In previous work the authors found the asymptotic expansion of the -norm of the solution of the strongly damped wave equation and also of the -norm of the difference between and its asymptotic approximation . This was done in space dimension . In the present work results are extended to the exceptional cases and . This extension is achieved by deriving new lemmas on the asymptotic expansion of some parameter dependent integrals.
We begin by considering the strongly damped wave equation in for
(1.1) admits a unique weak solution as determined by Ikehata–Todorova–Yordanov [12]. The squared -norm of this weak solution of (1.1) has been studied extensively by Ikehata [8] and, more recently, by Barrera–Volkmer [1] in space dimension . Ikehata [8] found sharp decay estimates as , while Barrera–Volkmer [1] followed up with the asymptotic expansion of under slightly different assumptions. Despite the differing assumptions, the common idea in obtaining the estimates and expansions is the use of weighted -initial data (to be defined). This technique has been used in the past to study both the linear [6,7,14] and strongly [1,8] damped wave equations. Furthermore, the use of weighted -data has been employed by Ikehata–Natsume [9] in their generalization of [12] to find energy decay estimates of the wave equation with fractional damping, and also by Ikehata–Soga [11] in their study of a strongly damped plate equation.
Regarding the weak solution u of (1.1), the low space dimension cases were known to Ikehata [8] to be exceptional, but sharp estimates on the long-term behavior of were unknown until Ikehata–Onodera [10]. They determined that as , in space dimension and in dimension . One of the two main goals of this paper is to find the asymptotic expansion of in space dimensions . In doing so, we will see that these low dimension cases are exceptional because more intricate integrals appear in the expansions, and as such, must be treated using different methods. Nonetheless this paper will carry over many preliminary results from the recent paper of Barrera–Volkmer [1].
The weak solution of (1.1) is found using the Fourier transform. In the Fourier space, Ikehata [8] found an asymptotic profile for , which exhibits a diffusion-like property in all space dimensions when is considered. He did so using a mean value theorem argument, which, along with the paper [14] of Volkmer, formed the motivation for [1] of Barrera–Volkmer. However due to the exceptional nature of the problem in space dimensions , the asymptotic expansion of in these dimensions is the other main goal of this paper.
Throughout this paper, will represent the positive integers and will represent the non-negative integers. The -norm is denoted by . For each we let denote the closed ball centered at the origin in , whereby we denote the -norm by .
For all we define the weighted -space
with norm . For all we define the Fourier transform
and the Fourier inverse
To extend to , consider functions such that as . Then is defined to be the unique -limit of as . See [4] for more details.
Finally, whenever a sum of the form or is encountered, it is taken to be the empty sum and evaluates to 0.
Assumptions
We assume that the space dimension is and that there exists such that , where the functions and are the initial data of (1.1). Under these assumptions both and are -times continuously differentiable on , and in particular at . Thus we may choose such that the Taylor approximations
hold in the closed δ-neighborhood of , where is a multi-index of order (see [4] for further details), and for all
We fix this chosen value of , and whenever δ is hereafter referred to, we mean this fixed value.
In this fixed closed δ-neighborhood of , we also have the Taylor approximations
where
and denotes the unit multi-index in the j-direction. Moreover,
With the definitions and , it is easy to see that and . Hence , , , and .
Preliminary work
Applying the Fourier transform to (1.1) we obtain the ordinary differential equation
The solution to (1.7) is
where
and
We define
Then . With the definition , we wish to find the asymptotic expansions of
Indeed is the profile determined by Ikehata in his paper [8].
Main results
It was determined by Ikehata [8] and Barrera–Volkmer [1] that in every space dimension , for all there is some such that
Thus all the interesting asymptotic behaviors of and are captured in any ϵ-neighborhood of the origin. We let ϵ equal the fixed value of , and hence we are interested in the expansions of
We will compute these expansions by first noting , where
and with denoting the -inner product over the closed ball of radius δ about the origin. Then , , and , where
Furthermore it is apparent that .
I accordance with the Notation section, the sums in the following theorems vanish when , leaving only the terms outside the sum and the O-term.
Letand. Letbe the weak solution of (
1.1
) under the Fourier transform with the complex-valued initial dataandsatisfyingand.
Foras, where γ is the Euler–Mascheroni constant.
Foras.
In both cases theare coefficients dependent on the space dimension N and the initial dataand.
Letand. Letbe the weak solution of (
1.1
) under the Fourier transform with the complex-valued initial dataandsatisfyingand. Consider the asymptotic profile offound by Ikehata in [
8
]:whereand. Then aswhere theare coefficients dependent on the space dimension N and the initial dataand.
In the process of proving Theorem 1.2 we will find the asymptotic expansions of , , and . Since as , we obtain the expansion of the squared -norm of the asymptotic profile .
Letand. Letbe the asymptotic profile offound by Ikehata in [
8
].
For, as,
For, as,
In both cases theare coefficients dependent on the space dimension N and the initial dataandof (
1.1
).
Our proofs of Theorem 1.1, Theorem 1.2 and Corollary 1.3 provide explicit formulas for the coefficients , , . For example, if , we have
For every , it is a routine argument to verify (using Lebesgue’s dominated convergence theorem and the mean value theorem) that , where is as in (2.3) and
By Lemma 2.2(b) with , thus has the expansion
Turning to , we begin by expanding in a Taylor series about . Since , for :
where is as given in (2.4) for . Substituting (2.6) into the definition of and estimating the integral with the -term, we obtain
We let and apply Lemma 2.1(b) to (2.7) with to obtain
Combining (2.5) and (2.8),
This implies that for some constant C
This fact is proven by modifying the proof given in Chapter 1 of [2].
To determine the constant C we consider the asymptotics of the following integral for (to be proved separately):
We now use the fact that for . Thus
Furthermore
This result together with (2.10) implies , which proves the lemma. □
Let , , and . Then by the mean value theorem and Lebesgue’s dominated convergence theorem, , where is as given in Lemma 2.1 and
We use the fact that to write
We observe the integral in the first term of (2.11) satisfies
From this fact and (2.1) we conclude that
where is as given and . Simplifying we obtain
Therefore there is some constant C such that
Now we must determine the constant C. To do so, we first note that from the integral definition in (2.9), , where for
It is easily verified that , so we instead study .
With the substitution we have . Integrating by parts we obtain
where
With the substitution ,
The integral
is a Laplace transform identity found in [3, §4.6(1)]. Therefore .
We now let , where is the characteristic function of the set . Then , and for all
By the Riemann–Lebesgue lemma found in Chapter 2 of [5], .
Lastly for we define
Then
where . We integrate (2.14) by parts and use the fact that to obtain
where . Again by the Riemann–Lebesgue lemma,
Combining the results of the analysis of , we have
From (2.12) we have
Thus and the proof is complete. □
Intermediate computations
Ikehata [8] showed that for the fixed , is exponentially small as . So we instead find the expansion of . Additionally, the overlying assumption is that with the initial data of (1.1) and .
Expansion of. Since
we may substitute (1.4) and (1.8) to obtain a sum of integrals indexed by the multi-indices σ plus an integral of a -term. We estimate the integral with the -term once, as all others may be estimated similarly:
Since any remaining integrals with an odd entry in the multi-index evaluate to zero, we omit them and then switch to polar coordinates to obtain
where
We substitute the expansion
into (2.15) with . We obtain
We apply Lemma 2.4 with to the term in the sum with , , and Lemma 2.2(b) to all other terms. Thus with the identity , we find
where
Expansion of. We refer back to the expansion of obtained in [1]. We see that all steps are valid here with . We arrive at
where
Expansion of. All steps are valid now with and we deduce
where
with
Asymptotic expansion of
We combine results (2.18), (2.19), and (2.20) to obtain the asymptotic expansion
where
For example, if then
We then simplify to obtain the expressions in Remark 2.
The space dimension case
Auxiliary results
For all,satisfies.
It follows from [3, §2.4 (21)] that , where denotes the error function. Therefore, using the known asymptotic behavior of the error function [13, Chapter 8]
proving the lemma. □
Forand, we defineIf, then.
Let , , and . We use the mean value theorem and Lebesgue’s dominated convergence theorem to justify differentiation within the integral. Hence
where is as given in Lemma 2.3 and
By Lemma 2.3(b) with ,
To determine the asymptotics of , we substitute (2.6) with . Hence
We apply Lemma 2.1(b) to (2.23) with . We also observe that since each () is even, every . Thus
We combine the results (2.22) and (2.24) to obtain . Hence . We must determine the constant C.
From the fact , Lemma 2.6 implies . Since for , we obtain
Further, for the given ,
Considering (2.25) and (2.26) together implies , completing the proof. □
Forand, we defineIf, then.
Let , , and . Using integration by parts, , where
We apply Lemma 2.2(a) with to . Therefore,
To analyze (2.28), we substitute
where each is as given in (2.4). Then
By Lemma 2.7, the first term of (2.31) is . We see the second term of (2.31) is by applying Lemma 2.1(b) with for each . Finally we observe
Thus, . Combining this result for with (2.27) and (2.29) completes the proof. □
Intermediate computations
Once again we compute with the assumptions that and the initial data of (1.1) satisfy and .
Expansion of. The work from the case in Section 2.1.2 carries over to this case. Since the space dimension is , the “multi-indices” are simply non-negative integers. We have
We substitute (2.16) into (2.32) with and find
We treat the term in the sum with by using Lemma 2.8 with , and all other terms by using Lemma 2.2(a) with . Then we obtain
where
Expansion of. The work done in [1] carries over to the case as well. We obtain
where
Expansion of. Given that
we substitute (1.6), (1.8), and (1.9). The integral with the -term is . Thus
With as given in (2.21),
So to find the expansion of , we substitute (2.37) into (2.36) with . Then
We use Lemma 2.7 with to treat the term of the sum with in (2.38), and Lemma 2.3(b) with to treat all other terms. Thus
Asymptotic expansion of
Combining (2.34), (2.35), and (2.39), we obtain the asymptotic expansion
where
For example, if then
Simplifying gives the expressions from Remark 2.
Formulas for and for small n are given in [1, (6.6), (3.7)].
Let,, and. Define
Ifis even,and, then
Ifis odd,and, then
Let,, and. Define
Ifis even,andthen
Ifis odd,and, then
The dimension case
Auxiliary result
Forand, defineIf, thenwhere
Let , , and . Using the mean value theorem and Lebesgue’s dominated convergence theorem, it is a routine argument to show that , where
and and are as given in Lemmas 3.2 and 3.3, respectively.
Similarly, by Lemma 3.3(a) with and , and the facts that and
To determine the asymptotic expansion of , we expand in a Taylor polynomial with remainder about as in (2.6). We then estimate the resulting integral with the -term and find it to be , where . Hence
Let and substitute the result of Lemma 3.3(a) into (3.3) with and so that both O-terms are instead . Thus
We use the fact that , , and to obtain
We now combine results (3.1), (3.2), and (3.4) with the fact that to obtain
where C is a constant. To determine the constant C we proceed as in the proof of Lemma 2.4 and compare to (see (2.9)). We note for and . Therefore
Furthermore
This result together with (3.5) implies , which proves the lemma. □
Intermediate computations
We may now set about proving the dimension case of Theorem 1.2. The proof will rely on the previous results for , , and , as well as the results of the following several sections. As usual, and the initial data of (1.1) satisfy and .
Expansion of. Since
we see that, upon switching to polar coordinates, , where is as given in (2.9). We apply Lemma 2.5 with to obtain the asymptotic expansion
where
Expansion of. Into
we substitute (1.3) and (1.8). The resulting integral with the -term is . We switch to polar coordinates and obtain
We substitute (2.37) into (3.7) with . Then
For the term in the sum of (3.8) with , , we use Lemma 3.4 with , and for all other terms we use Lemma 3.2(b) with and . We obtain
where
Asymptotic expansion of. We combine results (2.18), (3.6), and (3.9) with the fact that to obtain
where
For example, when we have
Expansions ofand. The analysis from Sections 3.2.4 and 3.2.5 of [1] fully carries over here with . Hence
where
and
Asymptotic expansion of. We combine results (2.19), (3.10), and (3.11) with the fact that to obtain the expansion
where
For example, when we have .
Expansions of,, and. The analysis from Sections 3.2.7, 3.2.8, and 3.2.9 of [1] also carries over with . We have
where
Asymptotic expansion of. We combine the results (2.20), (3.12), (3.13), and (3.14) with the fact that to obtain the expansion
where
We note that when .
Asymptotic expansion of
We recall from Section 1.3 that for the fixed there exists such that . We combine the results of the analysis for the case to obtain the full asymptotic expansion of . Further, we suppress the -term since it is dominated by the larger -term.
Let be an integer as given in the statement of Theorem 1.2. Then
where . The proof of Theorem 1.2 for dimension is complete.
Asymptotic expansion of
Let us again recall that for the fixed , . We then combine results (3.6), (3.10), and (3.14) to obtain the asymptotic expansion of Corollary 1.3(a) with
The space dimension case
Auxiliary results
Forand, we defineIf, then.
Let and . We first note that
The latter integral is . The former integral we denote by . Integrating by parts and using known integrals [3, §1.4(11), §2.4(21)], we find
This gives the desired statement. □
We omit the proof of the following lemma because it is very similar to the proof of Lemma 3.4.
Forand, defineIfandthen
Forand, defineIfthen
Let and . Using integration by parts, , where is as given in Lemma 3.2, is as given in Lemma 3.6, and
Using (2.30), we find
Therefore,
Lemma 3.6 gives
From Lemma 3.2(a) and , we have
Applying Lemma 3.3 with , we obtain
Using (3.18), (3.17), and (3.19) in (3.16) completes the proof. □
Intermediate computations
We are now in a position to prove the dimension case of Theorem 1.2. We assume that and the initial data of (1.1) satisfy and .
Expansion of. Observe that
with as given in (3.15). By Lemma 3.5 with ,
Expansion of. Using a similar argument for the expansion of in the case we find that
We substitute (2.37) into (3.21) with . Hence
To the term in (3.22) with we apply Lemma 3.7 with , and to all other terms Lemma 3.2(a) with . Then we obtain the asymptotic expansion
where
Asymptotic expansion of. We combine results (2.34), (3.20), and (3.23) for , , and , respectively, with the fact that to obtain the asymptotic expansion
where
For example, if then
Expansions ofand. The analysis of and from Sections 3.2.4 and 3.2.5 of [1] applies to the case as well. Hence
where
Asymptotic expansion of. Since we combine results (2.35), (3.24), and (3.25) to obtain the asymptotic expansion
where
We note that for .
Expansion of.
into which we substitute (1.3) and (1.8). With our overlying assumption that , the resulting integral with the -term can be shown to be . Hence
We substitute (2.37) into (3.26) with . Hence
We treat the term in the sum of (3.27) using Lemma 3.6 with , and all other terms by Lemma 3.3(b) with . Hence
where
Expansion of. We analyze similarly to and we find
We use Lemma 3.6 and Lemma 3.3(b) and obtain
where
Expansion of. From the definition of , we see that
where is as given in Lemma 2.6. Therefore
Asymptotic expansion of. We combine results (2.39), (3.28), (3.30), and (3.31) for , , , and , respectively, with the fact that to obtain the asymptotic expansion
where
We note that if .
Asymptotic expansion of
Again from Section 1.3, for the fixed there exists such that . We now combine the results we have for dimension to obtain the full asymptotic expansion of . The -term will hereafter be suppressed since it is dominated by the larger -term.
Let be an integer as given in the statement of Theorem 1.2. Then
where . Since cases are complete, here ends the proof of Theorem 1.2.
Asymptotic expansion of
Let us again recall that for the fixed , . We then combine results (3.20), (3.24), and (3.31) to obtain the asymptotic expansion of Corollary 1.3(b) with .
This completes the proof of Corollary 1.3. Furthermore, we have completed the proofs of all three main results.
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