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15 June 2020

On Inner Expansions for a Singularly Perturbed Cauchy Problem with Confluent Fuchsian Singularities

Département de mathématiques, Bât. M2, University of Lille, 59655 Villeneuve d’Ascq CEDEX, France

Abstract

A nonlinear singularly perturbed Cauchy problem with confluent Fuchsian singularities is examined. This problem involves coefficients with polynomial dependence in time. A similar initial value problem with logarithmic reliance in time has recently been investigated by the author, for which sets of holomorphic inner and outer solutions were built up and expressed as a Laplace transform with logarithmic kernel. Here, a family of holomorphic inner solutions are constructed by means of exponential transseries expansions containing infinitely many Laplace transforms with special kernel. Furthermore, asymptotic expansions of Gevrey type for these solutions relatively to the perturbation parameter are established.

1. Introduction

This work falls in the continuance of [1], where families of singularly perturbed initial value problems with the following shape
Q ( z ) y ( t , z , ϵ ) = Q 1 ( z ) y ( t , z , ϵ ) Q 2 ( z ) y ( t , z , ϵ ) + ( D ϵ , α ( t ) ) δ D R D ( z ) y ( t , z , ϵ ) + P ( 1 / a ( ϵ t , ϵ ) , z , ϵ , D ϵ , α ( t ) , z ) y ( t , z , ϵ ) + f ( 1 / a ( ϵ t , ϵ ) , z , ϵ )
for vanishing initial data y ( 0 , z , ϵ ) 0 were considered. There, Q , Q 1 , Q 2 , R D stand for polynomials with complex coefficients and δ D 2 is an integer. The operator
D ϵ , α ( t ) : = ( ϵ t 2 ϵ α ) t
is a fuchsian differential operator at the points t = ± ϵ α 1 2 for some odd integer α 3 and ϵ C is a non-vanishing complex parameter. This operator unfolds the basic singularly perturbed irregular operator ϵ t 2 t of rank 1 at t = 0 . Recent references about this so-called confluence process of Fuchsian singularities can be found in our work [1]. The function a ( ϵ t , ϵ ) (unveiled in (13)) represents a well-chosen logarithmic function in its arguments. The linear differential operator P ( T 1 , T 2 , T 3 , D ϵ , α ( t ) , z ) is chosen to be analytic in T 1 , T 3 near the origin in C and holomorphic w.r.t T 2 on a strip H β = { z C / | Im ( z ) | < β } for some width β > 0 ; moreover the forcing term f ( T 1 , z , ϵ ) is analytic near the origin in C relatively to T 1 , ϵ and holomorphic in z on H β . Notice that this function a ( ϵ t , ϵ ) is introduced to be able to construct nice representable solutions y ( t , z , ϵ ) to (1) as Laplace transforms in time t from which parametric asymptotic properties can be analyzed. The fact that both coefficients and forcing term in (1) are holomorphic maps in 1 / a ( ϵ t , ϵ ) is a strong technical condition, but they turn out to be good approximations of general analytic functions on appropriate domains in time t, for z H β , provided that ϵ remains small enough.
Two distinguished finite sets of holomorphic solutions y ( t , z , ϵ ) to (1) were constructed. The first family consists of the so-called outer solutions y p out ( t , z , ϵ ) , 0 p ι 1 for some integer ι 2 that are holomorphic on domains A × H β × E p out , where A is a fixed bounded sectorial annulus confined apart of the origin in C and E p out is a bounded sector centered at 0 which belongs to a set E ̲ out = { E p out } 0 p ι 1 that covers a full neighborhood of 0 in C called good covering in C (see Definition 2). The second family is comprised in the so-called inner solutions y p in ( t , z , ϵ ) , 0 p η 1 for some integer η 2 that are constructed on a domain T ϵ in = { ϵ α 1 2 x / x χ } w.r.t time t for some fixed bounded sectorial annulus χ far enough from the origin in C , z H β and ϵ in a sector E p in that is part of a good covering in C .
Both families y p out / in ( t , z , ϵ ) could be expressed as special Laplace transform and Fourier integrals
y p out / in ( t , z , ϵ ) = 1 ( 2 π ) 1 / 2 + L γ p out / in W p out / in ( τ , m , ϵ ) exp τ a ( ϵ t , ϵ ) e 1 z m d τ τ d m
for suitable Borel maps W p out / in . Furthermore, from these integral representations, asymptotic behavior could be extracted. Indeed, the outer solutions y p out ( t , z , ϵ ) (resp. inner solutions y p in ( t , z , ϵ ) ) share a common power series O ^ ( ϵ ) = k 0 O k ϵ k for bounded holomorphic coefficients O k on A × H β as asymptotic expansion of Gevrey order 1 (resp. I ^ ( ϵ ) = k 0 I k ϵ k for bounded holomorphic coefficients I k on T ϵ in × H β as asymptotic expansion of Gevrey order 2 α + 1 ), meaning that constants A p out / in , B p out / in > 0 can be found with
sup t A , z H β y p out ( t , z , ϵ ) k = 0 n 1 O k ϵ k A p out ( B p out ) n n ! | ϵ | n
for all n 1 , ϵ E p out and
sup x χ , z H β y p in ( ϵ α 1 2 x , z , ϵ ) k = 0 n 1 I k ϵ k A p in ( B p in ) n Γ ( 1 + 2 α + 1 n ) | ϵ | n
provided that n 1 , ϵ E p in .
In this paper, we turn our attention at a closely related singularly perturbed nonlinear Cauchy problem
P 2 D ϵ , α ( t ) z S u ( t , z , ϵ ) = P 1 ( t , z , ϵ , D ϵ , α ( t ) , z ) u ( t , z , ϵ ) + g ( t , ϵ )
under given Cauchy data
( z j u ) ( t , 0 , ϵ ) = φ j ( t , ϵ ) , 0 j S 1 .
Like in (1), the forcing term g ( t , ϵ ) is chosen to be a polynomial in the function 1 / a ( ϵ t , ϵ ) . A similar assumption is put on the Cauchy data (6). The choice of the function a ( ϵ t , ϵ ) is made for the same reason as in our former study (1). Moreover, P 2 stands for a polynomial with complex coefficients and S 2 is an integer. The novel feature is that the coefficients in the main part P 1 of (5) are assumed to be merely polynomials in t. As we will see in the work, this property has a deep impact on the structure of solutions to (5), (6) if compared with the ones y p out / in built up for (1).
For technical reasons that will be clear later in the paper, we impose that the operator P 2 D ϵ , α ( t ) can be factored out in the main part P 1 which allows us to reduce the problem (5), (6) to a Cauchy problem of Kowalevski type stated in (11), (12). Such a reduction is mandatory within our approach as explained in Section 5 of the work. The forcing term f ( t , ϵ ) of the resulting Equation (11) is asked to solve a simple singularly perturbed ODE
P 2 D ϵ , α ( t ) f ( t , ϵ ) = g ( t , ϵ ) .
As a result, the single Equation (5) is written as a coupling of a Kowalevski type Equation (11) and a singularly perturbed ODE (7). It is worthwhile noting that a more general forcing term g ( t , z , ϵ ) relying holomorphically on z and Cauchy data φ j ( t , ϵ ) , 0 j S 1 that are not only polynomials in 1 / a ( ϵ t , ϵ ) but also polynomials in t could be treated in a similar manner. However, such a general choice would lead to even more cumbersome and heavy computations which may avoid the reader to have a clear idea of the main purpose of the study.
The main striking difference with our previous work [1] is that now the analytic solutions fail to be constructed as a single special Laplace transform for the kernel exp τ a ( ϵ t , ϵ ) . Nevertheless, they can be expressed as exponential sums which involve infinitely many of Laplace transforms, which are called transseries in the literature (for an explanation of this terminology we refer to Chapters 4 and 5 of the excellent textbook [2]). Specifically, we can provide a finite set of analytic solutions ( t , z ) u p ( t , z , ϵ ) , 0 p ι 1 for some integer ι 2 on some domains T ϵ × D ( 0 , r ) . Here, D ( 0 , r ) represents a small disc centered at 0 with radius r > 0 and T ϵ = { ϵ α 1 2 x / x χ 1 } (which is similar to the domain T ϵ in introduced above) is a set where χ 1 stands for a tiny bounded sectorial annulus close to 1 in C , whenever ϵ E p , where E p is a bounded sector centered at 0 that belongs to a good covering in C . Since the domain T ϵ remains next to the Fuchsian singular point ϵ α 1 2 and borders the origin as ϵ tends to 0, we call the elements of this set inner solutions. Each solution u p ( t , z , ϵ ) has a convergent exponential transseries expansion
u p ( t , z , ϵ ) = n 0 L γ p W n ( τ , z , ϵ ) exp τ a ( ϵ t , ϵ ) d τ τ exp ( n ϵ α + 1 2 a ( ϵ t , ϵ ) )
on T ϵ × D ( 0 , r ) for ϵ E p (see Theorem 1). Actually, the appearance of such transseries stems from the very expansion of the monomials ( ϵ t ) l , l 1 as sums of special Laplace transforms as shown in Propositions 1 and 3. In the proof, an interesting small divisor phenomenon occurs which gives rise to the appearance of a special series (52) in the expansion of the basic monomial T, see (46). This special series turn out to carry an exponential series expansion displayed in Lemma 8. It is worthwhile noting that due to the specific arrangement of these expansions, this approach does not allow us to exhibit the so-called outer solutions as in the case of our previous study [1]. In a second main result (Theorem 2), we analyze the parametric asymptotic expansions of these inner solutions. It turns out that the functions ϵ u p ( t , z , ϵ ) , 0 p ι 1 , share a common formal series I ^ ( ϵ ) = k 0 I k ϵ k with bounded holomorphic coefficients I k on T ϵ × D ( 0 , r ) as Gevrey asymptotic expansion of order 2 α + 1 . This outcome is comparable to the one obtained in [1].
During the last two decades, exponential transseries expansions appear to be a central tool in the study of differential, partial differential and difference equations in the complex domain. Indeed, we refer to the seminal work by O. Costin and R. Costin, see [3], where these class of expansions have shown to be essential in the study of formation of complex singularities along Stokes directions for systems of nonlinear ODEs of the form
x 2 y ( x ) = A ( x ) y ( x ) + B ( x , y ( x ) )
where y ( x ) C n , for an integer n 1 , x C , A ( x ) is an analytic diagonal matrix and for a nonlinearity B ( x , Y ) analytic near the origin in C n + 1 . Later, the transseries approach was extended by B. Braaksma and R. Kuik, in [4], to nonlinear systems of difference equations
y ( x + 1 ) = Λ ( x ) y ( x ) + g ( x , y ( x ) )
for y ( x ) C n , with integer n 1 , Λ ( x ) an analytic diagonal matrix and g ( x , Y ) analytic near x = and Y = 0 . Adjustments of this approach applied to partial differential equations (beyond the integrable case) have been initiated in the paper [5]. More recently, transseries expansions (conjointly with a KAM-like approach) have been applied to the location of complex singularities of general first order nonlinear scalar equations y = F ( y ( x ) , 1 / x ) as x tends to infinity, see [6]. Similar strategies have been implemented on nonlinear second order ODEs such as the Painlevé equation P 1 in order to compute in closed form connection coefficients between solutions on sectors called Stokes multipliers, see [7]. For problems related to obstruction for analytic integrability of Hamiltonian systems and transseries expansions of first integrals, we refer to [8]. Another aspect for which transseries turn out to be a powerful tool is the resurgence property of formal power series solutions to differential or more general functional equations (i.e., analytic continuation of their Borel transforms). For systems of the form (8) and (9) resurgence properties stemming from transseries expansions of actual holomorphic solutions on sectors have been exhibited in the papers [9,10]. For parametric resurgence for WKB solutions of 1D complex Schrödinger equations
ϵ 2 y ( x ) = x 2 ( 1 x ) 2 y ( x )
w.r.t ϵ , based on exponential series techniques, we mention the work by A. Fruchard and R. Schäfke [11].
Our paper is arranged as follows.
In Section 2, we present the main problems (11), (12) and (23), (12) of the work. In the technical Propositins 1 and 3, we express the coefficients of (11) as convergent exponential transseries expansions that contain Laplace transforms with specific kernel, which leads to seek for solutions to (11), (12) expressed in the same manner as exponential series involving Laplace transforms of infinitely many Borel maps W n , n 0 . The principal accomplishment of this section is the layout of a sequence of convolution problems (100), (101) fulfilled by W n , n 0 .
In Section 3, the sequence of convolution problems is solved by means of a majorant series approach, the use of sequences of Banach spaces of sectorial holomorphic functions with exponential growth and the application of the classical Cauchy-Kowalevski theorem.
In Section 4, the two main results of the paper are stated. A set of inner holomorphic solutions to (11), (23), (12) are constructed, which are defined w.r.t ϵ on a good covering in C and relatively to time t on a domain that remains close to the moving fuchsian singularities of (23) (Theorem 1). In Theorem 2, the parametric asymptotic behavior of the latter solutions is analyzed by means of the classical Ramis–Sibuya approach.
The last section is devoted to the conclusion of the work where insights for prospective works are outlined.

3. Resolution of the Convolution Set of Equations within Banach Spaces of Holomorphic Functions

We seek for solutions W n ( τ , z , ϵ ) , n 0 of the convolution Equations (100) and (101) as formal power series w.r.t z, namely
W n ( τ , z , ϵ ) : = β 0 W n , β ( τ , ϵ ) β ! z β .
We first disclose a recursion formula, for each n 0 , for the sequence of expressions W n , β ( τ , ϵ ) , β 0 . We need to compute each piece of Equations (100) and (101). Specifically, for each n 0 , we get
z S W n ( τ , z , ϵ ) = β 0 W n , β + S ( τ , ϵ ) β ! z β
and
p + q = n ω l 1 , p ( τ , ϵ ) τ { ( τ + q ϵ α + 1 2 ) l 2 z l 3 W q ( τ , z , ϵ ) } + a l 1 , p ( ϵ ) ( τ + q ϵ α + 1 2 ) l 2 z l 3 W q ( τ , z , ϵ ) = β 0 p + q = n ω l 1 , p ( τ , ϵ ) τ ( τ + q ϵ α + 1 2 ) l 2 W q , β + l 3 ( τ , ϵ ) β ! + a l 1 , p ( ϵ ) ( τ + q ϵ α + 1 2 ) l 2 W q , β + l 3 ( τ , ϵ ) β ! ) z β .
Let the convergent Taylor expansion of d l ( z , ϵ ) w.r.t z at 0 be
d l ( z , ϵ ) = β 0 d l , β ( ϵ ) β ! z β
for all ϵ D ( 0 , ϵ 0 ) . Owing to (104) and (105), we get
d l ( z , ϵ ) × p + q = n ω l 1 , p ( τ , ϵ ) τ { ( τ + q ϵ α + 1 2 ) l 2 z l 3 W q ( τ , z , ϵ ) } + a l 1 , p ( ϵ ) ( τ + q ϵ α + 1 2 ) l 2 z l 3 W q ( τ , z , ϵ ) = β 0 β 1 + β 2 = β ( p + q = n ω l 1 , p ( τ , ϵ ) τ ( τ + q ϵ α + 1 2 ) l 2 W q , β 2 + l 3 ( τ , ϵ ) β 2 ! + a l 1 , p ( ϵ ) ( τ + q ϵ α + 1 2 ) l 2 W q , β 2 + l 3 ( τ , ϵ ) β 2 ! × d l , β 1 ( ϵ ) β 1 ! ) z β
and also
d l ( z , ϵ ) × ( τ + n ϵ α + 1 2 ) l 2 z l 3 W n ( τ , z , ϵ ) = β 0 β 1 + β 2 = β d l , β 1 ( ϵ ) β 1 ! ( τ + n ϵ α + 1 2 ) l 2 W n , β 2 + l 3 ( τ , ϵ ) β 2 ! z β .
On the other hand, we check that
p + q = n W p ( τ , z , ϵ ) τ W q ( τ , z , ϵ ) = β 0 p + q = n h 1 + h 2 = β W p , h 1 ( τ , ϵ ) h 1 ! τ W q , h 2 ( τ , ϵ ) h 2 ! z β
and if one expands e ( z , ϵ ) at z = 0 , namely
e ( z , ϵ ) = β 0 e β ( ϵ ) β ! z β
the next power series expansion for the nonlinear term holds
e ( z , ϵ ) p + q = n W p ( τ , z , ϵ ) τ W q ( τ , z , ϵ ) = β 0 β 1 + β 2 = β e β 1 ( ϵ ) β 1 ! × p + q = n h 1 + h 2 = β 2 W p , h 1 ( τ , ϵ ) h 1 ! τ W q , h 2 ( τ , ϵ ) h 2 ! z β .
As a result, we require that the sequence of expressions W 0 , β ( τ , ϵ ) , β 0 fulfills the next nonlinear recursive relation
W 0 , β + S ( τ , ϵ ) β ! = l = ( l 1 , l 2 , l 3 ) I , l 1 1 ϵ Δ l l 1 β 1 + β 2 = β ( ω l 1 , 0 ( τ , ϵ ) τ τ l 2 W 0 , β 2 + l 3 ( τ , ϵ ) β 2 ! + a l 1 , 0 ( ϵ ) τ l 2 W 0 , β 2 + l 3 ( τ , ϵ ) β 2 ! ) × d l , β 1 ( ϵ ) β 1 ! + l = ( l 1 , l 2 , l 3 ) I , l 1 = 0 ϵ Δ l l 1 β 1 + β 2 = β d l , β 1 ( ϵ ) β 1 ! τ l 2 W 0 , β 2 + l 3 ( τ , ϵ ) β 2 ! + β 1 + β 2 = β e β 1 ( ϵ ) β 1 ! × h 1 + h 2 = β 2 W 0 , h 1 ( τ , ϵ ) h 1 ! τ W 0 , h 2 ( τ , ϵ ) h 2 ! + P 1 ( τ ) P 2 ( τ ) δ 0 , β
where δ 0 , 0 = 1 and δ 0 , β = 0 whenever β 1 , under the assumption that
W 0 , j ( τ , ϵ ) = Q j ( τ ) , 0 j S 1 .
This latter constraint stems from the assumption (25) on the Cauchy data ( z j U d ) ( T , 0 , ϵ ) for 0 j S 1 . Furthermore, for each n 1 , we ask the sequence of expressions W n , β ( τ , ϵ ) , for n 1 , to be subjected to the next recursive relation
W n , β + S ( τ , ϵ ) β ! = l = ( l 1 , l 2 , l 3 ) I , l 1 1 ϵ Δ l l 1 β 1 + β 2 = β ( p + q = n [ ω l 1 , p ( τ , ϵ ) τ { ( τ + q ϵ α + 1 2 ) l 2 W q , β 2 + l 3 ( τ , ϵ ) β 2 ! } + a l 1 , p ( ϵ ) ( τ + q ϵ α + 1 2 ) l 2 W q , β 2 + l 3 ( τ , ϵ ) β 2 ! ] ) × d l , β 1 ( ϵ ) β 1 ! + l = ( l 1 , l 2 , l 3 ) I , l 1 = 0 ϵ Δ l l 1 β 1 + β 2 = β d l , β 1 ( ϵ ) β 1 ! ( τ + n ϵ α + 1 2 ) l 2 W n , β 2 + l 3 ( τ , ϵ ) β 2 ! + β 1 + β 2 = β e β 1 ( ϵ ) β 1 ! p + q = n h 1 + h 2 = β 2 W p , h 1 ( τ , ϵ ) h 1 ! τ W q , h 2 ( τ , ϵ ) h 2 !
provided that
W n , j ( τ , ϵ ) 0 , 0 j S 1
that originates from our requirement (25) on the Cauchy data of our problem (24).
We now need to specify in which spaces of functions our sequence of functions τ W n , β ( τ , ϵ ) are going to live, provided that ϵ D ( 0 , ϵ 0 ) { 0 } . These Banach spaces have already been introduced in a former work of the author in [15].
Definition 1.
Let S d be an unbounded sector centered at 0 with bisecting direction d R , D ( 0 , ρ ) be a disc centered at 0 with radius ρ > 0 and σ > 0 be a fixed real number. For each integer β 0 , we set F ( β , σ , S d , ρ ) as the vector space of holomorphic functions v : S d D ( 0 , ρ ) C such that the norm
| | v ( τ ) | | ( β , σ , S d , ρ ) : = sup τ S d D ( 0 , ρ ) | v ( τ ) | 1 + | τ | 2 | τ | exp ( σ r b ( β ) | τ | )
is finite, where r b ( β ) represents the partial Riemann series r b ( β ) : = n 0 β 1 / ( n + 1 ) b , for some integer b 2 .
The next technical proposition turns to be essential in the discussion that will lead to the fact that the sequence of functions τ W n , β ( τ , ϵ ) actually belong to the space F ( β , σ , S d , ρ ) for the direction d chosen as in Proposition 1 and for some small radius ρ > 0 .
Proposition 4.
Take a real number σ such that σ > M for M given in (31). Select a radius ρ > 0 such that the disc D ( 0 , ρ ) does not contain any element of the set R 2 of the roots of the polynomial P 2 ( τ ) .
(1) There exists a constant P 1 , 2 > 0 (which relies on σ , r b ( S ) , P 1 , P 2 ) such that
| | P 1 ( τ ) / P 2 ( τ ) | | ( S , σ , S d , ρ ) P 1 , 2 .
(2) Let n , β 0 be integers and l = ( l 1 , l 2 , l 3 ) I . Moreover, let 0 β 2 β , let p , q 0 satisfy the relation p + q = n . Finally, let 0 m 1 l 2 . We make the assumption that the map τ W q , β 2 + l 3 ( τ , ϵ ) belongs to the space F ( β 2 + l 3 , σ , S d , ρ ) , for all ϵ D ( 0 , ϵ 0 ) { 0 } . Then, the estimates
| | ω l 1 , p ( τ , ϵ ) τ τ m 1 W q , β 2 + l 3 ( τ , ϵ ) | | ( β + S , σ , S d , ρ ) K l 1 ( L l 1 ) p F m 1 m 1 e m 1 ( β + S + 1 ) b m 1 | | W q , β 2 + l 3 ( τ , ϵ ) | | ( β 2 + l 3 , σ , S d , ρ )
and
| | a l 1 , p ( ϵ ) τ m 1 W q , β 2 + l 3 ( τ , ϵ ) | | ( β + S , σ , S d , ρ ) A l 1 ( B l 1 ) p m 1 m 1 e m 1 ( β + S + 1 ) b m 1 | | W q , β 2 + l 3 ( τ , ϵ ) | | ( β 2 + l 3 , σ , S d , ρ )
hold where F is given by (84).
(3) Let n , β 0 be integers. Let p , q 0 be integers with p + q = n and h 1 , h 2 0 integers with h 1 + h 2 β . Take for granted that τ W p , h 1 ( τ , ϵ ) belongs to F ( h 1 , σ , S d , ρ ) and that τ W q , h 2 ( τ , ϵ ) belongs to F ( h 2 , σ , S d , ρ ) . Then, the next bounds
| | W p , h 1 ( τ , ϵ ) τ W q , h 2 ( τ , ϵ ) | | ( β + S , σ , S d , ρ ) F | | W p , h 1 ( τ , ϵ ) | | ( h 1 , σ , S d , ρ ) | | W q , h 2 ( τ , ϵ ) | | ( h 2 , σ , S d , ρ )
are valid for F displayed in (84).
Proof. 
We turn to the first point (1). By construction, both sets D ( 0 , ρ ) and S d a properly chosen in a way that they avoid the roots R 2 of the polynomial P 2 ( τ ) . We distinguish two cases.
First case: assume that deg ( P 1 ) < deg ( P 2 ) . Then, we can get a constant A 1 , 2 > 0 (which relies on P 1 , P 2 ) with
sup τ S d D ( 0 , ρ ) | P 1 ( τ ) / P 2 ( τ ) | 1 + | τ | 2 | τ | exp ( σ r b ( S ) | τ | ) sup x 0 A 1 , 2 exp ( σ r b ( S ) x ) = A 1 , 2 .
Second case: assume that deg ( P 1 ) deg ( P 2 ) . We need to recall the classical estimates for some real numbers m 1 0 , m 2 > 0 ,
sup x 0 x m 1 exp ( m 2 x ) = ( m 1 / m 2 ) m 1 e m 1
with the convention that 0 0 = 1 . Then, by construction, two constants A ^ 1 , 2 , B ^ 1 , 2 > 0 can be singled out with
sup τ S d D ( 0 , ρ ) | P 1 ( τ ) / P 2 ( τ ) | 1 + | τ | 2 | τ | exp ( σ r b ( S ) | τ | ) sup x 0 ( A ^ 1 , 2 x deg ( P 1 ) deg ( P 2 ) + 1 + B ^ 1 , 2 ) exp ( σ r b ( S ) x ) A ^ 1 , 2 deg ( P 1 ) deg ( P 2 ) + 1 σ r b ( S ) deg ( P 1 ) deg ( P 2 ) + 1 exp ( ( deg ( P 1 ) deg ( P 2 ) + 1 ) ) + B ^ 1 , 2 .
We now focus on the second point (2). From Proposition 3, one can choose two constants K l 1 , L l 1 > 0 and M > 0 introduced in (31) such that
| ω l 1 , p ( τ , ϵ ) | K l 1 ( L l 1 ) p | τ | 1 + | τ | 2 exp ( M | τ | )
holds for all τ C , provided that ϵ D ( 0 , ϵ 0 ) { 0 } . Moreover, from our hypothesis, we know that
| W q , β 2 + l 3 ( τ , ϵ ) | | | W q , β 2 + l 3 ( τ , ϵ ) | | ( β 2 + l 3 , σ , S d , ρ ) | τ | 1 + | τ | 2 exp ( σ r b ( β 2 + l 3 ) | τ | )
provided that τ S d D ( 0 , ρ ) and ϵ D ( 0 , ϵ 0 ) { 0 } . Furthermore, since r b ( β 2 + l 3 ) 1 , we observe that M σ r b ( β 2 + l 3 ) , and from the definition of F in (84), we deduce the next sequence of bounds
τ 0 τ ω l 1 , p ( τ s , ϵ ) s m 1 W q , β 2 + l 3 ( s , ϵ ) d s ( τ s ) s | τ | 0 | τ | K l 1 ( L l 1 ) p 1 1 + ( | τ | h ) 2 exp ( M ( | τ | h ) ) h m 1 | | W q , β 2 + l 3 ( τ , ϵ ) | | ( β 2 + l 3 , σ , S d , ρ ) × 1 1 + h 2 exp ( σ r b ( β 2 + l 3 ) h ) d h K l 1 ( L l 1 ) p | | W q , β 2 + l 3 ( τ , ϵ ) | | ( β 2 + l 3 , σ , S d , ρ ) × | τ | 0 | τ | 1 1 + ( | τ | h ) 2 1 1 + h 2 exp ( σ r b ( β 2 + l 3 ) ( | τ | h ) ) exp ( σ r b ( β 2 + l 3 ) h ) h m 1 d h K l 1 ( L l 1 ) p | | W q , β 2 + l 3 ( τ , ϵ ) | | ( β 2 + l 3 , σ , S d , ρ ) F | τ | 1 + | τ | 2 | τ | m 1 exp ( σ r b ( β 2 + l 3 ) | τ | ) K l 1 ( L l 1 ) p | | W q , β 2 + l 3 ( τ , ϵ ) | | ( β 2 + l 3 , σ , S d , ρ ) F × | τ | m 1 exp ( σ r b ( β 2 + l 3 ) σ r b ( β + S ) ) | τ | × | τ | 1 + | τ | 2 exp ( σ r b ( β + S ) | τ | )
for all τ S d D ( 0 , ρ ) and ϵ D ( 0 , ϵ 0 ) { 0 } . On the other hand, by construction of r b ( β ) , we observe that
r b ( β + S ) r b ( β 2 + l 3 ) = n = β 2 + l 3 + 1 β + S 1 ( n + 1 ) b β + S ( β 2 + l 3 ) ( β + S + 1 ) b = β 1 + S l 3 ( β + S + 1 ) b
for β 1 = β β 2 . Then, according to the exponential bounds (119), we observe that
| τ | m 1 exp ( σ r b ( β 2 + l 3 ) σ r b ( β + S ) ) | τ | | τ | m 1 exp σ β 1 + S l 3 ( β + S + 1 ) b | τ | sup x 0 x m 1 exp σ β 1 + S l 3 ( β + S + 1 ) b x = m 1 m 1 e m 1 ( β + S + 1 ) b m 1 ( β 1 + S l 3 ) m 1 m 1 m 1 e m 1 ( β + S + 1 ) b m 1
for all τ C . Finally, gathering (123) and (125) gives raise to (115).
For the second inequality of (2), we recall the bounds (73) from Proposition 3,
sup ϵ D ( 0 , ϵ 0 ) | a l 1 , p ( ϵ ) | A l 1 ( B l 1 ) p
and (122) from which the next estimates follow,
a l 1 , p ( ϵ ) τ m 1 W q , β 2 + l 3 ( τ , ϵ ) A l 1 ( B l 1 ) p | τ | m 1 | | W q , β 2 + l 3 ( τ , ϵ ) | | ( β 2 + l 3 , σ , S d , ρ ) × | τ | 1 + | τ | 2 exp ( σ r b ( β 2 + l 3 ) | τ | ) A l 1 ( B l 1 ) p | | W q , β 2 + l 3 ( τ , ϵ ) | | ( β 2 + l 3 , σ , S d , ρ ) | τ | m 1 exp ( σ r b ( β 2 + l 3 ) σ r b ( β + S ) ) | τ | ] × | τ | 1 + | τ | 2 exp ( σ r b ( β + S ) | τ | )
whenever τ S d D ( 0 , ρ ) and ϵ D ( 0 , ϵ 0 ) { 0 } . Calling in again (125) yields the expected bounds (116).
At last, we discuss the third point (3). Owing to our assumption, we can control the functions W p , h 1 and W q , h 2 from above as follows
| W p , h 1 ( τ , ϵ ) | | | W p , h 1 ( τ , ϵ ) | | ( h 1 , σ , S d , ρ ) | τ | 1 + | τ | 2 exp ( σ r b ( h 1 ) | τ | )
and
| W q , h 2 ( τ , ϵ ) | | | W q , h 2 ( τ , ϵ ) | | ( h 2 , σ , S d , ρ ) | τ | 1 + | τ | 2 exp ( σ r b ( h 2 ) | τ | )
for τ S d D ( 0 , ρ ) and ϵ D ( 0 , ϵ 0 ) { 0 } . Observing that r b ( h j ) r b ( β + S ) for j = 1 , 2 , and bearing in mind the definition of the constant F in (84), we deduce estimates for the convolution product
τ 0 τ W p , h 1 ( τ s , ϵ ) W q , h 2 ( s , ϵ ) d s ( τ s ) s | τ | 0 | τ | | | W p , h 1 ( τ , ϵ ) | | ( h 1 , σ , S d , ρ ) 1 1 + ( | τ | h ) 2 exp ( σ r b ( h 1 ) ( | τ | h ) ) × | | W q , h 2 ( τ , ϵ ) | | ( h 2 , σ , S d , ρ ) 1 1 + h 2 exp ( σ r b ( h 2 ) h ) d h F | | W p , h 1 ( τ , ϵ ) | | ( h 1 , σ , S d , ρ ) | | W q , h 2 ( τ , ϵ ) | | ( h 2 , σ , S d , ρ ) × | τ | 1 + | τ | 2 exp ( σ r b ( β + S ) | τ | )
provided that τ S d D ( 0 , ρ ) and ϵ D ( 0 , ϵ 0 ) { 0 } . This leads to (117). □
In the sequel, we define the next sequence of numbers
W n , β = sup ϵ D ( 0 , ϵ 0 ) { 0 } | | W n , β ( τ , ϵ ) | | ( β , σ , S d , ρ )
for all n , β 0 .
According to the recursion (110) together with the constraints (111) and taking into account the estimates of Proposition 4, we obtain the next inequalities for the sequence W 0 , β , β 0 ,
W 0 , β + S β ! l = ( l 1 , l 2 , l 3 ) I , l 1 1 ϵ 0 Δ l l 1 β 1 + β 2 = β ( K l 1 W 0 , β 2 + l 3 β 2 ! F l 2 l 2 e l 2 ( β + S + 1 ) b l 2 + A l 1 W 0 , β 2 + l 3 β 2 ! l 2 l 2 e l 2 ( β + S + 1 ) b l 2 ) × sup ϵ D ( 0 , ϵ 0 ) | d l , β 1 ( ϵ ) | β 1 ! + l = ( l 1 , l 2 , l 3 ) I , l 1 = 0 ϵ 0 Δ l l 1 β 1 + β 2 = β sup ϵ D ( 0 , ϵ 0 ) | d l , β 1 ( ϵ ) | β 1 ! W 0 , β 2 + l 3 β 2 ! l 2 l 2 e l 2 ( β + S + 1 ) b l 2 + β 1 + β 2 = β sup ϵ D ( 0 , ϵ 0 ) | e β 1 ( ϵ ) | β 1 ! × h 1 + h 2 = β 2 F W 0 , h 1 h 1 ! W 0 , h 2 h 2 ! + P 1 , 2 δ 0 , β
for δ 0 , 0 = 1 and δ 0 , β = 0 if β 1 , under the condition that
W 0 , j = sup ϵ D ( 0 , ϵ 0 ) { 0 } | | Q j ( τ ) | | ( j , σ , S d , ρ ) , 0 j S 1
which are, by construction, finite positive numbers. Moreover, owing to the recursion (112) subjected to the conditions (113), with the help of the binomial expansion
( τ + q ϵ α + 1 2 ) l 2 = m 1 + m 2 = l 2 l 2 ! m 1 ! m 2 ! τ m 1 ϵ α + 1 2 m 2 q m 2
for 0 q n , the bounds of Proposition 4 allows us to get inequalities for the whole sequence W n , β , for any n 1 , all β 0 . Specifically,
W n , β + S β ! l = ( l 1 , l 2 , l 3 ) I , l 1 1 ϵ 0 Δ l l 1 β 1 + β 2 = β ( p + q = n [ m 1 + m 2 = l 2 l 2 ! m 1 ! m 2 ! ϵ 0 α + 1 2 m 2 q m 2 × K l 1 ( L l 1 ) p W q , β 2 + l 3 β 2 ! F m 1 m 1 e m 1 ( β + S + 1 ) b m 1 + m 1 + m 2 = l 2 l 2 ! m 1 ! m 2 ! ϵ 0 α + 1 2 m 2 q m 2 × A l 1 ( B l 1 ) p W q , β 2 + l 3 β 2 ! m 1 m 1 e m 1 ( β + S + 1 ) b m 1 ] ) × sup ϵ D ( 0 , ϵ 0 ) | d l , β 1 ( ϵ ) | β 1 ! + l = ( l 1 , l 2 , l 3 ) I , l 1 = 0 ϵ 0 Δ l l 1 β 1 + β 2 = β sup ϵ D ( 0 , ϵ 0 ) | d l , β 1 ( ϵ ) | β 1 ! × [ m 1 + m 2 = l 2 l 2 ! m 1 ! m 2 ! ϵ 0 α + 1 2 m 2 n m 2 × W n , β 2 + l 3 β 2 ! m 1 m 1 e m 1 ( β + S + 1 ) b m 1 ] + β 1 + β 2 = β sup ϵ D ( 0 , ϵ 0 ) | e β 1 ( ϵ ) | β 1 ! × p + q = n h 1 + h 2 = β 2 W p , h 1 h 1 ! W q , h 2 h 2 ! F
under the additional condition that
W n , j = 0 , 0 j S 1 , n 1 .
At this point of the proof, we plan to apply a majorant series method in order to be able to provide upper bounds for the whole sequence W n , β , for any integers n , β 0 . Indeed, let us introduce a sequence of positive numbers W n , β for integers n , β 0 which are submitted to the next recursive relations.
For n = 0 , the sequence W 0 , β , β 0 fulfills
W 0 , β + S β ! = l = ( l 1 , l 2 , l 3 ) I , l 1 1 ϵ 0 Δ l l 1 β 1 + β 2 = β ( K l 1 W 0 , β 2 + l 3 β 2 ! F l 2 l 2 e l 2 ( β + S + 1 ) b l 2 + A l 1 W 0 , β 2 + l 3 β 2 ! l 2 l 2 e l 2 ( β + S + 1 ) b l 2 ) × sup ϵ D ( 0 , ϵ 0 ) | d l , β 1 ( ϵ ) | β 1 ! + l = ( l 1 , l 2 , l 3 ) I , l 1 = 0 ϵ 0 Δ l l 1 β 1 + β 2 = β sup ϵ D ( 0 , ϵ 0 ) | d l , β 1 ( ϵ ) | β 1 ! W 0 , β 2 + l 3 β 2 ! l 2 l 2 e l 2 ( β + S + 1 ) b l 2 + β 1 + β 2 = β sup ϵ D ( 0 , ϵ 0 ) | e β 1 ( ϵ ) | β 1 ! × h 1 + h 2 = β 2 F W 0 , h 1 h 1 ! W 0 , h 2 h 2 ! + P 1 , 2 δ 0 , β
for δ 0 , 0 = 1 and δ 0 , β = 0 if β 1 , strained to
W 0 , j = sup ϵ D ( 0 , ϵ 0 ) { 0 } | | Q j ( τ ) | | ( j , σ , S d , ρ ) , 0 j S 1 .
For any integer n 1 , the sequence W n , β obeys the next rule
W n , β + S β ! = l = ( l 1 , l 2 , l 3 ) I , l 1 1 ϵ 0 Δ l l 1 β 1 + β 2 = β ( p + q = n [ m 1 + m 2 = l 2 l 2 ! m 1 ! m 2 ! ϵ 0 α + 1 2 m 2 q m 2 × K l 1 ( L l 1 ) p W q , β 2 + l 3 β 2 ! F m 1 m 1 e m 1 ( β + S + 1 ) b m 1 + m 1 + m 2 = l 2 l 2 ! m 1 ! m 2 ! ϵ 0 α + 1 2 m 2 q m 2 × A l 1 ( B l 1 ) p W q , β 2 + l 3 β 2 ! m 1 m 1 e m 1 ( β + S + 1 ) b m 1 ] ) × sup ϵ D ( 0 , ϵ 0 ) | d l , β 1 ( ϵ ) | β 1 ! + l = ( l 1 , l 2 , l 3 ) I , l 1 = 0 ϵ 0 Δ l l 1 β 1 + β 2 = β sup ϵ D ( 0 , ϵ 0 ) | d l , β 1 ( ϵ ) | β 1 ! × [ m 1 + m 2 = l 2 l 2 ! m 1 ! m 2 ! ϵ 0 α + 1 2 m 2 n m 2 × W n , β 2 + l 3 β 2 ! m 1 m 1 e m 1 ( β + S + 1 ) b m 1 ] + β 1 + β 2 = β sup ϵ D ( 0 , ϵ 0 ) | e β 1 ( ϵ ) | β 1 ! × p + q = n h 1 + h 2 = β 2 W p , h 1 h 1 ! W q , h 2 h 2 ! F
for the given vanishing data
W n , j = 0 , 0 j S 1 , n 1 .
We can check by induction the important fact that
W n , β W n , β
for any integers n , β 0 . We build up the generating series
W ( X , Z ) = n 0 , β 0 W n , β β ! X n Z β .
Our next intention is to show that these series solve a Cauchy–Kowaleski type PDE, see (145), (146). Indeed, we define the next convergent series
G 1 , l 1 ( X ) = n 0 K l 1 ( L l 1 ) n X n , G 2 , l 1 ( X ) = n 0 A l 1 ( B l 1 ) n X n
and
D l ( Z ) = β 0 sup ϵ D ( 0 , ϵ 0 ) | d l , β ( ϵ ) | β ! Z β , E ( Z ) = β 0 sup ϵ D ( 0 , ϵ 0 ) | e β ( ϵ ) | β ! Z β
for l = ( l 1 , l 2 , l 3 ) I . We now briefly describe the action of basic differential operators on W ( X , Z ) , namely
z l W ( X , Z ) = n 0 , β 0 W n , β + l β ! X n Z β , ( Z Z ) m 1 W ( X , Z ) = n 0 , β 0 β m 1 W n , β β ! X n Z β , ( X X ) m 2 W ( X , Z ) = n 0 , β 0 n m 2 W n , β β ! X n Z β
for integers l , m 1 , m 2 1 and the product by convergent series
G ( X ) = n 0 G n X n , D ( Z ) = β 0 D β β ! Z β
with W which yields the expansions
G ( X ) W ( X , Z ) = n 0 , β 0 p + q = n G p W q , β β ! X n Z β , D ( Z ) W ( X , Z ) = n 0 , β 0 β 1 + β 2 = β D β 1 β 1 ! W n , β 2 β 2 ! X n Z β
together with
W ( X , Z ) W ( X , Z ) = n 0 , β 0 p + q = n h 1 + h 2 = β W p , h 1 h 1 ! W q , h 2 h 2 ! X n Z β .
From the recursions (134) and (136) under the Cauchy data (135) and (137), with the help of the above identities (142), (143) and (144) we obtain that W ( X , Z ) solves the next Cauchy problem
Z S W ( X , Z ) = l = ( l 1 , l 2 , l 3 ) I , l 1 1 ϵ 0 Δ l l 1 [ m 1 + m 2 = l 2 l 2 ! m 1 ! m 2 ! ϵ 0 α + 1 2 m 2 F m 1 m 1 e m 1 × ( Z Z + S + 1 ) b m 1 ( G 1 , l 1 ( X ) × ( X X ) m 2 Z l 3 W ( X , Z ) × D l ( Z ) ) + m 1 + m 2 = l 2 l 2 ! m 1 ! m 2 ! ϵ 0 α + 1 2 m 2 m 1 m 1 e m 1 × ( Z Z + S + 1 ) b m 1 ( G 2 , l 1 ( X ) × ( X X ) m 2 Z l 3 W ( X , Z ) × D l ( Z ) ) ] + l = ( l 1 , l 2 , l 3 ) I , l 1 = 0 ϵ 0 Δ l l 1 ( m 1 + m 2 = l 2 l 2 ! m 1 ! m 2 ! ϵ 0 α + 1 2 m 2 m 1 m 1 e m 1 ( Z Z + S + 1 ) b m 1 ( D l ( Z ) × ( X X ) m 2 Z l 3 W ( X , Z ) ) ) + E ( Z ) F ( W ( X , Z ) ) 2 + P 1 , 2
for given constant Cauchy data
( Z j W ) ( X , 0 ) W 0 , j , 0 j S 1 .
We now need to call upon the classical Cauchy-Kowalevski theorem (see [16], Chapter 1 for a reference), outlined below.
Theorem CK.
Consider a non-linear partial differential equation of the form
(a) 
x β u ( t , x ) = F ( t , x , ( t α 0 x α 1 u ( t , x ) ) ( α 0 , α 1 ) I )
for some integer β 1 , where I = { ( α 0 , α 1 ) N 2 : α 0 + α 1 β , α 1 < β } , and F is analytic in the variables t , x in a neighborhood of the origin in C 2 and polynomial in its other arguments, with Cauchy data
(b) 
( x k u ) ( t , 0 ) = φ k ( t ) , 0 k β 1
for 0 k β 1 , where φ k are analytic functions in a neighborhood of the origin in C . Then, the problem ( a ) , ( b ) has a unique solution u that is analytic in a neighborhood of the origin in C 2 .
Under the hypothesis that (10) hold, we observe that the above theorem applies. Hence, the problem (145), (146) has a unique analytic solution on some polydisc D ( 0 , X 0 ) × D ( 0 , Z 0 ) near 0 in C 2 for some X 0 , Z 0 > 0 . As a result, the constructed formal series W ( X , Z ) is actually convergent on the domain D ( 0 , X 0 ) × D ( 0 , Z 0 ) . This means that one can find constants W > 0 , X 1 , Z 1 > 0 such that
0 W n , β W ( X 1 ) n ( Z 1 ) β β !
for all n , β 0 .
In particular, from the lower bounds (138) and the definition of the sequence W n , β in (129), we deduce the next upper bounds for the set of functions W n , β ( τ , ϵ ) , n , β 0 that solve the recursive relations (110), (112) for Cauchy data (111), (113).
Proposition 5.
One can single out constants W , X 1 , Z 1 > 0 with
| W n , β ( τ , ϵ ) | W ( X 1 ) n ( Z 1 ) β β ! | τ | 1 + | τ | 2 exp ( σ r b ( β ) | τ | )
whenever ϵ D ( 0 , ϵ 0 ) { 0 } , for all τ S d D ( 0 , ρ ) , for a direction d (that relies on ϵ) constructed as in Proposition 1 and a small radius ρ chosen in a way that the domain S d D ( 0 , ρ ) avoids the set of the roots R 2 of the polynomial P 2 ( τ ) .
As a consequence of the latter proposition, the formal power series z W n ( τ , z , ϵ ) defined in (102) turns out to be be an analytic function on the disc D ( 0 , 1 / ( 2 Z 1 ) ) . More precisely, for all ϵ D ( 0 , ϵ 0 ) { 0 } , all integers n 0 , the map ( τ , z ) W n ( τ , z , ϵ ) is holomorphic on the product ( S d D ( 0 , ρ ) ) × D ( 0 , 1 / ( 2 Z 1 ) ) and suffers the next bounds
| W n ( τ , z , ϵ ) | 2 W ( X 1 ) n | τ | 1 + | τ | 2 exp ( σ ζ ( b ) | τ | )
where ζ ( b ) = n 0 1 / ( n + 1 ) b , provided that τ S d D ( 0 , ρ ) , z D ( 0 , 1 / ( 2 Z 1 ) ) . Furthermore, for n = 0 , W 0 ( τ , z , ϵ ) solves (100) and for n 1 , W n ( τ , z , ϵ ) fulfills (101) on the above domain.

4. Construction of Inner Analytic Solutions to the Main Problem and Their Parametric Asymptotic Expansions

We build up a set of genuine solutions to our initial problems (11) and (23) subjected to (12). We label these solutions as inner solutions in the terminology of the so-called boundary layer expansions since their domain of holomorphy in time turns out to depend on the parameter ϵ and comes close to the origin when ϵ tends to 0. This family of solutions is based on the following definition of so-called good covering in C .
Definition 2.
Let ι 2 be an integer. We consider a finite set E ̲ = { E p } 0 p ι 1 where E p stand for open sectors with vertex at 0 such that E p D ( 0 , ϵ 0 ) which fulfills the next three assumptions:
(i) 
E p E p + 1 for all 0 p ι 1 (with the convention that E ι = E 0 ).
(ii) 
E p 1 E p 2 E p 3 = for any distinct integers 0 p j ι 1 , j = 1 , 2 , 3 .
(iii) 
The union of all the sectors E p covers a punctured disc centered at 0 in C .
Then, the set E ̲ is called a good covering in C .
In the forthcoming definition, we describe the notion of admissible set of sectors relatively to a good covering.
Definition 3.
We consider a good covering E ̲ = { E p } 0 p ι 1 in C and a set of unbounded sectors S d p , 0 p ι 1 with bisecting direction d p R that fulfill the next two properties:
(1) The next inclusion
S d p ϵ E p S d
holds.
(2) There exists Δ > 0 such that for all ϵ E p , one can choose a direction γ p R (that may depend on ϵ) with L γ p = R + exp ( 1 γ p ) S d p { 0 } for which
cos ( γ p arg ( ϵ α + 1 2 ) + π ) < Δ
holds.
In that case, the family of sectors S = { S d p } 0 p ι 1 is called admissible relatively to E ̲ .
We now discuss the feasibility of such a construction. Indeed, for a given sector E p , we construct the sector
S d p = ϵ E p L arg ( ϵ ( α + 1 ) / 2 ) + Δ p
where
L arg ( ϵ ( α + 1 ) / 2 ) + Δ p = ( 0 , + ) exp ( 1 ( arg ( ϵ ( α + 1 ) / 2 ) + Δ p ) )
for some positive number Δ p > 0 (which is taken less than π / 2 and relies on p) and for each ϵ E p , we choose a sector S arg ( ϵ ( α + 1 ) / 2 ) + Δ p with bisecting direction arg ( ϵ ( α + 1 ) / 2 ) + Δ p and with large enough opening such that
S d p S arg ( ϵ ( α + 1 ) / 2 ) + Δ p
Furthermore, we adjust Δ p > 0 in a way that the union
ϵ E p S arg ( ϵ ( α + 1 ) / 2 ) + Δ p
avoids the set of the roots R 2 of the polynomial P 2 ( τ ) . Such an arrangement is achievable if the opening of E p is taken small enough. Therefore the first property (1) follows.
For the second point (2), let ϵ E p and set
γ p = arg ( ϵ ( α + 1 ) / 2 ) + Δ p .
Observe in particular that L γ p = R + e 1 γ p S d p { 0 } . By construction, we get that
cos ( γ p arg ( ϵ ( α + 1 ) / 2 ) + π ) = cos ( Δ p + π ) < Δ
for some Δ > 0 .
In the first main statement of the work, we construct a family of actual holomorphic solutions to our main problems (11) and (23) under the Cauchy data (12). These solutions are defined on the sectors of a good covering E ̲ = { E p } 0 p ι 1 in C w.r.t the perturbation parameter ϵ . We control the difference between neighboring solutions on the intersection of sectors E p E p + 1 where exponentially flat estimates are witnessed.
Theorem 1.
Assume that the requirement (10) on the shape of Equation (11) holds. We fix a good covering E ̲ = { E p } 0 p ι 1 in C together with an admissible set of sectors S = { S d p } 0 p ι 1 relatively to E ̲ .
Then, for all ϵ E p , one can exhibit a solution ( t , z ) u p ( t , z , ϵ ) of the main problems (11) and (23) submitted to the Cauchy data (12) that remains bounded holomorphic on a domain T ϵ × D ( 0 , r ) provided that r , ϵ 0 > 0 are taken small enough. This solution is represented as an exponential transseries expansion which contains infinitely many special Laplace transforms
u p ( t , z , ϵ ) = n 0 L γ p W n ( τ , z , ϵ ) exp ( τ a ( ϵ t , ϵ ) ) d τ τ exp n ϵ α + 1 2 a ( ϵ t , ϵ )
where W n ( τ , z , ϵ ) is the sequence of functions disclosed at the end of Section 3, for ϵ E p .
Furthermore, the functions
( x , z , ϵ ) u p ( ϵ α 1 2 x , z , ϵ )
are bounded holomorphic on the domain χ 1 × D ( 0 , r ) × E p , for 0 p ι 1 . These functions suffer the next bounds: There exist constants K p , M p > 0 such that
sup x χ 1 , z D ( 0 , r ) u p + 1 ( ϵ α 1 2 x , z , ϵ ) u p ( ϵ α 1 2 x , z , ϵ ) K p exp M p / | ϵ | α + 1 2
for all ϵ E p E p + 1 , for 0 p ι 1 (where by convention u ι = u 0 ).
Proof. 
In view of the feature (150) for the admissible set S , we remind the reader the construction we have reached at the end of Section 3. Specifically, we have singled out a sequence of functions W n ( τ , z , ϵ ) , n 0 satisfying the following property:
Let 0 p ι 1 and n 0 an integer, for all ϵ E p , the map ( τ , z ) W n ( τ , z , ϵ ) is holomorphic on the product ( S d p D ( 0 , ρ ) ) × D ( 0 , r ) , provided that 0 < r 1 / ( 2 Z 1 ) and is subjected to the bounds (149) whenever τ S d p D ( 0 , ρ ) and z D ( 0 , r ) .
For each 0 p ι 1 , we define the function
U p ( T , z , ϵ ) = n 0 L γ p W n ( τ , z , ϵ ) exp ( τ a ( T , ϵ ) ) d τ τ exp n ϵ α + 1 2 a ( T , ϵ )
where the integration halfline L γ p is chosen accordingly to Definition 3. We now show that when ϵ E p , the map ( T , z ) U p ( T , z , ϵ ) is well defined on the domain ϵ T ϵ × D ( 0 , r ) whenever the outer radius r 2 > 0 of χ 0 in (26) is taken small enough. Indeed, owing to the factorization (28), the next bounds hold
| U p ( T , z , ϵ ) | n 0 0 + 2 W ( X 1 ) n 1 1 + s 2 exp ( σ ζ ( b ) s ) × exp s 2 | ϵ | α + 1 2 log | x 1 x + 1 | | 1 + a in ( x ) | × cos γ p arg ( ϵ α + 1 2 ) + π + arg ( 1 + a in ( x ) ) d s × exp n 2 log | x 1 x + 1 | | 1 + a in ( x ) | × cos π + arg ( 1 + a in ( x ) )
for ϵ E p and ( T , z ) ϵ T ϵ × D ( 0 , r ) .
Bearing in mind (29), the lower bounds
| 1 + a in ( x ) | 1 δ
hold for x χ 1 , whenever δ > 0 is small enough and from (30), we deduce that
log | x 1 x + 1 | > log 2 r 2 r 2
provided that r 2 > 0 is small enough, when x χ 1 . Moreover, owing to the constraint (151), we deduce that
cos γ p arg ( ϵ α + 1 2 ) + π + arg ( 1 + a in ( x ) ) < Δ
for all x χ 1 whenever r 2 > 0 is taken small enough. Similarly, we can get a constant Δ 1 > 0 for which
cos π + arg ( 1 + a in ( x ) ) < Δ 1
when x belongs to χ 1 and r 2 > 0 is chosen close to 0.
Now, we choose r 2 > 0 in the vicinity of 0 in a way that both inequalities
0 < X 1 exp 1 2 log 2 r 2 r 2 ( 1 δ ) Δ 1 1 / 2
and
σ ζ ( b ) 1 2 ϵ 0 α + 1 2 log 2 r 2 r 2 ( 1 δ ) Δ 1 / 2
hold. Applying the lower bounds (155), (156) together with (157), (158) to (154) under the additional restrictions (159), (160), we deduce that
| U p ( T , z , ϵ ) | 2 W 0 + e s / 2 d s × n 0 ( 1 / 2 ) n = 8 W
for ϵ E p and ( T , z ) ϵ T ϵ × D ( 0 , r ) . Furthermore, from the bounds given above, for all ϵ E p , the series defining U p ( T , z , ϵ ) converge uniformly on the domain ϵ T ϵ × D ( 0 , r ) . Therefore, the map ( T , z ) U p ( T , z , ϵ ) is holomorphic on the domain ϵ T ϵ × D ( 0 , r ) . Since the function W 0 ( τ , z , ϵ ) solves the convolution Equation (100) and W n ( τ , z , ϵ ) satisfies (101) for all n 1 , the sequence of formal computations (95)–(99) are now justified and once performed they show that for all ϵ E p , the map ( T , z ) U p ( T , z , ϵ ) solves the Cauchy problem (24), (25) on the domain ϵ T ϵ × D ( 0 , r ) .
At last, for 0 p ι 1 , we set forth
u p ( t , z , ϵ ) = U p ( ϵ t , z , ϵ ) = n 0 L γ p W n ( τ , z , ϵ ) exp ( τ a ( ϵ t , ϵ ) ) d τ τ exp n ϵ α + 1 2 a ( ϵ t , ϵ ) .
According to the construction above, for each 0 p ι 1 , the function ( t , z ) u p ( t , z , ϵ ) is bounded, holomorphic and solves the main Cauchy problem (11), (12) (and hence the singularly perturbed Cauchy problem (23), (12)) on the domain T ϵ × D ( 0 , r ) . Furthermore, the maps
( x , z , ϵ ) u p ( ϵ α 1 2 x , z , ϵ )
represent bounded holomorphic functions on the domain χ 1 × D ( 0 , r ) × E p , for all 0 p ι 1 .
In the second part of the proof, we discuss the bounds (153). Let 0 p ι 1 . For all integers n 0 , the partial maps
τ W n ( τ , z , ϵ ) exp ( τ a ( ϵ t , ϵ ) ) / τ
are bounded and holomorphic on the disc D ( 0 , ρ ) , provided that ϵ E p E p + 1 and z D ( 0 , r ) . By Cauchy’s theorem, its integral must vanish along the next oriented path depicted as the union of
(a)
the segment joining 0 and ( ρ / 2 ) exp ( 1 γ p + 1 ) ,
(b)
the arc of circle with radius ρ / 2 which relates the two points ( ρ / 2 ) exp ( 1 γ p + 1 ) and ( ρ / 2 ) exp ( 1 γ p ) ,
(c)
the segment which attaches ( ρ / 2 ) exp ( 1 γ p ) and 0.
As a result, we can split the difference u p + 1 u p into a sum of three exponential transseries. Specifically,
u p + 1 ( ϵ α 1 2 x , z , ϵ ) u p ( ϵ α 1 2 x , z , ϵ ) = n 0 L ρ / 2 , γ p + 1 W n ( τ , z , ϵ ) exp ( τ a ( ϵ α + 1 2 x , ϵ ) ) d τ τ exp n ϵ α + 1 2 a ( ϵ α + 1 2 x , ϵ ) n 0 L ρ / 2 , γ p W n ( τ , z , ϵ ) exp ( τ a ( ϵ α + 1 2 x , ϵ ) ) d τ τ exp n ϵ α + 1 2 a ( ϵ α + 1 2 x , ϵ ) + n 0 C ρ / 2 , γ p , γ p + 1 W n ( τ , z , ϵ ) exp ( τ a ( ϵ α + 1 2 x , ϵ ) ) d τ τ exp n ϵ α + 1 2 a ( ϵ α + 1 2 x , ϵ )
where
L ρ / 2 , γ j = [ ρ / 2 , + ) exp ( 1 γ j ) , j = p , p + 1
are halflines in directions γ j at the distance ρ / 2 from the origin and C ρ / 2 , γ p , γ p + 1 represents an arc of circle with radius ρ / 2 that joins the above two lines.
We evaluate the first sum
I 1 = n 0 L ρ / 2 , γ p + 1 W n ( τ , z , ϵ ) exp ( τ a ( ϵ α + 1 2 x , ϵ ) ) d τ τ exp n ϵ α + 1 2 a ( ϵ α + 1 2 x , ϵ ) .
Bearing in mind the bounds (149) and the factorization (28), we get that
I 1 n 0 ρ / 2 + 2 W ( X 1 ) n 1 1 + s 2 exp ( σ ζ ( b ) s ) × exp s 2 | ϵ | α + 1 2 log | x 1 x + 1 | | 1 + a in ( x ) | × cos γ p + 1 arg ( ϵ α + 1 2 ) + π + arg ( 1 + a in ( x ) ) d s × exp n 2 log | x 1 x + 1 | | 1 + a in ( x ) | × cos π + arg ( 1 + a in ( x ) )
for ϵ E p E p + 1 , x χ 1 and z D ( 0 , r ) . The lower bounds (155), (156) and angles estimates (157) (for γ p replaced by γ p + 1 ), (158) yield that
I 1 n 0 ρ / 2 + 2 W ( X 1 ) n exp ( σ ζ ( b ) s ) × exp s 2 | ϵ | α + 1 2 log 2 r 2 r 2 ( 1 δ ) Δ d s × exp n 2 log 2 r 2 r 2 ( 1 δ ) Δ 1
for ϵ E p E p + 1 , x χ 1 , z D ( 0 , r ) . We select a positive real number δ 1 > 0 such that
σ ζ ( b ) ϵ 0 α + 1 2 1 2 log 2 r 2 r 2 ( 1 δ ) Δ δ 1
holds. Notice that such a δ 1 > 0 is ensured to exist if r 2 > 0 is taken close enough to 0. On the other hand, we take for granted that (159) is verified. Then, we obtain
I 1 2 W n 0 ( 1 / 2 ) n × ρ / 2 + exp δ 1 | ϵ | α + 1 2 s d s = 4 W | ϵ | α + 1 2 δ 1 exp δ 1 | ϵ | α + 1 2 ρ 2
provided that ϵ E p E p + 1 , x χ 1 , z D ( 0 , r ) .
In a similar manner, we can reach upper bounds for the second piece of the decomposition (161)
I 2 = n 0 L ρ / 2 , γ p W n ( τ , z , ϵ ) exp ( τ a ( ϵ α + 1 2 x , ϵ ) ) d τ τ exp n ϵ α + 1 2 a ( ϵ α + 1 2 x , ϵ ) .
Specifically,
I 2 4 W | ϵ | α + 1 2 δ 1 exp δ 1 | ϵ | α + 1 2 ρ 2
for all ϵ E p E p + 1 , x χ 1 , z D ( 0 , r ) and δ 1 > 0 chosen as above in (164).
For our last task, we handle the transseries integrated along an arc of circle
I 3 = n 0 C ρ / 2 , γ p , γ p + 1 W n ( τ , z , ϵ ) exp ( τ a ( ϵ α + 1 2 x , ϵ ) ) d τ τ exp n ϵ α + 1 2 a ( ϵ α + 1 2 x , ϵ ) .
Again the bounds (149) and the factorization (28) give rise to
I 3 n 0 γ p γ p + 1 2 W ( X 1 ) n ρ / 2 1 + ( ρ / 2 ) 2 exp ( σ ζ ( b ) ρ / 2 ) × exp ρ / 2 2 | ϵ | α + 1 2 log | x 1 x + 1 | | 1 + a in ( x ) | cos θ arg ( ϵ α + 1 2 ) + π + arg ( 1 + a in ( x ) ) d θ × exp n 2 log | x 1 x + 1 | | 1 + a in ( x ) | cos π + arg ( 1 + a in ( x ) ) .
Since the estimates (157) hold true for both angles γ p and γ p + 1 , one checks that
cos θ arg ( ϵ α + 1 2 ) + π + arg ( 1 + a in ( x ) ) < Δ
is valid for all θ ( γ p , γ p + 1 ) if γ p < γ p + 1 or θ ( γ p + 1 , γ p ) if γ p + 1 > γ p . Furthermore, taking into account the lower bounds (155), (156) together with the angle inequality (158), we come out with
I 3 n 0 | γ p γ p + 1 | 2 W ( X 1 ) n ρ / 2 1 + ( ρ / 2 ) 2 exp ( σ ζ ( b ) ρ / 2 ) × exp ρ / 2 2 | ϵ | α + 1 2 log 2 r 2 r 2 ( 1 δ ) Δ × exp n 2 log 2 r 2 r 2 ( 1 δ ) Δ 1
provided that ϵ E p E p + 1 , x χ 1 , z D ( 0 , r ) . We select δ 1 > 0 as in (164) and we assume that (159) to be valid. Then,
I 3 2 W | γ p γ p + 1 | ρ / 2 1 + ( ρ / 2 ) 2 exp δ 1 ρ 2 | ϵ | α + 1 2 n 0 ( 1 / 2 ) n = 4 W | γ p γ p + 1 | ρ / 2 1 + ( ρ / 2 ) 2 exp δ 1 ρ 2 | ϵ | α + 1 2
whenever ϵ E p E p + 1 , x χ 1 , z D ( 0 , r ) .
In conclusion, the collection of bounds (165), (166), (168) applied to the decomposition (161) give rise to the expected exponentially flat estimates (153). □
In the second central result of the paper, we show that the holomorphic inner solutions to (11) and (23) under the Cauchy data (12) obtained in Theorem 1 share a common asymptotic expansion relatively to ϵ on the sectors E p that turns out to be of Gevrey type.
Theorem 2.
Assume that the foregoing constraints listed in Theorem 1 hold. Let us denote O b ( χ 1 × D ( 0 , r ) ) the Banach space of C - valued bounded holomorphic functions on χ 1 × D ( 0 , r ) endowed with the sup norm.
Then, for all 0 p ι 1 , the holomorphic and bounded functions ϵ ( ( x , z ) u p ( ϵ α 1 2 x , z , ϵ ) ) built up in Theorem 1 and viewed as maps from E p into O b ( χ 1 × D ( 0 , r ) ) , admit a formal power series
I ^ ( ϵ ) = k 0 I k ϵ k O b ( χ 1 × D ( 0 , r ) ) [ [ ϵ ] ]
as Gevrey asymptotic expansion of order 2 α + 1 . This means that for all 0 p ι 1 , one can find constants A p , B p > 0 such that
sup x χ 1 , z D ( 0 , r ) u p ( ϵ α 1 2 x , z , ϵ ) k = 0 n 1 I k ϵ k A p ( B p ) n Γ ( 1 + 2 α + 1 n ) | ϵ | n
for all n 1 , whenever ϵ E p .
Proof. 
The proof leans on a cohomological criterion for the existence of Gevrey asymptotic expansions of order 1 / k , for real numbers k > 1 / 2 , for suitable families of sectorial holomorphic functions known as Ramis–Sibuya theorem in the literature, see [17], p.121 or [18] Lemma XI-2-6. Here we need a Banach valued version of this result that can be stated as follows.
Theorem Ramis–Sibuya. 
We set ( F , | | . | | F ) as a Banach space over C and consider a good covering { E p } 0 p ι 1 in C . For all 0 p ι 1 , G p stands for a holomorphic function from E p into the Banach space ( F , | | . | | F ) and let the cocycle Θ p ( ϵ ) = G p + 1 ( ϵ ) G p ( ϵ ) be a holomorphic function from the sector Z p = E p + 1 E p into E (under the convention that E ι = E 0 and G ι = G 0 ). We ask for the following requirements.
(1) The functions G p ( ϵ ) are bounded on E p , for all 0 p ι 1 .
(2) The functions Θ p ( ϵ ) suffer exponential flatness of order k on Z p , for all 0 p ι 1 . Specifically, there exist constants C p , A p > 0 such that
| | Θ p ( ϵ ) | | F C p e A p / | ϵ | k
for all ϵ Z p , all 0 p ι 1 .
Then, for all 0 p ι 1 , the functions G p ( ϵ ) share a common formal power series I ^ ( ϵ ) = k 0 I k ϵ k where the coefficients I k belong to F , as Gevrey asymptotic expansion of order 1 / k on E p . In other words, constants A p , B p > 0 can be selected with
| | G p ( ϵ ) k = 0 n 1 I k ϵ k | | F A p ( B p ) n Γ ( 1 + n k ) | ϵ | n
for all n 1 , provided that ϵ E p .
We apply the above theorem to the set of functions
G p ( ϵ ) : = ( x , z ) u p ( ϵ α 1 2 x , z , ϵ )
for 0 p ι 1 , which represent holomorphic and bounded functions from E p into the Banach space F = O b ( χ 1 × D ( 0 , r ) ) equipped with the sup norm over χ 1 × D ( 0 , r ) . Furthermore, the bounds (153) allow the cocycle Θ p ( ϵ ) = G p + 1 ( ϵ ) G p ( ϵ ) to fulfill the constraint (2) overhead. As a result, we deduce the existence of a formal power series I ^ ( ϵ ) that match the statement of Theorem 2. □

5. Conclusions and Perspectives

In this work we have considered Cauchy problems which are conjointly singularly perturbed and possess confluent fuchsian singularities relying on a single perturbation parameter. We constructed genuine solutions expressed as exponential transseries expansions which are shown to appear naturally from the polynomial structure of the coefficients in the equations involved.
It turns out that the nature of these special solutions and the extraction of their parametric asymptotic behavior impose rather strong constraints on the shape of the equations under study in this work, namely the reduction to an equation of Kowalevski type displayed in (11). Concerning that point we may provide some explanatory comments that may help to investigate future lines of research in this topic. Indeed, departing from the singularly perturbed Equation (23) under less restrictive conditions on the differential operator P would lead to corresponding sets of convolution equations similar to (101) that ought to be solved relatively to τ (and ϵ on a good covering E ̲ ) on a domain where the expression P 2 ( τ + n ϵ ( α + 1 ) / 2 ) is not equal to zero. Here P 2 is the polynomial introduced in Section 2. However, for τ = 0 , the quantity P 2 ( n ϵ ( α + 1 ) / 2 ) must vanish for a least some integer n 1 and some value of the parameter ϵ near 0. Consequently, the solution W n ( τ , z , ϵ ) to the convolution equation may not be defined at τ = 0 and the solutions to (23) would not be constructible by means of Laplace transforms with special kernel. Hence, relaxing those constraints would need a new framework and novel ideas. It is worthwhile noting that strong restrictions on the shape of the coefficients are also asked in related works on confluence problems, see the references in our previous contribution [1].
At last, we expect that our approach can be adapted to other related problems, for instance in the context of q - difference or difference equations.

Funding

This research was partially funded by the University of Lille.

Conflicts of Interest

The author declares no conflict of interest.

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