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Some new properties of composition operators associated with lens maps 2 1 0 Pascal Lefèvre,Daniel Li, 2 Hervé Queffélec, Luis Rodríguez-Piazza n a J January 4,2012 3 ] Abstract. Wegiveexamples ofresultsoncomposition operators connectedwith A lens maps. The first two concern the approximation numbers of those operators F acting on the usual Hardy space H2. The last ones are connected with Hardy- . h Orlicz and Bergman-Orlicz spaces Hψ and Bψ, and provide a negative answer t tothequestionof knowingif allcomposition operators which areweaklycompact a m on a non-reflexive space are norm-compact. [ Mathematics Subject Classification. Primary: 47 B 33 – Secondary: 28 B 1 99 ; 28 E 99 ; 46 E 30 v 6 Key-words. approximation numbers – Carleson measure – compact operator 3 – composition operator – Dunford-Pettis operator – Hardy space – lens map – 6 Orlicz function – Orlicz space – Schatten classes – weakly compact operator 0 . 1 0 1 Introduction 2 1 We first recall the context of this work, which appears as a continuation of : v [9], [10], [11], [14] and [15]. Xi Let D be the open unit disk of the complex plane and (D) be the space of holomorphic functions on D. To every analytic self-mapHϕ: D D (also ar called Schur function), a linear map C : (D) (D) can be→associated ϕ H → H by C (f) = f ϕ. This map is called the composition operator of symbol ϕ. ϕ ◦ A basic fact of the theory ([21], page 13, or [4], Theorem 1.7) is Littlewood’s subordination principle which allows to show that every composition operator induces a bounded linear map from the Hardy space Hp into itself, 1 p< . ≤ ∞ Inthiswork,wearespecificallyinterestedinaone-parameterfamily(asemi- group) of Schur functions: lens maps ϕ , 0 < θ < 1, whose definition is given θ below. They turn out to be very useful in the general theory of composition operators because they provide non trivial examples (for example, they gener- ate compact and even Hilbert-Schmidt operators on the Hardy space H2 [21], page 27). The aim of this work is to illustrate that fact by new examples. 1 We show in Section 2 that, as operatorsonH2, the approximationnumbers of Cϕθ behave as e−cθ√n. In particular, the composition operator Cϕθ is in all Schatten classes S , p > 0. In Section 3, we show that, when one “spreads” p these lens maps, their approximation numbers become greater, and the associ- ated composition operator C is in S if and only if p > 2θ. In Section 4, we ϕ˜θ p answertothenegativeaquestionofH.-O.Tylli: isittruethateveryweaklycom- pact composition operator on a non-reflexive Banach function space is actually compact ? We show that there are composition operators on a (non-reflexive) Hardy-Orliczspaces,whichareweaklycompactandDunford-Pettis,thoughnot compactand that there are compositionoperatorsona non-reflexiveBergman- Orlicz space which are weakly compact but not compact. We also show that therearecompositionoperatorsonanon-reflexiveHardy-Orliczspacewhichare weakly compact but not Dunford-Pettis. We give now the definition of lens maps (see [21], page 27). Definition 1.1 (Lens maps) The lens map ϕ : D D with parameter θ, θ → 0<θ <1, is defined by: (1+z)θ (1 z)θ (1.1) ϕ (z)= − − , z D. θ (1+z)θ+(1 z)θ ∈ − In a more explicit way, ϕ is defined as follows. Let H be the open right θ half-plane, and T: D H be the (involutive) conformal mapping given by → 1 z (1.2) T(z)= − 1+z · We denote by γ the self-map of H defined by θ (1.3) γ (w)=wθ =eθlogw, θ wherelogistheprincipalvalueofthelogarithmandfinallyϕ : D Disdefined θ → by (1.4) ϕ =T 1 γ T. θ − θ ◦ ◦ Those lens maps form a continuous curve of analytic self-maps from D into itself,andanabeliansemi-groupforthecompositionofmapssinceweobviously have from (1.4) and the rules on powers that ϕ (0)=0 and: θ (1.5) ϕθ ϕθ′ =ϕθ′ ϕθ =ϕθθ′. ◦ ◦ Acknowledgement. The fourth-named author is partially supported by a Spanish research project MTM 2009-08934. We thank the referee for a very quick answer and a very careful reading of this paper. 2 2 Approximation numbers of lens maps For every operator A: H2 H2, we denote by → a (A)= inf A R , n=1,2,... n rankR<nk − k its n-th approximation number. We refer to [2] for more details on those ap- proximation numbers. Recall ([24], page 18) that the Schatten class S on H2 is defined by p S = A: H2 H2; (a (A)) ℓp , p>0. p n n { → ∈ } S2 is theHilbert-SchmidtclassandthequantitykAkp = ∞n=1(an(A))p 1/p is a Banach norm on Sp for p 1. (cid:0)P (cid:1) ≥ We can now state the following theorem: Theorem 2.1 Let 0 < θ < 1 and ϕ be the lens map defined in (1.1). There θ are positive constants a,b,a,b depending only on θ such that ′ ′ (2.1) a e b′√n a (C ) ae b√n. ′ − ≤ n ϕθ ≤ − In particular, C lies in all Schatten classes S , p>0. ϕθ p The lower bound in (2.1) was proved in [15], Proposition 6.3. The fact that C lies in all Schatten classes was first provedin [22] under a qualitative form ϕθ (see the very end of that paper). The upper bound will be obtained below as a consequence of a result of O. G. Parfenov ([19]). However, an idea of infinite divisibility, which may be usedinothercontexts,leadstoasimplerproof,thoughitgivesaworseestimate in (2.1): √n is replaced by n1/3. We shall begin by giving this proof, because it is quite short. It relies on the semi-group property (1.5) and on an estimate of the Hilbert-Schmidt norm C in terms of α, as follows: k ϕαk2 Lemma 2.2 There exist numerical constants K ,K such that: 1 2 K K (2.2) 1 C 2 , for all 0<α<1. 1 α ≤k ϕαk2 ≤ 1 α − − In particular, we have K 2 (2.3) a (C ) n ϕα ≤ √n(1 α)· − Proof. The relation (2.3) is an obvious consequence of (2.2) since n a (C ) 2 n a (C ) 2 ∞ a (C ) 2 = C 2 K22 n ϕα ≤ j ϕα ≤ j ϕα k ϕαk2 ≤ (1 α)2 · (cid:2) (cid:3) Xj=1(cid:2) (cid:3) Xj=1(cid:2) (cid:3) − 3 For the first part, let a = cos(απ/2) = sin((1 α)π/2) 1 α and let − ≥ − σ = T(m) (m is the normalized Lebesgue measure dm(t) = dt/2π on the unit circle)be the probability measurecarriedby the imaginaryaxiswhich satisfies: ∞ dy fdσ = f(iy) ZH Z π(1+y2)· −∞ By definition, T, defined in (1.2), is a unitary operator from H2(D,m) into H2(H,σ), and we easily obtain, setting γ(y) = γ (iy) = ei(π/2)αsign(y) y α α | | (wheresignisthesignofyandγ isdefinedin(1.3)),that(see[21],section2.3): α dm dσ 1+γ 2 C 2 = = = | | dσ k ϕαk2 ZT 1−|ϕα|2 ZH 1− 11+−γγ 2 ZH 4Reγ +∞ 1+γ(y)2 dy(cid:12)(cid:12) (cid:12)(cid:12) = | | Z 4a y α π(1+y2) −∞ | | K +∞ 1+y2α dy 2K +∞ yα = dy ≤ 1 αZ yα 1+y2 1 αZ 1+y2 − 0 − 0 4K , ≤ (1 α)2 − where K is a numerical constant. This gives the upper bound in (2.2) and the lower one is obtained similarly. (cid:3) We cannowfinishthefirstproofofTheorem2.1. Letk be apositiveinteger and let α =θ1/k, k so that αk =θ. k Now use the well-known sub-multiplicativity a (vu) a (v)a (u) of p+q 1 p q − ≤ approximationnumbers([18],page61),aswellasthesemi-groupproperty(1.5) (which implies C =Ck ), and (2.3). We see that: ϕθ ϕαk k a (C )=a (Ck ) a (C ) k K2 . kn ϕθ kn ϕαk ≤(cid:2) n ϕαk (cid:3) ≤(cid:20)(1−αk)√n(cid:21) Observe that 1 αk 1 θ 1 α − k = − k − ≥ k k · We then get, c=c denoting a constant which only depends on θ: θ k k a (C ) . kn ϕθ ≤(cid:16)c√n(cid:17) Set d = c/e and take k = d√n, ignoring the questions of integer part. We obtain: a (C ) e k =e d√n. dn3/2 ϕθ ≤ − − 4 Setting N =dn3/2, we get (2.4) a (C ) ae bN1/3 N ϕθ ≤ − for an appropriate value of a and b and for any integer N 1. This ends our ≥ first proof, with an exponent slightly smaller that the right one (1/3 instead of 1/2), yet more than sufficient to prove that C S . (cid:3) ϕθ ∈∩p>0 p Remark. Since the estimate (2.3) is rather crude, it might be expected that, using (2.4), and iterating the process, we could obtain a better one. This is not the case, andthis iterationleads to (2.4) and the exponent 1/3 again(with different constants a and b). Proof of Theorem 2.1. This proof will give the correct exponent 1/2 in the upper bound. Moreover, it works more generally for Schur functions whose imageliesinpolygoninscribedintheunitdisk. Thisupperboundappears,ina differentcontextandunderaverycrypticform,in[19]. Firstnotethefollowing simple lemma. Lemma 2.3 Supposethat a,b D satisfy a b Mmin(1 a,1 b),where ∈ | − |≤ −| | −| | M is a constant. Then: M d(a,b) :=χ<1. ≤ √M2+1 Here d is the pseudo-hyperbolic distance defined by: a b d(a,b)= − a,b D. (cid:12)1 ab(cid:12) ∈ (cid:12) − (cid:12) Proof. Set δ =min(1 a,1 b). (cid:12)We hav(cid:12)e the identity −| | −| | 1 (1 a2)(1 b2) (1 a)(1 b) δ2 1 1= −| | −| | −| | −| | = , d2(a,b) − a b2 ≥ a b2 ≥ M2δ2 M2 | − | | − | hence the lemma. (cid:3) The second lemma gives an upper bound for a (C ). In this lemma, κ is N ϕ a numerical constant, S(ξ,h) the usual pseudo-Carleson window centered at ξ T (where T=∂D is the unit circle)andofradiush (0<h<1), definedby: ∈ (2.5) S(ξ,h)= z D; z ξ h , { ∈ | − |≤ } and m is the pull-back measure of m, the normalizedLebesgue measure on T, ϕ by ϕ . Recall that if f (D), one sets f (eit)= f(reit) for 0< r <1 and, if ∗ r ∈H the limit exists m-almost everywhere,one sets: (2.6) f (eit)= lim f(reit). ∗ r 1− → Actually,weshalldowritef insteadoff . RecallthatameasureµonDiscalled ∗ aCarleson measure ifthereisaconstantc>0suchthatµ S(ξ,h) chforall ξ T. Carleson’s embedding theorem says that µ is a Car(cid:2)leson m(cid:3)ea≤sure if and ∈ only if the inclusion map from H2 into L2(µ) is bounded (see [4], Theorem 9.3, for example). 5 Lemma 2.4 Let B be a Blaschke product with less than N zeroes (each zero being counted with its multiplicity). Then, for every Schur function ϕ, one has: (2.7) a2 := a (C ) 2 κ2 sup 1 B 2dm , N (cid:2) N ϕ (cid:3) ≤ 0<h<1,ξ∈T hZS(ξ,h)| | ϕ for some universal constant κ>0. Proof. The subspace BH2 is of codimension N 1. Therefore, a = N ≤ − c (C ) C , where the c ’s are the Gelfand numbers (see [2]), and N ϕ ≤ ϕBH2 N where we u(cid:13)sed t|he e(cid:13)quality a = c occurring in the Hilbertian case (see [2]). (cid:13) (cid:13) N N Now, since Bf = f for any f H2, we have: H2 H2 k k k k ∈ C 2 = sup B ϕ2 f ϕ2dm= sup B 2 f 2dm (cid:13)(cid:13) ϕ|BH2(cid:13)(cid:13) kfkH2≤1ZT| ◦ | | ◦ | kfkH2≤1ZD| | | | ϕ = R 2, µ k k where µ = B 2m and where R : H2 L2(µ) is the restriction map. Of ϕ µ | | → course, µ is a Carleson measure for H2 since µ m . Now, Carleson’s em- ϕ ≤ bmeadrdkinagftetrhetohreemprosoayfsofuTshtheoartemkR9µ.k32, a≤t tκh2esutopp0<ohf<p1,aξg∈eT1µ6[S3(h;ξ,ahc)]tu(asleley,[i4n],tRhaet- book, Carleson’s windows W(ξ,h) are used instead of pseudo-Carleson’s win- dows S(ξ,h), but that does not matter, since W(ξ,h) S(ξ,2h): if r 1 h ⊆ ≥ − and t t0 h, then reit eit0 reit eit + eit eit0 2h). That ends | − | ≤ | − | ≤ | − | | − | ≤ the proof of Lemma 2.4. (cid:3) The following lemma takes into account the behaviour of ϕ (eit), and will θ be useful to us in Section 3 as well. The notation u(t) v(t) means that ≈ au(t) v(t) bu(t), for some positive constants a,b. ≤ ≤ Lemma 2.5 Set γ(t) = ϕ (eit) = γ(t) eiA(t), with π t π, and π θ | | − ≤ ≤ − ≤ A(t) π. Then, for 0 t, t π/2, one has: ′ ≤ ≤| | | |≤ (2.8) 1 γ(t) 1 γ(t) tθ and γ(t) γ(t′) K t t′ θ. | − |≈ −| |≈| | | − |≤ | − | Moreover, we have for t π/2: | |≤ (2.9) A(t) tθ and A(t) tθ 1. ′ − ≈| | ≈| | Proof. First, recall that (1+z)θ (1 z)θ ϕ (z)= − − , θ (1+z)θ+(1 z)θ − so that ϕ (z) =ϕ (z) and ϕ ( z)= ϕ (z). It follows that γ( t)=γ(t) and θ θ θ θ − − − γ(t+π)= γ(t), so that we may assume 0 t,t π/2. Then, we have more ′ − ≤ ≤ precisely, setting c=e iθπ/2, s=sin(θπ/2) and τ = tan(t/2) θ: − (cid:0) (cid:1) (cost/2)θ e iθπ/2(sint/2)θ 1 cτ 1 τ2 2isτ γ(t)= − − = − = − + , (cost/2)θ+e iθπ/2(sint/2)θ 1+cτ 1+cτ 2 1+cτ 2 − | | | | 6 after a simple computation, since (1+eit)θ =eitθ/2(2cost/2)θ and (1 eit)θ = − e iθπ/2eitθ/2(2sint/2)θ. Note by the way that − ϕ (1)=1; ϕ (i)=itan(θπ/4); ϕ ( 1)= 1; ϕ ( i)= itan(θπ/4). θ θ θ θ − − − − Now, observe that 2 1+cτ Re(1+cτ) 1 and therefore that ≥| |≥ ≥ 2cτ 1 γ(t) = τ tθ, | − | (cid:12)1+cτ(cid:12)≈ ≈ (cid:12) (cid:12) (cid:12) (cid:12) andsimilarlyfor1 γ(t) since1 γ(cid:12)(t)2 =(cid:12)4(Rec)τ. Therelation(2.8)clearly −| | −| | 1+cτ 2 | | follows. To prove (2.9), we just have to note that, for 0 t π/2, we have ≤ ≤ A(t)=arctan 2sτ (cid:3) 1 τ2 · − Now, we prove Theorem 2.1 in the following form (in which q = q denotes θ a positive constant smaller than one), which is clearly sufficient. (2.10) a KqN. 4N2+1 ≤ The proof will come from an adequate choice of a Blaschke product of length 4N2, with zeroes on the curve γ(t) = ϕ (eit), π t π. Let t = π2 k and θ k − − ≤ ≤ p =γ(t ), with 1 k N, so that the points p are all in the first quadrant. k k k ≤ ≤ We reflect them through the coordinate axes, setting: q =p , r = p , s = q , 1 k N. k k k k k k − − ≤ ≤ Let now B be the Blaschke product having a zero of order N at each of the points p ,q ,r ,s , namely: k k k k N N z p z q z r z s k k k k B(z)= − − − − . (cid:20)1 p z · 1 q z · 1 r z · 1 s z(cid:21) kY=1 − k − k − k − k This Blaschke product satisfies, by construction, the symmetry relations: (2.11) B(z)=B(z), B( z)=B(z). − Of course, B =1 on the boundary of D, but B is small on a large portion of | | | | the curve γ, as expressed by the following lemma. Lemma 2.6 For some constant χ=χ <1, the following estimate holds: θ (2.12) t t t = B(γ(t)) χN. N 1 ≤ ≤ ⇒ | |≤ PThroeno,f.wiLthethteNlp≤oftL≤emtm1 aan2d.5k, wsuecsheethtahtattkt+h1e≤asstu≤mpttki.onLseotfBLke(mz)m=a 21z.−3−ppakkrze. satisfied with a = γ(t) and b = γ(t ), since t t t t = π2 k 1, so k k k k+1 − − | − | ≤ − that min(1 a,1 b) tθ 2 kθ and hence, for some constant M: −| | −| | ≈ k ≈ − a b K t t θ K2 kθ M min(1 a,1 b). k − | − |≤ | − | ≤ ≤ −| | −| | 7 We therefore have, by definition, and by Lemma 2.3, where we set χ = M/√M2+1: B (γ(t)) =d(γ(t),p ) χ<1. k k | | ≤ It then follows from the definition of B that: B(γ(t)) B (γ(t))N χN, k | |≤| | ≤ and that ends the proof of Lemma 2.6. (cid:3) Now fix ξ T and 0 < h 1. By interpolation, we may assume that h = 2 nθ. By∈symmetry, we m≤ay assume that Reξ 0 and Reγ(t) 0, − i.e. t π/2. Then, since ϕ (D) is contained in the sym≥metric angular se≥ctor θ | | ≤ of vertex 1 and opening θπ < π, there is a constant K > 0 such that 1 | − γ(t) K(1 γ(t)). The only pseudo-windows S(ξ,h) giving an integral not | ≤ −| | equal to zero in the estimation (2.7) of Lemma 2.4 satisfy ξ 1 (K +1)h. | − | ≤ Indeed, suppose that γ(t) ξ h. Then 1 γ(t) γ(t) ξ h and | − | ≤ − | | ≤ | − | ≤ 1 γ(t) K(1 γ(t)) Kh. If ξ 1 > (K + 1)h, we should have | − | ≤ − | | ≤ | − | γ(t) ξ ξ 1 γ(t) 1 >(K+1)h Kh=h, whichis impossible. Now, | − |≥| − |−| − | − for such a window, we have by definition of m : ϕ dt dt B 2dm = B(γ(t))2 B(γ(t))2 Z | | ϕθ Z | | 2π ≤Z | | 2π S(ξ,h) γ(t) ξ h γ(t) 1 (K+2)h | − |≤ | − |≤ B(γ(t))2 dt d=efI , h ≤Z | | 2π |t|≤Dtn since γ(t) 1 γ(t) ξ + ξ 1 h+(K+1)h and since γ(t) 1 atθ | − |≤| − | | − |≤ | − |≥ | | and γ(t) 1 (K +2)h together imply t Dt , where D > 1 is another n | − | ≤ | | ≤ constant (recall that h=2 nθ =(t /π)θ). − n To finish the discussion, we separate two cases. 1) If n N, we simply majorize B by 1. We set q =2θ 1 <1 and get: 1 − ≥ | | 1 1 Dtn dt 2Dt I B(γ(t))2 n =Dqn DqN. h h ≤ hZ | | 2π ≤ 2πh 1 ≤ 1 −Dtn 2) If n N 1, we write: ≤ − 1 2 DtN dt 2 Dtn dt I = B(γ(t))2 + B(γ(t))2 :=J +K . h N N h hZ | | 2π hZ | | 2π 0 DtN The term J is estimated above: J DqN. The term K is estimated N N ≤ 1 N through Lemma 2.6, which gives us: 2Dt K 2nθ n χ2N Dχ2N, N ≤ 2π ≤ since t 2nθ π, due to the fact that θ <1. n ≤ 8 If we now apply Lemma 2.4 with q =max(q ,χ2) and with N changed into 1 4N2+1, we obtain (2.10), by changing the value of the constant K once more. This ends the proof of Theorem 2.1. (cid:3) Theorem 2.1 has the following consequence (as in [21], page 29). Proposition 2.7 Let ϕ be a univalent Schur function and assume that ϕ(D) contains an angular sector centered on the unit circle and with opening θπ, 0<θ <1. Then a (C ) ae b√n, n=1,2,..., for some positive constants a n ϕ − ≥ and b, depending only on θ. Proof. Wemayassumethatthisangularsectoriscenteredat1. Byhypothesis, ϕ(D) contains the image of the “reduced” lens map defined by ϕ˜ (z)=ϕ ((1+ θ θ z)/2). Since ϕ is univalent, there is a Schur function u such that ϕ˜ = ϕ u. θ ◦ Hence C = C C and a (C ) C a (C ). Theorem 2.1 gives the ϕ˜θ ϕ ◦ u n ϕ˜θ ≤ k uk n ϕ result,sincethecalculationsforϕ˜ areexactlythesameasforϕ (becausethey θ θ are equivalent as z tends to 1). (cid:3) The same istrue if ϕis univalentandϕ(D)containsa polygonwithvertices on ∂D. 3 Spreading the lens map In [9], we studied the effect of the multiplication of a Schur function ϕ by 1+z thesingularinnerfunctionM(z)=e−1−z,andobservedthatthismultiplication spreads the values of the radial limits of the symbol and lessens the maximal occupation time for Carleson windows. In some cases this improves the com- pactness or membership to Schatten classes of C . More precisely, we proved ϕ the following result. Theorem 3.1 ([9], Theorem 4.2) For every p > 2, there exist two Schur functions ϕ and ϕ = ϕ M such that ϕ = ϕ and C : H2 H2 is not 1 2 1 | ∗1| | ∗2| ϕ1 → compact, but C : H2 H2 is in the Schatten class S . ϕ2 → p Here,wewillmeettheoppositephenomenon: thesymbolϕ willhaveafairly 1 bigassociatedmaximalfunctionρ ,butwillbelongtoallSchattenclassessince ϕ1 it“visits” aboundednumberofwindows(meaningthatthereexistsanintegerJ suchthat,for fixedn,atmostJ ofthe W arevisitedby ϕ (eit)). Thespread n,j ∗ symbol will have an improved maximal function, but will visit all windows, so that its membership in Schatten classes will be degraded. More precisely, we will prove that Theorem 3.2 Fix 0<θ <1. Then there exist two Schur functions ϕ and ϕ 1 2 such that: 1) C : H2 H2 is in all Schatten classes S , p>0, and even a (C ) ϕ1 → p n ϕ1 ≤ ae b√n; − 2) ϕ = ϕ ; | ∗1| | ∗2| 9 3) C S if and only if p>2θ; ϕ2 ∈ p 4) a (C ) K(logn/n)1/2θ, n=2,3,.... n ϕ2 ≤ Of course, it would be better to have a good lower bound for a (C ), but n ϕ2 we do not succeed in finding it yet. Proof. FirstobservethatC S ,sothatC S too,since ϕ = ϕ and ϕ1 ∈ 2 ϕ2 ∈ 2 | ∗1| | ∗2| since the membership of C in S only depends on the modulus of ϕ because ϕ 2 ∗ it amounts to ([21], page 26): π dt < . Z 1 ϕ (eit) ∞ −π −| ∗ | Theorem3.2saysthatwecanhardlyhavemore. Wefirstprovealemma. Recall (see[9],forexample)thatthemaximalCarleson function ρ ofaSchurfunction ϕ ϕ is defined, for 0<h<1, by: (3.1) ρ (h)= sup m [S(ξ,h)]. ϕ ϕ ξ=1 | | Lemma 3.3 Let 0 < θ < 1. Then, the maximal function ρ of ϕ satisfies ϕθ θ ρ (h) K1/θ(1 θ) 1/θh1/θ and, moreover, ϕθ ≤ − − (3.2) ρ (h) h1/θ. ϕθ ≈ Proof of the lemma. Let 0<h<1 and γ(t)=ϕ (eit). K and δ will denote θ constants which can change from a formula to another. We have, for t π/2: | |≤ 4(Rec)τ τ τ 1 γ(t)2 = δcos(θπ/2) δ(1 θ) −| | 1+cτ 2 ≥ 1+cτ 2 ≥ − 1+cτ 2 | | | | | | δ(1 θ)tθ. ≥ − | | Hence, we get, from Lemma 2.5: ρ (h) 2m( 1 γ(t) h and t π/2 ) 2m( (1 θ)δ tθ Kh ) ϕθ ≤ { −| |≤ | |≤ } ≤ { − | | ≤ } K1/θ(1 θ) 1/θh1/θ. − ≤ − Similarly, we have: ρ (h) m [S(1,h)] m( 1 γ(t) h ) m( tθ Kh ) Kh1/θ, ϕθ ≥ ϕθ ≥ {| − |≤ } ≥ {| | ≤ } ≥ and that ends the proof of the lemma. (cid:3) Going back to the proof of Theorem 3.2, we take ϕ = ϕ and ϕ (z) = 1 θ 2 ϕ (z)M(z2). WeuseM(z2)insteadofM(z)inordertotreatthepoints 1and 1 − 1 together. The first two assertions are clear. For the third one, we define the dyadic Carleson windows, for n=1,2,...,j =0,1,...,2n 1, by: − W = z D; 1 2 n z <1 and (2jπ)2 n arg(z)<(2(j+1))π)2 n . n,j − − − { ∈ − ≤| | ≤ } 10

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