N .

For any (t,x)+1+N, we define the open (in +1+N) backward cone

(1.5) C ( t , x ) = { ( s , y ) + 1 + N : | x - y | < t - s } .

Definition 1.3.

An open set Ω of +1+N is called an influence domain if (t,x)Ω implies C¯(t,x)Ω.

For Ω an influence domain containing {0}×N, define for any xN,

ϕ ( x ) = sup { t 0 : ( t , x ) Ω } .

From the above definition, either ϕ is identically , or it is finite for all xN. In the latter case, ϕ is a 1-Lipschitz continuous function.

Recall that by the Cauchy theory in the energy space H1(N)×L2(N), for any (u0,u1)H1(N)×L2(N) there exist T>0 and a solution (u,tu) of (1.1) belonging to C([0,T],H1(N))C([0,T],L2(N)). These solutions are unique in that class, except for the 3D critical case p=5, where uniqueness is known in C([0,T],H1(3))C([0,T],L2(3))L8((0,T)×3). (See Remark B.1 for details.)

From the local Cauchy theory, it is standard to define the notion of maximal solution and maximal time of existence Tmax(u0,u1)>0; if Tmax(u0,u1)=, the solution is globally defined, otherwise it blows up as tTmax(u0,u1) (in a suitable norm related to the resolution of the Cauchy problem).

To define the notion of maximal influence domain corresponding to an initial data, we first extend the Cauchy theory of N to truncated cones. For x0N and 0τR, we define

(1.6) E ( x 0 , R , τ ) = { ( t , x ) + 1 + N : 0 t < τ  and  | x - x 0 | < R - t } .

Suppose that x0N and R>0, and let (u0,u1)H1(B(x0,R))×L2(B(x0,R)). Consider any extension (u~0,u~1)H1(N)×L2(N) of (u0,u1), i.e. any function satisfying

u ~ 0 = u 0 and u ~ 1 = u 1 on  B ( x 0 , R ) .

Next, consider the solution (u~,tu~) of (1.1) corresponding to the initial data (u~0,u~1) defined on a time interval [0,τ~], where τ~>0, given by the above Cauchy theory. Note that if (uˇ0,uˇ1)H1(N)×L2(N) is another extension of (u0,u1) and (uˇ,tuˇ) is the corresponding solution of (1.1) on a time interval [0,τˇ] (τˇ>0), then by finite speed of propagation (see Proposition B.2), the two solutions (u~,tu~) and (uˇ,tuˇ) are identically equal on the truncated cone E(x0,R,min(τ~,τˇ)). In this way, we have defined a notion of solution of (1.1) on E(x0,R,τ) for some τ>0 which is independent of the extension chosen and includes a uniqueness property. From now on, for any (u0,u1)H1(B(x0,R))×L2(B(x0,R)) and any τ>0, we refer to the solution of (1.1) on E(x0,R,τ) in this sense.

By time-translation invariance of the equation and considering the map (t,x)E(x0,R,τ)u(t0+t,x), we extend this definition to any truncated cone in +1+N.

Now, we define the notion of solution in an influence domain.

Definition 1.4.

Let (u0,u1)H1(N)×L2(N). Let Ω be an influence domain. We say that (u,tu) is a solution of (1.1) on Ω with initial data (u0,u1) if the following hold:

  1. u H loc 1 ( Ω ) .

  2. For any t00, x0N and R>0 such that [0,t0]×B(x0,R)Ω, it holds

    u | [ 0 , t 0 ] × B ( x 0 , R ) C ( [ 0 , t 0 ] , H 1 ( B ( x 0 , R ) ) ) C 1 ( [ t 1 , t 2 ] , L 2 ( B ( x 0 , R ) ) ) ;

    moreover, u(0)u0 and tu(0)u1 on B(x0,R).

  3. For any (t0,x0)Ω and R>0 such that {t0}×B(x0,R)Ω, there exists τ with 0<τ<R such that (t,x)E(x0,R,τ)u(t0+t,x) is solution of (1.1) in the above sense.

Definition 1.5.

For any (u0,u1)H1(N)×L2(N), we denote Ωmax(u0,u1) the union of all the influence domains Ω such that there exists a solution (u,tu) with initial data (u0,u1) on Ω in the sense of Definition 1.4.

It follows that, for any initial data (u0,u1)H1(N)×L2(N), Ωmax(u0,u1) is the maximal influence domain on which a (unique) solution of (1.1) with initial data (u0,u1) exists. Finally, in the case Tmax(u0,u1)<+ the upper boundary of the maximal influence domain is the graph of the 1-Lipschitz application

x N ϕ ( x ) = sup { t 0 : ( t , x ) Ω max ( u 0 , u 1 ) } ( 0 , ) .

1.3 Previous Results

Under certain assumptions, it is known that the upper boundary of the maximal influence domain is a blow-up surface in the sense that the solution blows up (at the same rate as the ODE) on the surface, and the blow-up surface is C1. See [4, 3] and [1, Chapter III]. See also [9, 25, 26] and the references therein for further blow-up results.

Constructing solutions of the wave equation (1.1) with prescribed blow-up surface is a classical question. Results similar to Theorem 1.2 have been proved in several cases. For the wave equation with cubic nonlinearity, it is proved in [18, Theorem 10.14, p. 192] that there exist solutions (locally defined around the blow-up surface) blowing up exactly on a prescribed surface of class Hr(N) with r>N2+7. In [22, Theorem 1.1], an analogous result is proved in space dimension 1 for equation (1.1) for any p>1. For previous results, see [1, 20, 21, 17, 16].

A related question is the study of the blow-up set, which is the intersection of the blow-up surface with the hyperplane {t=Tmax}. In [22, Corollary 1.2], it is proved for (1.1) in space dimension 1 that, given any compact subset K of , there exist smooth initial data for which the blow-up set is precisely K. This result is extended in [6, Theorem 1.1] to any space dimension and any energy-subcritical p. See [19] for a related result.

1.4 Strategy of the Proof of Theorem 1.1

We follow closely the strategy of [6] (see also [7]). It is based on the construction of an appropriate approximate solution which blows up at t=0, combined with an energy method for the existence of an exact solution that also blows up at t=0. Here, we wish to prove blowup on a local space-like hypersurface. In order to apply the previously recalled strategy, we therefore apply a change of variable to reduce the problem to blowup at t=0 (Section 2.1). By doing so, we are led to study the transformed equation

( 1 - | ψ | 2 ) s s v - 2 ψ s v - ( Δ ψ ) s v - Δ v = f ( v )

in the dual variables (s,y)×N. The construction of an appropriate ansatz for this equation (Sections 2.2 and 2.3) is similar to the construction made in [6]. In particular, it is based on elementary ODE arguments. The energy method for this transformed equation requires a smallness condition on ψL, and yields an existence time that depends on ψ. See Section 3. This smallness condition can be met through a localization argument (Section 4.1) and a Lorentz transform (Sections 4.24.4). Going back to the original variables, to obtain a solution in the framework of H1×L2, we are forced to apply a trace argument which requires higher regularity of the solution v (Section 4.5). This is why we use the energy method for v in the framework of H2×H1. The restriction 1N4 implies that H2Lq for every 2q<, which simplifies the energy argument. The blow-up estimate (1.4) is a consequence of an ODE blow-up estimate for the solution of the transformed equation, and the change of variable (Section 4.6).

1.5 Notation

We fix a smooth, even function χ: satisfying

(1.7) χ 1  on  [ 0 , 1 ] χ 0  on  [ 2 , + ) χ 0 χ 1  on  [ 0 , + ) .

Let f(u)=|u|p-1u and F(u)=0uf(v)𝑑v. For future reference, we state and justify two Taylor formulas involving the functions F and f (see Introduction of [7] for proofs). Let p¯=min(2,p). For any u>0 and any v, it holds

(1.8) | F ( u + v ) - F ( v ) - F ( u ) v - 1 2 F ′′ ( u ) v 2 | | v | p + 1 + u p - p ¯ | v | p ¯ + 1 ,
(1.9) | ( f ( u + v ) - f ( u ) - f ( u ) v ) v | | v | p + 1 + u p - p ¯ | v | p ¯ + 1 ,
(1.10) | f ( u + v ) - f ( u ) | | u | - 1 | v | p + | u | p - 2 | v | ,
(1.11) | f ( u + v ) - f ( u ) - f ( u ) v - 1 2 f ′′ ( u ) v 2 | u - 1 | v | p + 1 + u p - p ¯ - 1 | v | p ¯ + 1 .

In the present article, we use multi-variate notation and results from [8]. For β=(β1,,βN)N and x=(x1,,xN)N, we set

| β | = j = 1 N β j , β ! = j = 1 N ( β j ! ) , x β = j = 1 N x j β j , x β = | β | x 1 β 1 x N β N for  | β | > 0 , x 0 = Id .

For β,βN, we write ββ provided βjβj, for all j=1,,N. Note that in this case |β-β|=|β|-|β|. For ββ, we denote

( β β ) = j = 1 N ( β j β j ) = β ! ( β ! ) ( β - β ) ! .

Recall that for two functions g,h:1+N, Leibniz’s formula writes

(1.12) x β ( g h ) = β β ( β β ) ( β g ) ( β - β h ) .

We write ββ provided one of the following holds:

  1. | β | < | β | ,

  2. | β | = | β | and β1<β1,

  3. | β | = | β | , β1=β1,,β=β and β+1<β+1 for some 1<N.

We recall the Faa di Bruno formula (see in [8, Corollary 2.10]). Let n=|β|1. Then, for functions f: and g:1+N,

(1.13) x β ( f g ) = r = 1 n ( f ( r ) g ) P ( β , r ) ( β ! ) = 1 n ( x β g ) r ( r ! ) ( β ! ) r

where

P ( β , r ) = { ( r 1 , , r n ; β 1 , , β n ) : there exists  1 m n  such that  r = 0  and  β = 0  for  1 n - m ;
r > 0  for  n - m + 1 n ;
and  0 β n - m + 1 β n  are such that  = 1 n r = r , = 1 n r β = β } .

We will also need to differentiate in space and time, so we define multi-index notation in space-time: 𝝂=(α,β1,,βN)1+N, β=(β1,,βN), and

| 𝝂 | = α + | β | , 𝝂 ! = α ! β ! , 𝝂 = s α x β .

For 𝝂,𝝂1+N, we write 𝝂𝝂 provided αα and βjβj, for all j=1,,N. In such a case, we denote

( 𝝂 𝝂 ) = ( α α ) ( β β ) .

Then, for two functions g,h:1+N,

(1.14) 𝝂 ( g h ) = 𝝂 𝝂 ( 𝝂 𝝂 ) ( 𝝂 g ) ( 𝝂 - 𝝂 h ) .

We write 𝝂𝝂 provided one of the following holds:

  1. | 𝝂 | < | 𝝂 | ,

  2. | 𝝂 | = | 𝝂 | and α<α,

  3. | 𝝂 | = | 𝝂 | , α=α and β1<β1,

  4. | 𝝂 | = | 𝝂 | , α=α, β1=β1,,β=β and β+1<β+1 for some 1<N.

Last, we write in this context the Faa di Bruno formula. Let n=|𝝂|1. Then, for functions f: and g:1+N,

(1.15) 𝝂 ( f g ) = r = 1 n ( f ( r ) g ) P ( 𝝂 , r ) ( 𝝂 ! ) = 1 n ( 𝝂 g ) r ( r ! ) ( 𝝂 ! ) r ,

where

P ( 𝝂 , r ) = { ( r 1 , , r n ; 𝝂 1 , , 𝝂 n ) : there exists  1 m n  such that  r = 0  and  𝝂 = 0  for  1 n - m ;
r > 0  for  n - m + 1 n ;
and  0 𝝂 n - m + 1 𝝂 n  are such that  = 1 n r = r , = 1 n r 𝝂 = 𝝂 } .

2 Blow-up Ansatz

2.1 Change of Variables

Let ψ𝒞q0(N,), where q0 is defined by (1.2), be such that for some R2,

(2.1) ψ ( x ) = 0 for  | x | R    and    ψ L < 1 .

We perform a change of variable related to ψ

u ( t , x ) = v ( s , x ) , s = ψ ( x ) - t

so that s>0 is equivalent to t<ψ(x). Then the following holds: for j=1,,N,

t t u = s s v ,
x j u = ( x j ψ ) s v + x j v ,
x j x j u = ( x j x j ψ ) s v + ( x j ψ ) 2 s s v + 2 ( x j ψ ) x j s v + x j x j v ,
Δ u = ( Δ ψ ) s v + | ψ | 2 s s v + 2 ψ s v + Δ v .

Therefore, equation (1.1) on u(t,x) rewrites

(2.2) ( 1 - | ψ | 2 ) s s v - 2 ψ s v - ( Δ ψ ) s v - Δ v = f ( v ) .

In this section, we focus on finding ansatz for this equation under assumption (2.1).

2.2 First Blow-up Ansatz

Let

(2.3) J = 2 p + 2 p - 1 so that q 0 = 2 J + 3 ,

where q0 is defined by (1.2), and let

(2.4) k q 0 + 1

be an integer.

We consider the function A:N[0,+[ given by

(2.5) A ( x ) := { 0 if  | x | 1 , ( | x | - χ ( x ) ) k if  1 < | x | 2 , | x | k if  | x | > 2 .

It follows that A is of class 𝒞k-1 and that, for any βN, with |β|k-1,

(2.6) { A 0  and  | x β A | A 1 - | β | k on  N , A ( x ) = | x | k for any  x N  such that  | x | 2 .

We define a basic blow-up ansatz V0, for s>0 and xN,

(2.7) V 0 ( s , x ) = κ ( x ) ( s + A ( x ) ) - 2 p - 1 ,

where

κ ( x ) = κ 0 ( 1 - | ψ ( x ) | 2 ) 1 p - 1 , κ 0 = [ 2 ( p + 1 ) ( p - 1 ) 2 ] 1 p - 1 ,

which satisfies

( 1 - | ψ | 2 ) s s V 0 = V 0 p on  ( 0 , + ) × N .

Since the functions ψ and A are of class 𝒞q0, we remark that the function V0 is of class 𝒞 in the variable s>0 and of class 𝒞q0-1 in the variable xN.

In view of (2.2), it is natural to set

0 = - ( 1 - | ψ | 2 ) s s V 0 + 2 ψ s V 0 + ( Δ ψ ) s V 0 + Δ V 0 + f ( V 0 )
(2.8) = 2 ψ s V 0 + ( Δ ψ ) s V 0 + Δ V 0 .

We gather in the next lemma the properties of V0 and 0.

Lemma 2.1.

The function V0 satisfies

(2.9) ( 1 - | ψ | 2 ) 1 2 s V 0 = - ( 2 p + 1 V 0 p + 1 ) 1 2 , ( 1 - | ψ | 2 ) s s V 0 = V 0 p .

Moreover, for any αN, βNN, ρR, 0<s<1, xRN, the following hold:

  1. If 0 | β | q 0 - 1 and | x | R , then

    (2.10) | s α x β ( V 0 ρ ) | V 0 ρ + ( α + | β | k ) p - 1 2 .

  2. If | β | q 0 - 3 and | x | R , then

    (2.11) | s α x β 0 | V 0 p + 1 2 + ( α + 1 + | β | k ) p - 1 2 .

  3. If | x | > R , then

    (2.12) | s α x β V 0 | | x | - ( 2 p - 1 + α ) k - | β | ,
    (2.13) | s α x β 0 | | x | - ( 2 p - 1 + α ) k - | β | - 2 .

Furthermore, if |x0|<1, then for any σ>0,

(2.14) lim inf s 0 s N + 2 - ( N - 2 ) p 2 ( p - 1 ) s V 0 ( s ) L 2 ( | x - x 0 | < σ s ) > 0 .

Proof.

First, we observe that the function κ is constant for |x|>R and satisfies κ1, |xβκ|1 on N, for any |β|q0-1.

Proof of (2.9). This follows from direct computations.

Proof of (2.10). For 0<s<1 and |x|R, one has 0<s+A(x)1 and thus, V01. We introduce some notation:

h ( z ) = z - 2 p - 1 for  z > 0 , W ( s , x ) = s + A ( x ) .

In particular, V0(s,x)=κ(x)h(W(s,x)). Let α0. Since |h(α)(z)||z|-2p-1-α, we have

s α V 0 = κ ( x ) h ( α ) ( W ( s , x ) ) and so | s α V 0 | | V 0 | 1 + α p - 1 2 .

Let βN be such that 1|β|q0-1. Using (1.12), we have

s α x β V 0 = β β ( β β ) ( x β - β κ ) ( x β [ h ( α ) ( W ) ] ) .

For 0ββ, it holds |xβ-βκ|1. Thus, for β=0 in the above sum, we have

| ( x β κ ) h ( α ) ( W ) | | V 0 | 1 + α p - 1 2 .

For 1|β|, ββ, setting n=|β| and using (1.13),

x β [ h ( α ) ( W ) ] = r = 1 n [ h ( α + r ) ( W ) ] P ( β , r ) ( β ! ) l = 1 n ( x β l W ) r l ( r l ! ) ( β l ! ) r l ,

where

P ( β , r ) = { ( r 1 , , r n ; β 1 , , β n ) : there exists  1 m n  such that  r = 0  and  β = 0  for  1 n - m ;
r > 0  for  n - m + 1 n ;
and  0 β n - m + 1 β n  are such that  = 1 n r = r , = 1 n r β = β } .

As before, we use for r1, |h(α+r)(W)|W-2p-1-r-α. Moreover, using the assumption (2.6) on A, we have, for 1|β|q0-1,

| x β W | | x β A | A 1 - | β | k .

Since =1nr=r, =1nr|β|=|β| and |β|q0-1k-1, we obtain

| x β [ h ( α ) ( W ) ] | r = 1 n W - 2 p - 1 - r - α P ( β , r ) [ A 1 - | β | k ] r
r = 1 n W - 2 p - 1 - r - α A r - | β | k W - 2 p - 1 - α - | β | k V 0 1 + ( α + | β | k ) p - 1 2 .

We obtain, for all 0|β|q0-1 and |x|R,

(2.15) | s α x β V 0 | V 0 1 + ( α + | β | k ) p - 1 2 ,

which proves (2.10) for ρ=1.

We use the notation 𝝂=(α,β1,,βN) as in the context of formula (1.15). Let n=|𝝂|1. Then, by (1.15), for ρ,

𝝂 ( V 0 ρ ) = r = 1 n [ ρ ( ρ - r + 1 ) ] V 0 ρ - r P ( 𝝂 , r ) ( 𝝂 ! ) = 1 n ( 𝝂 V 0 ) r ( r ! ) ( 𝝂 ! ) r ,

where

P ( 𝝂 , r ) = { ( r 1 , , r n ; 𝝂 1 , , 𝝂 n ) : there exists  1 m n  such that  r = 0  and  𝝂 = 0  for  1 n - m ;
r > 0  for  n - m + 1 n ;
and  0 𝝂 n - m + 1 𝝂 n  are such that  = 1 n r = r , = 1 n r 𝝂 = 𝝂 } .

Using (2.15) and =1nr=r, =1nrα=α, =1nrβ=β in P(𝝂,r), we estimate

| 𝝂 ( V 0 ρ ) | r = 1 n V 0 ρ - r P ( 𝝂 , r ) = 1 n V 0 r [ 1 + ( α + | β | k ) p - 1 2 ]
r = 1 n V 0 ρ - r V 0 r + ( α + | β | k ) p - 1 2 V 0 ρ + ( α + | β | k ) p - 1 2 .

Proof of (2.11). We estimate the three terms in (2.8). It follows from Leibniz’s formula (1.14), the properties of ψ, V01, and estimate (2.10) that, for |β|q0-3, and |x|R,

| s α x β [ ψ s V 0 ] | V 0 1 + ( 1 + α + 1 + | β | k ) p - 1 2 ,
| s α x β [ ( Δ ψ ) s V 0 ] | V 0 1 + ( 1 + α + | β | k ) p - 1 2 ,
| s α x β [ Δ V 0 ] | V 0 1 + ( α + 2 + | β | k ) p - 1 2 .

Using once more that V01 for |x|R and k1, these estimates imply (2.11).

Proof of (2.12). It follows from the properties of the functions ψ and A that

V 0 ( s , x ) = κ 0 ( s + | x | k ) - 2 p - 1 for any  | x | R .

Estimate (2.12) follows immediately. Then we have, for any |x|R,

| s α x β [ ψ s V 0 ] | = 0 ,
| s α x β [ ( Δ ψ ) s V 0 ] | = 0 ,
| s α x β [ Δ V 0 ] | | x | - ( 2 p - 1 + α ) k - | β | - 2 ,

which implies (2.13).

Proof of (2.14). Since |x0|<1, we have for s small |tV0|s-p+1p-1, and (2.14) follows. ∎

2.3 Refined Blow-up Ansatz

Starting from V0, we define by induction a refined ansatz to the nonlinear wave equation (2.2).

Let V0 be defined in (2.7) and let 0 be defined in (2.8). Let s0=1. For j1, let

v j = - 1 3 p + 1 [ 2 ( p + 1 ) 1 - | ψ | 2 ] 1 2 ( V 0 p + 1 2 0 s V 0 - p j - 1 𝑑 s + V 0 - p s s j - 1 V 0 p + 1 2 j - 1 𝑑 s ) ,
V j = V 0 + = 1 j χ v ,
j = - ( 1 - | ψ | 2 ) s s V j + 2 ψ s V j + ( Δ ψ ) s V j + Δ V j + f ( V j ) ,

where χj(x)=χ(A(x)rj) and 0<rj1, 0<sj1 are parameters to be defined for each j=1,,J. Since V0 is of class 𝒞 in s and of class 𝒞q0-1 in x, the above expressions make sense as continuous functions for j such that jJ. This restriction is due to the spatial derivatives in Vj in the expression of j.

Lemma 2.2.

There exist 0<rJr11 and 0<sJs11 such that for any 0jJ, for any αN, βNN, 0<ssj, xRN, the following hold:

  1. If 1 j J , |β|q0-2j-1 and |x|R, then

    (2.16) | s α x β v j | V 0 1 + ( - j + α + j + | β | k ) p - 1 2 .

  2. If 1 j J , then

    (2.17) | V j - V 0 | 1 4 ( 1 - 2 - j ) V 0 , | V j - V 0 | ( 1 - 2 - j ) ( 1 + V 0 ) - p - 1 4 V 0 ,
    (2.18) | s V j - s V 0 | V 0 1 + p - 1 2 k .

  3. If | β | q 0 - 2 ( j + 1 ) - 1 and | x | R , then

    (2.19) | s α x β j | V 0 p + 1 2 + ( - j + α + 1 + j + | β | k ) p - 1 2 .

  4. If | x | > R , then

    (2.20) | s α x β V j | | x | - ( 2 p - 1 + α ) k - | β | ,
    (2.21) | s α x β j | | x | - ( 2 p - 1 + α ) k - | β | - 2 .

Remark 2.3.

To complete the energy control in Section 3, we need an error estimate of the form

J L 2 s 2 p - 1 + δ ,

as in [6] (see (3.28)), as well as an estimate of the form sJL2s-1+δ (see the proof of (3.30)), with δ>0. This requires a sufficiently large J, see (2.3), and then a sufficiently large k. Compared with Lemma 2.3 (see also Remark 2.4) in [6], we need twice as many steps. This is due to the terms depending on sVj in the expression of the error term j. These necessary restrictions have the important consequence that the minimal regularity of the hypersurface that we can consider in Theorem 1.1 depends on p, see (2.3).

Proof of Lemma 2.2.

We observe that (2.19), (2.20) and (2.21) for j=0 are exactly (2.11), (2.12) and (2.13) in Lemma 2.1. We proceed by induction on j: for any 1jJ, we prove that estimate (2.19) for j-1 implies (2.16)–(2.19) for vj, Vj and j. Let s0=1.

Proof of (2.16). Let 1jJ. First, assuming (2.19) for j-1, we show the following estimates related to the two components of vj: for |β|q0-2j-1, 0<s<sj-1 and |x|R,

(2.22) | s α x β ( 0 s V 0 - p j - 1 𝑑 s ) | V 0 - p - 1 2 + ( - j + α + j + | β | k ) p - 1 2 ,
(2.23) | s α x β ( s s j - 1 V 0 p + 1 2 j - 1 𝑑 s ) | V 0 p + 1 + ( - j + α + j + | β | k ) p - 1 2 .

Indeed, we have by Leibniz’s formula

s α x β ( V 0 - p j - 1 ) = α α β β ( α α ) ( β β ) ( s α x β ( V 0 - p ) ) ( s α - α x β - β j - 1 ) ,

and thus using (2.10) and (2.19) for j-1, we obtain

| s α x β ( V 0 - p j - 1 ) | α α β β V 0 - p + ( α + | β | k ) p - 1 2 V 0 p + 1 2 + ( 1 - j + α - α + j + | β - β | k ) p - 1 2
V 0 ( - j + α + j + | β | k ) p - 1 2 .

For α=0, |β|q0-1k-1 and 1jJ, we note that

| x β ( V 0 - p j - 1 ) | V 0 - a p - 1 2 ( s + A ) a ,

where

a = j - j + | β | k = j ( 1 - 1 k ) - | β | k 0 .

This means that we can integrate this term on (0,s) for 0<ssj-1. We obtain

0 s | x β ( V 0 - p j - 1 ) | 𝑑 s ( s + A ) a + 1 V 0 - p - 1 2 + ( - j + j + | β | k ) p - 1 2 .

For α1,

| s α x β ( 0 s V 0 - p j - 1 𝑑 s ) | = | s α - 1 x β ( V 0 - p j - 1 ) | V 0 - p - 1 2 + ( - j + α + j + | β | k ) p - 1 2 ,

which proves (2.22). Similarly, using Leibniz’s formula, we check the estimate

| s α x β ( V 0 p + 1 2 j - 1 ) | V 0 p + 1 + ( 1 - j + α + j + | β | k ) p - 1 2 .

In particular, for α=0,

| x β ( V 0 p + 1 2 j - 1 ) | V 0 b p - 1 2 ( s + A ) - b ,

where, using 1jJ2p+2p-1,

b = 2 p + 2 p - 1 + 1 - j + j + | β | k 1 + j + | β | k > 1 .

Thus, by integration on (s,sj-1),

| x β ( s s j - 1 V 0 p + 1 2 j - 1 𝑑 s ) | ( s + A ) - b + 1 V 0 p + 1 + ( - j + j + | β | k ) p - 1 2 .

For α1,

| s α x β ( s s j - 1 V 0 p + 1 2 j - 1 𝑑 s ) | = | s α - 1 x β ( V 0 p + 1 2 j - 1 ) | V 0 p + 1 + ( - j + α + j + | β | k ) p - 1 2 ,

which proves (2.23).

Using estimates (2.10), (2.22), (2.23) and again Leibniz’s formula, we obtain, for all s(0,sj-1],

| s α x β ( V 0 p + 1 2 0 s V 0 - p j - 1 𝑑 s ) | V 0 1 + ( - j + α + j + | β | k ) p - 1 2 ,
| s α x β ( V 0 - p s s j - 1 V 0 p + 1 2 j - 1 𝑑 s ) | V 0 1 + ( - j + α + j + | β | k ) p - 1 2 .

These estimates imply (2.16) for vj on (0,sj-1].

Proof of (2.17)–(2.18). For j=1, we prove (2.17) as a consequence of (2.16). For 2jJ, we prove (2.17) as a consequence of (2.16) for j and (2.17) for j-1.

For |x|>R1, (2.6) implies A(x)2k2r12rj, thus χj=0 and Vj=V0.

For 0<ssj-1 and |x|<R, by (2.16) with α=0 and β=0, using the definition of χj and the bound V01, we have

χ j | v j | χ j V 0 1 - j ( 1 - 1 k ) p - 1 2 χ j V 0 1 - ( 1 - 1 k ) p - 1 2 χ j ( s + A ) 1 - 1 k V 0 ( s + r j ) 1 - 1 k V 0 .

Choosing 0<rj1 and 0<sjsj-1 sufficiently small, we impose, for s(0,sj],

χ j | v j | 2 - j - 2 V 0 and χ j | v j | 2 - j ( 1 + V 0 ) - p - 1 4 V 0 .

In the case j=1, this proves (2.17). For j2, combining this estimate with (2.17) for j-1, we find, for all s(0,sj] and xN,

= 1 j χ | v | 1 4 ( 1 - 2 - j ) V 0 and = 1 j χ | v | ( 1 - 2 - j ) ( 1 + V 0 ) - p - 1 4 V 0 ,

which is (2.17).

To prove (2.18), we note that by (2.16), and using AV0-p-12,

= 1 j χ | s v | = 1 j χ V 0 1 + ( 1 - ( 1 - 1 k ) ) p - 1 2 V 0 1 + p - 1 2 k .

Proof of (2.19). Note that (2.19) for j=0 was already checked. Now, for 1jJ, we prove (2.19) for j assuming (2.19) for j-1, (2.16) for vj and (2.17) for Vj. This suffices to complete the induction argument.

By direct computations, we briefly check that the function vj satisfies

(2.24) ( 1 - | ψ | 2 ) s s v j = f ( V 0 ) v j + j - 1 .

Indeed, we have

s v j = - 1 3 p + 1 [ 2 ( p + 1 ) 1 - | ψ | 2 ] 1 2 ( p + 1 2 s V 0 V 0 p - 1 2 0 s V 0 - p j - 1 𝑑 s - p s V 0 V 0 - p - 1 s s j - 1 V 0 p + 1 2 j - 1 𝑑 s ) ,

and thus, using (2.9),

( 1 - | ψ | 2 ) 1 2 s v j = 1 3 p + 1 [ 2 ( p + 1 ) 1 - | ψ | 2 ] 1 2 ( ( p + 1 2 ) 1 2 V 0 p 0 s V 0 - p j - 1 𝑑 s - p ( p + 1 2 ) - 1 2 V 0 - p + 1 2 s s j - 1 V 0 p + 1 2 j - 1 𝑑 s ) .

Differentiating in s again, and using (2.9), we obtain

( 1 - | ψ | 2 ) s s v j = p V 0 p - 1 v j + j - 1 ,

which is (2.24).

Using (2.24), Vj=Vj-1+χjvj and the definition of j-1, we have

j = j - 1 - χ j ( 1 - | ψ | 2 ) s s v j + 2 ψ s ( χ j v j ) + ( Δ ψ ) s ( χ j v j ) + Δ ( χ j v j ) + f ( V j ) - f ( V j - 1 )
= ( 1 - χ j ) j - 1 + 2 ψ s ( χ j v j ) + ( Δ ψ ) s ( χ j v j ) + Δ ( χ j v j ) + f ( V j ) - f ( V j - 1 ) - f ( V 0 ) χ j v j .

We estimate each term of the right-hand side above for |x|R.

For the first term, recall that for Arj, and any β, 1-χj=0 and xβχj=0. Moreover, for 0<s1, for x such that A(x)>rj and |x|R, one has A1 and V01. Thus, using (2.19) for j-1, we find

| s α x β [ ( 1 - χ j ) j - 1 ] | V 0 p + 1 2 + ( - j + α + 1 + j + | β | k ) p - 1 2 .

Now, we treat the next three terms in the expression of j. By Leibniz’s formula, the properties of ψ and χj, (2.16) and then V01, we have, for 0<ssj and |x|<R,

| s α x β [ ψ s ( χ j v j ) ] | α = 1 α + 1 | β | | β | + 1 | s α x β v j | V 0 1 + ( - j + 1 + α + 1 + j + | β | k ) p - 1 2 ,
| s α x β [ ( Δ ψ ) s ( χ j v j ) ] | α = 1 α + 1 | β | | β | | s α x β v j | V 0 1 + ( - j + 1 + α + j + | β | k ) p - 1 2 ,
| s α x β [ Δ ( χ j v j ) ] | α = 1 α | β | | β | + 2 | s α x β v j | V 0 1 + ( - j + α + 2 + j + | β | k ) p - 1 2 ;

we see that these three terms are estimated by V0p+12+(-j+α+1+j+|β|k)p-12.

Finally, we estimate sαxβ[f(Vj)-f(Vj-1)-f(V0)χjvj] using Taylor expansions on f and its derivatives. We start with the case α=β=0. Recall that by (2.17), we have 0<34V0Vj54V0. The following Taylor expansions hold:

| f ( V j ) - f ( V j - 1 ) - f ( V j - 1 ) χ j v j | χ j 2 V 0 p - 2 v j 2

and

| f ( V j - 1 ) - f ( V 0 ) | V 0 p - 2 = 1 j - 1 χ | v | .

These estimates imply

| f ( V j ) - f ( V j - 1 ) - f ( V 0 ) χ j v j | χ j V 0 p - 2 | v j | = 1 j χ | v | .

For 1j, using (2.16) and next V01, we have

V 0 p - 2 | v j | | v | V 0 p - 2 V 0 1 - j ( 1 - 1 k ) p - 1 2 V 0 1 - ( 1 - 1 k ) p - 1 2
V 0 p - ( j + ) ( 1 - 1 k ) p - 1 2 V 0 p - ( j + 1 ) ( 1 - 1 k ) p - 1 2 .

Thus, |f(Vj)-f(Vj-1)-f(V0)χjvj|V0p+12+(-j+1+jk)p-12 is proved.

Now, we consider the case |α|+|β|1. By the Taylor formula with integral remainder we have for any V and w,

f ( V + w ) - f ( V ) - f ( V ) w = w 2 0 1 ( 1 - θ ) f ′′ ( V + θ w ) 𝑑 θ .

Therefore, using the notation 𝝂=(α,β1,,βN), by the Leibniz formula (1.14),

𝝂 [ f ( V + w ) - f ( V ) - f ( V ) w ] = 𝝂 𝝂 ( 𝝂 𝝂 ) ( 𝝂 - 𝝂 ( w 2 ) ) 0 1 ( 1 - θ ) 𝝂 [ f ′′ ( V + θ w ) ] d θ

and, by the Faa di Bruno formula (1.15), for 𝝂0, denoting n=|𝝂|,

(2.25) 𝝂 [ f ′′ ( V + θ w ) ] = r = 1 n f ( r + 2 ) ( V + θ w ) P ( 𝝂 , r ) ( 𝝂 ! ) = 1 n ( 𝝂 ( V + θ w ) ) r ( r ! ) ( 𝝂 ! ) r j .

To estimate the term 𝝂[f(Vj)-f(Vj-1)-f(Vj-1)χjvj], we apply these formulas to V=Vj-1 and w=χjvj. First, for 𝝂𝝂, using (2.16) and the properties of χ, we obtain

| 𝝂 - 𝝂 [ ( χ j v j ) 2 ] | 𝝂 ′′ 𝝂 - 𝝂 | 𝝂 ′′ ( χ j v j ) | | 𝝂 - 𝝂 - 𝝂 ′′ ( χ j v j ) |
V 0 2 + ( α - α - 2 j + 2 j + | β - β | k ) p - 1 2 .

Thus, for 𝝂=0 and θ[0,1], from (2.17), we obtain

| 𝝂 [ ( χ j v j ) 2 ] f ′′ ( V j - 1 + θ χ j v j ) | V 0 2 + ( α - 2 j + 2 j + | β | k ) p - 1 2 V 0 p - 2
V 0 p + 1 2 + ( α - j + 1 + j + | β | k ) p - 1 2 .

Second, for 𝝂0, 𝝂𝝂 and θ[0,1], from formula (2.25), using (2.10) and (2.17), we have (the definition of P(𝝂,r) implies =1nr=r, =1nr𝝂=𝝂)

| 𝝂 [ f ′′ ( V j - 1 + θ χ j v j ) ] | r = 1 n V 0 p - r - 2 P ( 𝝂 , r ) = 1 n ( V 0 1 + ( α + | β | k ) p - 1 2 ) r
r = 1 n V 0 p - r - 2 V 0 r + ( α + | β | k ) p - 1 2 V 0 p - 2 + ( α + | β | k ) p - 1 2 .

Thus, we have proved

| 𝝂 - 𝝂 [ ( χ j v j ) 2 ] 𝝂 [ f ′′ ( V j - 1 + θ χ j v j ) ] | V 0 p + 1 2 + ( - j + α + 1 + j + | β | k ) p - 1 2 ;

and so by integration in θ[0,1],

(2.26) | 𝝂 [ f ( V j ) - f ( V j - 1 ) - f ( V j - 1 ) χ j v j ] | V 0 p + 1 2 + ( - j + α + 1 + j + | β | k ) p - 1 2 .

We now estimate 𝝂[f(Vj)-f(Vj-1)-f(V0)χjvj]. For any V,W,w, we have

f ( V ) - f ( W ) = ( V - W ) 0 1 f ′′ ( W + θ ( V - W ) ) 𝑑 θ ,

and thus

𝝂 [ w ( f ( V ) - f ( W ) ) ] = 𝝂 𝝂 ( 𝝂 𝝂 ) ( 𝝂 - 𝝂 [ w ( V - W ) ] ) 0 1 𝝂 [ f ′′ ( W + θ ( V - W ) ) ] d θ .

Moreover, for 𝝂0, formula (2.25) (with V replaced by W, and w by V-W) yields

𝝂 [ f ′′ ( W + θ ( V - W ) ) ] = r = 1 n f ( r + 2 ) ( W + θ ( V - W ) ) P ( 𝝂 , r ) ( 𝝂 ! ) = 1 n ( 𝝂 ( W + θ ( V - W ) ) ) r ( r ! ) ( 𝝂 ! ) r .

To estimate the term 𝝂[χjvj(f(Vj-1)-f(V0))], we apply these formulas to V=Vj-1, W=V0 and w=χjvj.

For 𝝂𝝂, using (2.16) and Leibniz’s formula, we have, for 1j-1,

| 𝝂 - 𝝂 [ χ j v j χ v ] | V 0 2 + ( - j - + α - α + j + + | β - β | k ) p - 1 2
V 0 - p - 5 2 + ( - j + α - α + 1 + j + | β - β | k ) p - 1 2 .

For 𝝂=0 and θ[0,1], from (2.17), we obtain

| 𝝂 [ χ j v j ( V j - 1 - V 0 ) ] f ′′ ( V 0 + θ ( V j - 1 - V 0 ) ) | V 0 p + 1 2 + ( - j + α + 1 + j + | β | k ) p - 1 2 .

Second, for 𝝂0, 𝝂𝝂 and θ[0,1], by formula (2.25), using (2.10), (2.16) and (2.17), we have

| 𝝂 [ f ′′ ( V 0 + θ ( V j - 1 - V 0 ) ) ] | r = 1 n V 0 p - r - 2 P ( 𝝂 , r ) = 1 n ( V 0 1 + ( α + | β | k ) p - 1 2 ) r
r = 1 n V 0 p - r - 2 V 0 r + ( α + | β | k ) p - 1 2 V 0 p - 2 + ( α + | β | k ) p - 1 2 .

Thus, we obtain

| 𝝂 - 𝝂 [ χ j v j ( V j - 1 - V 0 ) ] 𝝂 [ f ′′ ( V 0 + θ ( V j - 1 - V 0 ) ) ] | V 0 p + 1 2 + ( - j + α + 1 + j + | β | k ) p - 1 2 .

Integrating in θ[0,1] and summing in 𝝂𝝂, we obtain

(2.27) | 𝝂 [ χ j v j ( f ( V j - 1 ) - f ( V 0 ) ) ] | V 0 p + 1 2 + ( - j + α + 1 + j + | β | k ) p - 1 2 .

Combining (2.26) and (2.27), we have proved for s(0,sj], |x|R,

| 𝝂 [ f ( V j ) - f ( V j - 1 ) - f ( V 0 ) χ j v j ] | V 0 p + 1 2 + ( - j + α + 1 + j + | β | k ) p - 1 2 .

In conclusion, we have estimated all terms in the expression of j and (2.19) for j is proved.

Proof of (2.20)–(2.21). For |x|>R2, (2.6) implies A(x)2k2r12rj, thus χj=0 and Vj=V0, j=0. Thus, (2.20)–(2.21) follow from (2.12)–(2.13). ∎

3 Construction of a Solution of the Transformed Equation (2.2)

Let the function χ be given by (1.7), let ψ𝒞q0(N,), where q0 is defined by (1.2), satisfy (2.1), let J, q0 and k be as in (2.3)–(2.4). Set

(3.1) λ = min { 1 2 ( J - p + 3 p - 1 ) , 1 p } ( 0 , 1 2 ] ,

and impose the following additional condition on k:

(3.2) k 2 [ p + 1 + λ ( p - 1 ) ] λ ( p - 1 ) .

Recall that A:N[0,+[ is defined by (2.5), and let VJ be defined as in Section 2.3.

Our main result of this section is the following.

Proposition 3.1.

Assume that

(3.3) ψ L λ 8 p - 1 p + 1 .

There exist 0<δ0<1 and a function

(3.4) v C ( ( 0 , δ 0 ) , H 2 ( N ) ) C 1 ( ( 0 , δ 0 ) , H 1 ( N ) ) C 2 ( ( 0 , δ 0 ) , L 2 ( N ) ) ,

which is a solution of (2.2) in C((0,δ0),L2(RN)), and which satisfies

(3.5) ( v - V J ) ( s ) H 2 2 + s ( v - V J ) ( s ) H 1 2 C s λ for all  0 < s < δ 0 ,

with λ given by (3.1). In addition, there exist a constant C and a function gL((0,δ0),H1(RN)) such that

(3.6) | s v | 2 - | v | 2 1 4 | s V 0 | 2 - C - g 2

a.e. on (0,δ0)×RN.

We construct the solution v of Proposition 3.1 by a compactness argument. For any n large, let Sn=1n<sJ and

B n = sup s [ S n , s J ] V J ( s ) L so that lim n B n = .

We let n be sufficiently large so that Bn1, and we define the function fn:[0,) by

f n ( u ) = f ( u ) χ ( | u | B n ) so that f n ( u ) = { f ( u ) for  | u | < B n , 0 for  | u | > 2 B n .

Let Fn(u)=0ufn(w)𝑑w. Note that Taylor’s estimates such as (1.8)–(1.11) still hold for Fn and fn with constants independent of n. We will refer to these inequalities for Fn and fn with the same numbers (1.8), (1.9) and (1.11). In this proof, any implicit constant related the symbol is independent of n.

We define the sequence of solution vn of

(3.7) { ( 1 - | ψ | 2 ) s s v n - 2 ψ s v n - ( Δ ψ ) s v n - Δ v n = f n ( v n ) , v n ( S n ) = V J ( S n ) , s v n ( S n ) = s V J ( S n ) .

The nonlinearity fn being globally Lipschitz, the existence of a global solution (vn,svn) in H2×H1 is a consequence of standard arguments from semigroups theory, see Appendix A, and in particular Section A.4.

We set, for all s[Sn,sJ],

v n ( s ) = V J ( s ) + w n ( s ) ,

thus (wn,swn)𝒞([Sn,sJ],H2(N)×H1(N))𝒞1([Sn,sJ],H1(N)×L2(N)). The crucial step in the proof of Proposition 3.1 is the following estimate.

Proposition 3.2.

There exist C>0, n0>0 and 0<δ0<1 such that

(3.8) w n ( s ) H 2 2 + s w n ( s ) H 1 2 + s s w n ( s ) L 2 2 C ( s - S n ) λ

for all nn0 and s[Sn,Sn+δ0].

Proof.

We fix nn0 large, and we denote wn simply by w in this proof. By (3.7) and the definition of J, w satisfies the equation

(3.9) { ( 1 - | ψ | 2 ) s s w - 2 ψ s w - ( Δ ψ ) s w - Δ w = f n ( V J + w ) - f n ( V J ) + J , w ( S n ) = 0 , s w ( S n ) = 0 .

We define the auxiliary function Q as follows:

Q = ( 1 - χ + V 0 ) p + 1 ,

where, by abuse of notation, we denote χ(x)=χ(|x|). Note that Q1. We make the following preliminary observation:

s s w = s s [ Q 1 2 ( Q - 1 2 w ) ] = s s ( Q 1 2 ) ( Q - 1 2 w ) + 2 s ( Q 1 2 ) s ( Q - 1 2 w ) + Q 1 2 s s ( Q - 1 2 w )
= s s ( Q 1 2 ) ( Q - 1 2 w ) + Q - 1 2 s [ Q s ( Q - 1 2 w ) ] .

Thus, setting

G = f ( V 0 ) Q 1 2 - ( 1 - | ψ | 2 ) s s ( Q 1 2 )

(by the definition of Q and V0, we expect G to be small in some sense), we rewrite the equation of w as follows:

( 1 - | ψ | 2 ) s [ Q s ( Q - 1 2 w ) ] = Q 1 2 [ 2 ψ s w + ( Δ ψ ) s w + Δ w ]
(3.10) + Q 1 2 [ f n ( V J + w ) - f n ( V J ) - f n ( V 0 ) w ] + G w + Q 1 2 J .

The nonlinear term fn(VJ+w)-fn(VJ)-fn(V0)w is mostly quadratic in w (some linear terms in w remain but they are also small in VJ-V0), which is an important gain with respect to the previous formulation.

We define the following energy functional related to the above formulation of the equation of w:

= { ( 1 - | ψ | 2 ) [ Q s ( Q - 1 2 w ) ] 2 + Q 2 | ( Q - 1 2 w ) | 2 + λ 16 s - 2 Q w 2
- Q [ 2 F n ( V J + w ) - 2 F n ( V J ) - 2 F n ( V J ) w - F n ′′ ( V 0 ) w 2 ] } .

We also define a weighted norm related to the above functional

𝒩 = ( [ Q s ( Q - 1 2 w ) ] 2 + Q 2 | ( Q - 1 2 w ) | 2 + λ 16 s - 2 Q w 2 ) 1 2 .

Since we may be dealing with H1×L2 supercritical nonlinearities (but H2×H1 subcritical by the condition 1N4), we need higher order energy functionals. We set

𝒦 0 = { ( 1 - | ψ | 2 ) ( s s w ) 2 + | s w | 2 } ,
𝒦 = { ( 1 - | ψ | 2 ) ( s x w ) 2 + | x w | 2 } , 1 N ,

and

𝒦 = = 0 N 𝒦 , = ( w H 2 2 + s w H 1 2 + s s w L 2 2 ) 1 2 .

For future reference, we establish two estimates on sQ and Q. By the expression of V0 in (2.9), we have

(3.11) s Q = ( p + 1 ) s V 0 ( 1 - χ + V 0 ) p = ( p + 1 ) ( s V 0 ) Q p p + 1 = - 2 ( p + 1 ) ( 1 - | ψ | 2 ) - 1 2 V 0 p + 1 2 Q p p + 1 .

Thus, since Qp-12(p+1)s-1,

(3.12) | s Q | V 0 p + 1 2 Q p p + 1 Q 1 + p - 1 2 ( p + 1 ) s - 1 Q .

Similarly, by (2.10),

(3.13) | Q | = ( p + 1 ) | V 0 | ( 1 - χ + V 0 ) p V 0 1 + p - 1 2 k Q p p + 1 Q 1 + 1 k p - 1 2 ( p + 1 ) s - 1 k Q

and

(3.14) | Δ Q | s - 2 k Q , | s Q | s - 1 - 1 k Q .

Step 1: Coercivity. We claim the following estimates.

Lemma 3.3.

It holds

(3.15) 2 𝒩 2 + 𝒦 .

For 0<δsJ and 0<ω1 sufficiently small, for n large, if Nω and Mω, then

(3.16) 2 + 𝒦 𝒩 2 .

Proof.

First, we prove the following estimates. For any ρ0, the following holds on [Sn,δ0],

(3.17) Q ρ | w | 2 Q ρ + 1 | ( Q - 1 2 w ) | 2 + Q ρ + p - 1 k ( p + 1 ) w 2 ,
(3.18) Q ρ + 1 | ( Q - 1 2 w ) | 2 Q ρ | w | 2 + Q ρ + p - 1 k ( p + 1 ) w 2 ,
(3.19) Q ρ | s w | 2 Q ρ + 1 | s ( Q - 1 2 w ) | 2 + Q ρ + p - 1 p + 1 w 2 ,
(3.20) Q ρ + 1 | s ( Q - 1 2 w ) | 2 Q ρ | s w | 2 + Q ρ + p - 1 p + 1 w 2 .

We have, using (3.13),

Q ρ | w | 2 = Q ρ | Q 1 2 ( Q - 1 2 w ) + ( Q 1 2 ) Q - 1 2 w | 2
Q 1 + ρ | ( Q - 1 2 w ) | 2 + Q ρ - 1 | Q 1 2 | 2 w 2
Q 1 + ρ | ( Q - 1 2 w ) | 2 + Q ρ + p - 1 k ( p + 1 ) w 2 .

This proves (3.17) and the proof of (3.18) is similar. Moreover, using (3.12),

Q ρ | s w | 2 = Q ρ | Q 1 2 s ( Q - 1 2 w ) + ( s Q 1 2 ) Q - 1 2 w | 2
Q ρ + 1 s ( Q - 1 2 w ) | 2 + Q ρ - 1 | s Q 1 2 | 2 w 2
Q ρ + 1 | s ( Q - 1 2 w ) | 2 + Q ρ + p - 1 p + 1 w 2 ,

which proves (3.19); the proof of (3.20) is similar.

We prove (3.15). The inequality wL2𝒩 is obvious. Next, (3.19) with ρ=1 and Qp-1p+1s-2 show that

| s w | 2 Q | s w | 2 𝒩 2 .

Since ψL12 (from (3.3)), it follows (using wH2ΔwL2+wL2) that 2𝒩2+𝒦, which is (3.15).

Last, we prove (3.16). Let

(3.21) A 1 = | F n ( V J + w ) - F n ( V J ) - F n ( V J ) w - 1 2 F n ′′ ( V 0 ) w 2 | .

The triangle inequality and the Taylor inequality (1.8) yield

A 1 | F n ( V J + w ) - F n ( V J ) - F n ( V J ) w - F n ′′ ( V J ) 2 w 2 | + | F n ′′ ( V J ) - F n ′′ ( V 0 ) | w 2 Λ 1 ,

where

(3.22) Λ 1 = | w | p + 1 + V 0 p - p ¯ | w | p ¯ + 1 + V 0 p - 2 | V J - V 0 | w 2 .

From (2.17), VJV0 and |VJ-V0|(1+V0)-p-14V0Q-p-14(p+1)V0. Moreover, V0p+1Q. Thus,

(3.23) Λ 1 | w | p + 1 + Q p - p ¯ p + 1 | w | p ¯ + 1 + Q 3 4 p - 1 p + 1 w 2 ,

and so

Q Λ 1 Q | w | p + 1 + Q 1 + p - p ¯ p + 1 | w | p ¯ + 1 + Q 1 + 3 4 p - 1 p + 1 w 2 .

For the first term, we prove the following general estimate: for any 0<ζ1,

(3.24) Q ( 1 - ζ ) 2 p p + 1 | w | p + 1 𝒩 p + 1 + p + 1 .

Indeed, using Hölder’s inequality and the embedding H2(N)Lq(N) for 2q< (recall that N4),

Q ( 1 - ζ ) 2 p p + 1 | w | p + 1 s - 2 ( 1 - ζ ) Q 1 - ζ | w | p + 1 s - 2 ( 1 - ζ ) ( Q w 2 ) 1 - ζ ( | w | p - 1 ζ + 2 ) ζ 𝒩 2 ( 1 - ζ ) p - 1 + 2 ζ 𝒩 p + 1 + p + 1 .

In particular, from (3.24), it holds

Q | w | p + 1 𝒩 p + 1 + p + 1 .

In the case 1<p2, one has p¯=p and the second term is identical to the first one. In the case p>p¯=2, the second term is estimated as follows. Using the inequality |w|3aw2+a-(p-2)|w|p+1 with a=εQ1p-1, ε>0 to be chosen later, and the estimate Qp-1p+1s-2, we see that

Q 2 p - 1 p + 1 | w | 3 ε Q p - 1 p + 1 Q w 2 + ε - ( p - 2 ) Q | w | p + 1
ε s - 2 Q w 2 + ε - ( p - 2 ) Q | w | p + 1 ,

and so, using (3.24)

(3.25) Q 2 p - 1 p + 1 | w | p ¯ + 1 ε 𝒩 2 + ε - ( p - 2 ) ( 𝒩 p + 1 + p + 1 ) .

Last, since Qp-12(p+1)s-1, we observe that

Q 3 4 p - 1 p + 1 + 1 w 2 s - 3 2 Q w 2 s 1 2 𝒩 2 .

In conclusion, we have obtained, for 𝒩ω, ω, Snsδ,

Q A 1 ( ε + s 1 2 ) 𝒩 2 + ( 1 + ε - ( p - 2 ) ) ( 𝒩 p + 1 + p + 1 )
( ε + δ 1 2 ) 𝒩 2 + ( 1 + ε - ( p - 2 ) ) ω p - 2 2 ,

which, combined with (3.15), implies that for δ>0 and ω>0 small enough, it holds 2+𝒦𝒩2 on [Sn,δ0]. (Recall that 1-|ψ|234 by (3.3) and λ12.) ∎

Step 2: Energy Control. We claim that there exist C>0 such that

(3.26) d d s C s - 1 + λ 𝒩 + λ 4 s - 1 𝒩 2 + C s - 1 2 𝒩 2 + C s - 1 ( 𝒩 p + 1 + p + 1 )

provided 𝒩ω and ω with ω sufficiently small.

Proof of (3.26). We compute dds:

1 2 d d s = { ( 1 - | ψ | 2 ) Q s ( Q - 1 2 w ) s [ Q s ( Q - 1 2 w ) ]
    + Q 2 ( Q - 1 2 w ) s [ ( Q - 1 2 w ) ] + λ 16 s - 2 Q 3 2 w s ( Q - 1 2 w )
    - Q 3 2 [ f n ( V J + w ) - f n ( V J ) - f n ( V 0 ) w ] s ( Q - 1 2 w ) }
+ ( s Q ) Q | ( Q - 1 2 w ) | 2 + λ 32 s - 2 ( s Q ) w 2 - λ 16 s - 3 Q w 2
- 1 2 s Q [ 2 F n ( V J + w ) - 2 F n ( V J ) - 2 F n ( V J ) w - F n ′′ ( V 0 ) w 2 ]
- 1 2 s Q [ f n ( V J + w ) - f n ( V J ) - f n ( V 0 ) w ] w
- 1 2 Q s V 0 [ 2 f n ( V J + w ) - 2 f n ( V J ) - 2 f n ( V J ) w - f n ′′ ( V 0 ) w 2 ]
- 1 2 Q s ( V J - V 0 ) [ 2 f n ( V J + w ) - 2 f n ( V J ) - 2 f n ( V J ) w ]
= I 1 + I 2 + I 3 + I 4 + I 5 + I 6 .

First, we remark the negative contribution of I2. Since sQ0 by (3.11), we have

(3.27) I 2 - λ 16 s - 3 Q w 2 .

Second, we compute I1 using equation (3.10) of w:

I 1 = Q 3 2 s ( Q - 1 2 w ) [ 2 ψ s w + ( Δ ψ ) s w ]
+ { Q 3 2 s ( Q - 1 2 w ) ( Δ w ) + Q 2 ( Q - 1 2 w ) [ s ( Q - 1 2 w ) ] }
+ Q s ( Q - 1 2 w ) G w + Q 3 2 s ( Q - 1 2 w ) J + λ 16 s - 2 Q 3 2 w s ( Q - 1 2 w )
= I 7 + I 8 + I 9 + I 10 + I 11 .

For I7, we first observe that

2 Q 3 2 s ( Q - 1 2 w ) ( ψ s w ) = 2 Q 2 s ( Q - 1 2 w ) ( ψ s ( Q - 1 2 w ) ) + Q ( s ( Q - 1 2 w ) ) 2 ( ψ Q )
+ Q s Q s ( Q - 1 2 w ) ( ψ ( Q - 1 2 w ) ) + Q 1 2 w s ( Q - 1 2 w ) ( ψ s Q )
- 1 2 Q - 1 2 s Q w s ( Q - 1 2 w ) ( ψ Q ) .

Second, by integration by parts,

2 Q 2 s ( Q - 1 2 w ) ( ψ s ( Q - 1 2 w ) ) = Q 2 ψ [ ( s ( Q - 1 2 w ) ) 2 ]
= - Q 2 Δ ψ [ s ( Q - 1 2 w ) ] 2 - 2 Q [ s ( Q - 1 2 w ) ] 2 ( ψ Q ) .

By the definition of 𝒩, we estimate

| Q 2 Δ ψ [ s ( Q - 1 2 w ) ] 2 | 𝒩 2 .

Using (3.13), we also have

| Q ( s ( Q - 1 2 w ) ) 2 ( ψ Q ) | s - 1 k 𝒩 2 .

Now, by the expressions of Q and V0, we have

| s Q | = ( p + 1 ) | s V 0 | ( 1 - χ + V 0 ) p = 2 p + 1 p - 1 ( s + A ( x ) ) - 1 V 0 ( 1 - χ + V 0 ) p 2 p + 1 p - 1 s - 1 Q ,

and thus

| Q s Q s ( Q - 1 2 w ) ( ψ ( Q - 1 2 w ) ) | 2 p + 1 p - 1 s - 1 | ψ | Q 2 | s ( Q - 1 2 w ) | | ( Q - 1 2 w ) | p + 1 p - 1 s - 1 ψ L 𝒩 2 .

Similarly, using (3.12), (3.13), (3.14)

| Q 1 2 w s ( Q - 1 2 w ) ( ψ s Q ) | s - 1 k ( Q 2 | s ( Q - 1 2 w ) | 2 + s - 2 Q w 2 ) s - 1 k 𝒩 2

and

| Q - 1 2 s Q w s ( Q - 1 2 w ) ( ψ Q ) | s - 1 k 𝒩 2 .

Using the same estimates and then (3.19), we finish estimating I7 as follows:

| Q 3 2 s ( Q - 1 2 w ) ( Δ ψ ) s w | Q 2 | s ( Q - 1 2 w ) | 2 + Q ( s w ) 2 Q 2 | s ( Q - 1 2 w ) | 2 + s - 2 Q w 2 𝒩 2 .

Thus, for some constant C>0, using (3.3),

| I 7 | p + 1 p - 1 s - 1 ψ L 𝒩 2 + C s - 1 k 𝒩 2 λ 8 s - 1 𝒩 2 + C s - 1 k 𝒩 2 .

Next, integrating by parts, using the identities

Q 2 [ s ( Q - 1 2 w ) ] = Q 1 2 [ Q 3 2 ( s ( Q - 1 2 w ) ] - 3 2 s ( Q - 1 2 w ) Q ,
- w + Q 1 2 ( Q - 1 2 w ) = - Q - 1 2 ( Q 1 2 ) ,

and integrating again by parts, we find

I 8 = - ( Q 3 2 s ( Q - 1 2 w ) ) w + Q 2 ( Q - 1 2 w ) [ s ( Q - 1 2 w ) ]
= - [ ( Q 3 2 s ( Q - 1 2 w ) ) ( Q 1 2 ) ] Q - 1 2 w - 3 2 Q s ( Q - 1 2 w ) [ Q ( Q - 1 2 w ) ]
= - Q s ( Q - 1 2 w ) [ ( Q - 1 2 w ) Q ] + Δ ( Q 1 2 ) Q w s ( Q - 1 2 w ) .

By (3.13) and the definition of 𝒩,

| Q s ( Q - 1 2 w ) [ ( Q - 1 2 w ) Q ] | s - 1 k 𝒩 2 .

Similarly, using (3.13) and (3.14), we have |Δ(Q12)Q32||Q|2+|ΔQ|Qs-2kQ2, and thus

| Δ ( Q 1 2 ) Q w s ( Q - 1 2 w ) | Q 2 [ s ( Q - 1 2 w ) ] 2 + s - 4 k Q w 2 𝒩 2 .

For I9, we start by an estimate of G=fn(V0)Q12-(1-|ψ|2)ss(Q12). By the definition of Q=(1-χ+V0)p+1 and (2.9), we observe

s s ( Q 1 2 ) = s s [ ( 1 - χ + V 0 ) p + 1 2 ]
= p + 1 2 p - 1 2 ( s V 0 ) 2 ( 1 - χ + V 0 ) p - 3 2 + p + 1 2 s s V 0 ( 1 - χ + V 0 ) p - 1 2
= ( 1 - | ψ | 2 ) - 1 [ p - 1 2 V 0 p + 1 Q p - 3 2 ( p + 1 ) + p + 1 2 V 0 p Q p - 1 2 ( p + 1 ) ] .

Thus,

G = p V 0 p - 1 Q 1 2 - p - 1 2 V 0 p + 1 Q p - 3 2 ( p + 1 ) - p + 1 2 V 0 p Q p - 1 2 ( p + 1 ) = V 0 p - 1 Q p - 3 2 ( p + 1 ) [ p ( 1 - χ + V 0 ) + p - 1 2 V 0 ] ( 1 - χ ) .

For |x|>1, we have V01 and Q1; since also Q1, we see that GL1. Therefore,

| I 9 | G L 𝒩 2 𝒩 2 .

For I10, by the Cauchy–Schwarz inequality

| I 10 | = | Q 3 2 s ( Q - 1 2 w ) J | Q 1 2 J L 2 𝒩 ,

and we need only estimate Q12JL2. From (2.21), for |x|R, we have

Q 1 2 | J | | J | | x | - 2 k p - 1 - 2 .

Since 1N4, this implies Q12JL2(|x|>R)1. Next, from (2.19), for |x|R, we have

Q 1 2 | J | Q 1 2 V 0 p + 1 2 + ( - J + 1 + J k ) p - 1 2 V 0 p + 1 + ( - J + 1 + J k ) p - 1 2 V 0 p + 1 + 1 k p - 1 2 - J ( 1 - 1 k ) p - 1 2 .

Recall that by (3.1),

- J p - 1 2 - p + 3 2 - λ ( p - 1 )

and that (3.2) is equivalent to

p + 1 k - λ ( p - 1 ) ( 1 - 1 k ) - λ ( p - 1 ) 2 .

Thus, for |x|R,

Q 1 2 | J | V 0 p + 1 + 1 k p - 1 2 - p + 3 2 ( 1 - 1 k ) - λ ( p - 1 ) ( 1 - 1 k ) V 0 p - 1 2 + p + 1 k - λ ( p - 1 ) ( 1 - 1 k )
V 0 p - 1 2 - λ p - 1 2 ( s + A ( x ) ) - 1 + λ s - 1 + λ .

It follows that

(3.28) Q 1 2 J L 2 s - 1 + λ .

For this term, we have obtained

| I 10 | Q 1 2 J L 2 𝒩 s - 1 + λ 𝒩 .

Finally, by the Cauchy–Schwarz inequality,

| I 11 | s - 1 λ 16 Q 2 | s ( Q - 1 2 w ) | 2 + s - 3 λ 16 Q w 2 .

Using (3.27), we obtain

| I 11 | λ 16 s - 1 𝒩 2 - I 2 .

In conclusion for I1+I2, we find

I 1 + I 2 C s - 1 + λ 𝒩 + 3 λ 16 s - 1 𝒩 2 + C s - 1 k 𝒩 2 .

To continue with the proof of (3.26), we estimate the term I3. To that end, recall that p¯=min(2,p). First, by (3.21)–(3.23) and (3.12)

| s Q | A 1 | s Q | Λ 1 V 0 p + 1 2 Q p p + 1 Λ 1 Q 3 p + 1 2 ( p + 1 ) Λ 1
Q 3 p + 1 2 ( p + 1 ) | w | p + 1 + Q 3 p + 1 2 ( p + 1 ) Q p - p ¯ p + 1 | w | p ¯ + 1 + Q 9 p - 1 4 ( p + 1 ) w 2 .

Using (3.24), the first term is controlled as follows:

Q 3 p + 1 2 ( p + 1 ) | w | p + 1 𝒩 p + 1 + p + 1 .

In the case 1<p2, one has p¯=p and the second term is identical to the first one. In the case p>p¯=2, using Qp-12(p+1)s-1 and (3.25),

Q 3 p + 1 2 ( p + 1 ) Q p - p ¯ p + 1 | w | p ¯ + 1 = Q 5 p - 3 2 ( p + 1 ) | w | p ¯ + 1 s - 1 Q 2 p - 1 p + 1 | w | p ¯ + 1
ε s - 1 𝒩 2 + ε - ( p - 2 ) s - 1 ( 𝒩 p + 1 + p + 1 ) ,

where ε>0 is to be chosen. Last, we observe that Q9p-14(p+1)w2s-52Qw2, and thus

Q 9 p - 1 4 ( p + 1 ) w 2 s - 1 2 𝒩 2 .

In conclusion, we have proved

(3.29) | I 3 | | s Q | Λ 1 Q 3 p + 1 2 ( p + 1 ) Λ 1 ( s - 1 2 + ε s - 1 ) 𝒩 2 + ( 1 + ε - ( p - 2 ) s - 1 ) ( 𝒩 p + 1 + p + 1 ) .

We proceed similarly for I4. Indeed, setting

A 2 = | f n ( V J + w ) - f n ( V J ) - f n ( V J ) w | | w |
| f n ( V J + w ) - f n ( V J ) - f n ( V J ) w | | w | + | f n ( V 0 ) - f n ( V J ) | w 2 ,

by (1.9) and Taylor’s inequality,

A 2 | w | p + 1 + V 0 p - p ¯ | w | p ¯ + 1 + V 0 p - 2 | V J - V 0 | w 2 = Λ 1 .

Using (3.29), we conclude that

| I 4 | | s Q | Λ 1 ( s - 1 2 + ε s - 1 ) 𝒩 2 + ( 1 + ε - ( p - 2 ) s - 1 ) ( 𝒩 p + 1 + p + 1 ) .

Now, we estimate I5 and we set

A 3 = | 2 f n ( V J + w ) - 2 f n ( V J ) - 2 f n ( V J ) w - f n ′′ ( V 0 ) w 2 | .

By the triangle inequality, Taylor inequality (1.11), |sV0|V0p+12 (see (2.9)), we have

Q | s V 0 | A 3 Q V 0 p + 1 2 | 2 f n ( V J + w ) - 2 f n ( V J ) - 2 f n ( V J ) w - f n ′′ ( V J ) w 2 | + Q V 0 p + 1 2 | f n ′′ ( V J ) - f n ′′ ( V 0 ) | w 2
Q V 0 p - 1 2 Λ 1 Q 3 p + 1 2 ( p + 1 ) Λ 1 .

Using (3.29), we conclude that

| I 5 | ( s - 1 2 + ε s - 1 ) 𝒩 2 + ( 1 + ε - ( p - 2 ) s - 1 ) ( 𝒩 p + 1 + p + 1 ) .

Finally, we estimate I6 and we set

A 4 = | 2 f n ( V J + w ) - 2 f n ( V J ) - 2 f n ( V J ) w | .

By the triangle inequality and Taylor’s inequality (1.11)

A 4 | 2 f n ( V J + w ) - 2 f n ( V J ) - 2 f n ( V J ) w - f n ′′ ( V J ) w 2 | + | f n ′′ ( V J ) | w 2 V 0 - 1 | w | p + 1 + V 0 p - p ¯ - 1 | w | p ¯ + 1 + V 0 p - 2 w 2 .

Using (2.18), V0Q1p+1, Q1, Qs-2(p+1)p-1 and k1, we obtain

Q | s ( V J - V 0 ) | A 4 Q V 0 p - 1 2 k ( | w | p + 1 + V 0 p - p ¯ | w | p ¯ + 1 + V 0 p - 1 w 2 ) Q 1 + p - 1 2 k ( p + 1 ) ( | w | p + 1 + V 0 p - p ¯ | w | p ¯ + 1 ) + Q 1 + p - 1 p + 1 ( 1 + 1 2 k ) w 2 Q 3 p + 1 2 ( p + 1 ) ( | w | p + 1 + V 0 p - p ¯ | w | p ¯ + 1 ) + s - 2 k + 1 k Q w 2 Q 3 p + 1 2 ( p + 1 ) Λ 1 + s - 1 k s - 2 Q w 2 .

Using (3.29) and k2, we conclude that

| I 6 | ( s - 1 2 + ε s - 1 ) 𝒩 2 + ( 1 + ε - ( p - 2 ) s - 1 ) ( 𝒩 p + 1 + p + 1 ) .

Choosing ελ16, then ω sufficiently small, and collecting the above estimates, we have proved (3.26).

Step 3: Higher-Order Energy Terms. We claim that for any =0,1,,N,

(3.30) | d 𝒦 d s | s - 1 + λ ( 𝒩 + 𝒩 2 + 2 ) + 𝒩 p + 1 + p + 1 .

Differentiating (3.9) with respect to s, setting z0=sw, we have

(3.31) ( 1 - | ψ | 2 ) s s z 0 - 2 ψ s z 0 - ( Δ ψ ) s z 0 - Δ z 0 = f n ( V J + w ) z 0 + ( f n ( V J + w ) - f n ( V J ) ) s V J + s J .

Differentiating 𝒦0=(1-|ψ|2)(sz0)2+|z0|2, we find from (3.31) and integration by parts

1 2 d 𝒦 0 d s = { f n ( V J + w ) z 0 + ( f n ( V J + w ) - f n ( V J ) ) s V J + s J } s z 0
= I 12 + I 13 + I 14 .

First, by the Cauchy–Schwarz inequality

| I 12 | f n ( V J + w ) z 0 L 2 𝒦 0 1 2 f n ( V J + w ) z 0 L 2 .

From

| f n ( V J + w ) | | V 0 | p - 1 + | w | p - 1 s - p - 1 p Q p - 1 2 p + | w | p - 1 s - p - 1 p Q 1 2 + | w | p - 1

and then (3.19) with ρ=1, we have (recall that 1N4 and thus H2(N)Lq(N) for all q2, and H1(N)Lq(N) for all 2q4)

f ( V J + w ) z 0 L 2 2 s - 2 ( p - 1 ) p Q ( s w ) 2 + | w | 2 ( p - 1 ) ( s w ) 2
s - 2 ( p - 1 ) p 𝒩 2 + w L 4 p 2 ( p - 1 ) s w L 4 p p + 1 2
s - 2 ( p - 1 ) p 𝒩 2 + w H 2 2 ( p - 1 ) s w H 1 2 .

Thus, using also -p-1p-1+λ (since λ1p) we have

| I 12 | s - p - 1 p 𝒩 + p + 1 s - 1 + λ ( 𝒩 2 + 2 ) + p + 1 .

Second, using (2.10) and (2.18),

| s V J | V 0 1 + p - 1 2 + V 0 1 + p - 1 2 k V 0 Q p - 1 2 ( p + 1 ) ,

so that Taylor’s inequality (1.10) yields

| ( f n ( V J + w ) - f n ( V J ) ) s V J | Q p - 1 2 ( p + 1 ) | w | p + Q p - 1 2 ( p + 1 ) V 0 p - 1 | w |
Q p - 1 2 ( p + 1 ) | w | p + Q 3 ( p - 1 ) 2 ( p + 1 ) | w | .

We have

Q p - 1 p + 1 | w | 2 p ( Q w 2 ) p - 1 p + 1 | w | 2 p 2 + 1 p + 1 ( Q w 2 ) p - 1 p + 1 ( w p 2 + 1 ) 2 p + 1
𝒩 2 p - 1 p + 1 2 p 2 + 1 p + 1 ( 𝒩 + ) 2 p .

Moreover, since 2(p-2)p+1(2p-1)(p-1)p(p+1), Q1, Qs-2(p+1)p-1, and λ1p, we have

Q 3 ( p - 1 ) p + 1 w 2 Q 2 ( p - 2 ) p + 1 Q w 2 Q ( 2 p - 1 ) ( p - 1 ) p ( p + 1 ) Q w 2 s - 2 ( 2 p - 1 ) p Q w 2 s - 2 ( p - 1 ) p 𝒩 2 s - 2 ( 1 - λ ) 𝒩 2 .

Thus,

| I 13 | ( Q p - 1 2 ( p + 1 ) | w | p L 2 + Q 3 ( p - 1 ) 2 ( p + 1 ) L 2 )
( s - 1 + λ 𝒩 + ( 𝒩 + ) p ) s - 1 + λ ( 𝒩 2 + 2 ) + 𝒩 p + 1 + p + 1 .

Third, from (2.21), for |x|R, |sJ||x|-k(p+1)p-1-2 and thus, since 1N4, sJL2(|x|R)1. Now, from (2.19), for |x|R,

| s J | V 0 p + 1 2 + ( 1 - J + 1 + J k ) p - 1 2 V 0 p + 1 k p - 1 2 - J ( 1 - 1 k ) p - 1 2 ,

and thus, following the proof of (3.28), we have sJL2(|x|R)s-1+λ. Thus,

| I 14 | s J L 2 s - 1 + λ .

The above estimates prove (3.30) for 𝒦0.

We now prove (3.30) for {1,,N}. Differentiating (3.9) with respect to x, setting z=xw, we have

(3.32)

( 1 - | ψ | 2 ) s s z - 2 ψ s z - ( Δ ψ ) s z - Δ z = f n ( V J + w ) z + ( f n ( V J + w ) - f n ( V J ) ) x V J
+ x J + 2 ( ψ x ψ ) s s w
+ 2 x ψ s w + ( Δ x ψ ) s w .

Differentiating 𝒦=(1-|ψ|2)(sz)2+|z|2, we find from (3.32) and integration by parts

1 2 d 𝒦 d s = { f n ( V J + w ) z + ( f n ( V J + w ) - f n ( V J ) ) x V J + x J } s z
+ { 2 ( ψ x ψ ) s s w + 2 x ψ s w + ( Δ x ψ ) s w } s z
= I 15 + I 16 + I 17 + I 18 .

The term I15 is estimated exactly like I12. Next, it follows from (2.10), (2.16), (2.20) and the properties of χ that

| x V J | V 0 1 + p - 1 2 k ,

so that I16 is estimated like I13.

Moreover, from (2.21), for |x|R, |xJ||x|-3 and thus, since 1N4, sJL2(|x|R)1. Now, from (2.19), for |x|R,

| x J | V 0 p + 1 2 + ( - J + 2 + J k ) p - 1 2 V 0 p - 1 2 + 1 k p - 1 2 - J ( 1 - 1 k ) p - 1 2 ,

and thus, following the proof of (3.28), we have sJL2(|x|R)s-1+λ. Thus we see that I17 is estimated like I14.

Finally,

| 2 ( ψ x ψ ) s s w + 2 x ψ s w + ( Δ x ψ ) s w | | s s w | + | s w | + | s w | ,

so that I182. Therefore, estimate (3.30) holds for {1,,N}.

Step 4: Conclusion. Since (Sn)=𝒦(Sn)=0, the following is well defined:

S n = sup { s [ S n , δ ] : for all  s [ S n , s ] 𝒩 2 + 𝒦 min ( s λ , ω ) } ,

and by continuity, Sn(Sn,δ]. It follows from (3.26), (3.30), (3.15), and λ12 that

d d t ( + 𝒦 ) s - 1 + λ ( C 𝒩 + λ 4 s - λ 𝒩 2 + C ( 𝒩 2 + 𝒦 ) + C s - λ ( 𝒩 2 + 𝒦 ) p + 1 2 )

for some constant C>0 independent of δ. By the definition of Sn, we deduce that

d d t ( + 𝒦 ) λ s - 1 + λ ( C s 1 2 λ + C s p - 1 2 λ + 1 4 )

for some constant C>0 independent of δ. We fix 0<δ0δ such that

C δ 0 1 2 λ + C δ 0 p - 1 2 λ + 1 4 1 3 , δ 0 λ ω .

This gives, for all Snsmin(Sn,δ0), ddt(+𝒦)λ3s-1+λ.

By integration, using (sn)=𝒦(sn)=0, we find for Snsmin(Sn,δ0),

( s ) + 𝒦 ( s ) 1 3 ( s λ - S n λ ) 1 3 ( s - S n ) λ .

Thus, from (3.16), it holds, for Snsmin(Sn,δ0),

𝒩 2 ( s ) + 𝒦 ( s ) 2 3 ( s - S n ) λ .

It follows from (3.15) and the definition of Sn that Snδ0 and so, for all s[Sn,δ0],

( s ) ( s - S n ) λ 2 .

This completes the proof of the proposition. ∎

Proof of Proposition 3.1.

We set

Z n ( s ) = V J ( S n + s ) , η n ( s , y ) = w n ( S n + s ) , n ( s ) = J ( S n + s ) .

From Proposition 3.2, there exist C>0, n0>0 and 0<δ0<1 such that

(3.33) η n ( s ) H 2 + s η n ( s ) H 1 + s s η n ( s ) L 2 C s λ 2

for all nn0 and s[0,δ0]. Moreover, from (3.9),

(3.34) ( 1 - | ψ | 2 ) s s η n - 2 ψ s η n - ( Δ ψ ) s η n - Δ η n = f n ( Z n + η n ) - f n ( Z n ) + n .

It follows from estimate (3.33) that there exist a subsequence of (ηn) (still denoted by (ηn)) and a map ηL((0,δ0),H2(N))W1,((0,δ0),H1(N))W2,((0,δ0),L2(N)) such that

(3.35) η n n η in  L ( ( 0 , δ 0 ) , H 2 ( N ) )  weak* ,
(3.36) s η n n s η in  L ( ( 0 , δ 0 ) , H 1 ( N ) )  weak* ,
(3.37) s s η n n s s η in  L ( ( 0 , δ 0 ) , L 2 ( N ) )  weak* ,
(3.38) η n ( s ) n η ( s ) weakly in  H 2 ( N ) , for all  s [ 0 , δ 0 ] ,
(3.39) s η n ( s ) n s η ( s ) weakly in  H 1 ( N ) ) , for all  s [ 0 , δ 0 ]

It is then easy to pass to the limit in (3.34), and it follows that

( 1 - | ψ | 2 ) s s η - 2 ψ s η - ( Δ ψ ) s η - Δ η = f ( V J + η ) - f n ( V J ) + J

in L((0,δ0),L2(N)). Therefore, setting

v ( s ) = V J ( s ) + η ( s ) , s ( 0 , δ 0 ) ,

it holds

(3.40) v L loc ( ( 0 , δ 0 ) , H 2 ( N ) ) W loc 1 , ( ( 0 , δ 0 ) , H 1 ( N ) ) W loc 2 , ( ( 0 , δ 0 ) , L 2 ( N ) )

and, using the definition of J, we see that v is a solution of equation (2.2) in Lloc((0,δ0),L2(N)). Estimate (3.5) follows by letting n in (3.8) and using (3.38) and (3.39). We now prove that v satisfies (3.4). By standard semigroup theory (see Section A.3) it suffices to prove that |v|p-1vC((0,δ0),H1(N)). Since by (3.40) vC((0,δ0),H2-η(N)) for every η>0, and N4, we have by Sobolev’s embeddings vC((0,δ0),W1,q(N)) for all 2q<4 and |v|p-1C((0,δ0),Lr(N)) for max{1,2p-1}r<. Choosing for instance q=4(p+1)p+3 and r=4(p+1)p-1 yields |v|p-1vC((0,δ0),H1(N)).

Finally, we prove (3.6). We write

| s v | | s V 0 | - | s ( V J - V 0 ) | - | s ( v - V J ) | .

On the other hand, V01+p-12|sV0|, so that V01+p-12k|sV0|1-(p-1)(k-1)k(p+1). Therefore, given any η>0, there exists a constant Cη such that

(3.41) V 0 1 + p - 1 2 k η | s V 0 | + C η .

Since |s(Vj-V0)|V01+p-12k by (2.18), we see that there exists a constant C such that

(3.42) | s v | 2 1 2 | s V 0 | 2 - C | s ( v - V J ) | 2 - C .

Next, we write

| v | | ( v - V J ) | + | V J | | ( v - V J ) | + | V 0 | + j = 1 J | v j | .

It follows from (2.20) that |VJ|1 for |x|R. For |x|<R, by (2.16) and k2, |vj|V0 for j1; and

| V 0 | V 0 1 + p - 1 2 k

by (2.10). Using again (3.41), we conclude that

(3.43) | v | 2 1 4 | s V 0 | 2 - C | ( v - V J ) | 2 - C .

Since |s(v-VJ)|+|(v-VJ)|L((0,δ0),H1(N)) by (3.5), the lower estimate (3.6) follows from (3.42) and (3.43). ∎

4 Proof of Theorem 1.1

In this section, we use the following notation. We let {𝐞k:k=1,,N} be the canonical basis of N. If N2, then for xN, we denote x=(x1,x2,,xN) and x¯=(x2,,xN). We set Δ¯u=k=2Nxkxku. If N=1, we ignore x¯ and Δ¯.

4.1 Cut-Off of the Local Hypersurface

Let φ be a function satisfying (1.3) (see statement of Theorem 1.1). Without loss of generality, by the invariance by rotation of equation (1.1), we assume that

φ ( 0 ) = 𝐞 1 where  0 < 1 .

(For dimension 1, the reduction is done by possibly changing x-x.) For a positive real r<1 small to be defined later, set

φ ~ ( x ) = ( φ ( x ) - x 1 ) χ ( | x | r ) + x 1 .

On the one hand, from this definition and the properties of χ, it holds

(4.1) φ ~ ( x ) = φ ( x )  for  | x | < r , φ ~ ( x ) = x 1  for  | x | > 2 r , φ ~ ( 0 ) = 𝐞 1 .

On the other hand, from φ(0)=0 and φ(0)=𝐞1, there exists a constant C>1 such that for |x|<1, it holds |φ(x)-x1|C|x|2 and |φ(x)-𝐞1|C|x|. In particular, since

φ ~ ( x ) = ( φ ( x ) - 𝐞 1 ) χ ( | x | r ) + 𝐞 1 + 1 r ( φ ( x ) - x 1 ) χ ( | x | r ) x | x | ,

it holds on N,

| φ ~ ( x ) - 𝐞 1 | C r .

We fix r>0 small enough so that

(4.2) φ ~ - 𝐞 1 L ( 1 - ) min { λ 8 p - 1 p + 1 , 1 2 } .

The first constraint on φ~ is related to assumption (3.3) in Proposition 3.2, and the second implies

(4.3) φ ~ L + 1 2 < 1 .

4.2 Construction of the Function ψ

We claim that for any yN, there exists X1(y) such that

(4.4) y 1 = X 1 ( y ) - φ ~ ( X 1 ( y ) , y ¯ ) ( 1 - 2 ) 1 2 .

(As observed before, we ignore y¯ in dimension 1.) To prove the claim, we define

(4.5) Φ ( x 1 , y ¯ ) = x 1 - φ ~ ( x 1 , y ¯ ) ( 1 - 2 ) 1 2 ,

and we compute, using (4.3),

(4.6) x 1 Φ ( x 1 , y ¯ ) = 1 - x 1 φ ~ ( x 1 , y ¯ ) ( 1 - 2 ) 1 2 1 - ( 1 - 2 ) 1 2 = ( 1 - 1 + ) 1 2 > 0

and

(4.7) x 1 Φ ( x 1 , y ¯ ) 1 + ( 1 - 2 ) 1 2 ( 1 + 1 - ) 1 2 .

Thus, for fixed y¯N-1, the function x1Φ~y¯(x1)=:Φ(x1,y¯) is increasing and surjective. It has an inverse function Φ~y¯-1 on , which is also (strictly) increasing, and we set X1(y1,y¯)=Φ~y¯-1(y1) for y1. Setting X1(y)=X1(y1,y¯), we have proved the claim. Note that

X 1 ( Φ ( x 1 , y ¯ ) , y ¯ ) = Φ ~ y ¯ - 1 ( Φ ( x 1 , y ¯ ) ) = Φ ~ y ¯ - 1 ( Φ ~ y ¯ ( x 1 ) ) = x 1 ,

so that by (4.5)

(4.8) x 1 = X 1 ( x 1 - φ ~ ( x ) ( 1 - 2 ) 1 2 , x ¯ )

for all xN. Moreover, it follows from (4.6)–(4.7) that

(4.9) ( 1 - 1 + ) 1 2 X 1 y 1 ( 1 + 1 - ) 1 2

on N. Setting X(y)=(X1(y),y¯), it holds

(4.10) y 1 = X 1 ( y ) - φ ~ ( X ( y ) ) ( 1 - 2 ) 1 2 .

Moreover, using (4.9), we see that

(4.11) | X ( y ) | max { | X 1 ( y ) | , | y ¯ | } | y | .

For all yN, we define the function ψ: by

(4.12) ψ ( y ) = φ ~ ( X ( y ) ) - X 1 ( y ) ( 1 - 2 ) 1 2 .

Equivalently, the functions ψ and φ~ are uniquely related by the following relation on N:

(4.13) φ ~ ( x ) = ( 1 - 2 ) 1 2 ψ ( x 1 - φ ~ ( x ) ( 1 - 2 ) 1 2 , x ¯ ) + x 1 .

We check that ψ is of class 𝒞q0, where q0 is defined in (1.2), and satisfies assumptions (2.1) and (3.3).

First, since φ is of class 𝒞q0 and χ is of class 𝒞, it follows from their definitions that φ~ and then the functions X and ψ are of class 𝒞q0 in N. Since φ(0)=φ~(0)=0, from (4.13), we also have ψ(0)=0.

Second, from (4.1), it follows that φ~(x)=x1 for any |x|>2r. From (4.11) and (4.12), we see that ψ(y)=0 for |y| large.

Last, we estimate |ψ|. From (4.13)

(4.14) ( 1 - x 1 φ ~ ( x ) ) y 1 ψ ( x 1 - φ ~ ( x ) ( 1 - 2 ) 1 2 , x ¯ ) = x 1 φ ~ ( x ) - ,

and for j1,

(4.15) y j ψ ( x 1 - φ ~ ( x ) ( 1 - 2 ) 1 2 , x ¯ ) = ( 1 - 2 ) - 1 2 x j φ ~ ( x ) ( 1 + y 1 ψ ( x 1 - φ ~ ( x ) ( 1 - 2 ) 1 2 , x ¯ ) ) .

It follows from (4.3) that |1-x1φ~(x)|1-, so that (4.14) and (4.2) yield

y 1 ψ L 1 1 - x 1 φ ~ - L λ 8 p - 1 p + 1 .

In particular, we see that y1ψL1. Since xjφ~L(1-)λ8p-1p+1 by (4.2), we deduce from (4.15) that

y j ψ L ( 1 - 2 ) - 1 2 ( 1 - ) λ 8 p - 1 p + 1 ( 1 + ) = ( 1 - 2 ) 1 2 λ 8 p - 1 p + 1 λ 8 p - 1 p + 1

so that (3.3) is proved.

4.3 Definition of an Appropriate Solution of the Transformed Equation

We assume (2.3), (2.4), (3.1), (3.2) and we consider the function ψ defined in (4.12)–(4.13). Note that ψ is of class 𝒞q0 where q0 is defined in (1.2), and satisfies assumptions (2.1) and (3.3). Let the function A be given by (2.5). We consider the solution vC((0,δ0),H2(N))C1((0,δ0),H1(N))C2((0,δ0),L2(N)) of (2.2) given by Proposition 3.1.

4.4 Returning to the Original Variable

Let

(4.16) τ 0 = ( 1 - 1 + ) 1 2 δ 0 6 , ε 0 = 1 - 2 + τ 0 .

Recall (see (4.1) and (4.3)) that φ~(0)=0 and |φ~|+12, so that |φ~(x)|+12|x|. Thus we see that

(4.17) τ 0 + inf | x | τ 0 + ε 0 φ ~ ( x ) > 0 .

It follows that the space-time region

𝒯 = { ( t , x ) + 1 + N : 0 t < τ 0 + φ ~ ( x ) , | x | < τ 0 + ε 0 - t }

is an influence domain in the sense of Section 1.2. (See Figure 1.) Moreover, let |x|ε02. We have φ~(x)ε02. Therefore, if 0t<τ0+φ~(x), then t<τ0+ε02 so that |x|<τ0+ε0-t. It follows that

(4.18) | x | ε 0 2 max { t > 0 : ( t , x ) 𝒯 } = τ 0 + φ ~ ( x ) .

Figure 1

The set 𝒯 is the part of the cone |x|<τ0+ε0-t below the surface t=τ0+φ~(x).

Given 0<1 and τ0, we define the Lorentz transform Λ,τ0:1+N1+N by

Λ , τ 0 ( t , x ) = ( s , y ) = ( s , y 1 , y ¯ ) , where  s = t - τ 0 - x 1 ( 1 - 2 ) 1 2 , y 1 = x 1 - ( t - τ 0 ) ( 1 - 2 ) 1 2 , y ¯ = x ¯ .

It is well known that Λ,τ0 is a 𝒞 diffeomorphism with Jacobian determinant |detJΛ,τ0|=1. We also define the transformation Λψ:1+N1+N by

Λ ψ ( t , x ) = ( s , y ) , where  s = ψ ( x ) - t , y = x .

Since ψ is of class 𝒞q0 where q0 is defined in (1.2) (see Section 4.2), it follows easily that Λψ is a diffeomorphism of class 𝒞q0. Moreover, |detJΛψ|=1. We define the map Λ:1+N1+N as the composition of the above two maps, i.e.

Λ = Λ ψ Λ , τ 0 .

The map Λ has the expression

(4.19) Λ ( t , x ) = ( s , y ) = ( s , y 1 , y ¯ ) , where  s = ψ ( y ) - t - τ 0 - x 1 ( 1 - 2 ) 1 2 , y 1 = x 1 - ( t - τ 0 ) ( 1 - 2 ) 1 2 , y ¯ = x ¯

and it follows that Λ:1+N1+N is a diffeomorphism of class 𝒞q0 and that |detJΛ|=1.

We prove that

(4.20) s > 0 t < τ 0 + φ ~ ( x )

and that

(4.21) Λ ( 𝒯 ) ( 0 , δ 0 2 ) × N .

In the case where =0, by (4.4), we have X(y)=y and thus by (4.12), ψ(y)=φ~(y). Thus in this case,

(4.22) Λ ( t , x ) = ( φ ~ ( x ) - t + τ 0 , x ) .

Property (4.20) follows. Moreover,

s φ ~ ( x ) + τ 0 | x | + τ 0 2 τ 0 + ε 0 3 τ 0 < δ 0 2

by (4.16). Thus (4.21) is proved in this case.

In the case where 0, we observe that from (4.12),

s = φ ~ ( X ( y ) ) - X 1 ( y ) ( 1 - 2 ) 1 2 - t - τ 0 - x 1 ( 1 - 2 ) 1 2 .

Using (4.10), we replace φ~(X(y))=1(X1(y)-(1-2)12y1) so that

( 1 - 2 ) - 1 2 s = φ ~ ( X ( y ) ) - 2 X 1 ( y ) ( 1 - 2 ) - ( t - τ 0 ) - 2 x 1 ( 1 - 2 ) = X 1 ( y ) - y 1 ( 1 - 2 ) 1 2 + x 1 - ( t - τ 0 ) ( 1 - 2 ) - x 1 = X 1 ( y ) - x 1 .

Recall that by (4.8), we have

x 1 = X 1 ( x 1 - φ ~ ( x ) ( 1 - 2 ) 1 2 , x ¯ ) ,

which means that

(4.23) ( 1 - 2 ) - 1 2 s = X 1 ( x 1 - ( t - τ 0 ) ( 1 - 2 ) 1 2 , x ¯ ) - X 1 ( x 1 - φ ~ ( x ) ( 1 - 2 ) 1 2 , x ¯ ) ,

hence, using (4.9),

(4.24) - ( 1 + 1 - ) 1 2 s t - ( 1 - 1 + ) 1 2

on 1+N. Thus we see that s>0 is equivalent to t<τ0+φ~(x), i.e. (4.20) holds. Moreover, by (4.24), we have on 𝒯

s ( 1 + 1 - ) 1 2 | t - τ 0 - φ ~ ( x ) | = ( 1 + 1 - ) 1 2 ( τ 0 + φ ~ ( x ) - t ) .

Using (4.16), we see that τ0+φ~(x)-t<φ~(x)+τ03τ0, so that s<δ02. Thus (4.21) is proved in all cases.

We now set

(4.25) u ( t , x ) = v ( Λ ( t , x ) ) , ( t , x ) 𝒯 .

We refer to [18, Exercise 10.7.c] for a similar use of the Lorentz transform. Note that by (4.21), u is well defined.

Let ω be an open subset of N and let 0a<b. Suppose that [a,b]×ω¯𝒯. We claim that

(4.26) u H 2 ( ( a , b ) × ω ) ,
(4.27) u L q ( ( a , b ) × ω ) for all  1 q < ,
(4.28) t t u = Δ u + | u | p - 1 u in  L 2 ( ( a , b ) × ω ) .

Since [a,b]×ω¯ is a compact subset of 1+N, it follows that Λ([a,b]×ω¯) is a compact subset of 1+N. Moreover, it follows from (4.20)–(4.21) that Λ([a,b]×ω¯) is a compact subset of (0,δ0)×N. Let 1q<. Since vC((0,δ0),H2(N)) and H2(N)Lr(N) for every r< (because N4), we have vLq(Λ((a,b)×ω)); and so (4.27) follows from (4.25) and the change of variable formula. Next, let θCc((0,δ0)×N) such that θ(x)1 on Λ([a,b]×ω¯). Thus we may replace v by θv in formula (4.25), this does not change the values of u on (a,b)×ω. Since θvH2((0,δ0)×N), we can approximate θv in H2((0,δ0)×N) by a sequence (wn)n1Cc((0,δ0)×N) supported in a fixed compact of (0,δ0)×N. Setting un=wnΛ, we have

(4.29) ( a , b ) × ω | u n - u | 2 = Λ ( ( a , b ) × ω ) | w n - v | 2 | det J Λ | - 1 = Λ ( ( a , b ) × ω ) | w n - θ v | 2 n 0 .

Next, it follows from (4.25) that

( 1 - 2 ) t t u n = [ 2 ( y 1 ψ ( ) ) 2 + 2 y 1 ψ ( ) + 1 ] s s w n ( ) + 2 y 1 y 1 ψ ( ) s w n ( ) + 2 ( y 1 ψ ( ) + 1 ) s y 1 w n ( ) + 2 y 1 y 1 w n ( )

and

( 1 - 2 ) Δ u n = [ ( y 1 ψ ( ) ) 2 + ( 1 - 2 ) k 1 ( y k ψ ( ) ) 2 + 2 y 1 ψ ( ) + 2 ] s s w n ( ) + y 1 y 1 ψ ( ) s w n ( ) + 2 ( y 1 ψ ( ) + ) s y 1 w n ( ) + 2 ( 1 - 2 ) k 1 y k ψ ( ) s y k w n ( ) + y 1 y 1 w n ( ) + ( 1 - 2 ) Δ ¯ w n ( ) + ( 1 - 2 ) ( Δ ¯ ψ ( ) ) s w n ( ) ,

where the argument of ψ is y and the argument of wn is Λ.

Similar formulas hold for all first and second space-time derivatives of un, so arguing as in (4.29) we conclude that un is a Cauchy sequence in H2((a,b)×ω), from which (4.26) follows. In addition, the above two formulas imply that

t t u n - Δ u n = [ 1 - | ψ ( ) | 2 ] s s w n ( ) - 2 ψ ( ) s w n ( ) - Δ ψ ( ) s w n ( ) - Δ w n ( ) .

Since unu in H2((a,b)×ω) and wnθv in H2((0,δ0)×N), we may pass to the limit in the above equation. Since θv=v in Λ((a,b)×ω), we obtain using (2.2)

t t u - Δ u = [ 1 - | ψ ( ) | 2 ] s s v ( ) - 2 ψ ( ) s v ( ) - Δ ψ ( ) s v ( ) - Δ v ( ) = ( | v | p - 1 v ) ( ) = | u | p - 1 u

in L2((a,b)×ω). This proves (4.28).

Set

ρ ~ = τ 0 + ε 0 2

and

τ ~ = min { ε 0 2 , τ 0 + inf | x | τ 0 + ε 0 { φ ~ ( x ) } }

so that τ~>0 by (4.17). We see that (0,τ~)×Bρ~𝒯 so that uH2((0,τ~)×Bρ~)Lq((0,τ~)×Bρ~) for all q<. In particular, uC([0,τ~],H1(Bρ~))C1([0,τ~],L2(Bρ~)), so that u(0)H1(Bρ~) and tu(0)L2(Bρ~) are well defined.

4.5 Choice of a Solution of the Nonlinear Wave Equation

We apply Section 1.2 to extend u, which is a solution of (1.1) on 𝒯, to a solution of (1.1) on a maximal domain of influence that contains 𝒯. For this, we consider any pair (u~0,u~1)H1(N)×L2(N) such that u~0 and u~1 coincide with u(0) and tu(0), respectively, on Bρ~. The initial data (u~0,u~1) give rise to a solution u~ of (1.1) defined on the maximal influence domain Ωmax(u~0,u~1) in the sense of Section 1.2. We claim that this maximal influence domain contains

𝒯 ~ = 𝒯 { ( t , x ) [ 0 , ρ ~ ) × N : | x | < ρ ~ - t }

and that u~ coincides with u on 𝒯~. Indeed, let (t,x)𝒯~ and consider the corresponding open backward cone C(t,x). The cone C(t,x) is an influence domain, and it follows easily, using Proposition B.2 and (4.27), that u is a solution of (1.1) in C(t,x) with initial data (u0,u1), so that C(t,x)Ωmax(u~0,u~1). Since (t,x)𝒯~ is arbitrary, this proves the claim. From now on, we denote by u this solution.

4.6 Blowup on the Local Hypersurface and End of the Proof

We show blowup on the local hypersurface by proving (1.4). For this, we further restrict the size of the hypersurface. Arguing as in the proof of (4.18), we see that

| x | ε 0 4 max { t > 0 : ( t , x ) 𝒯 ~ } = τ 0 + φ ~ ( x ) .

Thus we see that if |x0|ε04, then the open backward cone C(τ0+φ~(x0),x0) is a subset of 𝒯~.

We fix <σ1 and |x0|ε04, and we prove (1.4). We use the geometric property that the image by the map Λ of a cone of slope σ contains at least a small cone (estimate (4.31)), and the lower estimate (3.6) for v on this small cone.

Let s00 and y0N be given by Λ(τ0+φ~(x0),x0)=(s0,y0). We first note that s0=0 by (4.12) and (4.19). Moreover, it follows from (4.19), (4.3) and (4.16) that

(4.30) | y 0 | ε 0 4 ( 1 + 2 ( 1 - 2 ) 1 2 ) 1 .

Given 0t<τ0+φ~(x0), we set

K ( t ) = { ( t , x ) 1 + N ; t < t < τ 0 + φ ~ ( x 0 ) , | x - x 0 | < σ ( τ 0 + φ ~ ( x 0 ) - t ) }

and, given s>0 and σ>0 we set

L ( s , σ ) = { ( s , y ) 1 + N ;  0 < s < s , | y - y 0 | < σ s } .

We claim that there exist σ>0 and η>0 such that

(4.31) L ( s ( t ) , σ ) Λ ( K ( t ) ) ,

where

(4.32) s ( t ) = η ( τ 0 + φ ~ ( x 0 ) - t ) .

Assuming (4.31)–(4.32), we conclude the proof of (1.4). Given (t,x)𝒯~, it follows from (4.25) and (4.19) that

t u ( t , x ) = - 1 ( 1 - 2 ) 1 2 [ s v ( Λ ( t , x ) ) + y 1 v ( Λ ( t , x ) ) ]

so that, using 2xy2x2+y2,

| t u ( t , x ) | 2 | s v ( Λ ( t , x ) ) | 2 - | y 1 v ( Λ ( t , x ) ) | 2 .

Therefore,

K ( t ) | t u | 2 Λ ( K ( t ) ) ( | s v | 2 - | y 1 v | 2 )

Applying (3.6) and (4.31), we deduce that

(4.33) K ( t ) | t u | 2 1 4 L ( s ( t ) , σ ) | s V 0 | 2 - C | Λ ( K ( t ) ) | - Λ ( K ( t ) ) g 2 .

It follows from (4.32), (2.14) and (4.30) that

(4.34) lim inf t τ 0 + φ ~ ( x 0 ) 1 τ 0 + φ ~ ( x 0 ) - t L ( s ( t ) , σ ) | s V 0 | 2 lim inf s 0 1 s L ( s , σ ) | s V 0 | 2 > 0 .

Furthermore,

(4.35) | Λ ( K ( t ) ) | | K ( t ) | ( τ 0 + φ ~ ( x 0 ) - t ) 1 + N .

Next, H1(N)L2(N+2)N(N), so that g2LN+2N((0,δ0)×N)); and so by (4.35),

(4.36) Λ ( K ( t ) ) g 2 | Λ ( K ( t ) ) | 2 N + 2 ( τ 0 + φ ~ ( x 0 ) - t ) 1 + N N + 2 .

Estimate (1.4) follows from (4.33)–(4.36).

It remains to prove the claim (4.31)–(4.32). Let (s,y)+1+N and (t,x)1+N such that (s,y)=Λ(t,x). In particular, tτ0+φ~(x) by (4.20). We prove that

(4.37) s ( 1 + 1 - ) 1 2 ( τ 0 + φ ~ ( x 0 ) - t + | x - x 0 | ) .

In the case =0, this follows from (4.22) and the inequality |φ~(x)-φ~(x0)||x-x0| (see (4.3)). In the case 0, then by (4.19) and (4.23),

( 1 - 2 ) - 1 2 s = X 1 ( y 1 , y ¯ ) - X 1 ( y 1 - ( τ 0 + φ ~ ( x ) - t ) ( 1 - 2 ) 1 2 , y ¯ ) .

Using the right-hand side inequality in (4.9), and then (4.3), we deduce

s ( 1 + 1 - ) 1 2 ( τ 0 + φ ~ ( x ) - t )

and (4.37) by using again (4.3).

Next we claim that

(4.38) | x - x 0 | | y - y 0 | + ( τ 0 + φ ~ ( x 0 ) - t ) .

Indeed, by (4.19) for (t,x) and for (τ0+φ~(x0),x0),

y 1 - ( y 0 ) 1 = x 1 - ( x 0 ) 1 ( 1 - 2 ) 1 2 + ( τ 0 + φ ~ ( x 0 ) - t ) ( 1 - 2 ) 1 2 ,
y ¯ - y ¯ 0 = x ¯ - x ¯ 0

so that

| x 1 - ( x 0 ) 1 | | y 1 - ( y 0 ) 1 | + ( τ 0 + φ ~ ( x 0 ) - t ) ,
| x ¯ - x ¯ 0 | = | y ¯ - y ¯ 0 | .

Estimate (4.38) follows by using the triangle inequality (a+b)2+c2a2+c2+|b|. Assuming now (s,y)L(s,σ) for some s>0 and σ>0, we deduce from (4.38) that

| x - x 0 | σ s + ( τ 0 + φ ~ ( x 0 ) - t ) .

Estimating s by (4.37), we obtain

( 1 - σ ( 1 + 1 - ) 1 2 ) | x - x 0 | ( + σ ( 1 + 1 - ) 1 2 ) ( τ 0 + φ ~ ( x 0 ) - t ) .

Since σ>, we see that if σ>0 and δ>0 are sufficiently small, then

(4.39) | x - x 0 | ( σ - δ ) ( τ 0 + φ ~ ( x 0 ) - t ) .

It now remains to prove that if sη(τ0+φ~(x0)-t) for some sufficiently small η>0, then tt. By (4.24), and then (4.3), we deduce

s ( 1 - 1 + ) 1 2 ( τ 0 + φ ~ ( x ) - t ) ( 1 - 1 + ) 1 2 ( τ 0 + φ ~ ( x 0 ) - t - | x - x 0 | ) .

Using (4.39), we obtain

s ( 1 - σ + δ ) ( 1 - 1 + ) 1 2 ( τ 0 + φ ~ ( x 0 ) - t ) ,

which proves the claim for η=(1-σ+δ)(1-1+)12.

Finally, we prove that the hypersurface {(t,x)+1+N:|x0|<ε04,t=τ0+φ~(x0)} is contained in the upper boundary of the maximal influence domain Ωmax of the solution u. Indeed, otherwise there would exist |x0|<ε04 and t>τ0+φ~(x0) such that C(t,x0)Ωmax with the notation (1.5). In particular,

t u C ( [ 0 , τ 0 + φ ~ ( x 0 ) ) , L 2 ( { | x - x 0 | < t - τ 0 - φ ~ ( x 0 ) 2 } ) ) .

This is absurd, since by (1.4), given <σ1, there exist a sequence tnτ0+φ~(x0) and δ>0 such that

{ | x - x 0 | < σ ( τ 0 + φ ~ ( x 0 ) - t n ) } | t u ( t n ) | 2 δ .

This completes the proof of the theorem, where τ0 and ε0 are given by (4.16), and ε=min{ε04,r} with r defined in Section 1.1 (recall that φ=φ~ on {|x|<r}).


Dedicated to Laurent Véron on the occasion of his 70th birthday



Communicated by Julian Lopez Gomez and Patrizia Pucci


Funding statement: Lifeng Zhao was partially supported by the NSFC Grant of China No. 11771415.

A The Wave Equation (2.2)

Let ψ𝒞2(N)W2,(N) satisfy ψL<1. It follows in particular that (1-|ψ|2)-1C1(N)W1,(N).

A.1 The Associated Semigroup

Let X be the Hilbert space H1×L2, equipped with the (equivalent) scalar product

( a , b ) , ( a ~ , b ~ ) X = ( a a ~ + a a ~ ) + b b ~ ( 1 - | ψ | 2 ) ,

and consider the linear operator 𝒜 on X defined by

𝒜 = ( 0 1 Δ - 1 1 - | ψ | 2 2 ψ + Δ ψ 1 - | ψ | 2 ) ,

with domain D(𝒜)=H2×H1. We compute

𝒜 ( a , b ) , ( a , b ) X = ( a b + a b ) + ( Δ a - a ) b + ( 2 ψ b + ( Δ ψ ) b ) b = 0 ,

which proves that 𝒜 is dissipative in X. Moreover, for any (c,d)X, there exist (a,b)D(𝒜) such that (a,b)-𝒜(a,b)=(c,d). Indeed, this system reduces to

{ b = a - c , 2 a - Δ a - 2 ψ a - ( Δ ψ ) a = - 2 ψ c - ( Δ ψ ) c + c + ( 1 - | ψ | 2 ) d .

It is easy to solve the second equation by the Lax–Milgram theorem, and we obtain a solution aH1(N). Since, by the equation, ΔaL2(N), we see that aH2(N). The first equation then yields bH1(N). In particular, 𝒜 is maximal dissipative, hence is the generator of a C0 semigroup of contractions (et𝒜)t0 on X. (See, e.g., [27, Chapter 1, Theorem 4.3, p. 14].)

A.2 The Nonlinear Equation

Using the notation U=(vsv), we rewrite equation (2.2) as

(A.1) s U = 𝒜 U + ( U ) ,

where

(A.2) ( a b ) = ( 1 - | ψ | 2 ) - 1 ( 0 f ( a ) + a ) .

A.3 Regularity

Suppose T>0 and UL((0,T),D(𝒜))W1,((0,T),X) is such that (U)L((0,T),X) and U satisfies equation (A.1) for a.a. 0<t<T. If (U)C((0,T),D(𝒜)), then UC((0,T),D(𝒜))C1((0,T),X). Indeed, U is weakly continuous (0,T)D(𝒜). In particular, U(t)D(𝒜) for all 0<t<T and the result follows easily, see, e.g., [27, Chapter 4, Corollary 2.6, p. 108].

A.4 The Case of Equation (3.7)

Equation (3.7) is equation (A.1), where f is replaced by fn in (A.2). Since fn(0)=0 and fn is globally Lipschitz , we see that the map ufn(u) is globally Lipschitz L2(N)L2(N). In particular, :XX is globally Lipschitz, and the existence and uniqueness of a global, mild solution UC([0,),X) of (A.1) with the initial condition U(0)=U0X is a direct consequence of standard semigroup theory. (See, e.g., [27, Chapter 6, Theorem 1.2, p. 184].) Moreover, since fn is globally Lipschitz and C1, it follows easily that the map ufn(u) is continuous H1(N)H1(N). Therefore is continuous XD(𝒜), so that (U)C([0,),D(𝒜)). It follows, again by the semigroup theory, that if the initial value is in D(𝒜), then UC([0,),D(𝒜))C1([0,),X) is a solution of (A.1). (See, e.g., [27, Chapter 4, Corollary 2.6, p. 108].)

B Uniqueness on Light Cones

We state and prove a uniqueness property for solutions of the nonlinear wave equation on light cones (Proposition B.2), for which we could not find a reference. We first recall in the following remark the relevant results concerning the local well-posedness of the Cauchy problem.

Remark B.1 (Local Well-Posedness).

Let N1, let p such that 1<pN+2N-2 (1<p< if N=1,2) and let (u0,u1)H1(N)×L2(N). We summarize some results on the existence of T>0 and a local solution

(B.1) u C ( [ 0 , T ] , H 1 ( N ) ) C 1 ( [ 0 , T ] , L 2 ( N ) )

of the wave equation

(B.2) { t t u - Δ u = | u | p - 1 u , u ( 0 ) = u 0 , t u ( 0 ) = u 1 .

We also discuss the property

(B.3) u L 2 ( N + 1 ) N - 2 ( ( 0 , T ) × N )

in the case N3.

(i) Case N=1,2. There exist T>0 and a unique solution u of (B.2) in the class (B.1). See, e.g., [5, Theorem 6.2.2].

(ii) Case N3, p<N+2N-2. There exist T>0 and a unique solution u of (B.2) in the class (B.1), and this solution satisfies (B.3) by possibly choosing T smaller. Indeed, existence follows from [12, Proposition 2.3] and uniqueness from [11, Proposition 3.1]. Moreover, applying [11, Lemma 3.3] with ρ=N2(N-1), r=2(N2-1)N2-2N+3 and q=2(N+1)N-1, we see that uLq((0,T),B˙r,2ρ(N)), hence (B.3) by Sobolev’s embedding.

(iii) Case N=3, p=5. There exist T>0 and a solution u of (B.2) in the class (B.1)–(B.3). See, e.g., [15, Theorem 2.7]. Moreover, solutions of (B.2) in the class (B.1)–(B.3) are unique. This last property is not explicitly stated in [15], but it easily follows from the proof. (It also follows from Proposition B.2.)

(iv) Case N4, p=N+2N-2. There exist T>0 and a unique solution u of (B.2) in the class (B.1), and this solution satisfies property (B.3) by possibly choosing T smaller. Indeed, existence is established in [10] (see also [15, Theorem 2.7] for the case N=4,5 and [2, Theorem 3.3] for the case N6). Uniqueness is proved in [28, Theorem 2] for N=4, in [28, Theorem 3] for N=5 and in [2, Theorem 3.4] for N6. Property (B.3) follows from [15, Theorem 2.7] in the case N=4,5. In the case N6, it follows from [2, Theorem 3.3] that uLq((0,T),B˙r,2ρ(N)) with ρ=N2(N-1), r=2(N2-1)N2-2N+3 and q=2(N+1)N-1, hence (B.3) by Sobolev’s embedding.

Proposition B.2 (Uniqueness on Light Cones).

Let N1 and let p satisfy 1<pN+2N-2 (1<p< if N=1,2). Let R>0, 0<τ<R, and let BR be the open ball of center 0 and radius R in RN. Let

u , v C ( [ 0 , τ ] , H 1 ( B R ) ) C 1 ( [ 0 , τ ] , L 2 ( B R ) ) C 2 ( [ 0 , τ ] , H - 1 ( B R ) ) )

be two solutions of the wave equation ttu=Δu+|u|p-1u in H-1(BR)) for tτ. If N3 and p>NN-2, suppose in addition that u,vL2(N+1)N-2((0,T)×BR). If u(0)=v(0) and tu(0)=tv(0), then

u = v on  { ( t , x ) ( 0 , τ ) × B R : | x | < R - t } .

The proof of Proposition B.2 relies on the following local estimates.

Lemma B.3.

Let R>0, 0<τ<R, hC([0,τ],Lq(BR)) for some q1, q2NN+2 (so that hC([0,τ],H-1(BR))), and let

z C ( [ 0 , τ ] , L 2 ( B R ) ) C 1 ( [ 0 , τ ] , H - 1 ( B R ) ) C 2 ( [ 0 , τ ] , H - 2 ( B R ) )

satisfy ttz=Δz+h in H-2(BR) for all 0tτ and if z(0)=tz(0)=0. If h|E(0,R,τ)L2(E(0,R,τ)) with the notation (1.6), then z(t)H1(BR-t) for all 0<t<τ, and

(B.4) z ( t ) H 1 ( B R - t ) C e C t h L 2 ( E ( 0 , R , t ) )

for all 0<t<τ. If N2 and hL2(N+1)N+3(E(0,R,τ)), then z|E(0,R,τ)L2(N+1)N-1(E(0,R,τ)) and

(B.5) z L 2 ( N + 1 ) N - 1 ( E ( 0 , R , τ ) ) C h L 2 ( N + 1 ) N + 3 ( E ( 0 , R , τ ) ) .

In (B.4) and (B.5), the constant C independent of h, R, τ and t.

Proof.

We define h~C([0,τ],Lq(N)) by

h ~ = { h on  ( 0 , τ ) × B R , 0 elsewhere .

We let z~C([0,τ],L2(N))C1([0,τ],H-1(N))C2([0,τ],H-2(N)) be the solution of the wave equation ttz~-Δz~=h~ on N with the initial conditions z~(0)=tz~(0)=0. Note that, given any 0<tτ<R and 1r,

h ~ L r ( E ( 0 , R , t ) ) = h L r ( E ( 0 , R , t ) ) .

Therefore, estimate (B.4) with z replaced by z~ follows from the standard energy inequality for z~; and (B.5) with z replaced by z~ follows from the Strichartz estimates (see [13, Corollary 1.3]).

To conclude the proof, we show that z and z~ coincide on E(0,R,τ). We let w(t)=(z(t)-z~(t))|BR for all 0tτ, so that

(B.6) w C ( [ 0 , τ ] , L 2 ( B R ) ) C 1 ( [ 0 , τ ] , H - 1 ( B R ) ) C 2 ( [ 0 , τ ] , H - 2 ( B R ) )

satisfies ttw=Δw in H-2(BR) for all 0tτ and w(0)=tw(0)=0. Thus we need to show that w=0 a.e. on E(0,R,τ). Let ρCc(N), ρ0, be radially symmetric, supported in B1, and satisfy ρ=1. Given ε>0, let ρε(x)=ε-Nρ(xε). Let 0<η<R and 0<ε<η2. Since ρε is supported in Bε, it follows that ρεw is well defined in BR-η, and we set wε=(ρεw)|BR-η. We claim that

(B.7) w ε C 2 ( [ 0 , τ ] × B R - η ¯ ) ,
(B.8) t t w ε = Δ w ε on  [ 0 , τ ] × B R - η ¯ ,
(B.9) w ε ( 0 ) = t w ε ( 0 ) = 0 on  B R - η .

By finite speed of propagation, it follows that wε identically vanishes on E(0,R-η,τ). Letting ε0, we deduce that w vanishes a.e. on E(0,R-η,τ); and letting η0, we see that w vanishes a.e. on E(0,R,τ). It remains to prove the claims (B.7)–(B.9). Given m and θH-m(BR)), recall that ρεθH-m(BR-η)) is given by

ρ ε θ , φ H - m ( B R - η ) , H 0 m ( B R - η ) = θ , ρ ε φ H - m ( B R ) , H 0 m ( B R )

for all φCc(BR-η). It is well known that

ρ ε θ C ( B R - η ¯ ) ) ,
D α ( ρ ε θ ) = ρ ε ( D α θ ) for all  α N ,
ρ ε θ C ( B R - η ¯ ) θ H - m ( B R ) .

On the other hand, it follows from (B.6) that DαtβwC([0,τ],H-2(BR)) for all αN and β such that |α|+β2. Thus we see that DαtβwεC([0,τ]×BR-η¯) and that

D α t β w ε = ρ ε D α t β w .

Properties (B.7)–(B.9) easily follow. ∎

Proof of Proposition B.2.

We need only prove the result for τ small, the general case follows by iteration.

The Case pNN-2 (any 1<p< if N=1,2). We note that r=2p satisfies 2<r2NN-2 (2<r< if N=1,2), so that by (B.4) and Sobolev’s embedding

( u - v ) ( t ) L r ( B R - t ) 2 C e C t 0 t | u | p - 1 u - | v | p - 1 v L 2 ( B R - s ) 2 𝑑 s .

Since |u|p-1u-|v|p-1vL2C(uLr+vLr)p-1u-vLr and u and v are bounded in H1, hence in Lr, the result follows by Gronwall’s inequality.

The Case N3 and p=N+2N-2. We note that, since pN+2N-2,

| | u | p - 1 u - | v | p - 1 v | ( | u | p - 1 + | v | p - 1 ) | u - v | ( 1 + | u | 4 N - 2 + | v | 4 N - 2 ) | u - v | .

By Hölder’s inequality, it follows that

| u | p - 1 u - | v | p - 1 v L 2 ( N + 1 ) N + 3 ( τ 2 N + 1 + u L 2 ( N + 1 ) N - 2 4 N - 2 + u L 2 ( N + 1 ) N - 2 4 N - 2 ) u - v L 2 ( N + 1 ) N - 1 ,

where all the integrals are on E(0,R,τ), with the notation (1.6). Applying the Strichartz inequality (B.5), we deduce that

u - v L 2 ( N + 1 ) N - 1 C ( τ 2 N + 1 + u L 2 ( N + 1 ) N - 2 4 N - 2 + u L 2 ( N + 1 ) N - 2 4 N - 2 ) u - v L 2 ( N + 1 ) N - 1 ,

where all the integrals are on E(0,R,τ). Since

u L 2 ( N + 1 ) N - 2 ( E ( 0 , R , τ ) ) + v L 2 ( N + 1 ) N - 2 ( E ( 0 , R , τ ) ) τ 0 0 ,

the conclusion follows by choosing τ sufficiently small. ∎

References

[1] S. Alinhac, Blowup for Nonlinear Hyperbolic Equations, Progr. Nonlinear Differential Equations Appl. 17, Birkhäuser, Boston, 1995. 10.1007/978-1-4612-2578-2Search in Google Scholar

[2] A. Bulut, M. Czubak, D. Li, N. Pavlović and X. Zhang, Stability and unconditional uniqueness of solutions for energy critical wave equations in high dimensions, Comm. Partial Differential Equations 38 (2013), no. 4, 575–607. 10.1080/03605302.2012.756520Search in Google Scholar

[3] L. A. Caffarelli and A. Friedman, Differentiability of the blow-up curve for one-dimensional nonlinear wave equations, Arch. Ration. Mech. Anal. 91 (1985), no. 1, 83–98. 10.1007/978-3-642-83743-2_1Search in Google Scholar

[4] L. A. Caffarelli and A. Friedman, The blow-up boundary for nonlinear wave equations, Trans. Amer. Math. Soc. 297 (1986), no. 1, 223–241. 10.1090/S0002-9947-1986-0849476-3Search in Google Scholar

[5] T. Cazenave and A. Haraux, An Introduction to Semilinear Evolution Equations, Oxford Lecture Ser. Math. Appl. 13, The Clarendon Press, New York, 1998. 10.1093/oso/9780198502777.001.0001Search in Google Scholar

[6] T. Cazenave, Y. Martel and L. Zhao, Solutions blowing up on any given compact set for the energy subcritical wave equation, preprint (2018), https://arxiv.org/abs/1812.03949; J. Differential Equations (2019), DOI 10.1016/j.jde.2019.08.030. 10.1016/j.jde.2019.08.030Search in Google Scholar

[7] T. Cazenave, Y. Martel and L. Zhao, Finite-time blowup for a Schrödinger equation with nonlinear source term, Discrete Contin. Dyn. Syst. 39 (2019), no. 2, 1171–1183. 10.3934/dcds.2019050Search in Google Scholar

[8] G. M. Constantine and T. H. Savits, A multivariate Faà di Bruno formula with applications, Trans. Amer. Math. Soc. 348 (1996), no. 2, 503–520. 10.1090/S0002-9947-96-01501-2Search in Google Scholar

[9] R. Donninger and B. Schörkhuber, Stable self-similar blow up for energy subcritical wave equations, Dyn. Partial Differ. Equ. 9 (2012), no. 1, 63–87. 10.4310/DPDE.2012.v9.n1.a3Search in Google Scholar

[10] J. Ginibre, A. Soffer and G. Velo, The global Cauchy problem for the critical nonlinear wave equation, J. Funct. Anal. 110 (1992), no. 1, 96–130. 10.1016/0022-1236(92)90044-JSearch in Google Scholar

[11] J. Ginibre and G. Velo, The global Cauchy problem for the nonlinear Klein–Gordon equation, Math. Z. 189 (1985), no. 4, 487–505. 10.1007/BF01168155Search in Google Scholar

[12] J. Ginibre and G. Velo, The global Cauchy problem for the nonlinear Klein–Gordon equation. II, Ann. Inst. H. Poincaré Anal. Non Linéaire 6 (1989), no. 1, 15–35. 10.1016/s0294-1449(16)30329-8Search in Google Scholar

[13] M. Keel and T. Tao, Endpoint Strichartz estimates, Amer. J. Math. 120 (1998), no. 5, 955–980. 10.1353/ajm.1998.0039Search in Google Scholar

[14] J. B. Keller, On solutions of nonlinear wave equations, Comm. Pure Appl. Math. 10 (1957), 523–530. 10.1002/cpa.3160100404Search in Google Scholar

[15] C. E. Kenig and F. Merle, Global well-posedness, scattering and blow-up for the energy-critical focusing non-linear wave equation, Acta Math. 201 (2008), no. 2, 147–212. 10.1007/s11511-008-0031-6Search in Google Scholar

[16] S. Kichenassamy, Fuchsian equations in Sobolev spaces and blow-up, J. Differential Equations 125 (1996), no. 1, 299–327. 10.1006/jdeq.1996.0033Search in Google Scholar

[17] S. Kichenassamy, The blow-up problem for exponential nonlinearities, Comm. Partial Differential Equations 21 (1996), no. 1–2, 125–162. 10.1080/03605309608821177Search in Google Scholar

[18] S. Kichenassamy, Fuchsian Reduction. Applications to Geometry, Cosmology, and Mathematical Physics, Progr. Nonlinear Differential Equations Appl. 71, Birkhäuser, Boston, 2007. 10.1007/978-0-8176-4637-0Search in Google Scholar

[19] S. Kichenassamy, Control of blow-up singularities for nonlinear wave equations, Evol. Equ. Control Theory 2 (2013), no. 4, 669–677. 10.3934/eect.2013.2.669Search in Google Scholar

[20] S. Kichenassamy and W. Littman, Blow-up surfaces for nonlinear wave equations. I, Comm. Partial Differential Equations 18 (1993), no. 3–4, 431–452. 10.1080/03605309308820936Search in Google Scholar

[21] S. Kichenassamy and W. Littman, Blow-up surfaces for nonlinear wave equations. II, Comm. Partial Differential Equations 18 (1993), no. 11, 1869–1899. 10.1080/03605309308820997Search in Google Scholar

[22] R. Killip and M. Visan, Smooth solutions to the nonlinear wave equation can blow up on Cantor sets, preprint (2011), https://arxiv.org/abs/1103.5257. Search in Google Scholar

[23] H. A. Levine, Instability and nonexistence of global solutions to nonlinear wave equations of the form Putt=-Au+(u), Trans. Amer. Math. Soc. 192 (1974), 1–21. 10.1090/S0002-9947-1974-0344697-2Search in Google Scholar

[24] H. Lindblad, Blow-up for solutions of u=|u|p with small initial data, Comm. Partial Differential Equations 15 (1990), no. 6, 757–821. 10.1080/03605309908820708Search in Google Scholar

[25] F. Merle and H. Zaag, Isolatedness of characteristic points at blow-up for a semilinear wave equation in one space dimension, Seminaire: Equations aux Dérivées Partielles. 2009–2010, Sémin. Équ. Dériv. Partielles, École Polytechnique, Palaiseau (2012), Exp. No. 11. Search in Google Scholar

[26] F. Merle and H. Zaag, On the stability of the notion of non-characteristic point and blow-up profile for semilinear wave equations, Comm. Math. Phys. 333 (2015), no. 3, 1529–1562. 10.1007/s00220-014-2132-8Search in Google Scholar

[27] A. Pazy, Semigroups of Linear Operators and Applications to Partial Differential Equations, Appl. Math. Sci. 44, Springer, New York, 1983. 10.1007/978-1-4612-5561-1Search in Google Scholar

[28] F. Planchon, On uniqueness for semilinear wave equations, Math. Z. 244 (2003), no. 3, 587–599. 10.1007/s00209-003-0509-zSearch in Google Scholar

Received: 2019-04-15
Accepted: 2019-08-17
Published Online: 2019-09-18
Published in Print: 2019-11-01

© 2019 Walter de Gruyter GmbH, Berlin/Boston

This work is licensed under the Creative Commons Attribution 4.0 International License.

Downloaded on 18.9.2025 from https://www.degruyterbrill.com/document/doi/10.1515/ans-2019-2059/html
Scroll to top button