Advances in Mathematical Physics

VolumeΒ 2010, Article IDΒ 504324, 35 pages

http://dx.doi.org/10.1155/2010/504324

## The Initial Value Problem for the Quadratic Nonlinear Klein-Gordon Equation

^{1}Department of Mathematics, Graduate School of Science, Osaka University, Osaka, Toyonaka 560-0043, Japan^{2}Instituto de MatemΓ‘ticas, UNAM Campus Morelia, AP 61-3 (Xangari), Morelia CP 58089, Mexico

Received 18 September 2009; Accepted 23 February 2010

Academic Editor: DonghoΒ Chae

Copyright Β© 2010 Nakao Hayashi and Pavel I. Naumkin. This is an open access article distributed under the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.

#### Abstract

We study the initial value problem for the quadratic nonlinear Klein-Gordon equation , , , , where and . Using the Shatah normal forms method, we obtain a sharp asymptotic behavior of small solutions without the condition of a compact support on the initial data which was assumed in the previous works.

#### 1. Introduction

Let us consider the Cauchy problem for the nonlinear Klein-Gordon equation with a quadratic nonlinearity in one dimensional case

where , and

Our purpose is to obtain the large time asymptotic profile of small solutions to the Cauchy problem (1.1) without the restriction of a compact support on the initial data which was assumed in the previous work [1]. One of the important tools of paper [1] was based on the transformation of the equation by virtue of the hyperbolic polar coordinates following to paper [2]. The application of the hyperbolic polar coordinates implies the restriction to the interior of the light cone, and therefore, requires the compactness of the initial data. Problem (1.1) is related to the Cauchy problem

where and are the real-valued functions, and Indeed we can put then satisfies

where

There are a lot of works devoted to the study of the cubic nonlinear Klein-Gordon equation

with When , the global existence of solutions to (1.4) can be easily obtained in the energy space, which is, however, insufficient for determining the large-time asymptotic behavior of solutions. The sharp - time decay estimates of solutions and nonexistence of the usual scattering states for (1.4) were shown in [3] by using hyperbolic polar coordinates under the conditions that the initial data are sufficiently regular and have a compact support.

The initial value problem for the nonlinear Klein-Gordon equation with various cubic nonlinearities depending on and having a suitable nonresonance structure was studied in [4β6], where small solutions were found in the neighborhood of the free solutions when the initial data are small and regular and decay rapidly at infinity. Hence the cubic nonlinearities are not necessarily critical; however the resonant nonlinear term was excluded in these works. In paper [4], the nonresonant nonlinearities were classified into two types, one of them can be treated by the nonlinear transformation which is different from the method of normal forms [7] and the other reveals an additional time decay rate via the operator which was used in [2]. This nonlinear transformation was refined in [8] and applied to a system of nonlinear Klein-Gordon equations in one or two space dimensions with nonresonant nonlinearities. It seems that the method of normal forms is very useful in the case of a single equation; however it does not work well in the case of a system of nonlinear Klein-Gordon equations. Some sufficient conditions on quadratic or cubic nonlinearities were given in [1], which allow us to prove global existence and to find sharp asymptotics of small solutions to the Cauchy problem including (1.2) with small and regular initial data having a compact support. Moreover it was proved that the asymptotic profile differs from that of the linear Klein-Gordon equation. See also [9, 10] in which asymptotic behavior of solutions to (1.4) was studied as in [1] by using hyperbolic polar coordinates. Compactness condition on the data was removed in [11] in the case of the cubic nonlinearity and a real-valued solution. Final value problem with the cubic nonlinearity was studied in [12] for a real-valued solution. As far as we know the problem of finding the large-time asymptotics is still open for the case of the cubic nonlinearity and the complex valued initial data. When the initial data are complex-valued, global existence and -time decay estimates of small solutions to the Klein-Gordon equation with cubic nonlinearity were obtained in paper [13] under the conditions that the initial data are smooth and have a compact support.

The scattering problem and the time decay rates of small solutions to (1.4) with super-critical nonlinearities and with were studied in papers of [14, 15]. Finally, we note that the Klein-Gordon equation (1.4) with quadratic nonlinearities in two space dimensions was studied in [16], where combining the method of the normal forms of [7] and the time decay estimate through the operator of [17], it was shown that every quadratic nonlinearity is nonresonant.

We denote the Lebesgue space by , with the norm if and if The weighted Sobolev space is

for , where For simplicity we write . The index we usually omit if it does not cause a confusion. We denote by the Fourier transform of the function Then the inverse Fourier transformation is .

Our main result of this paper is the following.

Theorem 1.1. *Let and the norm . Then there exists such that for all the Cauchy problem (1.1) has a unique global solution
**
satisfying the time decay estimate
**
Furthermore there exists a unique final state such that
**
where , *

An important tool for obtaining the time decay estimates of solutions to the nonlinear Klein-Gordon equation is implementation of the operator

which is analogous to the operator in the case of the nonlinear SchrΓΆdinger equations used in [18]. The operator was used previously in paper of [15] for constructing the scattering operator for nonlinear Klein-Gordon equations with a supercritical nonlinearity. We have ; therefore the commutator , where is a linear part of (1.1). Since is not a purely differential operator, it is apparently difficult to calculate the action of on the nonlinearity in (1.1). So, instead we use the first-order differential operator

which is closely related to by the identity and acts easily on the nonlinearity. Moreover, it almost commutes with , since .

Also we use the method of normal forms of [7] by which we transform the quadratic nonlinearity into a cubic one with a nonlocal operator. We multiply both sides of equation (1.1) by the free Klein-Gordon evolution group and put to get

where Integrating (1.11) with respect to time, we find

Then we integrate by parts with respect to taking into account (1.11),

Returning to the function , we obtain the following equation:

with the symmetric bilinear operator

where

and Our main point in this paper is to show that the right-hand side of (1.14) can be decomposed into two terms; one of them is a cubic nonlinearity

and the other one is a remainder term with an estimate like

*Remark 1.2. * We believe that all quadratic nonlinear terms of problem (1.3) also could be considered by this approach. In the same way as in the derivation of (1.14) we get from (1.3)
where
with Some more regularity conditions are necessary to treat the bilinear operators . Also we have to show that
are the nonresonant terms (i.e., remainders) and to remove the resonant terms
by an appropriate phase function. We will dedicate a separate paper to this problem.

We prove our main result in Section 3. In the next section we prove several lemmas used in the proof of the main result.

#### 2. Preliminaries

First we give some estimates for the symmetric bilinear operator

where

Denote the kernel as follows:

Lemma 2.1. *The representation is true
**
where the kernel obeys the following estimate:
**
for all Moreover the following estimates are valid:
**
for , provided that the right-hand sides are bounded.*

*Proof. *To prove representation (2.4), we substitute the direct Fourier transforms
into the definition of the operator . Then changing , we find
where the kernel is
Changing the variables of integration and (the prime we will omit), we get
where We change and ) and denote
For the case of we integrate by parts using the identity where Then we get
Note that
Then
Hence we can estimate the kernel as follows:
for the case of For the case of we integrate three times by parts with respect to
Note that
Hence we can estimate the kernel as follows:
for all For the case we integrate by parts three times with respect to
Note that Hence
Finally for the case of we integrate by parts three times with respect to and
Since
then we can estimate the kernel as follows:
for all Hence estimate (2.5) is true.

By virtue of estimate (2.5) applying the HΓΆlder inequality with and the Young inequality with and , we find
where .

We now estimate the operator as follows:
Then by virtue of estimate (2.4) applying the HΓΆlder and Young inequalities, we get
Lemma 2.1 is proved.

We now decompose the free Klein-Gordon evolution group where similarly to the factorization of the free SchrΓΆdinger evolution group. We denote the dilation operator by

Define the multiplication factor where for and for We introduce the operator

The inverse operator acts on the functions defined on as follows:

for all since and We now introduce the operators

so that we have the representation for the free Klein-Gordon evolution group

The first term of the right-hand side of (2.31) describes inside the light cone the well-known leading term of the large-time asymptotics of solutions of the linear Klein-Gordon equation with initial data . The second term of the right-hand side of (2.31) is a remainder inside of the light cone, whereas the last term represents the large time asymptotics outside of the light cone which decays more rapidly in time. We also have

where the right-inverse operators are

where

In the next lemma we state the estimates of the operators .

Lemma 2.2. *The estimates hold as follows:
**
where and
**
where provided the right-hand sides are finite.*

*Proof. *Changing the variable of integration , we see that
Hence

Consider the estimate for the derivative . Define Note that and Hence integrating by parts one time yields
where . Also we have
Hence the estimate is true
Since , we get
Consider the -estimate of the integral
We have
where the kernel
After a change , we find
We now change the contour of integration in as then
Since , using (2.38) and the inequality for we get ; also we have
for . Therefore we obtain the estimate
if we choose and Thus we get
since

In the same manner we consider the estimate of the integral
where the kernel
since by a direct calculation
In the same way as in (2.47) we have
if we choose , and Therefore we get
Hence Thus we have the second estimate of the lemma.

Consider the estimate for the derivative . Note that and Hence integrating by parts one time yields
where and The estimate is true
Consider the -estimate of the integral
We have, changing and ,
where the kernel
We now change the contour of integration in as ; then
Since and by (2.55) for , and also
for we obtain the estimate
if we choose and Therefore we get

In the same manner we consider the estimate of the integral with Hence
where Thus we have the second estimate of the lemma. Lemma 2.2 is proved.

In the next lemma we prove an auxiliary asymptotics for the integral

Lemma 2.3. *The estimate holds as follows:
**
provided the right-hand side is finite, where .*

*Proof. *We represent the integral
where the remainder term is
In the remainder term we integrate by parts via identity
since
Thus we have the estimate for the remainder in the asymptotic formula. Lemma 2.3 is proved.

In the next lemma we obtain the asymptotics for the operator and the right-inverse operator

Lemma 2.4. *The estimates hold as follows:
**
for all where provided the right-hand sides are finite.*

*Proof. *We have the identities
and We now change We denote The inverse functions by so that and

Thus the stationary point transforms into Hence we can write the representation
By a direct calculation we find