A semilinear diffusion equation is considered in the de Sitter spacetime with the spatially flat curvature. Global solutions for small initial data and their asymptotic behaviors in high order are obtained. Some effects of the spatial expansion and contraction are studied through the problem.
In this paper, we consider the Cauchy problem for a semilinear diffusion equation
for and , where , , is the Hubble constant, , is a weight function defined by
is a semilinear term defined by
for , is a given initial datum, and is defined by
The de Sitter spacetime is the solution of the Einstein equations with the cosmological constant in the vacuum. We consider the de Sitter spacetime with the spatially flat curvature whose metric is given by , which describes the spatial expansion and contraction when and , respectively, where c denotes the speed of the light, and τ denotes the proper time. We note that the case yields the Minkowski spacetime. The derivation of the first equation in (1.1) by the nonrelativistic limit of a semilinear field equation has been shown in [18]. In this paper, we study the effects of the spatial expansion and contraction through the Cauchy problem of the semilinear diffusion equation in the de Sitter spacetime. Our main purpose is to study the large time behavior of the solution of (1.1).
The corresponding Cauchy problem for the semilinear Schrödinger equation in the de Sitter spacetime has been considered in [17]. The global solutions for small data for the Klein–Gordon equation have been shown in asymptotically de Sitter spacetime in [3]. The wave equation with quadratic nonlinear term in asymptotically de Sitter and Kerr–de Sitter spacetimes has been considered in [11]. The global solutions for semilinear wave equations have been shown on the manifold with the time slices being real hyperbolic spaces in [1,2,13,14]. The Klein-Gordon equation in the de Sitter spacetime has been considered in [4] for the tachyonic field, in [27] for the Huygens principle, and in [26] for the Higgs scalar field. The Cauchy problem of the semilinear Klein–Gordon equations has been considered in [8,16,25] in the de Sitter spacetime, and in [7] in the Friedmann–Lemaître–Robertson–Walker spacetime.
We denote the Lebesgue space of order by with the norm . Put for . For any real number , we define the weighted Lebesgue space by
with the norm . For and , we denote the Sobolev space by
with the norm . We also denote the homogeneous Sobolev space by
with .
We denote the set of natural numbers by . For any real number , we denote the largest integer which is less than r or equal to r by . For , we define the function space defined by
with the metric , where we have put
For real numbers and , we put
We denote the Gauss kernel for the diffusion equation by
for and , and we define the operator by , where denotes the convolution for the variables x. We regard the solution of the Cauchy problem (1.1) as the fixed point of the mapping Φ defined by
First, we show the existence of the solutions of the Cauchy problem (1.1) for .
(Global solutions for ).
Let,,. Let p satisfyLet. Ifis sufficiently small, then there exist,and a unique global solution u of (
1.1
) insatisfying the estimatesfor.
The global solutions in Theorem 1.1 have the following asymptotic behaviors.
(Asymptotic behaviors for ).
Under the assumption in Theorem
1.1
, moreover, assumeLet. The solution u obtained in Theorem
1.1
satisfiesas, whereandHere,andhold for j and α with.
The corresponding result in Theorem 1.2 in the case has been shown in [12] with a different expression of the asymptotic function v, and the result in Theorem 1.1 in the case follows from the estimates in it (see [21]). Our results extend the results in the case into , and our proofs show how the spatial contraction by affects the problem compared with the case . The basic idea of our proofs is based on the method in [5] and [15] (see also [10,22]), which obtained a higher order expansion of the solutions of the Navier–Stoke equations in terms of Gaussian-like functions. We can find similar argument in [23], which dealt with nonlinear damped wave equations. The exponent in (1.7) is called the Fujita exponent. When , it is well-known for (1.1) that any nontrivial and nonnegative solution blows up in finite time when , while the solution u exists globally for small data when [6,9,24]. Theorem 1.1 shows that the Fujita exponent disappears if the space is contracting (i.e., ). We note that holds if and only if .
Next, we show the existence of solutions of the Cauchy problem (1.1) for . We say that the solution u of (1.1) is global if u exists on . Let . For integers and , we define the function spaces D and Y by
and with the metric
where is defined by
for . For , put
(Global solutions for ).
Let,,,,. Let p satisfy. Let. Then the following results hold.
There exists constantsandsuch that ifsatisfies, then there exists a unique global solution u of (
1.1
) in.
The solution u in (1) satisfies, whereis defined by
The solution u in (1) is unique in.
The solutions in Theorem 1.3 have the following asymptotic behaviors.
(Asymptotic behaviors for ).
Under the assumption in Theorem
1.3
, let. Putfor. Then the following results hold.for. Especially,as.
One might consider to obtain the same result in Theorem 1.4 with replaced by defined by
In this case, we need to show as . When , since we have
by Lemma 2.1, below, the additional condition is required to show , while this condition is not necessary in the theorem by the use of .
The global solutions in Theorem 1.1 when and in Theorem 1.3 when have been shown in [19] with their asymptotic behaviors based on the different method in [20]. Our results extend those results to the general order , and , which require the estimates for the higher order terms in the Taylor expansion of the Gauss kernel and the heat operator given by Lemma 2.3 and (6.2).
For A and B, the notation denotes the inequality for some constant which is not essential for the argument throughout the paper.
Preliminaries
In this section, we prepare several estimates to prove our theorems. We recall three fundamental lemmas known as the estimate, the expansion of the Gauss kernel, and the asymptotic behavior for the free solution of the diffusion equation. We prove them for the convenience of readers.
Let,, and let α denote arbitrary multi-index. Thenhold for.
(1) Put , , . We define functions inductively by
and
for . By , we have . We are able to show inductively for . We obtain
for and any multi-index α. So that, we have
which yields the required inequality.
(2) By , the Young inequality and (1), we have
where s is defined by , which is the required result. □
Let. The expansionholds for.
For and , put . Since h has the expansion
we have
by . Taking the Fourier transform and its inverse for the both sides, we obtain the required result. □
For any, the equationholds for any,.
The required result follows from the fundamental theorem of calculus. □
For and , put
Letand. Put. Then the following inequalities hold for.
if.
if.
.
We have as . By , the function g is increasing if , g is constant if , and g is decreasing if . Thus, we have if , and if . We note that is equivalent to “ and ” or “ and ,” and is equivalent to “ and ” or “ and ” under . So that, we obtain the required results in (1) and (2). The result in (3) follows from and by the results in (1), (2) and the definition of . □
(Nonlinear estimates).
For, α withanddefined by (
1.3
), the estimateholds for any.
Since we have
and by the definition of and , we have
for any . So that, we obtain
where we have used by the definition of . □
Let, and let,. Let,. Let,for a.e.if. Then the function u defined byforsatisfies.
For , we have
where we have put
Since the function is uniformly continuous by
for , the function is uniformly continuous for any α with if . We have
Since we have
by Lemma 2.1, we have
as or , where we have used that are uniformly continuous when . Similarly, we have
by Lemma 2.1, where is the characteristic function on the interval . Since we have
and
as or , where we use that are uniformly continuous for a.e. when , we obtain
as or by the Lebesgue convergence theorem. We have
as or by Lemma 2.1 and . By (2.4), (2.5), (2.6) and (2.7), the function u is continuous. □
We show some weighted estimates for the operator as follows.
Let. Let. For any multi-index α, the following results hold.whereis a constant dependent on α, β, γ and j.
(1) The required result follows from
where is a constant dependent on j and β, and we note .
(2) By the result (1) and (2.2), we have
Since we have
by the interpolation, we obtain the last result. □
Let k be a nonnegative integer. If h satisfies, thenas.
For any α with , we have
by (1) in Lemma 2.7, where we have put
Since we have
by (2.2), we obtain as . Since we have
we obtain
as by as required. □
Let k be a nonnegative integer. Let. The following results hold for any rapidly decaying function h on.
(1) When , we have
by (2.2). When , we divide the interval into and . For each interval, we have
and
by (2.2). So that, we obtain the required result.
For , we have
by (2.2). We also have
by Lemma 2.7. Put . We have
by (1.6). Put
By Corollary 2.9, we have
which yields
by (3) and (4) in Lemma 2.10. Thus, we obtain
for under the conditions
Similarly to (3.3), we have
Put
By Corollary 2.9, we have
which yields
by (4) in Lemma 2.10. Thus, we obtain
under the conditions
Especially, putting , we obtain
under the same condition (3.5). So that, Φ is a mapping from into itself under the conditions (3.4) and (3.5).
Next, we consider the metric. Put . Since we have
we have
by Corollary 2.9 and Lemma 2.10. So that, we obtain
for any under the second condition in (3.5). Similarly, we also have
by Corollary 2.9 and Lemma 2.10. So that, we obtain
for any under the second condition in (3.5). Especially, taking , we also obtain
Therefore, Φ is a contraction mapping on under the conditions (3.4) and (3.5). We obtain the fixed point of Φ by the Banach fixed point theorem.
Since we have
for by the definition of in (1.2), we obtain
for by the definition of in (2.9). So that, the conditions (3.4) and (3.5) are satisfied if and are sufficiently small, which require the smallness of . Especially, taking and , we obtain the solution , which shows
for by the definition (1.4) as required in (1.8) and (1.9).
Next, let us show . Let . Since u satisfies
we have
Thus, we have
where we have put
We have
as or if by Lemma 2.7 and Corollary 2.8. We consider for since when . Since is rewritten as
where is the characteristic function on the interval , we have
We have
as or if for by Lemma 2.7 and Corollary 2.8. We also have
by which we obtain
by Lemma 2.10. Thus, we obtain
as or by (3.8) and (3.9) and the Lebesgue convergence theorem. We have
as or by Lemma 2.7 and Lemma 2.10. By (3.6), (3.7), (3.10) and (3.11), we obtain is continuous in for . Since the above argument is also valid for the case , we have . So that, we obtain as required.
For any integer , let v be the function defined by (1.14).
For the solution u obtained in Theorem
1.1
, we havewhere we have put
Put . Since u is the fixed point of Φ defined by (1.6), and we have
we obtain
On the other hand, since v is defined by (1.14), we have
by dividing the interval into and . So that, we have
as required. □
In the following, we estimate in Lemma 4.1, respectively.
(Estimate for ).
Letand. Letandbe defined by (
1.12
) andThen the following estimates hold.
(2) Since we have
and
by Lemma 2.1, we have
for . By (4.1) and (4.2), we obtain the required result.
(3) Put and
Then we have
where we have decomposed into the regions and for any . Since is rewritten as
by Lemma 2.3, we have
By and
we have
Next, we estimate . Since is rewritten as
where we have used Lemma 2.3 for the last equality. Thus, we have
by (4.4), which yields
By (4.3), (4.5) and (4.6), we have
which is the required estimate. □
(Estimate for ).
Letbe an integer. Let. Let u be the global solution of (
1.1
) in Theorem
1.1
. Then the following results hold.
The solution u satisfiesfor.
Ifor, thenfor. Especially,for any integerifby putting.
Letbe the constant defined by (
2.3
). Ifand, thenfor. Especially,for any integerifby putting.
(2) By the result (1), we have
where we have used
for by Lemma 2.1, and
by the definition of . Since when or , we have
We obtain the required result by (4.9) and (4.10).
(3) Since we have when and , we have
We obtain the required result by (4.9) and (4.11). □
(Decomposition of ).
Put.is decomposed aswhereandare defined byandHere,is ignored if.
The decomposition follows directly from the definition of since is the case of in , and is the case of in . □
(Estimate for ).
Let, and let. The following estimates hold.
Ifor, thenMoreover,if.
Ifand, thenMoreover,if.
We rewrite as
by
For any , we decompose into three parts given by
where we have put
and
Here, is ignored when . We estimate I. Since we have
by Lemma 2.3, we have
where we have used ,
for by Lemma 2.1,
by Lemma 2.5, and we have put
We have
by Lemma 2.4. When or , we have
by which we obtain
When and , we have
by which we obtain
We estimate . By Lemma 2.3, we have
Thus, we obtain
where we have used Lemma 2.1, and
by Lemma 2.5. When or , we obtain
by (4.14). Especially, we have
if by the Lebesgue convergence theorem for (4.19). When and , we obtain
by (4.16). Especially, we have
if by the Lebesgue convergence theorem for (4.19).
We estimate . We have
directly from the definition of . Analogously to the argument starting from (4.18), we obtain the same estimates (4.20), (4.21), (4.22), (4.23) with replaced by .
The result in (1) follows from (4.12), (4.15), (4.20) with the same estimate for , and (4.21). The result in (2) follows from (4.12), (4.17), (4.22) with the same estimate for , and (4.23). □
(Estimate for ).
Letand. The following estimates hold.
Ifor, thenMoreover,if.
Ifand, thenMoreover,if.
We rewrite as
by
Since we have
by Lemma 2.3, we obtain
Taking -norm of the both sides, we have
Here, we have
by Lemma 2.1,
by Lemma 2.5. So that, we obtain
where we have used (4.13) and we have put
(1) When or , we have
by which we obtain the required result. Since holds when , we obtain
if .
(2) When and , we have
by which we obtain the required result. Since holds when , we obtain if . □
(Estimate for ).
Letand. The following inequalities hold.
Ifor, thenfor. Especially,if.
Ifand, thenfor. Especially,if.
We have
and
by the Hölder inequality. By the interpolation and the definition of , we have
By (4.13), we obtain
By (4.28) and (4.29), we have the required results (4.24) and (4.26). The results (4.25) and (4.27) follow directly from (4.24) and (4.26), respectively, since is rewritten as , and is rewritten as . □
(Estimate for ).
Letand. The following results hold.
Letor. Let p satisfy. ThenEspecially,
Letand. Let p satisfy. ThenEspecially,
By the definition of , we have
where we have used (2.1) and Lemma 2.5.
(1) Since by Lemma 2.4 when or , we have
if . So that, we obtain (4.30) by (4.35) and (4.36). The result (4.31) follows from (4.30) since holds by .
(2) Since by Lemma 2.4 when and , we have
if . So that, we obtain (4.32) by (4.35) and (4.37). The result (4.33) follows from (4.32) since holds by . □
Now, we prove Theorem 1.2. Let v be the function defined by (1.14). By Lemma 4.1, we have
We have
as if by (3) in Lemma 4.2. We have
under the condition (1.10) by Lemmas 4.3, 4.7 and 4.8. We have
under the condition (1.10) by Lemmas 4.4, 4.5 and 4.6. So that, we obtain
as , which is the required result in the theorem.
For any multi-index α with , we have
where are constants dependent on α, . Thus, when , we have
where is defined by (1.15) for and we have used
Since we also have
for , we obtain
Similarly, we have
for by (5.2), where we note .
Let Φ be the operator defined by (1.6). By (2.2) and (5.3), we have
for some constant , where we have used
Thus, we have
for any . We also have
for by (1.6), (5.5) and
for any u, v. Thus, we have
for any . By (5.6) and (5.7), the operator Φ is a contraction mapping on the ball in Y if R satisfies and .
(2) (i) Let us consider the case with or . In this case, we have and by their definitions. We have for a.e. by (5.4). By this result, and Lemma 2.6, we have .
(ii) Let us consider the case . Since , we have by Lemma 2.6.
(3) Let be an another solution which has the initial data . Put
We assume and show a contradiction. Since and , we have . Since u and v are rewritten as
for , we have
by . By (2.2) and the Hölder inequality, we have
Thus, we have
Since , we obtain
for sufficiently small . This result shows for , which is a contradiction to the definition of . So that, we have , which yields the required uniqueness of the solution.
This section is devoted to the proof of Theorem 1.4. The following lemma is useful to obtain the asymptotic profiles of the solutions of (1.1) when .
Let. Letwith. Let. Thenfor.
Put . For , we use the expansion
Defining the operator
we have
Since we have
we have
by the Young inequality, where we have put and
We have
where we have put . Since we have
we have by the Young inequality. Since is rewritten as
we have
where we have put . Since is rewritten as
we have . Thus, we have
Combining (6.4) and (6.5), we have
We obtain the required result by (6.3) and (6.6). □
Now, let us prove the theorem. Let , and v be the functions defined in the theorem. Since satisfies
we have
for any multi-index α by Lemma 2.1. Thus, we have
for . Replacing t and T with and in (6.2), respectively, we have
Thus, we have
where we have put and defined by
We have
by Lemma 2.1. Since we have by (5.1), and we also have by simple calculation, we obtain
Analogously, we have
by
(1) Since v satisfies , we obtain
by (6.7) and (6.9). So that, as required.
(2) Since we have , we obtain
by Lemma 6.1 and (6.8), which is the required result.
Footnotes
Acknowledgements
This work was supported in part by JSPS KAKENHI Grant Number (B)16H03940 for the first author, and by JSPS KAKENHI Grant Number (C)19K03596 for the second author. The authors are thankful to the anonymous referee for several comments to revise the paper.
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