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Modulation type spaces for generators of polynomially bounded groups and Schrödinger equations

Peer Christian Kunstmann

CRC Preprint 2018/4 (revised), March 2019

KARLSRUHE INSTITUTE OF TECHNOLOGY

KIT – The Research University in the Helmholtz Association www.kit.edu Participating universities

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ISSN 2365-662X

2 MODULATION TYPE SPACES FOR GENERATORS OF POLYNOMIALLY BOUNDED GROUPS AND SCHRODINGER¨ EQUATIONS

PEER CHRISTIAN KUNSTMANN

Abstract. We introduce modulation type spaces associated with the generators of polynomially bounded groups. Besides strongly continuous groups we study in detail the case of bi-continuous groups, e.g. weak∗-continuous groups in dual spaces. It turns out that this gives new insight in situations where generators are not densely defined. Classical modulation spaces are covered as a special case but the abstract formulation gives more flexibility. We illustrate this with an application to a nonlinear Schr¨odingerequation. Mathematics Subject Classification (2010). 47 D 06, 47 A 60, 47 D 08, 35 Q 55. Keywords. Polynomially bounded groups, , spaces associated with opera- tors, modulation spaces

1. Introduction and main results

s d Classical modulation spaces Mp,q(R ) (or more general on locally compact abelian groups) have been introduced by Feichtinger in the 80s (we refer to[4] and the literatue cited there) by means of the short time Fourier transform (see (19) below for the definition of the latter). There is an equivalent description of these spaces by so-called “uniform” decompositions of the Fourier transforms of their elements ([4]), and we shall rely on that one here. Modulation spaces have been succesfully used in time-frequency analysis and related fields (see, e.g., the survey [5]). s d In recent years, modulation spaces Mp,q(R ) have been used in the theory of dispersive partial differential equations such as the (nonlinear) Schr¨odingerequation (see, e.g., [17, 2]). One of the it∆ appealing features of modulation spaces in this context is that operators e , t ∈ R, are bounded s d (polynomially in |t|) on Mp,q(R ) for all s ∈ R, 1 ≤ p, q ≤ ∞ (see, e.g., [1]), which is in sharp q d contrast to Lebesgue spaces L (R ), where this only holds for q = 2. In this paper we propose a different and in a sense more abstract point of view on this phenomenon, within the realm of semigroup theory and with a variant of the Phillips functional calculus as the main technical tool. We start with a general polynomially bounded group (T (t)) = (e−itB) in a s X and construct modulation type spaces MX,q(B) associated with the “generator” −itB −itB2 s B. Then we study the groups (e ) and (e ) in MX,q(B) and apply the results to Schr¨odinger type equations  2 iu˙(t) = B u(t), t ∈ R, u(0) = x. Note that we do not restrict to bounded groups. Moreover, we are particularly interested in the case where B is not densely defined in X. It turns out that the theory of bi-continuous (semi- )groups (see [11]) is well suited to the study of this case, and that this also gives new insight with respect to continuity properties in the case q = ∞. In the abstract situation one cannot, in general, resort to some kind of weak∗-continuity, and it turns out that, even when this is possible, one might have other possibilities to choose a suitable topology.

The author acknowledges support by the DFG through CRC 1173. 1 To be more precise, let T (·) = (T (t))t∈R be a C0-group in a complex Banach space X. We assume that (T (t))t∈R is polynomially bounded, i.e. there exist M ≥ 1 and α ≥ 0 such that α (1) kT (t)xkX ≤ Mhti kxkX , t ∈ R, x ∈ X, 2 1/2 −itB where hti = (1 + |t| ) . We denote the generator of T (·) by −iB and write T (t) = e , t ∈ R. We shall use the Phillips functional calculus for the operator B (see, e.g. [7, Sect. 3.3]) and R α denote the space of complex Borel measures µ satisfying hti d|µ|(t) < ∞ by α( ). Observe R M R R α that α( ) is a for convolution (letting kµk := (1 + |t|) d|µ|(t) we have M R Mα R kµ ∗ νkMα ≤ kµkMα kνkMα ). If µ ∈ Mα(R) and Z −iτξ φ(ξ) = µb(ξ) = e dµ(τ), ξ ∈ R, R is its Fourier transform then Z Z (2) φ(B)x := e−iτBx dµ(τ) = T (τ)x dµ(τ), x ∈ X, R R defines a in X. Moreover, φ 7→ φ(B) is an algebra homomorphism from the space FMα(R) := {µb : µ ∈ Mα(R)} into L(X), the space of bounded linear operators on X. We denote by S (R) the , by Z −iτr φb(τ) := (F φ)(τ) := e φ(r) dr, τ ∈ R, R −1 the Fourier transform of φ ∈ S (R), and by F φ the inverse Fourier transform of φ, given by Z −1 1 iτr F φ(r) = e φ(τ) dτ, r ∈ R. 2π R We clearly have S (R) ⊆ FMα(R) for any α ≥ 0, and for φ ∈ S (R) the operator φ(B) is given by Z Z 1 iτB −1 −iτB (3) φ(B)x = φb(τ)e x dτ = (F φ)(τ)e x dτ, φ ∈ S (R). 2π R R The map S (R) → L(X), φ 7→ φ(B), is an algebra homomorphism and we have the estimate

M α (4) kφ(B)k ≤ kh·i φbk 1 , φ ∈ S ( ), L(X) 2π L R in particular, φ 7→ φ(B) is continuous for the usual topology on S (R). Remark 1.1. Letting 1 α 1 Lα(R) := {f : h·i fb ∈ L (R)} α 1 equipped with the norm kfk 1 := k(1 + | · |) fk 1 , we have that L ( ) is a Banach subalgebra Lα b L α R 1 of FMα(R). By (4) we obtain a bounded functional calculus for B on Lα(R). Observe that, by 1 k the Riemann-Lebesgue lemma, Lα(R) ⊆ C0 (R) for any k ∈ N0 with k ≤ α. Nevertheless, we shall mostly work with the functional calculus for Schwartz functions and use the formulae in (3). The following example has to kept in mind throughout the paper and shall give the relation to classical modulation spaces. 2 p Example 1.2. Let X = L (R) with p ∈ [1, ∞) and let T (t)f := f(· − t), t ∈ R be the right d translation group with generator − dx . The group is bounded, even isometric, and M = 1, α = 0 d −iτB in (1). We have B = −i dx , e f = T (τ)f = f(· − τ) and we see from the second formula in (3) that d −1 −1  p φ(B)f = φ(−i )f = (F φ) ∗ f = F ξ 7→ φ(ξ)fb(ξ) , φ ∈ S ( ), f ∈ L ( ). dx R R Boundedness of the Phillips functional calculus here just means that, for any complex Borel p measure µ on R, its Fourier transform µb is an L -Fourier multiplier and that µb(B)f = µ ∗ f. We shall associate with B a scale of “modulation type” spaces. The basic idea is to take φ ∈ S (R) \{0} and put, for s ∈ R and q ∈ [1, ∞], Z 1/q s  s q  (5) M := {x : kxk s := hti kφ(B − t)xk dt < ∞} X,q,φ MX,q,φ X R with obvious modification in case q = ∞ (observe that it makes no difference whether we plug B into φ(· − t) or B − t into φ to obtain φ(B − t)). We shall show below that different φ give s s rise to equivalent norms, so that we can denote this space by MX,q (or MX,q(B) if we want to specify the operator B in notation). In the context of Example 1.2 this will yield the classical s modulation spaces Mp,q(R). However, we have to be a bit careful about the x we admit in (5). 0 In the classical case we have the space S (R) of tempered distributions as an ambient space. For sufficiently large s we can take x ∈ X, but for s small (depending on q) or for negative s we have to resort to a scale X−k, k ∈ N, of extrapolation spaces, see Section 2. Just as there is an analogy of classical modulation spaces with classical Besov spaces, our con- struction can be viewed as a counterpart to the construction of abstract Besov type spaces for sectorial operators (see, e.g., the “intermediate spaces” in [7, Sect. 6.4.1]). The results in this paper can clearly be extended to finitely many commuting groups, and one s d d can thus recover classical modulation spaces Mp,q(R ) on R for d > 1. Moreover, iterating the procedure presented here one can define anisotropic versions of these spaces with different integrability exponents in different directions. We shall not go into further details here. The paper is organized as follows: In Section 2 we show basic properties of the functional calculus for Schwartz functions and introduce the extrapolation scale we shall use. In Section 3 we define s the spaces MX,q(B) in the case of a strongly continuous group and establish their basic properties. In Section 4 we consider the situation of a bi-continuous group with not necessarily densely defined s B. Even if the original group in X is strongly continuous, the induced group in MX,∞(B) is not strongly continuous, in general. Resorting to the notion bi-continuous groups allows to study this −itB2 s case in a satisfying setting. Section 5 is devoted to the study of (e ) in MX,q(B), and this relies very much on (extensions of) the Phillips calculus. We give an application of our result to a nonlinear Schr¨odingerequation in Section 6. In the Appendix we have gathered two auxiliary results and give their proofs for convenience.

2. Basic definitions and properties We start with fundamental properties of the functional calculus for Schwartz functions.

Lemma 2.1. Let φ ∈ S (R). (1) For x ∈ X we have φ(B)x ∈ D(B) and Bφ(B)x = ψ(B)x where ψ(r) := rφ(r). k (2) For any k ∈ N the operator φ(B) maps X into D(B ). (3) For λ ∈ C \ R we have R(λ, B)φ(B)x = ψ(B)x where ψ(r) := φ(r)/(λ − r). 3 S (4) The set ρ∈S ρ(B)(X) is dense in X and ρ(B)x = 0 for all ρ ∈ S (R) implies x = 0. Proof. For the proof of (1) let t > 0. Then 1 Z 1 Z T (t)φ(B)x = φb(τ)ei(τ−t)Bx dτ = φb(τ + t)eiτBx dτ 2π R 2π R hence T (t)φ(B)x = e−it(·)φ(B)x (in fact, this also follows from the Phillips calculus). We −t R ∞ multiply with e , integrate 0 . . . dt and use Fubini to get R(1, −iB)φ(B)x = φe(B)x, where φe(r) = (1 + ir)−1φ(r). This implies (1). (2) follows from (1) by induction, and (3) also follows from (1). √ −t2/(2k) −kτ 2/2 For k ∈ N let gk(t) := e . Then gk ∈ S (R) and gbk(τ) = 2πke . For x ∈ X and k → ∞ we have r 1 Z Z k 2 g (B)x = g (τ)eiτBx dτ = e−kτ /2eiτBx dτ → eiτBx = x k bk τ=0 2π R R 2π as k → ∞. This proves (4).  Lemma 2.2. Let φ ∈ S (R). (1) The map R → L(X), t 7→ φ(B − t) is uniformly continuous in operator norm. (2) If x ∈ X is such that R kφ(B − t)xk dt < ∞ then R φ(B − t)x dt = φ(0)x. R X R b Proof. The estimate (4) implies Z M α −itξ −isξ ˆ kφ(B − t) − φ(B − s)kL(X) ≤ hξi e − e |φ(ξ)| dξ 2π R Z M α −i(t−s)ξ = hξi e − 1 |φˆ(ξ)| dξ, 2π R and we can use dominated convergence to prove (1). −t2/(2k) To see (2), let again gk(t) = e , k ∈ N. Then we have Z Z φ(B − t)x dt = lim gk(t)φ(B − t)x dt k→∞ R R and Z Z Z 1 −iτt iτB gk(t)φ(B − t)x dt = gk(t)e φb(τ)e x dτ dt R 2π R R Z 1 iτB = gbk(τ)φb(τ)e x dτ. 2π R r Z k 2 = e−kτ /2φb(τ)eiτBx dτ. R 2π iτB As k → ∞ this tends to φb(τ)e x|τ=0 = φb(0)x in k · kX .  The following construction of extrapolation spaces is well established (see, e.g., [7, Sect. 6.3]). As −iB generates a C0-group satisfying (1), B is densely defined and ±i belong to the resolvent set k of B. For k ∈ N, we denote by Xk the Banach space D(B ) equipped with the norm kxkXk := 4 k k(i + B) xkX . We let X0 := X, and for k ∈ N we denote by X−k the completion of X for the −k norm kxkX−k := k(i + B) xk. Then

... ⊆ Xk+1 ⊆ Xk ⊆ ... ⊆ X1 ⊆ X0 = X ⊆ X−1 ⊆ ... ⊆ X−k ⊆ X−(k+1) ⊆ ... with continuous and dense embeddings. For each k ∈ Z there is an operator Bk in Xk with D(Bk) = Xk+1 such that i + Bk : Xk+1 → Xk is an isometry, Bk is an extension of Bk+1 and Bk+1 is the part of Bk in Xk+1 (we recall that, for an operator A in a Banach space X and another Banach space Y ⊆ X, the part AY of A in Y is the operator given by the restriction of A to D(AY ) = {y ∈ Y ∩ D(A): Ay ∈ Y }). Moreover, we set X := T X and X := S X (as we do not need topologies on these ∞ k∈N k −∞ k∈N −k spaces, we simply consider them as sets). By similarity, each operator −iBk generates a C0-group −itBk (e )t∈R in Xk, and this group satisfies again (4) in Xk. So everything we have done so far can be carried over from X to any of the spaces Xk, k ∈ Z. Moreover, we have consistency of spaces and operators in the sense of (Xk)l = Xk+l and (Bk)l = Bk+l for all k, l ∈ Z. For simplicity, we omit in notation the subscript for the different versions of B.

Remark 2.3. (a) By Lemma 2.1 we have φ(B): X−∞ → X∞ for any φ ∈ S (R). p (b) In the case of the translation group on X = L (R), 1 < p < ∞, we obtain the scale of Sobolev k,p T k,p spaces Xk = W (R), k ∈ Z, and X∞ = k≥0 W (R), which is sometimes denoted by DLp and 0 can be equipped with the natural Fr´echetspace topology. In this notation X−∞ = (DLp0 ) would be the of DLp0 . R R Lemma 2.4. Let x ∈ X−∞ and φ, ψ ∈ ( ). Then kφ(B − t)ψ(B)xk dt < ∞ and φ(B − S R R X R t)ψ(B)x dt = φb(0)ψ(B)x.

Proof. By Lemma 2.2 the integrand is continuous in k · kX . For any k ∈ N we have k kφ(B − t)ψ(B)kL(X−k,X) = kφ(B − t)(i + B) ψ(B)kL(X). k Thus it suffices to estimate kφ(B − t)ψe(B)kL(X) where ψe := (i + (·)) ψ ∈ S (R). We simply use the estimate (4) (for the definition of Vgf we refer to the appendix): Z M α kφ(B − t)ψe(B)kL(X) ≤ hξi |F {φ(· − t)ψe}(ξ)| dξ 2π R Z M α = hξi |(Vφ ψe)(t, ξ)| dξ. 2π R By Lemma A.1, the integral is finite for each t ∈ R and can be integrated with respect to t. 

3. Modulation type spaces associated with B With the scale of extrapolation spaces from the previous section at hand we can now give the precise definition of the modulation type spaces associated with B. Definition 3.1. For s ∈ R, q ∈ [1, ∞) and φ ∈ S (R) \{0} we define Z 1/q s  s q  (6) M := {x ∈ X : kxk s := hti kφ(B − t)xk dt < ∞} X,q,φ −∞ MX,q,φ X R and s s (7) M := {x ∈ X : kxk s := sup hti kφ(B − t)xk < ∞}. X,∞,φ −∞ MX,∞,φ X t∈R We start with a lemma on simple inclusions. 5 s 1 Lemma 3.2. We have X,→ MX,q,φ for s < − q (and for s ≤ 0 if q = ∞). If ρb(0) = 1 then s 1 MX,q,ρ ,→ X for s > q0 (and s ≥ 0 if q = 1). Proof. By (4) we have for x ∈ X the estimate

M α s (8) kxkM s ≤ kh·i φbk 1 kh·i kLq kxkX X,q,φ 2π L s 1 where kh·i kLq < ∞ for s < − q (and for s ≤ 0 if q = ∞). This proves the first assertion. 1 s Take now ρ ∈ S (R) with ρb(0) = 1 and s > q0 (s ≥ 0 if q = 1). For x ∈ MX,q,ρ we then have by H¨older Z −s s −s kρ(B − t)xk dt ≤ kh·i k q0 kh·i ρ(B − ·)xk q = kh·i k q0 kxk s . X L L (X) L MX,q,ρ R R Now we use Lemma 2.2 to obtain ρ(B − t)x dt = x and consequently kxk kxk s . X . MX,q,ρ 

We now prove that different φ ∈ S (R) \{0} induce equivalent norms. We also show that the continuous type norms involving integrals can be replaced by semi-discrete norms involving sums. We shall study fully discrete norms below.

Theorem 3.3. Let s ∈ and q ∈ [1, ∞]. Then all norms k · k s , φ ∈ ( ) \{0}, are R MX,q,φ S R equivalent. Moreover, they are equivalent to the norms given for φ ∈ S (R) \{0} by 1/q ∼  X s q kxkM s := sup hki kφ(B − k + t)xkX , X,q,φ t∈[0,1] k∈Z again with obvious modification for q = ∞.

∼ Proof. It is clear that kxkM s kxk s for all q ∈ [1, ∞] and that the reverse inequality X,q,φ . MX,q,φ ∼ holds for q = ∞. So it rests to show kxk s kxkM s for fixed φ, ψ ∈ S ( ) \{0} and MX,q,ψ . X,q,φ R q ∈ [1, ∞]. We give the proof for q ∈ [1, ∞), the modifications for q = ∞ being obvious. Let φ ∈ ( ) \{0}, c := kφk2 , and set φ := c−1φ. Then R φ(r)φ(r) dr = 1. We let S R L2 e R e Z 1 ρ(t) := φ(r + t)φe(r + t) dr, t ∈ R. 0 Then ρ ∈ ( ), 0 ≤ ρ ≤ 1, and R ρ(r − t) dt = 1 for all r ∈ . For ψ ∈ ( ) \{0} and t ∈ [0, 1] S R R R S R we have, using Lemma 2.4, 1/q  X sq q  hki kψ(B − k + t)xkX k Z 1/q  X sq q  = hki kψ(B − k + t) ρ(B − k + σ)x dσkX k R Z 1 Z 1 1/q X  X sq q  ≤ hki kψ(B − k + t) (φφe )(B − k + j + σ + r)x dr dσkX j k 0 0 We write k + j for j: Z 1 Z 1 1/q X  X sq q  = hk + ji k ψ(B − (k + j) + t)(φφe )(B − k + σ + r)x dr dσkX j k 0 0 6 sq sq |s|q Now we use hk + ji . hki hji and Jensen: Z 1 Z 1 1/q X |s| X sq q  . hji hki kψ(B − (k + j) + t)(φφe )(B − k + σ + r)x dr dσkX j k 0 0  X |s|  ≤ hji sup kψ(B − (k + j) + t)φe(B − k + σ + r)kX j σ,r∈[0,1],k∈Z Z 1 1/q  X sq q  × sup hki kφ(B − k + σ + r)xkX dσ r∈[0,1] k 0 = I1 × I2.

For I1 we use (4) and let s := σ + r ∈ [0, 2]. As in the proof of Lemma 2.4 we then obtain

kψ(B − (k + j) + t)φe(B − k + σ + r)kX α α . kh·i F {ψ(· − j + t)φe(· + s)}kL1 = kh·i F {ψ(· − j + t − s)φe}kL1 Z α ≤ hξi |(Vψφe)(j + s − t, ξ)| dξ, R −β −γ where the integrand is . hξi hji for all β, γ > 0 by Lemma A.1. Hence I1 is finite. For the estimate of I2 we fix r ∈ [0, 1] and estimate the term in brackets by Z 1/q  sq q  . hσi kφ(B − σ + r)xkX dσ , R which is independent of r and equals kxk s . MX,q,φ  s s Definition 3.4. According to Theorem 3.3 we can define MX,q := MX,q,φ for s ∈ R, q ∈ [1, ∞] where φ ∈ S (R) \{0} is arbitrary. As announced above we now give fully discrete norms for special ρ ∈ S (R) \{0}. Proposition 3.5. Let ρ ∈ ( ) \{0} satisfy supp ρ ⊆ [−1, 1] and P ρ(· − k) = 1 on . Then S R k∈Z R 1/q d  X sq q  kxk s := hki kρ(B − k)xk MX,q,ρ X k∈Z s (obvious modification in case q = ∞) defines an equivalent norm on MX,q for any s ∈ R and q ∈ [1, ∞].

d ∼ Proof. It is clear that kxk s ≤ kxk s . To see the reverse estimate we observe that, for MX,q,ρ MX,q,ρ P2 t ∈ [0, 1], ρ(· + t) = j=−1 ρ(· + t)ρ(· + j). Hence we have, for k ∈ Z and t ∈ [0, 1], 2 X kρ(B − k + t)xkX = (ρ(B − k + t)ρ(B − k + j))x X j=−1 2 X ≤ kρ(B − k + t)ρ(B − k + j)xkX j=−1 2 X . kρ(B − k + j)xkX , j=−1 ∼ d since supk∈ ,t∈[0,1] kρ(B − k + t)kL(X) < ∞ by (4). Now kxk s kxk s follows. Z MX,q,ρ . MX,q,ρ  7 s+1 s Proposition 3.6 (Lifting property). The operator i + B is an isomorphism MX,q → MX,q for any s ∈ , q ∈ [1, ∞]. Moreover, M s (B) = M s+1 (B ) with equivalent norms. R X,q X−1,q −1

q Proof. For φ ∈ S (R)\{0}, φ1(r) := rφ(r), and x with t 7→ φ1(B −t)x ∈ Ls, the basic observation q q s+1 is that t 7→ Bφ(B − t)x ∈ Ls is equivalent to t 7→ tφ(B − t)x ∈ Ls. Hence we have x ∈ MX,q if s s and only if x ∈ MX,q(R) and Bx ∈ MX,q(R). The assertions now follow easily. 

1 As a corollary, we can replace X−∞ in Definition 3.1 by any X−k, k > q0 − s if q ∈ (1, ∞] and k ≥ −s if q = 1.

s Proposition 3.7 (Completeness). For s ∈ R and q ∈ [1, ∞] the space MX,q,ρ is a Banach space.

1 s Proof. We give the proof here for s > q0 (and s ≥ 0 if q = 1) and can exploit MX,q,ρ ,→ X. For the general case we then use the lifting property. s q Let (x ) be Cauchy for k · k s . Then (h·i ρ(B − ·)x ) is Cauchy in L ( ,X) and there exists n MX,q,ρ n R s q s s q h·i f ∈ L (R,X) such that h·i ρ(B − ·)xn → h·i f in the norm of L (R,X). The assumption on s implies that (xn) is Cauchy in k·k so that xn → x ∈ X in k·kX . But then ρ(B −t)xn → ρ(B −t)x in k · kX for any t ∈ R. Thus f(t) = ρ(B − t)x for a.e. t ∈ R, and dominated convergence yields s x ∈ M and x → x in k · k s . X,q,ρ n MX,q,ρ 

We close this section by the following result on denseness and the group induced by (e−itB) in modulation type spaces associated with B.

s Proposition 3.8. For q ∈ [1, ∞) and any s ∈ R, X∞ is dense in MX,q. The part of −iB in s s+1 s MX,q which has domain MX,q generates a C0-group in MX,q that is consistent with the group −itB (e )t∈R we started with and satisfies again (1).

0 Proof. By lifting we resort to s > 1/q (s ≥ 0 if q = 1). Choose ρ ∈ S (R) \{0} as in Proposi- s P tion 3.5. Take x ∈ MX,q and, for n ∈ N, set xn := |l|≤n ρ(B − l)x. Then  ρ(B − k)x , |k| ≤ n − 1 X  ρ(B − k)xn = ρ(B − l)ρ(B − k)x = , |l|≤n  0 , |k| ≥ n + 2 so clearly x ∈ X and x ∈ T M s . Moreover n ∞ n s∈R X,q

q X sq q kx − xnk s ≤ C hki kρ(B − k)xk → 0 (n → ∞). Mx,q X |k|≥n

s −itB Clearly, the spaces MX,q are invariant under the group operators e and the induced group s still satisfies (1). Similarly, MX,q is invariant under resolvents of B and norm estimates in X carry s s s+1 over to MX,q. The resolvent operators induce an operator B in MX,q with domain MX,q . s+1 s+1 s By X∞ ⊆ MX,q , the domains MX,q of B is dense in MX,q. Now Hille-Yosida implies that the −itB s induced group (e ) is strongly continuous in MX,q. 

We shall study the case q = ∞ in the next section. 8 4. The case of bi-continuous groups In our considerations, we also want to include the translation group in spaces such as L∞ where it is not strongly continuous and the supposed “generator” is not densely defined. However, the ∗ ∞ s translation semigroup is weak -continuous on L . Also, in our spaces MX,∞ the induced group is not densely defined, but it is strongly continuous for a weaker norm (namely in X−k if k is sufficiently large). So we resort to the theory of bi-continuous (semi-)groups and recall basic definitions and properties (cf. [11]).

Assumption 4.1. Let X be Banach space with norm k·kX and let τX be a locally convex topology on X such that

(i) Any norm-bounded τX -Cauchy sequence converges in (X, τX ). (ii) The embedding (X, k · kX ) ,→ (X, τX ) is continuous. 0 (iii) The space (X, τX ) is norming for X, i.e. for any x ∈ X we have 0 kxkX = sup{|hx, ψi| : ψ ∈ (X, τX ) , kφkX0 ≤ 1}, 0 where kψk 0 := sup |hz, ψi| is the usual norm on the dual space (X, k · k ) of X kzkX ≤1 X (X, k · kX ).

By (iii), τX is necessarily Hausdorff. In the following we use the notation 0 ΦX (τX ) := Φ(τX ) := {ψ ∈ (X, τX ) : kψkX0 ≤ 1}, then we can rewrite (iii) as kxk = sup |hx, ψi| for any x ∈ X. Observe that (iii) is X ψ∈Φ(τX ) invariant if we multiply k · kX by a positive constant. We rephrase [11, Def. 3] for our purposes. Observe that here we are only interested in the poly- nomially bounded case.

Definition 4.2. Suppose that τX is as above and that (T (t))t∈R is a group satisfying (1). Then (T (t)) is called bi-continuous (with respect to τX ) if

(i) R → X, t 7→ T (t)x is τX -continuous for any x ∈ X, (ii) for any a > 0 the set {T (t): |t| ≤ a} is bi-equicontinuous, i.e. for every k · k-bounded sequence (xn) in X that is τX -convergent to 0 we have

τX − lim T (t)(xn) = 0 n→∞ uniformly in |t| ≤ a.

Following [11, Def. 9], the generator of (T (t)) is the unique operator A on X such that Z ∞ (9) R(λ, A)x = e−λtT (t)x dt, x ∈ X, Re λ > 0. 0 R a −λt The integral here is the limit lima→∞ in operator norm of the integrals 0 e T (t)x dt which in turn have to be understood as τX -Riemann integrals (we refer also to Proposition A.2 in the appendix and to the arguments in the proof of Proposition 4.4). Then (see [11, Cor. 13]) A is bi-closed, i.e. if (xn) is a norm-bounded sequence, τX -convergent to x and such that (Axn) is norm-bounded and τX -convergent to y, then x ∈ D(A) and Ax = y. Moreover, the domain D(A) of A is bi-dense in X, i.e. for any x ∈ X there is a norm-bounded sequence (xn) in D(A) that is τX -convergent to x (see [11, Cor. 13]). The following are our main motivations to include the present section. 9 ∞ Examples: 1. The translation group given by T (t)f = f(· − t) is isometric in X = L (R) = 1 0 ∗ L (R) . It is not strongly continuous, but it is bi-continuous for the . −itB 2. More general, if X is not reflexive and (T (t)) = (e ) is a C0-group in X satisfying (1) then the dual group (T (t)0) in X0 satisfies (1) and is bi-continuous for the weak∗ topology on X0. Its generator is the dual operator (−iB)0 of −iB whose domain is bi-dense in X0. 3. The translation group is also not strongly continuous on the space Cb(R) of bounded and continuous functions equipped with the sup-norm. But it is bi-continuous for the topology τc of uniform convergence on compact subsets of R (see [11]). −itB s 4. In the situation of Section 3, the induced group (e ) is not strongly continuous in MX,∞ (unless B is bounded). We shall see below that it is bi-continuous for the norm of Xk where s+1 k < s − 1 and its generator is the operator −iB with domain MX,∞. In the following we assume

Assumption 4.3. Let (X, k · kX ) be a Banach space and τX a topology on X satisfying As- sumption 4.1. We assume that (T (t))t∈R is a group in X that satisfies (1) and is bi-continuous with respect to the topology τX . As before we denote the generator of (T (t)) by −iB and write T (t) = e−itB. Before we continue we establish the Phillips calculus for the group (T (t)) in X. We shall use that, for a τX -continuous and norm-bounded function f :[a, b] → X and a complex Borel measure R µ ∈ Mα(R), the integral [a,b] f(t) dµ(t) exists in a Riemann sense. For convenience, we prove this in the appendix (cf. Proposition A.2).

Proposition 4.4 (Phillips calculus). For µ ∈ Mα(R) and x ∈ X the limit Z µb(B)x := lim T (t)x dµ(t) a→−∞,b→∞ [a,b] exists in operator norm and x 7→ µb(B) defines a linear operator µb(B) ∈ L(X) satisfying the estimate Z α (10) kµb(B)kL(X) ≤ M hti d|µ|(t). R The map FMα(R) → L(X), µb 7→ µb(B) is an algebra homomorphism. Moreover, if F ⊆ Mα(R) is a k · kMα -bounded subset satisfying Z (11) lim sup htiα d|µ|(t) = 0 a→∞ µ∈F |t|>a then {µb(B): µ ∈ F} is bi-equicontinuous. R Proof. Let µ ∈ Mα(R) and x ∈ X. By Proposition A.2 the integral [a,b] T (t)x dµ(t) exists in a τX -Riemann sense. By Assumption 4.1 (iii) we have

Z Z Z α T (t)x dµ(t) = sup hT (t)x, ψi dµ(t) ≤ M hti d|µ|(t) kxkX . [a,b] ψ∈Φ(τ ) [a,b] [a,b] X X R R Denoting the operator x 7→ [a,b] T (t)x dµ(t) by [a,b] T (t) dµ(t) this estimate implies R [a,b] T (t) dµ(t) ∈ L(X). Moreover, it implies that Z lim T (t) dµ(t) a→−∞,b→∞ [a,b] 10 exists in operator norm. Denoting this limit by µb(B) as in the assertion, the estimate finally shows (10). For the following we observe that, for ψ ∈ Φ(τX ), we have Z Z Z hµ(B)x, ψi = lim h T (t)x dµ(t), ψi = lim hT (t)x, ψi dµ(t) = hT (t)x, ψi dµ(t), b a→−∞ a→−∞ b→∞ [a,b] b→∞ [a,b] R where the last integral is a Lebesgue integral. For the algebra property we only have to show multiplicativity, i.e. for µ, ν ∈ Mα(R) we have to show µb(B)νb(B) = µ[∗ ν(B). We do this by applying functionals ψ ∈ Φ(τX ): Z hµ[∗ ν(B)x, ψi = hT (t)x, ψi d(µ ∗ ν)(t) R Z Z = hT (t + s)x, ψi dµ(t) dν(s) R R Z Z = hT (s) T (t)x dµ(t), ψi dν(s) R R = hνb(B)µb(B)x, ψi.

Now suppose that F ⊆ Mα(R) is k · kMα -bounded and satisfies (11). Let (xn) be a norm-bounded sequence that is τX -convergent to 0. Let p be continuous seminorm and ε > 0. We may assume p ≤ k · kX . By assumption we find a > 0 such that Z sup htiα d|µ|(t) ≤ ε. µ∈F |t|>a For µ ∈ F we write ! Z Z

p(µb(B)xn) ≤ p T (t)xn dµ(t) + T (t)xn dµ(t) . [−a,a] |t|>a X

Using τX -continuity of p and (10) we obtain Z Z α p(µb(B)xn) ≤ p(T (t)xn) d|µ|(t) + M hti d|µ|(t) [−a,a] |t|>a

≤ sup p(T (t)xn) sup kµkMα + Mε. |t|≤a µ∈F

By Assumption 4.3 we have sup|t|≤a p(T (t)xn) → 0 as n → ∞, and this implies the assertion. 

−α The result on bi-equicontinuity can be used to show that {hti eT (t): t ∈ R} is bi-equicontinuous for any αe > α. It can also be used to reprove bi-equicontinuity assertions on (powers of) resolvent operators in [11]. Remark 4.5 (Extrapolation scale). Also under Assumption 4.3, it is possible to construct the scale of Banach spaces (Xk, k · kXk )k∈Z such that i + B : Xk → Xk−1 is an isometry for every k ∈ Z, since the construction essentially only uses that ±i ∈ ρ(B) (we refer to, e.g., [7, Sect. 6.3]). Similarly, we can use the operator i + B and its powers to transfer the topology τX to the spaces

Xk, k ∈ Z, and we shall denote the induced topologies by τXk . In this way i + B :(Xk, τXk ) →

(Xk−1, τXk−1 ) is an isomorphism for each k ∈ Z. Moreover, in each space Xk we have an induced −itB group (e ) which satisfies (1) and is bi-continuous with respect to τXk . Its generator is the operator −iB with domain Xk+1. 11 s We now comment on the construction of the spaces MX,q under the given assumptions. By Proposition 4.4 the operators φ(B) are well-defined for φ ∈ S (R). Moreover, we still have the estimate (4). In particular, the argument which shows continuity of t 7→ φ(B − t) in operator norm of X is still valid. We also note that, if we apply ψ ∈ Φ(τX ), we have 1 Z (12) hφ(B)x, ψi = φb(τ)heiτBx, ψi dτ 2π R where the integral is a Lebesgue integral. Using this observation we can apply functionals ψ ∈ Φ(τX ) in the argument of the proof of Lemma 2.1 (1). Thus we obtain that the assertions of Lemma 2.1 (1)-(3) still hold. Concerning the assertion of Lemma 2.1 (4) we take a continuous seminorm p for τX and have (with notations as in the proof of Lemma 2.1) Z r k −kτ 2/2 iτB p(gk(B)x − x) ≤ e p(e x − x) dτ → 0 (k → ∞). R 2π S Hence the set ρ∈S ρ(B)(X) is bi-dense in X and ρ(B)x = 0 for all ρ ∈ S (R) still implies x = 0. s Now it is obvious that the spaces MX,q(B) can be defined as before. We summarize all this in Proposition 4.6. Under Assumption 4.3 the assertions of Lemma 2.1 (1)-(3) still hold. In the assertion of Lemma 2.1 (4) “dense” has to be replaced by “bi-dense”. The assertions of Lemma 2.2 s and Lemma 2.4 still hold. We can define the spaces MX,q,φ(B) as in Definition 3.1. The assertions of Lemma 3.2, Theorem 3.3, and of the Propositions 3.5, 3.6, and 3.7 are still valid.

−itB s We now study the induced group (e ) and its properties in the spaces MX,q and give the analog of Proposition 3.8.

s s+1 Proposition 4.7. For q ∈ [1, ∞), the part of −iB in MX,q which has domain MX,q generates a s −itB C0-group in MX,q that is consistent with the group (e )t∈R we started with and satisfies again s s+1 (1). For q = ∞, the part of −iB in MX,∞ which has domain MX,∞ generates a bi-continuous s s group in MX,q w.r.t. the topology τXk restricted to MX,∞ where k < s−1. The group is consistent −itB with the group (e )t∈R we started with and satisfies again (1). s Observe that the range of k in the assertion is such that MX,∞ ,→ Xk.

s −itB Proof. As before, the spaces MX,q are invariant under the group operators e and the induced s group still satisfies (1). Similarly, MX,q is invariant under resolvents of B and norm estimates in s s s+1 X carry over to MX,q. The resolvent operators induce an operator B in MX,q with domain MX,q . s+1 s For q ∈ [1, ∞) the space MX,q is dense in MX,q (by the same arguments as in the proof of Proposition 3.8). Again, Hille-Yosida implies that the induced group (e−itB) is strongly continuous s in MX,q if q ∈ [1, ∞). −itB s We turn to the case q = ∞. For s ∈ R, the induced group (e ) in the space MX,∞ is bi- continuous with respect to the topology τ | s whenever k ∈ satisfies s > k + 1. By the Xk MX,∞ Z lifting property it suffices to prove the case k = 0, s > 1. We denote by τM the restriction of τX s s to MX,∞. First we show that τM satisfies Assumption 4.1 in MX,∞ in place of X. The inclusion s s M ,→ (X, k · k ) implies (ii). For the proof of (i) let (x ) be k · k s -bounded in M and X,∞ X n MX,∞ X,∞ τM -Cauchy. Then (xn) is also k · kX -bounded in X and τX -Cauchy and thus converges in (X, τX ) s by (i) for τX in X. We denote the limit by x and have to show x ∈ MX,∞. Let ρ ∈ S (R) \{0}. 12 Taking ψ ∈ ΦX (τX ) we have, for any t ∈ R,

|hρ(B − t)x, ψi| = lim |hρ(B − t)xn, ψi| ≤ sup kρ(B − t)xnkX . n n

Hence using (iii) for τX in X we get kρ(B − t)xkX ≤ supn kρ(B − t)xnkX for every t ∈ R which implies in turn s s kxkM s = suphti kρ(B − t)xkX ≤ suphti kρ(B − t)xnkX = sup kxnkM s < ∞. X,∞,ρ t t,n n X,∞,ρ s So x ∈ MX,∞,ρ, and (i) is proved. s For the proof of (iii) we take x ∈ MX,∞,ρ. For t ∈ R we then have, by (iii) for τX in X,

kρ(B − t)xkX = sup |hρ(B − t)x, ψi|, ψ∈ΦX (τX ) and for every ψ ∈ ΦX (τX ) we have Z s 1 s hti hρ(B − t)x, ψi = lim hρ(B − r)x, hri 1[t−δ,t+δ](r)ψi dr. δ→0+ 2δ R 0 1 s Defining ψδ : R → X by ψδ(r) = 2δ hri 1[t−δ,t+δ](r)ψ we have kψδkL1(X0) ≤ 1. Then we see easily that the functional Z Z t+δ 1 s Ψδ : x 7→ hρ(B − r)x, ψδ(r)i dr = h hri ρ(B − r)x dr, ψi R 2δ t−δ s is τM -continuous on MX,∞,ρ and −s |hx, Ψ i| ≤ kxk s kh·i ψ k 1 0 ≤ kxk s . δ MX,∞,ρ δ L (X ) MX,∞,ρ

So we have Ψ ∈ Φ s (τ ). Using the above we thus have δ MX,∞,ρ M s hti kρ(B − t)xk ≤ sup |hx, Ψ i| ≤ sup{|hx, Ψi| :Ψ ∈ Φ s (τ )}. X δ MX,∞,ρ M δ s Taking the sup over t ∈ R we obtain (iii) for τM in MX,∞,ρ. The same arguments can be used for d the norms k · k s where ρ satisfies the additional assumptions that are needed. MX,∞,ρ −itB s Now we show that the induced group (e ) in MX,∞ is bi-continuous with respect to τM by checking the conditions in Definition 4.2. Property (i) is obvious from (i) for τX in X. Property (ii) also follows from (ii) for τX in X and Assumption 4.1 (ii).  Still under the Assumptions 4.1 and 4.3 we comment on another choice of a topology that makes s the induced group on MX,∞(B) bi-continuous.

[ Remark 4.8. We denote by X the k · kX -closure of D(B) in X and by k · kX[ the restriction of [ [ [ [ −itB[ k·kX to X . Then the restriction (T (t) ) of (T (t)) to X is strongly continuous, and T (t) = e [ [ [ [ [ where B is the part of B in X . Denoting by (Xk)k∈Z the extrapolation scale w.r.t. X and B [ [ [ we clearly have Xk+1 ⊆ Xk ⊆ Xk for any k ∈ Z which implies X−∞ = X−∞ and X∞ = X∞. By the results of Section 2 we conclude s s [ MX,∞(B) = MX[,∞(B ), s > 1. −itB2 s Now, Proposition 4.7 tells us that, for s > 1, the group (e ) in MX,∞(B) is bi-continuous s w.r.t. to the topology induced by k · kX , restricted to MX,∞(B). 13 [ We also want to remark that a similar argument applies to, e.g., MX,1(B) in place of X : we have

X2 ,→ MX,1 ,→ X, so MMX,1,∞(B) ,→ MX,∞(B). On the other hand, we have, for a suitable ρ and any k ∈ Z, by an argument as in the proof of Proposition 3.8 1 s s X s X hki kρ(B − k)xkMX,1 = hki kρ(B − l)ρ(B − k)xkX ≤ Chki kρ(B − l)xk, l l=−1 so that kxkM s kxkM s . We conclude that MX,1,∞ . X,∞ M s (B) = M s (B), s > 1, X,∞ MX,1,∞ −itB2 s as Banach spaces. Again, Proposition 4.7 tells us that, for s > 1, the group (e ) in MX,∞(B) s is bi-continuous w.r.t. to the topology induced by k · kMX,1 , restricted to MX,∞(B). We remark that, in the same way, it can be shown that we have s s+σ M σ (B) = M (B) MX,r(B),q X,q for all s, σ ∈ R and r, q ∈ [1, ∞] which yields more choices for an appropriate topology on s MX,∞(B).

−itB2 s 5. The group e in the spaces MX,q(B) In this section we briefly consider a functional calculus of unbounded operators for B in X before −itB2 we concentrate on the operators e , t ∈ R, and their properties in the modulation type spaces s ∞ ∞ ∞ MX,q(R). If F : R → C is C , then F φ ∈ Cc (R) ⊆ S (R) for any φ ∈ Cc (R) and we define the operator F (B) in X by ∞ x ∈ D(F (B)) and F (B)x = y :⇐⇒ ∀φ ∈ Cc (R):(F φ)(B)x = φ(B)y. An application of Lemma 2.2 (2) yields that F (B) is a well-defined single-valued linear operator (the extension procedure used here is the upper extension in the sense of [9], note that the functional calculus we started with is upper non-degenerate in the sense of [9], in this context and for the following poperties we also refer to [7, Chapter 1] and [10, Chapter 2]). Moreover, F (B) is a closed operator in X and the map F 7→ F (B) has the properties of an unbounded functional ∞ ∞ calculus: C (R) is an algebra and for F,G ∈ C (R) it is not hard to see that we have (13) F (B) + G(B) ⊆ (F + G)(B) and F (B)G(B) ⊆ (FG)(B) where D(F (B) + G(B)) := D(F (B)) ∩ D(G(B)) and D(F (B)G(B)) := {x ∈ D(G(B)) : G(B)x ∈ D(F (B))} equals D((FG)(B)) ∩ D(G(B)). Examples of such F are: −1 (a) If F (r) = (λ − r) where λ ∈ C \ R, then F (B) = R(λ, B). −itr −itB (b) If F (r) = e where t ∈ R, then F (B) = T (t) = e . (c) If F (r) = rk, then F (B) = Bk. −itr2 (d) We are especially interested in the case F (r) = e for t ∈ R. In case (a) and (b), F (B) is already in the Phillips calculus: in (a) by the usual representation of the resolvent operators as Laplace transform of the semigroup, and in (b) we have µ = δt in (2). We shall study (d) in the following.

Proposition 5.1. Suppose that Assumptions 4.1 and 4.3 hold. There is a constant Cα only depending on α and M such that, for all s ∈ R and all q ∈ [1, ∞], we have −itB2 α+1/2 s+α (14) ke xkM s ≤ Cαhti kxk s+α , t ∈ R, x ∈ M . X,q MX,q X,q 14 −itB2 s In case α = 0, (e ) is a group of bounded operators in MX,q(B) for each s ∈ R. If q ∈ [1, ∞) then this group is strongly continuous, for q = ∞ this group is bi-continuous w.r.t. the restriction s of τXk to MX,∞(B) where k < s − 1.

Proof. We first prove the estimate (14). We take φ ∈ S (R) \{0} and show −itB2 α+1/2 α (15) ke φ(B − k)kL(X) ≤ Cαhti hki , k, t ∈ R. This will prove (14) since we then have

−itB2 2 α+1/2 α ke φ (B − k)xkX ≤ Cαhti hki kφ(B − k)xkX , which in turn implies −itB2 α+1/2 ke xkM s ≤ Cαhti kxk s+α . X,q,φ2 MX,q,φ For the proof of (15) we write

2 2 2 e−itB φ(B − k) = eitk e−2iktBe−it(B−k) φ(B − k) and use (1) and (4) (the latter for B − k in place of B) to obtain 2 −itB2 M α α ke φ(B − k)k ≤ h2kti kh·i ψbtk 1 , L(X) 2π L −itr2 where ψt ∈ S (R) is given by ψt(r) = e φ(r). Then we use h2ktiα ≤ chtiαhkiα.

α In order to get the right dependence on t and α we calculate kh·i ψbtkL1 for the special case φ(r) = e−r2 . Then r −itr2 −r2 −(1+it)r2 π −ξ2/(4(1+it)) ψt(r) = e e = e , ψbt(ξ) = e 1 + it as can be seen by analytic continuation. Hence Z α √ −1/2 α −ξ2/(4hti2) kh·i ψbtkL1 = π hti hξi e dξ. R For α = 0 we substitute ξ = htiη and obtain Z √ 1/2 −η2/4 kψbtkL1 = π hti e dη. R For α > 0 we use hξiα ≤ 2α/2(1 + |ξ|α) and get with the same substitution as before

Z 2 2 Z 2 hti−1/2 |ξ|αe−ξ /(4hti ) dξ = htiα+1/2 |η|αe−η /4 dη. R R This proves (15). We also infer from Proposition 4.4 that, for any a, N > 0 and φ ∈ S (R), the set

2 (16) {eitB φ(B − k): |t| ≤ a, |k| ≤ N} ⊆ L(X) is bi-equicontinuous w.r.t. τX . Now let α = 0. The group property follows from (13). We have to 2 s+2 prove continuity properties and that −iB with domain MX,q is the generator. We shall use 15 −itB2 s Case q < ∞: We show that ke x − xk s → 0 as t → 0 for any x ∈ M (B). So let MX,q X,q s x ∈ MX,q(B). For the calculation of the norm we take a φ ∈ S (R) \{0} with compact support. −it(·)2 Then we have, for any k ∈ R,(e − 1)φ(· − k) → 0 in S (R), which implies (again by (4)) −itB2 k(e − I)φ(B − k)xkX → 0 (t → 0). Since q < ∞ the assertion now follows by dominated convergence. The argument is the same if the original group (e−itB) is just bi-continuous in the sense of Section 4. −itB2 s Case q = ∞: We have to show that, for s > 1, the group (e ) is bi-continuous in MX,∞(B) s w.r.t. the restriction of the topology τX to MX,∞(B)), which we again denote by τM . We already s know that τM satisfies Assumption 4.1 in MX,∞(B). So we only have to show (i) and (ii) of s Definition 4.2. We start with (ii) and take a sequence (x ) in M (B) such that kx k s ≤ n X,∞ n MX,∞(B) C and xn → 0 w.r.t. τX , and we let a, ε > 0. We choose ρ ∈ S (R) as in Proposition 3.5. Since P s s < 1, y = k ρ(B − k)y for each y ∈ MX,∞ where the series converges in k · kX and we can find N > 0 such that X −itB2 X −s s −itB2 0 X −s k ρ(B − k)e xnkX ≤ hki hki kρ(B − k)e xnkX ≤ C hki ≤ ε |k|>N |k|>N |k|>N 0 −itB2 for any n ∈ , |t| ≤ a, where C := C sup ke k s . For a τ -continuous seminorm N |t|≤a L(MX,∞) X p ≤ k · kX and |t| ≤ a we then have −itB2 X −itB2  p(e xn) ≤ p e ρ(B − k)xn + ε, |k|≤N where the sum tends to 0 uniformly in t as n → ∞ by bi-equicontinuity of the set in (16). Now s s −itB2 let x ∈ MX,∞(B). By MX,∞ ,→ MX,1 ,→ X,→ (X, τX ) we get τX -continuity of t 7→ e x from continuity in k · kMX,1 (the case q = 1 is already proved). The generation property is checked via resolvents and the Phillips calculus.  Remark 5.2. Taking into account Remark 4.8 we also obtain that, for s > 1, the group (eitB2 ) s s is bi-continuous in MX,∞(B) w.r.t. the norm-topology of X restricted to MX,∞(B) or w.r.t. the s norm-topology of MX,1(B), restricted to MX,∞(B). Remark 5.3. Concerning only boundedness of operators F (B), the more general result is, of course, the following (cf. also [6, Thm. 17(1)] for the classical setting): Take ρ ∈ S (R) \{0} with compact support and suppose that the set {F (B)ρ(B − k): k ∈ R} ⊆ L(X) is uniformly bounded in operator norm. Then F (B) acts as a bounded operator in every space s MX,q, s ∈ R, q ∈ [1, ∞].

6. Application to a nonlinear Schrodinger¨ equation We illustrate our results briefly by a simple application. The cubic nonlinear Schr¨odinger equation (NLS) in one space dimension is  iu + u ± |u|2u = 0, t ∈ , x ∈ (17) t xx R R u(0, x) = u0(x), x ∈ R. d We take T (t)f = f(· − t), the right translation group, as in Example 1.2, hence B = −i dx , and we consider the function space X = Cb(R) of bounded continuous on R, which is an algebra 16 for pointwise multiplication. Denoting by BUC(R) the space of bounded uniformly continuous functions on R we have ∞ [ ∞ L (R) = BUC(R) ⊆ X ⊆ L (R). s s s Thus MX,∞(B) equals the classical modulation space ML∞,∞(B) = M∞,∞(R). Since the trans- lation group is bi-continuous on X w.r.t. the topology τc of uniform convergence on compact 2 intervals, Proposition 5.1 tells us that, for s > 1, the Schr¨odinger group (eitdx ) is bi-continuous on s s s M∞,∞(R) w.r.t. the topology τc restricted to M∞,∞. On the other hand, M∞,∞(R) is an algebra (see, e.g., [4]), moreover pointwise multiplication is τc-continuous, at least on k·k∞-bounded sets. We rewrite (17) as a fixed point equation in the space

b s s s Cτc ([0,T ],M∞,∞(R)) := {v : [0,T ] → M∞,∞(R): v is k · kM∞,∞ -bounded and τc-continuous },

s which equipped with the norm kvk∞ := supt∈[0,T ] kv(t)kM∞,∞ is a Banach space. The fixed point equation is Z t itd2 i(t−s)d2 2  (18) u(t) = e x u0 ± i e x |u(s)| u(s) ds, t ∈ [0,T ]. 0 b s We call a solution u ∈ Cτc ([0,T ],M∞,∞(R)) a mild solution of (17). The only thing that we now need to solve this via Banach’s Fixed Point Theorem in the usual way is the following on the convolution part.

2 itdx b s Lemma 6.1. The convolution with the semigroup (e ) maps Cτc ([0,T ],M∞,∞) into itself and we have the estimate

2 i(·)dx 1/2 b s ke ∗ vk∞ ≤ C0T hT i kvk∞, v ∈ Cτc ([0,T ],M∞,∞), where C0 is the constant from Proposition 5.1.

We omit the easy proof. By standard means (see, e.g., [2, Proof of Theorem 1.1]) we then have

s Proposition 6.2. Let s > 1 and u0 ∈ M∞,∞(R). Then there exists T > 0 only depending on b s s ku0kM∞,∞ such that (17) has a unique mild solution u ∈ Cτc ([0,T ],M∞,∞(R)).

s Remark 6.3. Doing the fixed point argument in the space of k · kM∞,∞ -bounded and k · k∞- s continuous or in the space of k · kM∞,∞ -bounded and k · kM∞,1 -continuous functions, which is possible since pointwise multiplication is also continuous for these norms, yields existence of a more regular solution. However, using the τc-topology we get uniqueness in a larger space.

Appendix A. Two auxiliary results Here we provide proofs for a well-known result on the short time Fourier transform and for the contruction of τX -Riemann type integrals with respect to measures µ ∈ M (R). 0 Fix g ∈ S (R)\{0}. The short-time Fourier transform with window g of f ∈ S (R) is the function Vgf : R × R → C is defined by Z −iyξ iξ(·) (19) Vgf(x, ξ) := e f(y)g(y − x) dy = hf, e g(· − x)i, R 2 where the duality bracket extends the usual scalar product in L (R). We shall only need that Vg maps S (R) to rapidly decreasing functions. 17 Lemma A.1. For g ∈ S (R) \{0} and f ∈ S (R) the function k l (x, ξ) 7→ hxi hξi Vgf(x, ξ) is bounded on R × R for all k, l > 0. This is well-known but we reprove it here for convenience.

Proof. We have Z |Vgf(x, ξ)| ≤ |f(y)||g(y − x)| dy = |f| ∗ |σg|(x), R k where σg(y) = g(−y). By f, g ∈ S (R) we infer that hxi Vgf(x, ξ) is bounded for any k > 0. For any l ∈ N we use integration by parts to obtain Z l l   l l −iyξ d  l X l (j) (−iξ) V f(x, ξ) = (−1) e f(y)g(y − x) dy = (−1) V (l−j) f (x, ξ). g dyl j g R j=0 Since S (R) is invariant under taking derivatives we can combine both arguments to obtain the assertion. 

For the following result on τX -Riemann type integrals we suppose that Assumption 4.1 holds.

Proposition A.2. Let f :[a, b] → X be a τX -continuous and norm-bounded function and let µ ∈ M (R) be a complex Borel measure. For any partition a = t0 < t1 < . . . < tn = b and any vector (ξ1, . . . , ξn) with ξj ∈ [tj−1, tj) we define the Riemann type sum n X   S(f, tj, ξj) := f(ξj)µ [tj−1, tj) + f(b)µ {b} . j=1

Then the τX -limit of S(f, tj, ξj) exists in X as maxj |tj − tj−1| tends to 0. This limit is denoted R [a,b] f(t) dµ(t). We have the estimate

Z

f(t) dµ(t) ≤ sup kf(t)kX |µ|([a, b]) [a,b] t∈[a,b] X and for any τX -continuous seminorm p we have Z ! Z p f(t) dµ(t) ≤ pf(t) d|µ|(t) ≤ sup pf(t) |µ|([a, b]). [a,b] [a,b] t∈[a,b]

Proof. If kf(t)kX ≤ C we easily get  kS(f, tj, ξj)kX ≤ C|µ| [a, b] . By Assumption 4.1 (i) it thus suffices to show the Cauchy property. So we let δ > 0 and take two partitions (tj) and (sk) such that maxj |tj − tj−1| and maxk |sk − sk−1| are ≤ δ and we take two corresponding vectors (ξj) and (ηk). Then we rewrite X   S(f, tj, ξj) − S(f, sk, ηk) = f(ξel) − f(ηel) µ [ul, ul−1) , l where (ul) is a partition obtained by the union of the tj and the sk and we have {ξel} = {ξj}, {ηel} = {ηk} as sets, but we have to repeat ξj according to the splitting of the interval [tj−1, tj). 18 Then not necessarily ξel ∈ [ul−1, ul) but we have at least |ξel − ul| ≤ δ and |ξel − ul−1| ≤ δ. The same holds for the ηel so that |ξel − ηel| ≤ 2δ. Taking a τX -continuous seminorm p we thus have  X   p S(f, tj, ξj) − S(f, sk, ηk) ≤ p f(ξel) − f(ηel) |µ| [ul−1, ul) l ≤ sup pf(ξ) − f(η)|µ|[a, b). |ξ−η|≤2δ

The assertion thus follows from uniform τX -continuity of f on [a, b]. The p-estimates are immedi- ate, for the norm estimate we use Assumption 4.1 (iii) and the p-estimates for p := |h·, ψi| where ψ ∈ Φ(τX ). 

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Karlsruhe Institute of Technology (KIT), Institute for Analysis, Englerstr. 2, D – 76128 Karlsruhe, Germany, e-mail: [email protected]

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