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Dedicated to Professor Tohru Ozawa on the occasion of his sixties birthday \rcvdate \rvsdate

Recent developments on the lifespan estimate for classical solutions of nonlinear wave equations
in one space dimension

Hiroyuki Takamura Mathematical Institute, Tohoku University, Aoba, Sendai 980-8578, Japan. [email protected]
Abstract.

In this paper, we overview the recent progresses on the lifespan estimates of classical solutions of the initial value problems for nonlinear wave equations in one space dimension. There are mainly two directions of the developments on the model equations which ensure the optimality of the general theory. One is on the so-called “combined effect” of two kinds of the different nonlinear terms, which shows the possibility to improve the general theory. Another is on the extension to the non-autonomous nonlinear terms which includes the application to nonlinear damped wave equations with the time-dependent critical case.

Key words and phrases:
nonlinear wave equation, initial value problem, one space dimension, classical solution, lifespan
2010 Mathematics Subject Classification:
primary 35L71, secondary 35B44

1. Introduction.

In order to illustrate our purpose, let us turn back to the general theory for nonlinear wave equations in one space dimension which was introduced by Li, Yu and Zhou [19, 20] more than 30 years ago.

We consider the initial value problem of the form;

{uttuxx=H(u,ut,ux,uxx,uxt)in𝐑×(0,T),u(x,0)=εf(x),ut(x,0)=εg(x)forx𝐑,\left\{\begin{array}[]{ll}\displaystyle u_{tt}-u_{xx}=H(u,u_{t},u_{x},u_{xx},u_{xt})&\quad\mbox{in}\ {\bf R}\times(0,T),\\ u(x,0)={\varepsilon}f(x),\quad u_{t}(x,0)={\varepsilon}g(x)&\quad\mbox{for}\ x\in{\bf R},\end{array}\right. (1)

where T>0T>0, f,gC0(𝐑)f,g\in C_{0}^{\infty}({\bf R}) and ε>0{\varepsilon}>0 is a sufficiantly small parameter. Let λ~=(λ;(λi),i=0,1;(λij),i,j,=0,1,i+j1).\widetilde{\lambda}=(\lambda;\ (\lambda_{i}),i=0,1;\ (\lambda_{ij}),i,j,=0,1,i+j\geq 1). Assume that H=H(λ~)H=H(\widetilde{\lambda}) is a sufficiently smooth function with

H(λ~)=O(|λ~|1+α)H(\widetilde{\lambda})=O(|\widetilde{\lambda}|^{1+\alpha})

in a neighborhood of λ~=0\widetilde{\lambda}=0, where α𝐍\alpha\in{\bf N}. Let us define the lifespan T~(ε)\widetilde{T}({\varepsilon}) as the maximal existence time of the classical solution of (1) with arbitrary fixed data. We are interested in the long-time stability of the trivial solution due to the fact that we cannot expect any time-decay of the solution of the free wave equation in one space dimension. Indeed, the general theory is to express the lower bound of T~(ε)\widetilde{T}({\varepsilon}) by means of the smallness of the initial data, i.e. ε{\varepsilon}, for which, Li, Yu and Zhou [19, 20] obtained

T~(ε){Cεα/2in general case,Cεα(α+1)/(α+2)if𝐑g(x)𝑑x=0,Cεmin{β0/2,α}ifuβH(0)=0for 1+αββ0,\widetilde{T}({\varepsilon})\geq\left\{\begin{array}[]{lll}C{\varepsilon}^{-\alpha/2}&\mbox{in general case,}\\ C{\varepsilon}^{-\alpha(\alpha+1)/(\alpha+2)}&\mbox{if}\ \displaystyle\int_{{\bf R}}g(x)dx=0,\\ C{\varepsilon}^{-\min\{\beta_{0}/2,\alpha\}}&\mbox{if}\ \partial_{u}^{\beta}H(0)=0\ \mbox{for}\ 1+\alpha\leq\forall\beta\leq\beta_{0},\end{array}\right. (2)

where CC is a positive constant independent of ε{\varepsilon}. This result has been expected complete more than 30 years.

Beyond the general theory, our interest went to its optimality or to extending the general theory by studying the morel problem;

{uttuxx=A(x,t)|ut|p|u|q+B(x,t)|u|rin𝐑×(0,T),u(x,0)=εf(x),ut(x,0)=εg(x),x𝐑,\left\{\begin{array}[]{ll}\displaystyle u_{tt}-u_{xx}=A(x,t)|u_{t}|^{p}|u|^{q}+B(x,t)|u|^{r}&\mbox{in}\quad{\bf R}\times(0,T),\\ u(x,0)={\varepsilon}f(x),\ u_{t}(x,0)={\varepsilon}g(x),&x\in{\bf R},\end{array}\right. (3)

where p,q,r>1p,q,r>1 (qq could be zero) and A,BA,B are non-negative functions of space-time variables. Let us write the lifespan of classical solutions of (3) by T(ε)T({\varepsilon}). According to the series of our studies on the estimates of T(ε)T({\varepsilon}), we will see later that the general theory can be improved in some case, which arises from the constant coefficient case. This part is presented in Section 2. Moreover, the principle in extending the nonlinear term HH in (1) of the general theory to the non-autonomous one H=H(x,t,u,ut,ux,uxx,uxt)H=H(x,t,u,u_{t},u_{x},u_{xx},u_{xt}) must be initiated by variable coefficient case. This part is presented in Section 3.

2. Case of constant coefficients and the combined effect.

In this section, we assume that

A(x,t)A0andB(x,t)B0.A(x,t)\equiv A_{0}\quad\mbox{and}\quad B(x,t)\equiv B_{0}.

where A0A_{0} and B0B_{0} are non-negative constants.

2.1. The generalized combined effect.

When A0=0A_{0}=0 and B0>0B_{0}>0, Zhou [38] obtained the estimates of T(ε)T({\varepsilon});

T(ε){Cε(r1)/2if𝐑g(x)𝑑x0,Cεr(r1)/(r+1)if𝐑g(x)𝑑x=0.T({\varepsilon})\sim\left\{\begin{array}[]{lll}C{\varepsilon}^{-(r-1)/2}&\mbox{if}&\displaystyle\int_{{\bf R}}g(x)dx\neq 0,\\ C{\varepsilon}^{-r(r-1)/(r+1)}&\mbox{if}&\displaystyle\int_{{\bf R}}g(x)dx=0.\end{array}\right. (4)

Here we denote the fact that there are positive constants, C1C_{1} and C2C_{2}, independent of ε{\varepsilon} satisfying E(ε,C1)T(ε)E(ε,C2)E({\varepsilon},C_{1})\leq T({\varepsilon})\leq E({\varepsilon},C_{2}) by T(ε)E(ε,C)T({\varepsilon})\sim E({\varepsilon},C). The classification by total integral of the initial speed gg is caused by strong Huygens’ principle such as (17). On the other hand, when A0>0A_{0}>0 and B0=0B_{0}=0, we have

T(ε)Cε(p+q1)T({\varepsilon})\sim C{\varepsilon}^{-(p+q-1)} (5)

For q=0q=0, the upper bound in this estimate was obtained by Zhou [39], and the lower bound is due to Kitamura, Morisawa and Takamura [15]. For q>1q>1, (5) was verified by Zhou [40] for the upper bound with integer p,qp,q satisfying p1,q0,p+q2p\geq 1,q\geq 0,p+q\geq 2, and by Li,Yu and Zhou [19, 20] for the lower bound with integer p,qp,q satisfying p+q2p+q\geq 2 including more general but smooth terms. Note that [40] is a preprint version of Zhou [39] in which only the case of q=0q=0 is considered. But it is easy to apply its argument to the case of q>1q>1. The lower bound in this case is due to Kido, Sasaki, Takamatsu and Takamura [12].

Therefore the natural expectation is that

T(ε){Cεmin{(p+q1),(r1)/2}if𝐑g(x)𝑑x0,Cεmin{(p+q1),r(r1)/(r+1)}if𝐑g(x)𝑑x=0T({\varepsilon})\sim\left\{\begin{array}[]{ll}C{\varepsilon}^{-\min\{(p+q-1),(r-1)/2\}}&\mbox{if}\ \displaystyle\int_{{\bf R}}g(x)dx\not=0,\\ C{\varepsilon}^{-\min\{(p+q-1),r(r-1)/(r+1)\}}&\mbox{if}\ \displaystyle\int_{{\bf R}}g(x)dx=0\end{array}\right. (6)

in the case where A0>0A_{0}>0 and B0>0B_{0}>0. But, surprisingly, we have the following fact.

Theorem 1 (Morisawa, Sasaki and Takamura [24, 25], Kido, Sasaki, Takamatsu and Takamura [12]).

The conjecture (6) is true except for the case where

𝐑g(x)𝑑x=0andr+12<p+q<r.\int_{{\bf R}}g(x)dx=0\quad\mbox{and}\quad\frac{r+1}{2}<p+q<r. (7)

In this case, we have that

T(ε)Cε(p+q)(r1)/(r+1),T({\varepsilon})\sim C{\varepsilon}^{-(p+q)(r-1)/(r+1)}, (8)

which is strictly shorter than the second case in (6).

The brief proof of (8) will appear at the end of this section. We shall call this special phenomenon by “generalized combined effect” of two nonlinearities. The original “combined effect”, which means the case of q=0q=0, was first observed by Han and Zhou [5] which targeted to show the optimality of the result by Katayama [10] on the lower bound of the lifespan of classical solutions of nonlinear wave equations with a nonlinear term ut3+u4u_{t}^{3}+u^{4} in two space dimensions including more general nonlinear terms. It is known that T(ε)exp(Cε2)T({\varepsilon})\sim\exp\left(C{\varepsilon}^{-2}\right) for the nonlinear term ut3u_{t}^{3} and T(ε)=T({\varepsilon})=\infty for the nonlinear term u4u^{4}, but Katayama [10] obtained only a much worse estimate than their minimum as T(ε)cε18T({\varepsilon})\geq c{\varepsilon}^{-18}. Surprisingly, more than ten years later, Han and Zhou [5] showed that this result is optimal as T(ε)Cε18T({\varepsilon})\leq C{\varepsilon}^{-18}. They also considered (3) with q=0q=0 for all space dimensions nn bigger than 1 and obtain the upper bound of the lifespan. Its counter part, the lower bound of the lifespan, was obtained by Hidano, Wang and Yokoyama [6] for n=2,3n=2,3. See the introduction of [6] for the precise results and references. We note that the estimate (8) with q=0q=0 coincides with the lifespan estimate for the combined effect in [5, 6] if one sets n=1n=1 formally. Indeed, [5] and [6] showed that

T(ε)Cε2p(r1)/{2(r+1)(n1)p(r1)}T({\varepsilon})\sim C{\varepsilon}^{-2p(r-1)/\{2(r+1)-(n-1)p(r-1)\}} (9)

holds for n=2,3n=2,3 provided

(r1){(n1)p2}<4, 2pr2p1,r>2n1.(r-1)\{(n-1)p-2\}<4,\ 2\leq p\leq r\leq 2p-1,\ r>\frac{2}{n-1}. (10)

Later, Dai, Fang and Wang [4] improved the lower bound of lifespan for the critical case in [6]. They also show that T(ε)<T({\varepsilon})<\infty for all p,r>1p,r>1 in case of n=1n=1, i.e. (3) with q=0q=0. For the non-Euclidean setting of the results above, see Liu and Wang [21] for example, in which the application to semilinear damped wave equations is included.

2.2. Comparison with the general theory.

Here we strongly remark that our estimate in (8) is better than that of the general theory by Li, Yu and Zhou [19, 20] in the case of (7) with integer p,q,r2p,q,r\geq 2. Because our result on the lower bound of the lifespan can be established also for the smooth terms as uttuxx=utpuq+uru_{tt}-u_{xx}=u_{t}^{p}u^{q}+u^{r}. We note that there are infinitely many examples of (p,q,r)=(m,m,2m+1)(p,q,r)=(m,m,2m+1) as the inequality

r+12=m+1<p+q=2m<r=2m+1\frac{r+1}{2}=m+1<p+q=2m<r=2m+1

holds for m=2,3,4,m=2,3,4,\ldots. This fact shows a possibility to improve the general theory. We also note that, even for the original combined effect of q=0q=0, the integer points satisfying (10) are (p,r)=(2,3),(3,3),(3,4)(p,r)=(2,3),(3,3),(3,4) for n=2n=2 and (p,r)=(2,2)(p,r)=(2,2) for n=3n=3, but (9) with p=rp=r agrees with the case of A0=0A_{0}=0 and B0>0B_{0}>0. See Introduction of Imai, Kato, Takamura and Wakasa [7] for references on the case of A0=0A_{0}=0 and B0>0B_{0}>0. Hence one can say that only the lifespan estimates with (p,r)=(2,3),(3,4)(p,r)=(2,3),(3,4) for n=2n=2 are essentially in the combined effect case. If q0q\neq 0, pp is replaced with p+qp+q in the results above. Therefore it has less meaningful to consider (3) in higher space dimensions, n2n\geq 2, if we discuss the optimality of the general theory. In spite of this situation, Han and Zhou [5] studied

uttΔu=u|ut|p1+u|u|q1in𝐑2×(0,T)u_{tt}-\Delta u=u|u_{t}|^{p-1}+u|u|^{q-1}\quad\mbox{in}\ {\bf R}^{2}\times(0,T)

with 1<p4,q>11<p\leq 4,q>1 to show the blow-up part of the generalized combined effect.

Of course, some special structure of the nonlinear terms such as “null condition” guarantees the global-in-time existence. See Tartar [32], Bianchini and G. Staffilani [3], Nakamura [23], Luli, Yang and Yu [22], Zha [36, 37] for this direction. But we are interested in the optimality of the general theory.

From now on, let us make sure the fact above. If one applies the result of the general theory (2) to our problem (3) with

H(u,ut,ux,uxx,uxt)=utpuq+urwithp,q,r𝐍,H(u,u_{t},u_{x},u_{xx},u_{xt})=u_{t}^{p}u^{q}+u^{r}\quad\mbox{with}\ p,q,r\in{\bf N}, (11)

one has the following estimates in each cases.

  • When p+q<rp+q<r,

    then, we have to set α=p+q1\alpha=p+q-1 and β0=r1\beta_{0}=r-1 which yield that

    T~(ε){Cε(p+q1)/2in general,Cε(p+q)(p+q1)/(p+q+1)if𝐑g(x)𝑑x=0,Cεmin{(r1)/2,p+q1}if uβH(0)=0for p+qβr1.\widetilde{T}({\varepsilon})\geq\left\{\begin{array}[]{ll}C{\varepsilon}^{-(p+q-1)/2}&\mbox{in general},\\ C{\varepsilon}^{-(p+q)(p+q-1)/(p+q+1)}&\mbox{if}\ \displaystyle\int_{{\bf R}}g(x)dx=0,\\ C{\varepsilon}^{-\min\{(r-1)/2,p+q-1\}}&\begin{array}[]{l}\mbox{if $\partial_{u}^{\beta}H(0)=0$}\\ \mbox{for $p+q\leq\forall\beta\leq r-1$}.\end{array}\end{array}\right.

    We note that the third case is available for (11). Therefore, for p+q(r+1)/2p+q\leq(r+1)/2, we obtain that

    T~(ε)cε(p+q1)\widetilde{T}({\varepsilon})\geq c{\varepsilon}^{-(p+q-1)}

    whatever the value of 𝐑g(x)𝑑x\displaystyle\int_{{\bf R}}g(x)dx is. On the other hand, for (r+1)/2<p+q(r+1)/2<p+q, i.e.

    r12<p+q1,\frac{r-1}{2}<p+q-1,

    we obtain

    T~(ε){Cε(r1)/2if𝐑g(x)𝑑x0,Cεmax{(r1)/2,(p+q)(p+q1)/(p+q+1)}if𝐑g(x)𝑑x=0.\widetilde{T}({\varepsilon})\geq\left\{\begin{array}[]{ll}C{\varepsilon}^{-(r-1)/2}&\mbox{if}\ \displaystyle\int_{{\bf R}}g(x)dx\neq 0,\\ C{\varepsilon}^{-\max\{(r-1)/2,(p+q)(p+q-1)/(p+q+1)\}}&\mbox{if}\ \displaystyle\int_{{\bf R}}g(x)dx=0.\\ \end{array}\right.
  • When p+qrp+q\geq r,

    then, similarly to the case above, we have to set α=r1\alpha=r-1, which yields that

    T~(ε){Cε(r1)/2in general,Cεr(r1)/(r+1)if𝐑g(x)𝑑x=0,Cεmin{β0/2,(r1)}if uβH(0)=0 for rββ0.\widetilde{T}({\varepsilon})\geq\left\{\begin{array}[]{ll}C{\varepsilon}^{-(r-1)/2}&\mbox{in general},\\ C{\varepsilon}^{-r(r-1)/(r+1)}&\mbox{if}\ \displaystyle\int_{{\bf R}}g(x)dx=0,\\ C{\varepsilon}^{-\min\{\beta_{0}/2,(r-1)\}}&\mbox{if $\partial_{u}^{\beta}H(0)=0$ for $r\leq\forall\beta\leq\beta_{0}$}.\end{array}\right.

    We note that the third case does not hold for (11) by urH(0)0\partial_{u}^{r}H(0)\neq 0.

As a conclusion, for the special nonlinear term in (11), the result of the general theory is

T~(ε){Cε(p+q1)forp+qr+12,Cε(r1)/2forr+12p+qif𝐑g(x)𝑑x0\widetilde{T}({\varepsilon})\geq\left\{\begin{array}[]{ll}C{\varepsilon}^{-(p+q-1)}&\mbox{for}\ p+q\leq\displaystyle\frac{r+1}{2},\\ C{\varepsilon}^{-(r-1)/2}&\mbox{for}\ \displaystyle\frac{r+1}{2}\leq p+q\end{array}\right.\mbox{if}\ \int_{{\bf R}}g(x)dx\not=0\\

and

T~(ε){Cε(p+q1)forp+qr+12,Cεmax{(r1)/2,(p+q)(p+q1)/(p+q+1)}forr+12p+qr,Cεr(r1)/(r+1)forrp+qif𝐑g(x)𝑑x=0.\widetilde{T}({\varepsilon})\geq\left\{\begin{array}[]{l}C{\varepsilon}^{-(p+q-1)}\\ \qquad\displaystyle\mbox{for}\ p+q\leq\displaystyle\frac{r+1}{2},\\ C{\varepsilon}^{-\max\{(r-1)/2,(p+q)(p+q-1)/(p+q+1)\}}\\ \qquad\displaystyle\mbox{for}\ \displaystyle\frac{r+1}{2}\leq p+q\leq r,\\ C{\varepsilon}^{-r(r-1)/(r+1)}\\ \qquad\mbox{for}\ r\leq p+q\\ \end{array}\right.\mbox{if}\ \displaystyle\int_{{\bf R}}g(x)dx=0.

Therefore a part of our results in (8) is larger than the lower bound of T~(ε)\widetilde{T}({\varepsilon}) in that case. If one follows the proof of Theorem 1, one can find that it is easy to see that our results on the lower bounds also hold for a special term (11) by estimating the difference of nonlinear terms from above after employing the mean value theorem. This fact indicates that we still have a possibility to improve the general theory in the sense that the optimal results in (8) should be included at least.

2.3. An improvement of the general theory.

Inspired by Theorem 1, Takamatsu [30] has recently proved the following theorem which is an improvement of the general theory related to the generalized combined effect.

Theorem 2 (Takamatsu [30]).

The fourth case,

uβH(0,0,0)=0forα+1ββ0<2αand𝐑g(x)𝑑x=0,\partial_{u}^{\beta}H(0,0,0)=0\quad\mbox{for}\ \alpha+1\leq\forall\beta\leq\beta_{0}<2\alpha\quad\mbox{and}\ \displaystyle\int_{{\bf R}}g(x)dx=0,

should be added in the result of the general theory (2) with a new estimate,

T~(ε)Cεβ0(α+1)/(β0+2).\widetilde{T}({\varepsilon})\geq C{\varepsilon}^{-\beta_{0}(\alpha+1)/(\beta_{0}+2)}. (12)

We note that (12) is stronger than both the second and the third cases in (2) because we have

β0(α+1)β0+2>α(α+1)α+2byα+1β0\frac{\beta_{0}(\alpha+1)}{\beta_{0}+2}>\frac{\alpha(\alpha+1)}{\alpha+2}\quad\mbox{by}\ \alpha+1\leq\beta_{0}

and

β0(α+1)β0+2>β02byβ0<2α.\frac{\beta_{0}(\alpha+1)}{\beta_{0}+2}>\frac{\beta_{0}}{2}\quad\mbox{by}\ \beta_{0}<2\alpha.

The sharpness of (12) can be verified by setting

p=α+1,q=0,r=β0+1,p=\alpha+1,\ q=0,\ r=\beta_{0}+1,

or

p+q=α+1,r=β0+1withq0p+q=\alpha+1,\ r=\beta_{0}+1\ \mbox{with}\ q\neq 0

in Theorem 1.

We shall omit the proof of Theorem 2, but point out that it is initiated by that of Thereom 1, especially the key is how to split LL^{\infty} norm of the solution itself according to the appropriate domains. Let us see it in the next section.

2.4. Strategy of the proof of Theorem 1.

The key of our success to prove the generalized combined effect case, especially the lower bound of the lifespan estimate in (8), in Theorem 1 is to handle the system of integral equations of (uεu0,utεut0)(u-{\varepsilon}u^{0},u_{t}-{\varepsilon}u^{0}_{t}), where u0u^{0} is a solution of the free wave equation with the same initial data (u,ut)|t=0=(f,g)(u,u_{t})|_{t=0}=(f,g);

u0(x,t)=12{f(x+t)+f(xt)}+12xtx+tg(y)𝑑y.u^{0}(x,t)=\frac{1}{2}\{f(x+t)+f(x-t)\}+\frac{1}{2}\int_{x-t}^{x+t}g(y)dy. (13)

The basic argument is due to John [8] in which classical solutions of semilinear wave equations in three space dimensions are constructed in a weighted LL^{\infty} space.

Assume that

suppf,g{|x|R}withR>1,\mbox{supp}\ f,g\subset\{|x|\leq R\}\ \mbox{with}\ R>1, (14)

which yields that the finiteness of the propagation seed of the wave,

supp u(x,t){|x|t+R}\mbox{supp\ }u(x,t)\subset\{|x|\leq t+R\} (15)

by standard argument on small solutions of nonlinear wave equations. For example, see Appendix in John [9]. Then, set an “interior” domain DD by

D:={t|x|R}D:=\{t-|x|\geq R\}

and define a sequence {(Uj,Vj)}\{(U_{j},V_{j})\} by

{Uj+1=L(A0|Vj+εut0|p|Uj+εu0|q+B0|Uj+εu0|r),U1=0,Vj+1=L(A0|Vj+εut0|p|Uj+εu0|q+B0|Uj+εu0|r),V1=0,\left\{\begin{array}[]{l}U_{j+1}=L(A_{0}|V_{j}+{\varepsilon}u_{t}^{0}|^{p}|U_{j}+{\varepsilon}u^{0}|^{q}+B_{0}|U_{j}+{\varepsilon}u^{0}|^{r}),\\ U_{1}=0,\\ V_{j+1}=L^{\prime}(A_{0}|V_{j}+{\varepsilon}u_{t}^{0}|^{p}|U_{j}+{\varepsilon}u^{0}|^{q}+B_{0}|U_{j}+{\varepsilon}u^{0}|^{r}),\\ V_{1}=0,\end{array}\right.

where L(v)L(v) for a function vv of space-time variables is from Duhamel’s term defined by

L(v)(x,t):=120t𝑑sxt+sx+tsv(y,s)𝑑y,L(v)(x,t):=tL(v)(x,t).\begin{array}[]{l}\displaystyle L(v)(x,t):=\frac{1}{2}\int_{0}^{t}ds\int_{x-t+s}^{x+t-s}v(y,s)dy,\\ \displaystyle L^{\prime}(v)(x,t):=\frac{\partial}{\partial t}L(v)(x,t).\end{array} (16)

This sequence {(Uj,Vj)}\{(U_{j},V_{j})\} will converge to (uεu0,utεut0)(u-{\varepsilon}u^{0},u_{t}-{\varepsilon}u_{t}^{0}) in a function space

X:={(U,V){C1(𝐑×[0,T])}2:(U,V)X<,supp(U,V){|x|t+R}},\begin{array}[]{ll}X:=&\{(U,V)\in\{C^{1}({\bf R}\times[0,T])\}^{2}\\ &\quad:\|(U,V)\|_{X}<\infty,\ \mbox{supp}\ (U,V)\subset\{|x|\leq t+R\}\},\end{array}

where

(U,V)X:=U1+Ux1+V2+Vx2,U1:=sup(x,t)𝐑×[0,T](t+|x|+R)1|U(x,t)|,V2:=sup(x,t)𝐑×[0,T]{χD(x,t)+(1χD(x,t))(t+|x|+R)1}|V(x,t)|\begin{array}[]{l}\|(U,V)\|_{X}:=\|U\|_{1}+\|U_{x}\|_{1}+\|V\|_{2}+\|V_{x}\|_{2},\\ \|U\|_{1}:=\displaystyle\sup_{(x,t)\in{\bf R}\times[0,T]}(t+|x|+R)^{-1}|U(x,t)|,\\ \|V\|_{2}:=\displaystyle\sup_{(x,t)\in{\bf R}\times[0,T]}\{\chi_{D}(x,t)\\ \qquad+(1-\chi_{D}(x,t))(t+|x|+R)^{-1}\}|V(x,t)|\end{array}

and χD\chi_{D} is a characteristic function of the interior domain DD. In view of the expression of u0u^{0} in (13), it follows from (14) and the assumption on gg yield the strong Huygens’ principle,

u0(x,t)𝐑g(x)𝑑x=0inD.u^{0}(x,t)\equiv\int_{{\bf R}}g(x)dx=0\quad\mbox{in}\ D. (17)

Then we have main a priori estimates;

L(|V|p|U|q)1CV2pU1q(T+R)p+q,L(|U|r)1CU1r(T+R)r+1,L(|V|p|U|q)2CV2pU1q(T+R)p+q,L(U|r)2CU1r(T+R)r+1\begin{array}[]{ll}\|L(|V|^{p}|U|^{q})\|_{1}\leq C\|V\|_{2}^{p}\|U\|_{1}^{q}(T+R)^{p+q},\\ \|L(|U|^{r})\|_{1}\leq C\|U\|_{1}^{r}(T+R)^{r+1},\\ \|L^{\prime}(|V|^{p}|U|^{q})\|_{2}\leq C\|V\|_{2}^{p}\|U\|_{1}^{q}(T+R)^{p+q},\\ \|L^{\prime}(U|^{r})\|_{2}\leq C\|U\|_{1}^{r}(T+R)^{r+1}\end{array}

with some positive constant CC independent of ε{\varepsilon} and TT which give us the key estimates for p+q<rp+q<r;

Uj+11εp+q+Vj2pUj1qTp+q+Uj1rTr+1+harmless terms,Vj+12the same as above,\begin{array}[]{ll}\|U_{j+1}\|_{1}\lesssim&{\varepsilon}^{p+q}+\|V_{j}\|_{2}^{p}\|U_{j}\|_{1}^{q}T^{p+q}+\|U_{j}\|_{1}^{r}T^{r+1}+\mbox{harmless terms},\\ \|V_{j+1}\|_{2}\lesssim&\mbox{the same as above},\end{array}

where \lesssim stands for mod constant independent of ε{\varepsilon} and TT. Therefore the boundedness of the sequence, Uj1,Vj2εp+q\|U_{j}\|_{1},\|V_{j}\|_{2}\lesssim{\varepsilon}^{p+q} for all j𝐍j\in{\bf N}, follows from the competition between the second and third terms in the right-hand side. When (r+1)/2<p+q(r+1)/2<p+q, the third term is major, so that

εr(p+q)Tr+1εp+q{\varepsilon}^{r(p+q)}T^{r+1}\lesssim{\varepsilon}^{p+q}

is the required condition. The difference to convergence of the sequence as well as those for the spatial derivative is almost the same as the boundedness above. Therefore we obtain the desired lower bound;

T(ε)Cε(p+q)(r1)/(r+1).T({\varepsilon})\geq C{\varepsilon}^{-(p+q)(r-1)/(r+1)}.

For the upper bound in this generalized combined effect, its proof is easy if we follow the argument by higher dimensional case by Han and Zhou [5]. In fact, assume that f(x)0(0),g(x)0f(x)\geq 0(\not\equiv 0),\ g(x)\equiv 0. Set

F(t):=𝐑u(x,t)𝑑x.F(t):=\displaystyle\int_{{\bf R}}u(x,t)dx.

Then, the equation and (15) imply that

F′′(t)=𝐑(A0|ut|p|u|q+B0|u|r)𝑑x.F^{\prime\prime}(t)=\int_{{\bf R}}(A_{0}|u_{t}|^{p}|u|^{q}+B_{0}|u|^{r})dx.

The second term and Hölder’s inequality yield that

F′′(t)(t+R)(r1)|F(x)|rfort0.F^{\prime\prime}(t)\gtrsim(t+R)^{-(r-1)}|F(x)|^{r}\quad\mbox{for}\ t\geq 0. (18)

This is the main inequality. Next we shall make use of the first term to obtain the better estimate than the single term. For this purpose, assume further that

f(x),f(x)c>0forx(R/2,0).f(x),-f^{\prime}(x)\geq\exists c>0\ \quad\mbox{for}\ x\in(-R/2,0).

Then, we have that

{u(x,t)εf(xt)ε,ut(x,t)εf(xt)εfort<x<t+R.\left\{\begin{array}[]{l}u(x,t)\gtrsim{\varepsilon}f(x-t)\gtrsim{\varepsilon},\\ u_{t}(x,t)\gtrsim-{\varepsilon}f^{\prime}(x-t)\gtrsim{\varepsilon}\end{array}\right.\mbox{for}\ t<x<t+R.

Plugging these estimates into the first term in (18), we obtain that

F′′(t)εp+qfor large tF^{\prime\prime}(t)\gtrsim{\varepsilon}^{p+q}\quad\mbox{for large $t$}

which implies that

F(t)εp+qt2for large t.F(t)\gtrsim{\varepsilon}^{p+q}t^{2}\quad\mbox{for large $t$}. (19)

These estimates (18) and (19) will give us the desired result according to the improved Kato’s lemma by Takamura [31]. But here we show a brief feeling that the result is correct as follows. Plugging (19) into (18), we obtain that

F′′(t)εr(p+q)tr+1for large t\begin{array}[]{l}F^{\prime\prime}(t)\gtrsim{\varepsilon}^{r(p+q)}t^{r+1}\quad\mbox{for large $t$}\end{array}

which implies that

F(t)εr(p+q)tr+3for large t.\begin{array}[]{l}F(t)\gtrsim{\varepsilon}^{r(p+q)}t^{r+3}\quad\mbox{for large $t$}.\end{array} (20)

The difference of the lower bound of FF between (19) and (20) is

ε(p+q)(r1)tr+1.{\varepsilon}^{(p+q)(r-1)}t^{r+1}.

This quantity is larger than some constant, we will reach to the desired lifespan estimate

T(ε)Cε(p+q)(r1)/(r+1)T({\varepsilon})\leq C{\varepsilon}^{-(p+q)(r-1)/(r+1)}

by standard iteration argument. Because we don’t have to cut the time interval in each step, which means that this procedure can be repeated infinitely many times in the fixed time interval. In this way, we obtain the sharp estimate of the lifespan in the generalized combined effect case.

Other cases except for the generalized combined effect are similar to those above. However, we point out that the existence part under the assumption of 𝐑g(x)𝑑x0\displaystyle\int_{{\bf R}}g(x)dx\neq 0 is most difficult practically among all the proofs in choosing appropriate weight functions.

3. The case of variable coefficients

In this section, we assume for our model (3) that A(x,t)A(x,t), or B(x,t)B(x,t), is of

1t+x1+atx1+bx1+c,or0,\frac{1}{\langle t+\langle x\rangle\rangle^{1+a}\langle t-\langle x\rangle\rangle^{1+b}\langle x\rangle^{1+c}},\ \mbox{or}\ \equiv 0,

where a,b,c𝐑a,b,c\in{\bf R} and x:=1+x2\langle x\rangle:=\sqrt{1+x^{2}}. The reason to take many \langle\ \rangles is to ensure the differentiability of A,BA,B to construct a classical solution. We will see that this kind of models will be a key in extending the general theory for (1) to the non-autonomous terms as stated at the end of Introduction. The weights of this kind were firstly introduced by Belchev, Kepka and Zhou [2], later Liu and Zhou [18] in higher space dimensions to show a blow-up result. But they set a special weight to make use of some geometric transform to absorb it, and reduced the equation to ordinary differential inequality of the functional without any argument on the local existence of the solution as well as the lifespan estimates.

3.1. Motivation of the problem

Our motivation to consider such AA and BB above comes from an initial value problem for the semilinear damped wave equations;

{vttvxx+21+tvt=|v|pin𝐑×(0,),v(x,0)=εf(x),vt(x,0)=εg(x)forx𝐑\left\{\begin{array}[]{ll}\displaystyle v_{tt}-v_{xx}+\frac{2}{1+t}v_{t}=|v|^{p}&\quad\mbox{in}\ {\bf R}\times(0,\infty),\\ v(x,0)={\varepsilon}f(x),\quad v_{t}(x,0)={\varepsilon}g(x)&\quad\mbox{for}\ x\in{\bf R}\end{array}\right. (21)

with the same setting on the initial data. This problem is a very important model as it has a critical decay in damping term, namely scaling invariant damping. The time-decay (1+t)1(1+t)^{-1} is a threshold between heat-like with weaker decay and wave-like with stronger decay in the sense that the each critical exponent is the same as Fujita one and Strauss one respectively. In the critical case, the size of the constant in front of the damping term is important. There is also a threshold on the constant and this case “2” is in the domain of heat-like in one dimension. See the introduction of Kato, Takamura and Wakasa [11] for precise results and references. In fact, D’Abbicco [1] showed for p>3p>3 that the energy solution of (21) exists globally-in-time, while Wakasugi [35] obtained its counter part of finite-time blow-up of the energy solution for 1<p31<p\leq 3. This critical exponent 33 is Fujita one in one space dimension, so one may expect that the solution behaves like one of semilinear heat equations for which uttu_{tt} is neglected from (21). But, this is not true.

In fact, Liouville transform u(x,t)=(1+t)v(x,t)u(x,t)=(1+t)v(x,t) shows that (21) is equivalent to

{uttuxx=|u|p(1+t)p1in𝐑×(0,),u(x,0)=εf(x),ut(x,0)=ε{f(x)+g(x)}forx𝐑,\left\{\begin{array}[]{ll}\displaystyle u_{tt}-u_{xx}=\frac{|u|^{p}}{(1+t)^{p-1}}&\mbox{in}\ {\bf R}\times(0,\infty),\\ u(x,0)={\varepsilon}f(x),\ u_{t}(x,0)={\varepsilon}\{f(x)+g(x)\}&\mbox{for}\ x\in{\bf R},\end{array}\right. (22)

so that all the technique for semilinear wave equations are applicable to this problem, and we have the following results on the lifepsan estimates for (21). Wakasa [33] obtained that

T(ε){Cε(p1)/(3p)for1<p<3,exp(Cε(p1))forp=3if𝐑{f(x)+g(x)}𝑑x0\begin{array}[]{c}T({\varepsilon})\sim\left\{\begin{array}[]{lll}C{\varepsilon}^{-(p-1)/(3-p)}&\mbox{for}&\displaystyle 1<p<3,\\ \exp(C{\varepsilon}^{-(p-1)})&\mbox{for}&\displaystyle p=3\\ \end{array}\right.\\ \mbox{if}\ \displaystyle\int_{{\bf R}}\{f(x)+g(x)\}dx\neq 0\end{array} (23)

This is the heat-like estimate in the sense that it coincides with the corresponding semilinear heat equations for which uxxu_{xx} is neglected in (21). In the original paper [33], the condition on the initial data is missing, but it was expected to be natural as the critical exponent is Fujita one. Later, Kato, Takamura and Wakasa [11] proved that

T(ε){Cεp(p1)/(1+2pp2)for1<p<2,Cb(ε)forp=2,Cεp(p1)/(3p)for2<p<3,exp(Cεp(p1))forp=3if𝐑{f(x)+g(x)}𝑑x=0,\begin{array}[]{c}T({\varepsilon})\sim\left\{\begin{array}[]{lll}C{\varepsilon}^{-p(p-1)/(1+2p-p^{2})}&\mbox{for}&\displaystyle 1<p<2,\\ Cb({\varepsilon})&\mbox{for}&\displaystyle p=2,\\ C{\varepsilon}^{-p(p-1)/(3-p)}&\mbox{for}&\displaystyle 2<p<3,\\ \exp(C{\varepsilon}^{-p(p-1)})&\mbox{for}&\displaystyle p=3\end{array}\right.\\ \mbox{if}\ \displaystyle\int_{{\bf R}}\{f(x)+g(x)\}dx=0,\end{array} (24)

where b=b(ε)b=b({\varepsilon}) is a positive number satisfying ε2blog(1+b)=1{\varepsilon}^{2}b\log(1+b)=1. This is the wave-like estimate. In deed, the cases 1<p<21<p<2 and p=3p=3 are the same forms as those of 3-dimensional semillinear wave equations.

In this way, it is very important to study the weighted nonlinear terms, and it is natural to extend the results to more general weighted terms than (22). The first simple question may go to the case of xx-decay.

3.2. Spatially weighted nonlinear terms.

First we consider the following case of spatial weights;

A(x,t)0andB(x,t)=1x1+c,A(x,t)\equiv 0\quad\mbox{and}\quad B(x,t)=\frac{1}{\langle x\rangle^{1+c}}, (25)

where c𝐑c\in{\bf R}, in (3). This setting was first introduced by Suzuki [29] under the supervision by Prof. M. Ohta (Tokyo Univ. of Sci. Japan), but with the assumption that the initial data is of non-compact support. Later, Kubo, Osaka and Yazici [17] improved the result and Wakasa [34] finalized it. For the compactly supported case, we have the following result.

Theorem 3 (Kitamura, Morisawa and Takamura [14]).

Assume (25). Then, the lifespan of a classical solution of (3) satisfies the following estimates.

T(ε){Cε(p1)/(1c)forc<0,ϕ1(Cε(p1))forc=0,Cε(p1)forc>0if𝐑g(x)𝑑x0T({\varepsilon})\sim\left\{\begin{array}[]{ll}C{\varepsilon}^{-(p-1)/(1-c)}&\mbox{for}\ c<0,\\ \phi^{-1}(C{\varepsilon}^{-(p-1)})&\mbox{for}\ c=0,\\ C{\varepsilon}^{-(p-1)}&\mbox{for}\ c>0\end{array}\right.\quad\mbox{if}\ \int_{\bf R}g(x)dx\neq 0 (26)

and

T(ε){Cεp(p1)/(1pc)forc<0,ψ1(Cεp(p1))forc=0,Cεp(p1)forc>0if𝐑g(x)𝑑x=0,T({\varepsilon})\sim\left\{\begin{array}[]{ll}C{\varepsilon}^{-p(p-1)/(1-pc)}&\mbox{for}\ c<0,\\ \psi^{-1}(C{\varepsilon}^{-p(p-1)})&\mbox{for}\ c=0,\\ C{\varepsilon}^{-p(p-1)}&\mbox{for}\ c>0\end{array}\right.\quad\mbox{if}\ \int_{\bf R}g(x)dx=0, (27)

where ϕ1\phi^{-1} and ψ1\psi^{-1} are inverse functions defined by ϕ(s)=slog(2+s)\phi(s)=s\log(2+s) and ψ(s)=slogp(2+s)\psi(s)=s\log^{p}(2+s), respectively.

Remark 1.

Wakasa [34] established the estimate in (26) with the assumption that fL(𝐑),gL1(𝐑)f\in L^{\infty}({\bf R}),\ g\in L^{1}({\bf R}) and c1c\geq-1. The last condition ensures the existence of local-in-time solutions with non-compactly supported data. We also remark that |u|p|u|^{p} in the nonlinear term can be replaced with |u|p1u|u|^{p-1}u in [34] due to the fact that the positiveness of the solution can be obtained easier than the compactly supported case.

The strategy of the proof of Theorem 3 for the existence part is similar to the one of Theorem 1 based on weighted LL^{\infty} estimates of the solution, so we don’t comment about it here. For the blow-up part, the iteration argument of the point-wise estimate is employed. The functional method like the proof of Theorem 1 cannot be applied to this case due to the effect of the weight.

After the work [14], one may study the counter case of

A(x,t)=1x1+candB(x,t)0,A(x,t)=\frac{1}{\langle x\rangle^{1+c}}\quad\mbox{and}\quad B(x,t)\equiv 0, (28)

where c𝐑c\in{\bf R}, in (3) with q=0q=0. For this equation, one may expect that the result is not so interesting as |x|t|x|\sim t in dealing with the nonlinear term |ut|p|u_{t}|^{p}. But the result is

Theorem 4 (Zhou [39], Kitamura, Morisawa and Takamura [15]).

Assume (28) with q=0q=0. Then, the lifespan of a classical solution of (3) satisfies the following estimates.

T(ε){Cε(p1)/(c)forc<0,exp(Cε(p1))forc=0,T(ε)=forc>0.\begin{array}[]{l}T({\varepsilon})\sim\left\{\begin{array}[]{ll}C{\varepsilon}^{-(p-1)/(-c)}&\mbox{for}\ c<0,\\ \exp(C{\varepsilon}^{-(p-1)})&\mbox{for}\ c=0,\end{array}\right.\\ T({\varepsilon})=\infty\quad\mbox{for}\ c>0.\end{array} (29)

We note that Zhou [39] established the blow-up part with c=1c=-1, namely non-weighted case. The proof of Theorem 4 is similar to the one of Theorem 3, so we don’t comment about it here also. The main difference between (25) and (28) is a possibility to obtain the global-in-time existence for (28) while there is no such a situation due to the effect of the origin in space for (25).

According to the result on (21) and Theorems 3 and 4, one may expect that it is sufficient to study the weights in the nonlinear terms by powers of (1+t)(1+t) or x\langle x\rangle for the purpose to extend the general theory, but we have to take into account of “characteristic weights” in handling nonlinear wave equations. Let’s see it in the next subsection.

3.3. Weighted nonlinear terms in the characteristic directions.

It is well-known that the wave propagates along with the characteristic directions, so that it is not sufficient to study the weights of powers by (1+t)(1+t) or x\langle x\rangle only. Therefore, as a breakthrough to this direction, we set

A(x,t)0andB(x,t)=1t+x1+atx1+b,A(x,t)\equiv 0\quad\mbox{and}\quad B(x,t)=\frac{1}{\langle t+\langle x\rangle\rangle^{1+a}\langle t-\langle x\rangle\rangle^{1+b}}, (30)

where a,b𝐑a,b\in{\bf R}, in (3). Then, we obtained the following result.

Theorem 5 (Kitamura, Wakasa and Takamura [16]).

Assume (30). Then, the lifespan T(ε)T({\varepsilon}) of the classical solution of (3) satisfies the following estimates;

T(ε)=fora+b>0anda>0,T({\varepsilon})=\infty\quad\mbox{for}\ a+b>0\ \mbox{and}\ a>0, (31)

and

T(ε){exp(Cε(p1))fora+b=0anda>0,ora=0andb>0,exp(Cε(p1)/2)fora=b=0,Cε(p1)/(a)fora<0andb>0,ϕ11(Cε(p1))fora<0andb=0,Cε(p1)/(ab)fora+b<0andb<0T({\varepsilon})\sim\left\{\begin{array}[]{lllll}\exp(C{\varepsilon}^{-(p-1)})&\mbox{for}&\begin{array}[]{l}a+b=0\ \mbox{and}\ a>0,\\ \mbox{or}\ a=0\ \mbox{and}\ b>0,\end{array}\\ \exp(C{\varepsilon}^{-(p-1)/2})&\mbox{for}&a=b=0,\\ C{\varepsilon}^{-(p-1)/(-a)}&\mbox{for}&a<0\ \mbox{and}\ b>0,\\ \phi_{1}^{-1}(C{\varepsilon}^{-(p-1)})&\mbox{for}&a<0\ \mbox{and}\ b=0,\\ C{\varepsilon}^{-(p-1)/(-a-b)}&\mbox{for}&a+b<0\ \mbox{and}\ b<0\\ \end{array}\right. (32)

if

𝐑g(x)𝑑x0,\int_{{\bf R}}g(x)dx\neq 0,

where ϕ11\phi_{1}^{-1} is an inverse function defined by

ϕ1(s)=salog(2+s).\phi_{1}(s)=s^{-a}\log(2+s). (33)

On the other hand, it holds that

T(ε){exp(Cε(p1))fora=0andb>0,exp(Cεp(p1))fora+b=0anda>0,exp(Cεp(p1)/(p+1))fora=b=0,Cε(p1)/(a)fora<0andb>0,ψ11(Cεp(p1))fora<0andb=0,Cεp(p1)/(pab)fora<0andb<0,ψ21(Cεp(p1))fora=0andb<0,Cεp(p1)/(ab)fora+b<0anda>0T({\varepsilon})\sim\left\{\begin{array}[]{lllll}\exp(C{\varepsilon}^{-(p-1)})&\mbox{for}&a=0\ \mbox{and}\ b>0,\\ \exp(C{\varepsilon}^{-p(p-1)})&\mbox{for}&a+b=0\ \mbox{and}\ a>0,\\ \exp(C{\varepsilon}^{-p(p-1)/(p+1)})&\mbox{for}&a=b=0,\\ C{\varepsilon}^{-(p-1)/(-a)}&\mbox{for}&a<0\ \mbox{and}\ b>0,\\ \psi_{1}^{-1}(C{\varepsilon}^{-p(p-1)})&\mbox{for}&a<0\ \mbox{and}\ b=0,\\ C{\varepsilon}^{-p(p-1)/(-pa-b)}&\mbox{for}&a<0\ \mbox{and}\ b<0,\\ \psi_{2}^{-1}(C{\varepsilon}^{-p(p-1)})&\mbox{for}&a=0\ \mbox{and}\ b<0,\\ C{\varepsilon}^{-p(p-1)/(-a-b)}&\mbox{for}&a+b<0\ \mbox{and}\ a>0\end{array}\right. (34)

if

𝐑g(x)𝑑x=0,\int_{{\bf R}}g(x)dx=0,

where ψ11\psi_{1}^{-1} and ψ21\psi_{2}^{-1} are inverse functions defined by

ψ1(s)=spalog(2+s)andψ2(s)=sblogp1(2+s).\psi_{1}(s)=s^{-pa}\log(2+s)\ \mbox{and}\ \psi_{2}(s)=s^{-b}\log^{p-1}(2+s). (35)
Remark 2.

The estimates (34) with a=p2a=p-2 and b=1b=-1 coincide with (23) and (24) because (1+t)(1+t) is equivalent to t+x{\langle{t+{\langle{x}\rangle}}\rangle} by finite propagation speed of the wave like (15).

The strategy of the proof of Theorem 5 is also almost the same as the one of Theorem 3, but the weights cause many technical difficulties, but we shall skip the details fot the purpose of this paper. The main concern of Theorem 5 is that we have interactions among two characteristic directions as the critical line a+b=0a+b=0 with b0b\leq 0 and a=0a=0 with b0b\geq 0 which divides abab-plane into two domains of the global-in-time existence and the blow-up in finite time.

In contrast, if

A(x,t)=1t+x1+atx1+bandB(x,t)0,A(x,t)=\frac{1}{\langle t+\langle x\rangle\rangle^{1+a}\langle t-\langle x\rangle\rangle^{1+b}}\quad\mbox{and}\quad B(x,t)\equiv 0, (36)

where a,b𝐑a,b\in{\bf R}, in (3) with q=0q=0, then we obtained the different critical line on abab-plane from Theorem 5 as follows.

Theorem 6 (Kitamura [13]).

Assume (28) with q=0q=0. Then, the lifespan of a classical solution of (3) satisfies the following estimates.

T(ε){Cε(p1)/(a)fora<0andbp,Cεp(p1)/{p(1+a)b}forp(1+a)+b<0andb<p,exp(Cε(p1))fora=0andbp,exp(Cεp(p1))fora>0andp(1+a)+b=0,T(ε)=fora>0andp(1+a)+b>0.\begin{array}[]{l}T({\varepsilon})\sim\left\{\begin{array}[]{l}C{\varepsilon}^{-(p-1)/(-a)}\\ \qquad\mbox{for}\ a<0\ \mbox{and}\ b\geq-p,\\ C{\varepsilon}^{-p(p-1)/\{-p(1+a)-b\}}\\ \qquad\mbox{for}\ p(1+a)+b<0\ \mbox{and}\ b<-p,\\ \exp(C{\varepsilon}^{-(p-1)})\\ \qquad\mbox{for}\ a=0\ \mbox{and}\ b\geq-p,\\ \exp(C{\varepsilon}^{p(p-1)})\\ \qquad\mbox{for}\ a>0\ \mbox{and}\ p(1+a)+b=0,\end{array}\right.\\ T({\varepsilon})=\infty\quad\mbox{for}\ a>0\ \mbox{and}\ p(1+a)+b>0.\end{array} (37)

We note again that all the estimates above are established whatever the value of 𝐑g(x)𝑑x\displaystyle\int_{{\bf R}}g(x)dx is, due to the nonlinear term |ut|p|u_{t}|^{p}. The strategy of the proof of Theorem 6 is also almost the same as the one of Theorem 3.

Concluding remark The series of our theorems above are major if one intends to extend the general theory for non-autonomous equations. But they are not sufficient still as we never try to analyze the combined effect for variable coefficients case including the different order of AA and BB.

3.4. Other models.

Finally we shall comment on the different nonlinear terms. Recently we obtained the following result.

Theorem 7 (Sasaki, Takamatsu and Takamura [28]).

Assume that A1,B0,q=0A\equiv 1,B\equiv 0,q=0 in (3). Moreover, |ut|p|u_{t}|^{p} is replaced with |ux|p|u_{x}|^{p}. Then we have that

T(ε)Cε(p1).T({\varepsilon})\sim C{\varepsilon}^{-(p-1)}. (38)

One may feels that this result is trivial according to Theorem 3 with c=1c=-1. But the proof is different from each others. Especially there is a difficulty on the blow-up part as the point-wise positivity of uxu_{x} cannot be obtained by

xL(v)(x,t),\frac{\partial}{\partial x}L(v)(x,t),

where L(v)L(v) is the one in (16). This situation is overcome by taking suitably weighted functional of the solution which was introduced by Rammaha [26, 27]. We believe that Theorem 7 will contribute to analysis of the “blow-up boundary” for the equation

uttuxx=|ux|pu_{tt}-u_{xx}=|u_{x}|^{p}

for which there is no result til now. See [28] for references therein to the blow-up boundary.

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