Home Schauder estimates on bounded domains for KFP operators with coefficients measurable in time and Hölder continuous in space
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Schauder estimates on bounded domains for KFP operators with coefficients measurable in time and Hölder continuous in space

  • Stefano Biagi and Marco Bramanti EMAIL logo
Published/Copyright: September 19, 2024

Abstract

We consider degenerate Kolmogorov-Fokker-Planck operators

u = i , j = 1 q a i j ( x , t ) u x i x j + k , j = 1 N b j k x k u x j u t ,

such that the corresponding model operator having constant a i j is hypoelliptic, translation invariant w.r.t. a Lie group operation in R N + 1 and 2-homogeneous w.r.t. a family of nonisotropic dilations. We assume that the a i j ’s are globally bounded and Hölder continuous in x (w.r.t. some intrinsic distance induced by ); the matrix { a i j } i , j = 1 q is symmetric and uniformly positive on R q . We prove “partial Schauder a priori estimates” on a bounded open set Ω R N + 1 , of the kind

i , j = 1 q ( [ u x i x j ] , α , 2 x + [ u x i x j ] , 2 ) c { [ u ] , α , 2 x + [ u ] , 2 + sup Ω u }

for suitable functions u , where

[ u ] , α , 2 x = sup ( x , t ) ( y , t ) Ω d ( x , t ) , ( y , t ) 2 + α u ( x , t ) u ( y , t ) x y α [ u ] , 2 = sup ξ Ω d ξ 2 u ( ξ ) .

Here is a homogeneous norm in R N , while d ξ = dist ( ξ , Ω ) and d ξ , η = min { d ξ , d η } . We also prove that the derivatives u x i x j are locally Hölder continuous in space and time.

MSC 2010: 35K65; 35K70; 35B45; 35A08

We wish to dedicate this note to prof. Ermanno Lanconelli on the occasion of his 80th birthday. We warmly thank Ermanno for his precious teachings through the years, for his esteem and his friendship.

1 Introduction and main results

In his 1936 seminal paper on the Theory of gases [12], Kolmogorov introduced the parabolic operator (nowadays called the Kolmogorov operator)

K u = Δ v u + v , x u u t  with  ( v , x ) R n × R n  and  t R .

This operator K enjoys the following interesting features:

  1. K is ultra-parabolic, since the diffusive term Δ x is missing;

  2. K possesses an explicit, global fundamental solution p , found by Kolmogorov himself: more precisely, introducing the notation

    X = ( v , x ) , Y = ( w , y ) , Z = ( ω , ξ ) ,

    for the points of R 2 n , we have

    p t , s ( X , Y ) = p ˆ t s ( v w , x ( s t ) w y ) , where p ˆ τ ( Z ) = c n τ 2 n exp 1 τ ω 2 3 τ ω , ξ + τ ω + 3 τ 2 ξ + τ ω 2 1 { τ > 0 } .

    In particular, since p ˆ is clearly smooth outside the origin of R 2 n × R , the operator K is C -hypoelliptic (despite its degeneracy).

  3. K can be written as a sum of squares (of smooth vector fields) plus a drift:

    K u = i = 1 n X i 2 u + Y u ,

    where X i = v i (with 1 i n ) and Y u = v , x u u t .

In view of properties (i)–(iii), the operator K is presented by Hörmander as the main inspiration for his study in his 1967 celebrated paper [10]; in fact, we see that K is a degenerate and hypoelliptic sum of squares plus a drift, but it does not satisfy the sufficient conditions for hypoellipticity established by Hörmander himself in his previous work [9]. This example led Hörmander to formulate the so-called (Hörmander) Rank Condition for hypoellipticity.

Inspired by [10], at the beginning of the 90s, a large class of degenerate and hypoelliptic operators (of which the Kolmogorov operator K is the main prototype) has been deeply studied by Lanconelli and Polidoro [13]: more precisely, they considered parabolic operators of the form

(1.1) u = i , j = 1 q a i j u x i x j + B x , u u t i , j = 1 q a i j u x i x j + Y u on  R N + 1 = R x N × R t ,

which satisfy the following structural assumptions.

  1. Assumption on the principal part of :

    1. 1 q N ;

    2. the constant matrix A 0 = ( a i j ) i , j = 1 q is symmetric and positive definite.

  2. Assumption on the drift Y:

    1. the N × N matrix B takes the block form

      (1.2) B = B 1 O B 2 O O B k ,

      where the entries of the blocks denoted by are arbitrary, while every block B j is an m j × m j 1 matrix of rank m j (for j = 1 , 2 , , k ), with

      m 0 = q , m 0 m 1 m k and m 0 + m 1 + + m k = N .

These operators are usually called Kolmogorov-Fokker-Planck (KFP) operators. We explicitly note that the Kolmogorov operator K actually fits into this class, since it can be obtained by choosing

N = 2 n ( with  n 1 ) q = m 1 = n A = Id m 0 B = O n O n Id n O n .

Under the above assumptions, Lanconelli and Polidoro [13] proved that any KFP operator satisfies the Hörmander Rank Condition, so that is C -hypoelliptic; moreover, it possesses a rich underlying geometric structure:

  1. is left-invariant on the non-commutative Lie group G = ( R N + 1 , ) , where the composition law is defined as follows:

    ( y , s ) ( x , t ) = ( x + E ( t s ) y , t + s )

    and E ( t ) = e t B . This means that, defining τ y , s ( x , t ) = ( y , s ) ( x , t ) , for every u C ( R N + 1 ) and every ( y , s ) R N + 1 , we have

    ( u τ y , s ) = ( u ) τ y , s .

  2. If, in addition, the blocks in the matrix B vanish, is also homogeneous of degree 2 w.r.t. the non-isotropic dilations (automorphisms of G )

    (1.3) D ( λ ) ( x , t ) ( D 0 ( λ ) ( x ) , λ 2 t ) = ( λ q 1 x 1 , , λ q N x N , λ 2 t ) ,

    where the N -tuple ( q 1 , , q N ) is given by

    ( q 1 , , q N ) = ( 1 , , 1 m 0 , 3 , , 3 m 1 , , 2 k + 1 , , 2 k + 1 m k ) .

    This means that, for every u C ( R N + 1 ) and every λ > 0 , we have

    ( u D λ ) = λ 2 ( u ) D λ .

After [13], more general families of (degenerate) KFP operators have been deeply studied; in particular, a great attention has been gained by KFP operators with variable coefficients a i j ( x , t ) , which play an important role in the theory of Stochastic Differential Equations (e.g., [2, Section 2.1]), as well as in collisional kinetic theory (e.g., [19,21]). In this perspective, recent research studies in the field of Stochastic Differential Equations suggest the importance of developing a theory allowing the coefficients a i j to be rough in t (say, L ), and more regular only w.r.t. the space variables.

Motivated by this fact, in [1], we studied a suitable class of KFP operators (1.1) on R N + 1 with variable coefficients a i j ( x , t ) , which are L in t and Hölder continuous in x (in a sense which will be made precise in a moment). For these operators, we proved partial Schauder estimates on unbounded strips S T = R N × ( , T ) , i.e., a control of the supremum in t of the Hölder norms in space of u x i x j , assuming the finiteness of the analogous quantity for the coefficients a i j and the right-hand side of the equation. We also proved a local Hölder continuity estimate in the joint variables ( x , t ) for the derivatives u x i x j , without assuming any continuity in t on the coefficients nor on u .

On the other hand, since the drift Y = B x , t has unbounded coefficients, requiring the global boundedness of u (which is encoded in the boundedness assumption of the full Hölder norm of u ) seems a quite demanding assumption. Therefore, it can be interesting also to establish a version of the aforementioned a priori estimates on bounded domains of R N + 1 , in the spirit of the classical interior Hölder estimates in cylinders. However, these local estimates cannot be easily deduced directly by the global bounds proved in [1], but require some nontrivial work, which is exactly the content of the present study. We will prove partial Schauder estimates for u x i x j (with 1 i , j q ) and for Y u on a bounded domain of R N + 1 (Theorem 1.6), as well as a Hölder continuity estimate in ( x , t ) of u x i x j (Theorem 1.7).

Comparison with the existing literature. Schauder estimates for KFP operators have been proved first by Manfredini [18] and later, under more general assumptions on B , by Di Francesco and Polidoro [5], on bounded domains, assuming the coefficients a i j Hölder continuous (in ( x , t ) ) with respect to the intrinsic distance induced in R N + 1 by the vector fields x 1 , x q , Y . For related issues about Schauder estimates for KFP operators, we point out also the research by Lunardi [17], Priola [20], Imbert and Mouhot [11], Henderson and Snelson [8], Lorenzi [14], and references therein.

Partial Schauder estimates for degenerate KFP operators, of the kind dealt in our previous study [1], have been proved also by Chaudru de Raynal et al. [4], with different techniques and without obtaining the Hölder control in time of second-order derivatives. Concerning the same class of KFP operators with coefficients Hölder continuous in space and L in time, we quote the research by Lucertini et al. [15], dealing with the construction of a fundamental solution for these operators, with consequent results about the Cauchy problem, and the research by Henderson and Wang [7], containing partial Schauder estimates for a special class of KFP operators, with applications to the Landau equation. The results in [15] and [7] are independent from and do not contain our results. We also point out the preprint by Dong and Yastrzhembskiy [6] dealing with kinetic KFP operators, and the more recent preprint by Lucertini et al. [16], where the authors prove optimal global Schauder estimates, which improve some of the results in [1].

Main results. We now turn to give the precise statements of our main results; to this end we first need to introduce the appropriate metric and functional setting.

We begin by recalling that, if 0 is a KFP operator as in (1.1) with constant coefficients and with vanishing blocks in the “drift” matrix B , see (1.2), Lanconelli and Polidoro [13] proved the following facts:

  1. 0 is C -hypoelliptic;

  2. 0 is left-invariant w.r.t. the composition law

    ( y , s ) ( x , t ) = ( x + E ( t s ) y , t + s ) ;

  3. 0 is 2-homogeneous w.r.t. the dilations

    D ( λ ) ( x , t ) ( D 0 ( λ ) ( x ) , λ 2 t ) = ( λ q 1 x 1 , , λ q N x N , λ 2 t ) .

Since we aim to study KFP operators with variable coefficients a i j ( x , t ) such that the corresponding model operator 0 with constant a i j satisfies (a)–(c), it is convenient to endow R N + 1 with a structure of homogeneous quasi-metric space adapted to and to { D λ } λ > 0 .

First of all, we consider in R N + 1 , the following D λ -homogeneous norm:

ρ ( ξ ) = i = 1 N x i ( 2 q N ) ! q i + t q N ! 1 ( 2 q N ) ! ( with  ξ = ( x , t ) R N + 1 ) ,

and we also set

x = ρ ( x , 0 ) = i = 1 N x i ( 2 q N ) ! q i 1 ( 2 q N ) ! .

Accordingly, we define a translation-invariant quasi-distance as follows:

d ( ξ , η ) = ρ ( η 1 ξ ) ( with  ξ = ( x , t ) , η = ( y , s ) R N + 1 ) .

It is easy to see that ρ and d satisfy the following properties:

  1. ρ ( ξ ) 0 for every ξ R N + 1 , and ρ ( ξ ) = 0 ξ = 0 ;

  2. ρ ( D ( λ ) ξ ) = λ ρ ( ξ ) for every ξ R N + 1 , λ > 0 ;

  3. d ( ξ , η ) 0 for every ξ , η R N + 1 , and d ( ξ , η ) = 0 ξ = η ;

  4. there exists κ > 0 such that, for every ξ , η , ζ R N + 1 , we have

    d ( ξ , η ) κ ( d ( ξ , ζ ) + d ( η , ζ ) ) and d ( ξ , η ) κ d ( η , ξ ) ;

  5. d ( ξ , η ) = d ( η 1 ξ , 0 ) for every ξ , η R N + 1 .

Moreover, by the explicit expression of , we have

(1.4) d ( ( x , t ) , ( y , t ) ) = ρ ( ( y , t ) 1 ( x , t ) ) = x y .

It should be noted that ρ ( ) and are not the ones defined in [1]; however, they are globally equivalent to them, and have the advantage of being smooth outside the origin.

Remark 1.1

Another way to construct a geometric setting adapted to the composition law and to the dilations D λ is to consider the so-called Carnot-Carathéodory distance d CC associated with the (Hörmander) vector fields

X 1 = x 1 , X m 0 = x q , Y .

This d CC is a true distance in R N + 1 , but it has not a simple explicit expression; since d and d CC are globally equivalent, we thus prefer to work with d and with the associated d -balls, defined as follows:

B r ( ξ ) { η R N + 1 : d ( η , ξ ) < r } ( for  ξ R N + 1  and  r > 0 ) .

Assumptions 1.2

We consider a KFP operator of the form (1.1) and with variable coefficients a i j = a i j ( x , t ) : R N + 1 R , i.e.,

u = i , j = 1 q a i j ( x , t ) u x i x j + B x , u u t i , j = 1 q a i j ( x , t ) u x i x j + Y u in  R N + 1 = R x N × R t ,

with 1 q N . Throughout the study, the points of R N + 1 will be sometimes denoted by the compact notation ξ = ( x , t ) .

We make the following assumptions.

  1. For some α ( 0 , 1 ) , we have

    (1.5) a i j C x α ( R N + 1 ) for every 1 i , j q ,

    where we have used the notation

    ( ) C x α ( R N + 1 ) = { f L ( R N + 1 ) : [ f ] α x < } ( ) [ f ] α x = sup ( x , t ) ( y , t ) R N + 1 u ( x , t ) u ( y , t ) x y α .

  2. The matrix A 0 ( x , t ) = ( a i j ( x , t ) ) i , j = 1 q is a symmetric uniformly positive matrix on R q ; this means, precisely, that

    (1.6) ν ξ 2 i , j = 1 q a i j ( x , t ) ξ i ξ j ν 1 ξ 2

    for some constant ν > 0 , every ξ R q , every x R N , and a.e. t R .

  3. The (constant) matrix B takes the block form in (1.2), and all the blocks vanish; more explicitly (and for a future reference), this means that

    B = O O O O B 1 O O B 2 O O O O B k O ,

    where every block B j is an m j × m j 1 matrix of rank m j , and

    m 0 = q , m 0 m 1 m k , and m 0 + m 1 + + m k = N .

Now, we have defined a good structure in R N + 1 , we can introduce the appropriate function spaces allowing to state our main results. Throughout the following, Ω R N + 1 is a fixed bounded domain; if ξ = ( x , t ) Ω , we set

d ξ Ω = dist ( ξ , Ω ) = inf { d ( η , ξ ) : η Ω } .

Moreover, given any ξ = ( x , t ) , η = ( y , s ) Ω , we also set

d ξ , η Ω = min { d ξ Ω , d η Ω } .

When the open set Ω is understood, we simply write d ξ and d ξ , η .

Definition 1.3

Let u : Ω R . Given any α ( 0 , 1 ) and k 0 , we introduce the following seminorms:

[ u ] , α , k Ω = sup ξ η Ω d ξ , η k + α u ( ξ ) u ( η ) d ( ξ , η ) α u , α , k Ω = sup ( x , t ) ( y , s ) Ω d ( x , t ) , ( y , s ) k + α u ( x , t ) u ( y , s ) d ( ( x , t ) , ( y , s ) ) α + t s α q N [ u ] , α , k x , Ω = sup ( x , t ) ( y , t ) Ω d ( x , t ) , ( y , t ) k + α u ( x , t ) u ( y , t ) x y α , [ u ] , k Ω = sup ξ Ω d ξ k u ( ξ ) ,

where q N 3 is the greatest exponent appearing in the dilations D λ , see (1.3). In order to avoid cumbersome notation, the dependence on Ω of the above norms will be often left understood.

Definition 1.4

We define S 0 ( Ω ) as the space of functions u : Ω ¯ R satisfying the following properties:

  1. u C ( Ω ¯ ) ;

  2. for every 1 i , j q , the distributional derivatives u x i , u x i x j L ( Ω ) ;

  3. the distributional derivative Y u L ( Ω ) .

Moreover, given any number α ( 0 , 1 ) , we define

S α ( Ω ) { u S 0 ( Ω ) : [ u x i ] , α , 1 x , Ω , [ u x i x j ] , α , 2 x , Ω , [ Y u ] , α , 2 x , Ω < for 1 i , j q } .

Remark 1.5

On account of assumption (H2), we immediately obtain the following facts which shall be repeatedly used throughout the rest of the study:

  1. If u S 0 ( Ω ) , then u L ( Ω ) .

  2. If u S α ( Ω ) , then u L ( Ω ) and [ u ] , α , 2 x < .

We are now ready to state the main results of this note. Our first result is a version of the Schauder estimates on the domain Ω , controlling the local Hölder continuity w.r.t. x of u x i x j (and the full Hölder continuity of u x i and u ) with the local Hölder continuity w.r.t. x of u and sup u .

Theorem 1.6

Let the above assumptions (H1)–(H3) be in force.

Then, there exists a constant c > 0 , depending on α in (1.5) and on Ω , such that, for every u S α ( Ω ) , we have the following estimate:

(1.7) i , j = 1 q ( [ u x i x j ] , α , 2 x + [ u x i x j ] , 2 ) + [ Y u ] , α , 2 x + [ Y u ] , 2 + i = 1 q ( [ u x i ] , α , 1 + [ u x i ] , 1 ) + [ u ] , α , 0 + sup Ω u c ( [ u ] , α , 2 x + [ u ] , 2 + sup Ω u ) .

Under the same assumptions, we will also improve our estimate on u x i x j controlling their local Hölder continuity also w.r.t. time.

Theorem 1.7

Let the assumptions of Theorem 1.6 be in force.

Then, there exists a constant c > 0 , depending on α and on diam ( Ω ) such that for every u S α ( Ω ) , we have the following estimate:

(1.8) i , j = 1 q u x i x j , α , 2 c ( [ u ] , α , 2 x + [ u ] , 2 + sup Ω u ) .

Remark 1.8

We explicitly stress that the finiteness of the seminorms

i = 1 q ( [ u x i ] , α , 1 + [ u x i ] , 1 ) , [ u ] , α , 0 , u x i x j , α , 2

appearing in the left-hand sides of (1.7) and (1.8), respectively, are not obvious a priori for a function in S α ( Ω ) ; they will be actually proved.

2 Proof of the main results

We are now ready to begin the proofs of Theorems 1.6 and 1.7.

2.1 Some interpolation inequalities

To begin with, we state and prove several interpolation inequalities, which will be used in the sequel. In order to do this, and to make this note as self-contained as possible, we recall here the following definitions given in [1].

Definition 2.1

Let u : Ω R , and let α ( 0 , 1 ) . We set

( i ) [ u ] α Ω = sup ξ η Ω u ( ξ ) u ( η ) d ( ξ , η ) α ; ( i i ) u α Ω = sup ( x , t ) ( y , s ) Ω u ( x , t ) u ( y , s ) d ( ( x , t ) , ( y , s ) ) α + t s α q N ; ( i i i ) [ u ] α x , Ω = sup ( x , t ) ( y , t ) Ω u ( x , t ) u ( y , t ) x y α .

The first inequality we prove is the following.

Proposition 2.2

There exists c > 0 and, for every ε > 0 small enough, there exists c ε > 0 such that for every u S α ( Ω )

(2.1) [ u x i ] , 1 c ε sup Ω u + ε max i , j = 1 , , q [ u x i x j ] , 2 ,

(2.2) [ u x i x j ] , 2 c ε sup Ω u + ε [ u x i x j ] , α , 2 x .

Proof

We first prove that there exists some absolute c > 0 such that, given any ε > 0 small enough, we have

[ u x i ] , 1 c ε sup Ω u + ε [ u x i x i ] , 2

for every u S α ( Ω ) ; this clearly implies (2.1).

Let ξ = ( x , t ) Ω , and let B r ( ξ ) Ω with r = μ d ξ and μ small enough to be chosen later. There exist ξ 1 , ξ 2 B r ( ξ ) , belonging to the line ξ ( τ ) = ξ + τ e i and such that (see (1.4) and recall the definition of )

d ( ξ 1 , ξ 2 ) = ξ 2 1 ξ 1 = ξ 1 ξ 2 r .

Applying Lagrange theorem to the function τ u ( ξ + τ e i ) , we obtain the existence of ξ ¯ ξ ( τ ) B r ( ξ ) such that

u x i ( ξ ¯ ) = u ( ξ 1 ) u ( ξ 2 ) ξ 1 ξ 2 2 r sup B r ( ξ ) u .

We can also write

u x i ( ξ ) = u x i ( ξ ¯ ) + ( ξ i ξ ¯ i ) 0 1 u x i x i ( ξ ¯ + s ( ξ ξ ¯ ) ) d s 2 r sup B r ( ξ ) u + ξ ξ ¯ sup B r ( ξ ) u x i x i 2 r sup B r ( ξ ) u + r sup B r ( ξ ) u x i x i .

Then,

d ξ u x i ( ξ ) d ξ 2 r sup B r ( ξ ) u + d ξ r sup B r ( ξ ) u x i x i 2 μ sup B r ( ξ ) u + μ d ξ 2 sup B r ( ξ ) u x i x i .

Finally, for μ small enough and some absolute c > 0 , we have d ζ c d ξ for every ζ B r ( ξ ) . Hence, that last expression is

2 μ sup B r ( ξ ) u + μ c 2 sup ζ B r ( ξ ) d ζ 2 u x i x i ( ζ ) .

Shrinking again the constant μ , by the arbitrariness of ξ , we conclude (2.1). In view of (2.1), to prove (2.2), it suffices to show that, for every ε > 0

[ u x i x j ] , 2 c ε [ u x i ] , 1 + ε [ u x i x j ] , α , 2 x .

Let us apply the above reasoning to the function u x i (and the line ξ ( τ ) = ξ + τ e j ). For ξ = ( x , t ) Ω , B r ( ξ ) Ω with r = μ d ξ and μ small enough to be chosen later, there exists ξ ¯ B r ( ξ ) such that

u x i x j ( ξ ¯ ) 2 r sup B r ( ξ ) u x i .

Then,

u x i x j ( ξ ) u x i x j ( ξ ¯ ) + u x i x j ( ξ ) u x i x j ( ξ ¯ ) 2 r sup B r ( ξ ) u x i + r α u x i x j ( ξ ) u x i x j ( ξ ¯ ) ξ ¯ ξ α 2 r sup B r ( ξ ) u x i + r α sup ( z , s ) ( y , s ) B r ( ξ ) u x i x j ( z , s ) u x i x j ( y , s ) z y α .

Hence, reasoning like above

d ξ 2 u x i x j ( ξ ) 2 μ d ξ sup B r ( ξ ) u x i + μ α d ξ 2 + α sup ( z , s ) ( y , s ) B r ( ξ ) u x i x j ( z , s ) u x i x j ( y , s ) z y α c μ [ u x i ] , 1 + c μ α [ u x i x j ] , α , 2 x

so that

[ u x i x j ] , 2 c ε [ u x i ] , 1 + ε [ u x i x j ] , α , 2 x .

This completes the proof.□

The next result is actually just a more precise version of [1, Theorem 4.2].

Proposition 2.3

There exist constants c > 0 and γ > 1 such that for every ε ( 0 , 1 ) , every u S α ( Ω ) , and every r > 0 such that B 8 r Ω ,

(2.3) r 1 + α i = 1 q [ u x i ] α B r + r i = 1 q u x i L ( B r ) + r α [ u ] α B r + sup B r u ε r 2 i , j = 1 q u x i x j L ( B 4 r ) + r 2 Y u L ( B 4 r ) + c ε γ sup B 4 r u .

Proof

First of all, we recall that, by [1, Theorem 4.2], there exists some constant c > 0 such that, given any ε > 0 , for every u S 0 ( R N + 1 ) and every ξ ¯ R N + 1 , we have the following interpolation inequality:

(2.4) h = 1 q [ u x h ] α B 1 ( ξ ¯ ) + u x h L ( B 1 ( ξ ¯ ) ) + [ u ] α B 1 ( ξ ¯ ) + sup B 1 ( ξ ¯ ) u ε h , k = 1 q x k x h 2 u L ( B 4 ( ξ ¯ ) ) + Y u L ( B 4 ( ξ ¯ ) ) + c ε γ sup B 4 ( ξ ¯ ) u .

As a consequence, if u S 0 ( R N + 1 ) and if B 8 r = B 8 r ( η ) (for some η R N + 1 ), by applying (2.4) to the function v = u D ( r ) and with the choice ξ ¯ = D ( 1 r ) η , we readily obtain (2.3).

For a general u S 0 ( Ω ) , it suffices to apply the above argument to the function v = u ϕ , where ϕ C 0 ( B 8 r ) is such that

ϕ 1 in B 4 r .

This completes the proof.□

A third interpolation result of different kind (for compactly supported functions) is as follows:

Proposition 2.4

There exists a constant c > 0 such that, for every r > 0 and every u S α ( Ω ) with supp ( u ) B r = B r ( ξ ¯ ) Ω , we have

[ u x i ] α B r c r 1 α j = 1 q u x j x j L ( B r ) + Y u L ( B r ) [ u ] α B r c r 2 α j = 1 q u x j x j L ( B r ) + Y u L ( B r ) .

Proof

Let 0 be a KFP operator belonging to our class but with constant a i j = δ i j , so that for every u S α ( Ω ) , compactly supported in some ball B r ( ξ ¯ ) Ω , we can write the representation formulas contained in [1, Thm.3.11, Coroll. 3.12]:

(2.5) u ( x , t ) = B r ( ξ ¯ ) Γ ( x , t ; y , s ) 0 u ( y , s ) d y d s

(2.6) u x i ( x , t ) = B r ( ξ ¯ ) Γ x i ( x , t ; y , s ) 0 u ( y , s ) d y d s

for every ( x , t ) B r ( ξ ¯ ) , i = 1 , 2 , , q . Next we note that the kernels Γ , Γ x i are fractional integral kernels satisfying the assumptions of [1, Thm.2.4] with β = 2 , β = 1 , respectively, so that

[ u ] α B r c r 2 α 0 u L ( B r ) [ u x i ] α B r c r 1 α 0 u L ( B r ) .

Since 0 u = j = 1 q u x j x j + Y u , we obtain the assertion.□

2.2 Proof of Theorem 1.6

The proof is split in several steps, each one obtaining the estimate on a separate term of the left-hand side of (1.7). The technique of the proof in the several steps is somehow similar.

Step (1). We start by proving the estimate

(2.7) i , j = 1 q ( [ u x i x j ] , α , 2 x + [ u x i x j ] , 2 ) c { [ u ] , α , 2 x + [ u ] , 2 + sup Ω u } .

Let ξ = ( x , t ) , η = ( y , t ) Ω be such that

d ξ , η 2 + α u x i x j ( ξ ) u x i x j ( η ) x y α 1 2 [ u x i x j ] , α , 2 x .

We assume, to fix the ideas, that

d ξ , η = d ξ

and we turn to distinguish two cases.

Case (1): x y d ξ 16 . In this first case, we have

(2.8) [ u x i x j ] , α , 2 x 2 d ξ , η 2 + α u x i x j ( x , t ) u x i x j ( y , t ) x y α c α { d ξ 2 u x i x j ( ξ ) + d η 2 u x i x j ( η ) } c α [ u x i x j ] , 2 .

Case (2): x y < d ξ 16 . In this second case, we set r = 3 d ξ 16 , and we consider the ball B r = B r ( ξ ) ; then, we choose ϕ C 0 ( B r ) such that

  1. 0 ϕ 1 and ϕ = 1 in B r 3 = B ( ξ , r 3 ) ;

  2. there exists c > 0 such that, for every ζ R N + 1 , one has

    ϕ ( ζ ) + d ξ i = 1 q ϕ x i ( ζ ) + d ξ 2 i , j = 1 q ϕ x i x j ( ζ ) c .

We explicitly stress that the existence of a cut-off function satisfying (a) and (b) follows from the fact that the distance d associated with our balls is smooth outside the origin.

We now observe that, since u S α ( Ω ) and ϕ C 0 ( Ω ) , the function v = u ϕ satisfies the assumptions of [1, Theorem 4.1]; hence, we have

[ ( u ϕ ) x i x j ] α x , B r + u ϕ L ( B r ) c [ ( u ϕ ) ] α x , B r .

From this, since ξ , η B r 3 and ϕ 1 on B r 3 , we have:

u x i x j ( ξ ) u x i x j ( η ) x y α c [ u ] α x , B r + u L ( B r ) d ξ α + 1 d ξ h = 1 q [ u x h ] α x , B r + 1 d ξ 1 + α h = 1 q u x h L ( B r ) + [ u ] α x , B r d ξ 2 + sup B r u d ξ 2 + α .

Multiplying both left- and right-hand sides with d ξ 2 + α , we obtain

[ u x i x j ] , α , 2 x 2 d ξ 2 + α u x i x j ( ξ ) u x i x j ( η ) x y α c d ξ 2 + α [ u ] α x , B r + d ξ 2 u L ( B r ) + d ξ 1 + α h = 1 q [ u x h ] α x , B r + d ξ h = 1 q u x h L ( B r ) + d ξ α [ u ] α x , B r + sup B r u .

Applying Proposition 2.3 (with ε = 1 ), and since in our situation, the radius r is comparable to d ξ , we obtain

[ u x i x j ] , α , 2 x c d ξ 2 + α [ u ] α x , B r + d ξ 2 u L ( B r ) + d ξ 2 h , k = 1 q u x h x k L ( B 4 r ) + Y u L ( B 4 r ) + sup B 4 r u .

From the equation, we can bound Y u obtaining

[ u x i x j ] , α , 2 x c d ξ 2 + α [ u ] α x , B r + d ξ 2 u L ( B 4 r ) + d ξ 2 h , k = 1 q u x h x k L ( B 4 r ) + sup B 4 r u .

We now observe that, since ξ = ( x , t ) is the center of B r and since B 4 r Ω , we have d ξ c d ζ for every ζ B 4 r ; hence,

(2.9) i , j = 1 q [ u x i x j ] , α , 2 x c [ u ] , α , 2 x + [ u ] , 2 + i , j = 1 q [ u x i x j ] , 2 + sup B 4 r u .

Gathering (2.8) and (2.9) we conclude that, in any case, we have

(2.10) i , j = 1 q [ u x i x j ] , α , 2 x c [ u ] , α , 2 x + [ u ] , 2 + i , j = 1 q [ u x i x j ] , 2 + sup B 4 r u .

By adding to both left- and right-hand sides of (2.10), the term [ u x i x j ] , 2 , we clearly obtain

i , j = 1 q ( [ u x i x j ] , α , 2 x + [ u x i x j ] , 2 ) c [ u ] , α , 2 x + [ u ] , 2 + i , j = 1 q [ u x i x j ] , 2 + sup B 4 r u .

Then, by applying Proposition 2.2 (with ε > 0 sufficiently small), we obtain

i , j = 1 q [ u x i x j ] , α , 2 x c { [ u ] , α , 2 x + [ u ] , 2 + sup Ω u } .

This, together with (2.10), implies (2.7).

Step (2). Exploiting (2.7) and the equation, we immediately obtain

(2.11) i , j = 1 q ( [ u x i x j ] , α , 2 x + [ u x i x j ] , 2 ) + [ Y u ] , α , 2 x + [ Y u ] , 2 c { [ u ] , α , 2 x + [ u ] , 2 + sup Ω u } .

Step (3). We now come to the estimates of the full Hölder seminorms

[ u x i ] , α , 1 , [ u x i ] , α , 0 .

To begin with, we choose ξ = ( x , t ) , η = ( y , s ) Ω in such a way that

(2.12) d ξ , η 1 + α u x i ( ξ ) u x i ( η ) d ( ξ , η ) α 1 2 [ u x i ] , α , 1 ;

we assume, to fix ideas, that d ξ , η = d ξ and we distinguish two cases.

Case (1): d ( ξ , η ) d ξ 16 . In this first case, we have

(2.13) [ u x i ] , α , 1 2 d ξ , η 1 + α u x i ( ξ ) u x i ( η ) d ( ξ , η ) α c α { d ξ u x i ( ξ ) + d ξ u x i ( η ) } c α [ u x i ] , 1 .

Case (2): d ( ξ , η ) < d ξ 16 . In this second case, we set r = 3 d ξ 16 , and we consider the ball B r = B r ( ξ ) ; then, we choose ϕ C 0 ( B r ) such that

  1. 0 ϕ 1 and ϕ = 1 in B r 3 = B ( ξ , r 3 ) ;

  2. there exists c > 0 such that, for every ζ R N + 1 , one has

    ϕ ( ζ ) + d ξ i = 1 q ϕ x i ( ζ ) + d ξ 2 i , j = 1 q ϕ x i x j ( ζ ) + Y ϕ ( ζ ) c .

We now observe that, since u S α ( Ω ) and ϕ C 0 ( Ω ) , the function v = u ϕ satisfies the assumptions of Proposition 2.4; hence, we have

[ ( u ϕ ) x i ] α B r c r 1 α h , k = 1 q ( u ϕ ) x h x k L ( B r ) + Y ( u ϕ ) L ( B r ) ( recalling that r = 3 16 d ξ ) c d ξ 1 α h , k = 1 q ( u ϕ ) x h x k L ( B r ) + Y ( u ϕ ) L ( B r ) .

From this, since ξ , η B r 3 and since ϕ 1 on B r 3 , we have

u x i ( ξ ) u x i ( η ) d ( ξ , η ) α c d ξ 1 α h , k = 1 q u x h x k L ( B r ) + Y u L ( B r ) + 1 d ξ h = 1 q u x h L ( B r ) + 1 d ξ 2 sup B r u c d ξ 1 α h , k = 1 q u x h x k L ( B r ) + u L ( B r ) + 1 d ξ h = 1 q u x h L ( B r ) + 1 d ξ 2 sup B r u .

Multiplying both left- and right-hand sides with d ξ 1 + α , and recalling (2.12), we obtain

[ u x i ] , α , 1 2 d ξ , η 1 + α u x i ( ξ ) u x i ( η ) d ( ξ , η ) α c h , k = 1 q d ξ 2 u x h x k L ( B r ) + d ξ 2 u L ( B r ) + d ξ h = 1 q u x h L ( B r ) + sup B r u .

Starting from this last estimate, and reasoning as in Step (1), we then obtain

(2.14) [ u x i ] , α , 1 c h , k = 1 q [ u x h x k ] , 2 + [ u ] , 2 + h = 1 q [ u x h ] , 1 + sup Ω u .

Gathering (2.13) and (2.14) we conclude that, in any case, we have

(2.15) [ u x i ] , α , 1 c h , k = 1 q [ u x h x k ] , 2 + [ u ] , 2 + h = 1 q [ u x h ] , 1 + sup Ω u ,

and this completes the estimate of [ u x i ] , α , 1 . As for the estimate of [ u ] , α , 0 , instead, by exploiting the second inequality in Proposition 2.4 and by proceeding in a completely analogous way, we can prove that

(2.16) [ u ] , α , 0 c h , k = 1 q [ u x h x k ] , 2 + [ u ] , 2 + h = 1 q [ u x h ] , 1 + sup Ω u .

With estimates (2.11), (2.15), and (2.16) at hand, we can complete the proof of the theorem: by adding to both left- and right-hand sides of (2.11) the term

h = 1 q ( [ u x h ] , α , 1 + [ u x h ] , 1 ) + [ u ] , α , 0 + sup Ω u ,

we obtain

i , j = 1 q ( [ u x i x j ] , α , 2 x + [ u x i x j ] , 2 ) + [ Y u ] , α , 2 x + [ Y u ] , 2 + h = 1 q ( [ u x h ] , α , 1 + [ u x h ] , 1 ) + [ u ] , α , 0 + sup Ω u c { [ u ] , α , 2 x + [ u ] , 2 + sup Ω u } + h = 1 q ( [ u x h ] , α , 1 + [ u x h ] , 1 ) + [ u ] , α , 0 + sup Ω u .

From this, by exploiting (2.15)–(2.16), jointly with the interpolation inequalities of Proposition 2.2 and again (2.7), we obtain (1.7).

2.3 Proof of Theorem 1.7

We now improve the estimates on u x i x j contained in Theorem 1.6 by proving the Hölder continuity of these second-order derivatives also w.r.t. time.

We split the proof into two steps.

Step (A). First, we prove estimate (1.8) for all functions u S α ( Ω ) satisfying the additional property that u x i x j , α , 2 < . To this end, as in the proof of Theorem 1.6, we let ξ = ( x , t ) , η = ( y , s ) Ω be such that

(2.17) d ξ , η 2 + α u x i x j ( ξ ) u x i x j ( η ) d ( ξ , η ) α + t s α q N 1 2 u x i x j , α , 2 .

We assume, to fix ideas, that d ξ , η = d ξ , and we distinguish two cases.

Case (1): d ( ξ , η ) d ξ 16 . In this first case, we have

u x i x j , α , 2 2 d ξ , η 2 + α u x i x j ( ξ ) u x i x j ( η ) d ( ξ , η ) α + t s α q N c α d ξ , η 2 u x i x j ( ξ ) u x i x j ( η ) c α { d ξ 2 u x i x j ( ξ ) + d η 2 u x i x j ( η ) } c α [ u x i x j ] , 2 .

Case (2): d ( ξ , η ) < d ξ 16 . In this second case, we set r = 3 d ξ 16 , and we consider the ball B r = B r ( ξ ) ; then, we choose ϕ C 0 ( B r ) such that

  1. 0 ϕ 1 and ϕ = 1 in B r 3 = B ( ξ , r 3 ) ;

  2. there exists c > 0 such that, for every ζ R N + 1 , one has

    ϕ ( ζ ) + d ξ i = 1 q ϕ x i ( ζ ) + d ξ 2 i , j = 1 q ϕ x i x j ( ζ ) c .

We now observe that, since u S α ( Ω ) and ϕ C 0 ( Ω ) , the function v = u ϕ satisfies the assumptions of [1, Theorem 4.9]; hence, we have

( u ϕ ) x i x j α B r c { [ ( u ϕ ) ] α x , B r + ( u ϕ ) L ( B r ) + sup B r u } .

From this, since ξ , η B r 3 and since ϕ 1 on B r 3 , we have

u x i x j ( ξ ) u x i x j ( η ) d ( ξ , η ) α + t s α q N c [ u ] α x , B r + u L ( B r ) d ξ α + 1 d ξ h = 1 q [ u x h ] α x , B r + 1 d ξ 1 + α h = 1 q u x h L ( B r ) + [ u ] α x , B r d ξ 2 + sup B r u d ξ 2 + α + u L ( B r ) + 1 d ξ h = 1 q u x h L ( B r ) + 1 d ξ 2 sup B r u + sup B r u .

Multiplying both left- and right-hand sides with d ξ 2 + α , and recalling (2.17) (jointly with the fact that, since Ω is bounded, we have d ξ diam ( Ω ) ), we obtain

u x i x j , α , 2 2 d ξ , η 2 + α u x i x j ( ξ ) u x i x j ( η ) d ( ξ , η ) α + t s α q N c d ξ 2 + α [ u ] α x , B r + d ξ 2 u L ( B r ) + d ξ 1 + α h = 1 q [ u x h ] α x , B r + d ξ h = 1 q u x h L ( B r ) + d ξ α [ u ] α x , B r + sup B r u .

Applying Proposition 2.3 (with ε = 1 ), and since in our situation, the radius r is comparable to d ξ we obtain

u x i x j , α , 2 c { d ξ 2 + α [ u ] α x , B r + d ξ 2 u L ( B r ) + d ξ 2 h , k = 1 q u x h x k L ( B 4 r ) + Y u L ( B 4 r ) + sup B 4 r u .

From the equation, we can bound Y u obtaining

u x i x j , α , 2 c d ξ 2 + α [ u ] α x , B r + d ξ 2 u L ( B 4 r ) + d ξ 2 h , k = 1 q u x h x k L ( B 4 r ) + sup B 4 r u .

We now observe that, since ξ = ( x , t ) is the center of B r and since B 4 r Ω , we have d ξ c d ζ for every ζ B 4 r ; hence,

(2.18) i , j = 1 q u x i x j , α , 2 c [ u ] , α , 2 x + [ u ] , 2 + i , j = 1 q [ u x i x j ] , 2 + sup B 4 r u .

Gathering (2.17) and (2.18) we conclude that, in any case, we have

(2.19) i , j = 1 q u x i x j , α , 2 c [ u ] , α , 2 x + [ u ] , 2 + i , j = 1 q [ u x i x j ] , 2 + sup B 4 r u .

By combining (2.19) with Theorem 1.6, we obtain

i , j = 1 q u x i x j , α , 2 c { [ u ] , α , 2 x + [ u ] , 2 + sup Ω u } ,

and this is exactly the desired (1.8).

Step (B). We now complete the proof by considering a general function u S α ( Ω ) , not satisfying a priori the property

u * , α , 2 < .

To this end, we consider an increasing sequence { Ω k } k of domains invading Ω , and we let { ϕ k } k C 0 ( Ω ) be a sequence of cut-off functions such that

0 ϕ k 1 and ϕ k = 1 in Ω k .

Now, since ϕ k C 0 ( Ω ) , it is readily seen that the function v k = u ϕ k satisfies the regularity assumptions in [1, Theorem 4.9]; thus, we obtain

( u ϕ ) x i x j α Ω k = u x i x j α Ω k < for every  k N .

From this, since Ω k is bounded, we infer that

(2.20) u x i x j , α , 2 Ω k diam ( Ω k ) α + 2 u x i x j α Ω k diam ( Ω ) α + 2 u x i x j α Ω k < + .

In view of (2.20), we can then apply estimate (1.8) to the function u S α ( Ω k ) on the domain Ω k : this gives

(2.21) i , j = 1 q u x i x j , α , 2 Ω k c { [ u ] , α , 2 x , Ω k + [ u ] , 2 Ω k + sup Ω k u } c { [ u ] , α , 2 x , Ω + [ u ] , 2 Ω + sup Ω u } ,

where we have used the fact that d ζ Ω k d ζ Ω for every ζ Ω k , and the constant c > 0 depends on Ω k only through its diameter (hence, it can be chosen independent of k ). We can then pass to the limit as k in the above (2.21), thus obtaining both the finiteness of u x i x j , α , 2 and the desired (1.8).

Acknowledgments

The authors are members of the research group “Gruppo Nazionale per l’Analisi Matematica, la Probabilità e le loro Applicazioni” of the Italian “Istituto Nazionale di Alta Matematica.”

  1. Funding information: Stefano Biagi was partially supported by the PRIN 2022 project 2022R537CS NO 3 - Nodal Optimization, Nonlinear elliptic equations, Nonlocal geometric problems, with a focus on regularity, funded by the European Union – Next Generation EU; Marco Bramanti was partially supported by the PRIN 2022 project Partial differential equations and related geometric-functional inequalities, financially supported by the EU, in the framework of the “Next Generation EU initiative.”

  2. Author contributions: The authors contributed equally to the preparation of this work.

  3. Conflict of interest: The authors state no conflict of interest.

References

[1] S. Biagi and M. Bramanti, Schauder estimates for Kolmogorov-Fokker-Planck operators with coefficients measurable in time and Hölder continuous in space. J. Math. Anal. Appl. 533 (2024), no. 1, Paper No. 127996. 10.1016/j.jmaa.2023.127996Search in Google Scholar

[2] M. Bramanti, An invitation to hypoelliptic operators and Hörmander’s vector fields, Springer Briefs Math. Springer, Cham, 2014, xii+150 pp. 10.1007/978-3-319-02087-7Search in Google Scholar

[3] M. Bramanti and S. Polidoro, Fundamental solutions for Kolmogorov-Fokker-Planck operators with time-depending measurable coefficients, Math. Eng. 2 (2020), no. 4, 734–771. Search in Google Scholar

[4] P.-E. Chaudru de Raynal, I. Honoré, and S. Menozzi, Sharp Schauder estimates for some degenerate Kolmogorov equations, Ann. Sc. Norm. Super. Pisa Cl. Sci. (5) 22 (2021), no. 3, 989–1089. 10.2422/2036-2145.201811_011Search in Google Scholar

[5] M. Di Francesco and S. Polidoro, Schauder estimates, Harnack inequality and Gaussian lower bound for Kolmogorov-type operators in non-divergence form, Adv. Differential Equations 11 (2006), no. 11, 1261–1320. 10.57262/ade/1355867597Search in Google Scholar

[6] H. Dong and T. Yastrzhembskiy, Global Schauder estimates for kinetic Kolmogorov-Fokker-Planck equations, 2022, arXiv:2209.00769. 10.1007/s00205-022-01786-0Search in Google Scholar

[7] C. Henderson and W. Wang, Kinetic Schauder estimates with time-irregular coefficients and uniqueness for the Landau equation, Discrete Contin. Dyn. Syst. 44 (2024), no. 4, 1026–1072. 10.3934/dcds.2023137Search in Google Scholar

[8] C. Henderson and S. Snelson, C∞ smoothing for weak solutions of the inhomogeneous Landau equation, Arch. Ration. Mech. Anal. 236 (2020), no. 1, 113–143. 10.1007/s00205-019-01465-7Search in Google Scholar

[9] L. Hörmander, Pseudo-differential operators and hypoelliptic equations, Singular Integrals (Proc. Sympos. Pure Math., Vol. X, Chicago, Ill., 1966), American Mathematical Society, Providence, R.I., 1967, pp. 138–183. 10.1090/pspum/010/0383152Search in Google Scholar

[10] L. Hörmander, Hypoelliptic second order differential equations, Acta Math. 119 (1967), 147–171. 10.1007/BF02392081Search in Google Scholar

[11] C. Imbert and C. Mouhot, The Schauder estimate in kinetic theory with application to a toy nonlinear model, Ann. H. Lebesgue 4 (2021), 369–405. 10.5802/ahl.75Search in Google Scholar

[12] A.N. Kolmogorov, Zufällige Bewegungen (Zur Theorie der Brownschen Bewegung), Ann. Math. 35 (1934), no. 2, 116–117. 10.2307/1968123Search in Google Scholar

[13] E. Lanconelli and S. Polidoro, On a class of hypoelliptic evolution operators, Partial Differential Equations, II (Turin, 1993), Rend. Sem. Mat. Univ. Politec. Torino 52 (1994), no. 1, 29–63. Search in Google Scholar

[14] L. Lorenzi, Schauder estimates for degenerate elliptic and parabolic problems with unbounded coefficients in RN. Differential Integral Equations 18 (2005), no. 5, 531–566. 10.57262/die/1356060184Search in Google Scholar

[15] G. Lucertini, S. Pagliarani, and A. Pascucci, Optimal regularity for degenerate Kolmogorov equations in non-divergence form with rough-in-time coefficients. J. Evol. Equ. 23 (2023), no. 4, Paper No. 69, 37pp. 10.1007/s00028-023-00916-9Search in Google Scholar

[16] G. Lucertini, S. Pagliarani, and A. Pascucci, Optimal Schauder estimates for kinetic Kolmogorov equations with time measurable coefficients, 2024, arXiv:2304.13392v2. Search in Google Scholar

[17] A. Lunardi, Schauder estimates for a class of degenerate elliptic and parabolic operators with unbounded coefficients in RN, Ann. Scuola Norm. Sup. Pisa Cl. Sci. (4) 24 (1997), no. 1, 133–164. Search in Google Scholar

[18] M. Manfredini, The Dirichlet problem for a class of ultraparabolic equations, Adv. Differential Equations 2 (1997), no. 5, 831–866. 10.57262/ade/1366638967Search in Google Scholar

[19] C. Mouhot, De Giorgi–Nash–Moser and Hörmander theories: New interplays, World Scientific Publishing Co. Pte. Ltd., Hackensack, NJ, 2018, pp. 2467–2493. 10.1142/9789813272880_0146Search in Google Scholar

[20] E. Priola, Global Schauder estimates for a class of degenerate Kolmogorov equations. Studia Math. 194 (2009), no. 2, 117–153. 10.4064/sm194-2-2Search in Google Scholar

[21] C. Villani, A review of mathematical topics in collisional kinetic theory, Handbook of Mathematical Fluid Dynamics, Vol. I, North-Holland, Amsterdam, 2002, pp. 71–305. 10.1016/S1874-5792(02)80004-0Search in Google Scholar

Received: 2024-04-06
Revised: 2024-06-20
Accepted: 2024-07-22
Published Online: 2024-09-19

© 2024 the author(s), published by De Gruyter

This work is licensed under the Creative Commons Attribution 4.0 International License.

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