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Global instability in Hamiltonian systems

Gonçalves Schaefer, Rodrigo

Abstract

In Chapters 1 and 2 of this thesis, we prove that for any non-trivial perturbation depending on any two independent harmonics of a pendulum and a rotor there is global instability. The proof is based on the geometrical method and relies on the concrete computation of several scattering maps. A complete description of the different kinds of scattering maps takes place. We separate the proof of the general system in two cases. The first one is studied in Chapter 1. There, a proof is given for the simplest perturbation function. Besides, we find out some very special diffusion orbits, called "highways", and we give estimates of the time of diffusion for these orbits. The second case is considered in Chapter 2, and the proof of diffusion is completed. In Chapter 2, the existence of piecewise smooth global scattering maps is also provided. In Chapter 3, we consider a similar Hamiltonian with 3 degrees of freedom. We prove the diffusion using a combination of scattering maps and inner dynamics with concrete diffusion paths.We also compare the results obtained in this case with the results in Chapter 1. Closing the thesis, we comment some open problems remained of the study that we have done along the three previous Chapters.

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Global Ins abili y in Hamil onian Sys ems Thesis p esen ed o ob ain he Ph. D. in Applied Ma hema ics by Uni e si a Poli `ecnica de Ca alunya Rod igo Gon¸cal es Schae e Supe iso : Amadeu Delshams May 29, 2018 Con en s 1 In oduc ion 4 2 The i s case o 2 + 1/2 deg ees o eedom 11 2.1 TheSys em ................................... 11 2.2 The inne and he ou e dynamics . . . . . . . . . . . . . . . . . . . . . . . 13 2.2.1 Inne map................................ 13 2.2.2 Sca e ing map: Melniko po en ial and c es s . . . . . . . . . . . . 14 2.3 A nolddi usion................................. 28 2.3.1 A geome ical p oposi ion: The le el cu es o L∗(I, θ) ....... 29 2.3.2 Resul s abou global ins abili y . . . . . . . . . . . . . . . . . . . . 33 2.4 The imeo di usion .............................. 37 2.4.1 Accu acy o he sca e ing map . . . . . . . . . . . . . . . . . . . . 38 2.4.2 Es ima e o he ime o di usion . . . . . . . . . . . . . . . . . . . 40 3 Second case o 2+1/2 deg ees o eedom 46 3.1 Inne dynamics ................................. 46 3.2 Sca e ingmap ................................. 48 3.2.1 C es s and NHIM lines . . . . . . . . . . . . . . . . . . . . . . . . . 50 3.2.2 Cons uc ion o sca e ing maps . . . . . . . . . . . . . . . . . . . . 57 3.3 A noldDi usion ................................ 64 3.3.1 P oo o Theo em1........................... 67 3.4 Piecewise smoo h global sca e ing maps . . . . . . . . . . . . . . . . . . . 68 4 A case o 3+1/2 deg ees o eedom 71 4.1 Unpe u bedcase................................ 72 4.2 Inne dynamics ................................. 72 4.3 Sca e ingmap ................................. 73 4.3.1 De ini ion o sca e ing map . . . . . . . . . . . . . . . . . . . . . . 73 4.3.2 C es s and NHIM lines . . . . . . . . . . . . . . . . . . . . . . . . . 74 4.3.3 Symme y o he sca e ing map . . . . . . . . . . . . . . . . . . . . 78 4.4 Highways .................................... 83 1 5 Some open ques ions 87 5.1 Highways in piecewise smoo h global sca e ing maps . . . . . . . . . . . . 87 5.2 Abou he case wi h 3 + 1/2 deg ees o eedom . . . . . . . . . . . . . . 87 5.3 Abou Shadowing lemmas . . . . . . . . . . . . . . . . . . . . . . . . . . . 88 5.4 Rela ion be ween he o mulas o he sca e ing and sepa a ix maps . . . . 88 5.5 Abou he amoun o di usion ajec o ies . . . . . . . . . . . . . . . . . . 89 5.6 Andmo eandmo e............................... 89 2 Acknowledgmen s Ag aeixo especialmen al meu u o , Amadeu Delshams, pe ha e accep a eballa amb mi, pe la solida i a , la paci`encia i la dedicaci´o. Ag aeixo amb´e a en Jos´e Tom´as L´aza o pe la simpa ia in ini a i la som iu e cada eg- ada que ens obem al depa amen . A l’E a Mi anda pe l’in e `es i la se a disponibili a . Als p o esso s A u o Viei o i Ca les Sim´o pels comen a is desp ´es dels semina is. Me gus a ´ıa ag adece a Albe o, mi compa˜ne o de despacho po es os 4 a˜nos, siemp e una buena compa˜n´ıa en los ca ´es y cong esos. Que o ag adece aos meus amigos de Cabo F io que se man i e am semp e p esen es apesa da dis ˆancia, Gab iel, Paulo, Lucas, Ma cus, Rhenan, Guilhe me e Jona has. Aos amigos do “Regen Mendie a” que ize am poss´ı el a sob e i ˆencia no p imei o ano de dou o ado, Ma cos, Jo˜ao e Danilo. Aos colegas de Ce danyola Mu ilo, Leona do, e Jackson. A Juliana pela companhia no pe ´ıodo que es e e em Ba celona. E cla o, ao O ´a io e ao Glads on, se ei e e namen e g a o pela amizade de ocˆes... ocˆes sabem o qu˜ao di ´ıcil oi. Gos a ia de ag adece amb´em a S e anella Boa o, po e me dado a p imei a opo - unidade pa a que esse dou o ado se o nasse ealidade. Seu apoio e sua amizade. Gos a ia amb´em de ag adece a minha am´ılia pelo apoio e amo que me ansmi em a cada momen o, meus pais Selma e Luiz, minhas i m˜as Juliana e Ana Ca olina e aos meus sob inhos Caio e Camila. I ag aeixo mol especialmen a la N´u ia i a la se a am´ılia, que ja conside o com me a. Sense u, es d’aix`o se ia possible. Enca a enim mol es coses pe conque i jun s. Thanks o he e e ees o ead his hesis. I was suppo ed by he PhD g an CNPq- Conselho Nacional de Desen ol imen o Cien ´ı ico e Tecnol´ogico. 3 Chap e 1 In oduc ion This hesis conce ns abou global ins abili y in nea ly-in eg able Hamil onian sys ems, also called “A nold di usion”. In [A n64], V.I. A nold p oposed an example o a nea ly- in eg able Hamil onian wi h 2 + 1/2 deg ees o eedom H(q, p, ϕ, I, ) = 1 2p2+I2+ε(cos q−1) (1 + µ(sin ϕ+ cos )) , and asse ed ha gi en any δ, K > 0, o any 0 < µ ε0, he e exis s a ajec o y o his Hamil onian sys em such ha I(0) < δ and I(T)> K o some ime T > 0. No ice ha his a global ins abili y esul o he a iable I, since ˙ I=−∂H ∂ϕ =−εµ(cos q−1) cos ϕ is ze o o ε= 0, so I emains cons an , whe eas Ican ha e a d i o ini e size o any ε > 0 small enough. A nold’s Hamil onian can be w i en as a nea ly-in eg able Hamil onian wi h 3 deg ees o eedom H∗(q, p, ϕ, I, s, A) = 1 2p2+I2+A+ε(cos q−1) (1 + µ(sin ϕ+ cos s)) , which o ε= 0 is an in eg able Hamil onian h(p, I, A) = 1 2(p2+I2) + A. Since hsa is ies he (A nold) isoene ge ic non-degene acy D2h Dh Dh>0=−16= 0, by he KAM heo em p o en by A nold in [A n63], he 5D phase space o His illed, up o a se o ela i e measu e O(√ε) , wi h 3D-in a ian o i Tωwi h Diophan ine equencies ω= (ω1, ω2,1): |k1ω1+k2ω2+k0| ≥ γ/|k|τ o any 0 6= (k1, k2, k0)∈Z, 4 whe e γ=O(√ε), and τ≥2. Since he 3D KAM in a ian o i do no sepa a e he 5D phase space, he e can exis i egula o bi s ‘ a eling’ be ween o i. A nold conjec u ed in he KAM heo em in 1963 ha his was he gene al case. In he i s pa o his hesis we conside an a p io i uns able Hamil onian wi h 2+1/2 deg ees o eedom Hε(p, q, I, ϕ, s) = ±p2 2+ cos q−1+I2 2+εh(q, ϕ, s) (1.1) consis ing o a pendulum and a o o plus a ime pe iodic pe u ba ion h(q, ϕ, s). A p io i uns able Hamil onian sys ems like he abo e one we e in oduced by [Loc92, CG94]. They consis on a o o in he a iables (I, ϕ) as an in eg able Hamil onian in ac ion-angle a iables, a pendulum in he a iables (p, q) which ca ies ou a sepa a ix associa ed o a saddle poin , plus a small pe u ba ion o size ε. Fo ε= 0, Hamil onian (1.1) is in eg able and, in pa icula , he ac ion Iis cons an . We wan o desc ibe he global ins abili y in he a iable I o |ε|non-ze o bu o he wise a bi a y small. Fo simplici y, we e e o global ins abili y in his pape simply as A nold di usion. Ne e heless, i is wo h ema king ha o iginally he e m A nold di usion was coined o a p io i s able Hamil onian sys ems, which a e pe u ba ions o in eg able Hamil onian sys ems w i en in ac ion-angle a iable. See [Be 10] o a ca e ul exposi ion o a p io i uns able and a p io i s able Hamil onian sys ems. Fo ins ance, eplacing V(q) by εV (q), ou Hamil onian (1.1) becomes a p io i s able. In ha case, A nold di usion would con- sis ing on inding ajec o ies wi h la ge de ia ions (p(T), I(T)) −(p(0), I(0)). This would be a much mo e di icul p oblem ha he one conside ed he e, because one has o con on o exponen ially small spli ing o in a ian mani olds wi h espec o he pa ame e εas well as o he passage h ough double esonances in he ac ion a iables p, I. In pa icula , exponen ial la ge es ima es o he ime o di usion wi h espec o εdue o Nekho oshe [Nek77, LM05, BM11] would apply. The main cha ac e is ic o an a p io i uns able Hamil onian sys em wi h 2+1/2 deg ees o eedom is ha he e exis s a 3D No mally Hype bolic In a ian Mani old (NHIM) which is a la ge in a ian objec wi h 4D uns able and s able in a ian mani olds. Inside his NHIM he e exis s an inne dynamics gi en by a Hamil onian sys em wi h 1+1/2 deg ees o eedom. This Hamil onian possesses 2D in a ian o i which p e en global ins abili y inside he 3D NHIM. Fo ε= 0, he s able and uns able in a ian mani old coincide along a huge sepa a ix illed wi h homoclinic o bi s o he NHIM. Fo small |ε| 6= 0, he uns able and s able mani olds o he NHIM in gene al do no coincide, bu o he wise in e sec ans e sely along 3D homoclinic in a ian mani olds. Th ough each poin on each 3D homoclinic mani old, he e exis s a homoclinic o bi which begins in a poin o he NHIM and inishes on ano he poin o he NHIM, no necessa ily he same one. This assignmen be ween an ini ial and he inal poin on he NHIM is called he sca e ing map. In p ac ice, one mus selec an adequa e domain o any sca e ing map. 5 Unde he ac ion o a sca e ing map, he a iable Ican inc ease (o dec ease). The geome ic mechanism o global ins abili y consis s on looking o ajec o ies o he sca e - ing map wi h a la ge change on he a iable I. S anda d shadowing a gumen s p o ide he exis ence o nea by ajec o ies o Hamil onian (1.1) wi h a la ge change on he a iable I. We a e going o assume ha he pe u ba ion h(q, ϕ, s) depends on wo ha monics in he a iables (ϕ, s): h(q, ϕ, s) = (q)g(ϕ, s), (q) = cos q, g(ϕ, s) = a1cos(k1ϕ+l1s) + a2cos(k2ϕ+l2s),(1.2) wi h k1, k2, l1, l2∈Z. One o he main goals o his hesis is o p o e ha o any non- i ial pe u ba ion a1a26= 0 depending on any wo independen ha monics k1k2 l1l26= 0, he e is global ins a- bili y o he ac ion I o any ε > 0 small enough. Ou i s esul is ha he global ins abili y happens o any a bi a y pe u ba ion (1.2). Theo em 1. Assume ha a1a26= 0 and k1l2−k2l16= 0 in Hamil onian (1.1)-(1.2). Then, o any I∗>0, he e exis s ε∗=ε∗(I∗, a1, a2)>0such ha o any ε,0< ε < ε∗, he e exis s a ajec o y (p( ), q( ), I( ), ϕ( )) such ha o some T > 0 I(0) ≤ −I∗< I∗≤I(T). Rema k 2. Fo a ough es ima e o ε∗∼exp(−πI∗/2) a leas o |a1/a2|<0.625, k1= l2= 1 and l1=k2= 0, and T=T(ε∗, I∗, a1, a2)∼(Ts(I∗, a1, a2)/ε) log(C(I∗, a1, a2)/ε) o he di usion ime, see 2.4. Analogous es ima es could be ob ained o all he o he alues o he pa ame e s. The p oo is based on he geome ical me hod in oduced in [DLS06] and elies on he conc e e compu a ion o se e al sca e ing maps. A sca e ing map is a map o ans e se homoclinic o bi s o a NHIM. Fo Hamil onian (1.1), he NHIM u ns ou o be simply ˜ Λε=˜ Λ = (0,0, I, ϕ, s):(I, ϕ, s)∈R×T2.(1.3) In he unpe u bed case, i.e., ε= 0, o any I∗>0 he NHIM ˜ Λ possesses a 4D sepa a ix, ha is o say, coinciden s able and uns able in a ian mani olds W0˜ Λ = (p0(τ), q0(τ), I, ϕ, s) : τ∈R, I ∈[−I∗, I∗],(ϕ, s)∈T2, whe e (p0, q0) a e he sepa a ices o he saddle equilib ium poin o he pendulum (p0( ), q0( )) = ±2 cosh ,4 a c an e± . In he pe u bed case, i.e., o small ε > 0, Wu(˜ Λε) and Ws(˜ Λε) do no coincide ( his is he so-called spli ing o sepa a ices), and e e y local ans e sal in e sec ion be ween 6 hem gi es ise o a (local) sca e ing map which is simply he co espondence be ween a pas asymp o ic mo ion in he NHIM o he co esponding u u e asymp o ic mo ion ollowing a homoclinic o bi . Since he NHIM has also an inne dynamics, an adequa e combina ion o hese wo dynamics on he NHIM, he inne one and he ou e one p o ided by he sca e ing map, gene a es he A nold di usion as long as he ou e dynamics does no p ese e he in a ian objec s o he inne dynamics. Necessi y o he assump ions I he de e minan ∆ := k1l2−k2l1o some coe icien a1,a2 anishes, o ins ance, i he e is only one ha monic in g, he e is no global ins abili y o he ac ion I. Indeed, looking a he equa ions associa ed o Hamil onian (1.1) ˙q=±p˙p= [±1 + ε(a1cos(k1ϕ+l1s) + a2cos(k2ϕ+l2s))] sin q ˙ϕ=I˙ I=εcos q(k1a1sin(k1ϕ+l1s) + k2a2sin(k2ϕ+l2s)) (1.4) ˙s= 1 his is clea o k1=k2= 0, since in his case Iis a cons an o mo ion. I k1o k26= 0, say k16= 0, he change o a iables ¯ϕ=k1ϕ+l1s, ¯ϕ−¯s=k2ϕ+l2s, ¯ I=k1I+l1, whe e =k2/k1can be assumed o sa is y 0 ≤ ≤1 wi hou loss o gene ali y, cas s sys em (1.4) in o ˙q=±p˙p= [±1 + ε(a1cos ¯ϕ+a2cos( ¯ϕ−¯s))] sin q ˙ ¯ϕ=¯ I˙ ¯ I=εk2 1cos q(a1sin ¯ϕ+ a2sin( ¯ϕ−¯s)) ˙ ¯s= ∆/k1 which is a Hamil onian sys em wi h he Hamil onian gi en by ¯ Hε(p, q, ¯ I, ¯ϕ, ¯s) = ±p2 2+ cos q−1+¯ I2 2 +εk2 1cos q(a1cos ¯ϕ+a2cos( ¯ϕ−¯s)) . (1.5) I ∆ = 0 Hamil onian (1.5) is au onomous wi h 2 deg ees o eedom, and he e o e a global d i o he ac ion Iis no possible. Only d i s o size √εa e possible due o KAM heo em. Analogously one easily checks ha o a1a2= 0 Hamil onian (1.1) is in eg able o au onomous. Reduc ion o he ha monic ypes Unde he hypo hesis (k1l2−k2l1)a1a26= 0 o Theo em 1, he case k2= 0 o Theo em 1 is p o ed in Chap e 2. Indeed, k2= 0 implies := k2/k1= 0 and i u ns ou om (1.5) 7 ha Hamil onian (1.1) is equi alen o he one wi h k1= 1, k2= 0, l1= 0, l2= 1: Hε(p, q, I, ϕ, ) = ±p2 2+ cos q−1+I2 2+εcos q(a1cos ϕ+a2cos s),(1.6) which is jus he Hamil onian s udied in Chap e 2. In Chap e 3 we p o e Theo em 1 o k1k26= 0 o equi alen ly o ∈(0,1]. Fo he sake o cla i y we will explain in ull de ail and p o e Theo em 1 along Sec ion 3.3 jus o = 1, which by (1.5) is equi alen o he case k1= 1, k2= 1, l1= 0, l2=−1: Hε(p, q, I, ϕ, ) = ±p2 2+ cos q−1+I2 2+εcos q(a1cos ϕ+a2cos(ϕ−s)) .(1.7) To inish he p oo o Theo em 1, in Sec ion 3.3 we will ske ch he modi ica ions needed o he case ∈(0,1). Sca e ing map ypes By he de ini ion gi en a Sec ion 2.2.2, a sca e ing map is in p inciple only locally de ined, ha is, o a small ball o alues o he a iables (I, ϕ, s) o (I, θ =ϕ−Is), since i depends on a non-degene a e c i ical poin τ∗=τ∗(I, ϕ, s) o a eal unc ion (2.6), depend- ing smoo hly on he a iables (I, ϕ, s), al eady in oduced in [DLS06]. In he s udy ca ied ou in Sec ion 3.2, i will be desc ibed whe he , in e ms o he pa ame e µ:= a1/a2 and he a iable I, a local sca e ing map can o canno be smoo hly de ined o all he alues o he angles (ϕ, s) o θ=ϕ−Is, becoming hus a global o ex ended sca e ing map. This desc ip ion will depend essen ially on a geome ical cha ac e iza ion o he unc- ion τ∗(I, ϕ, s) in e ms o he in e sec ion o c es s and NHIM lines, ollowing [DH11]. Any degene a ion o he c i ical poin τ∗=τ∗(I, ϕ, s) may gi e ise o mo e non-degene a e c i - ical poin s and a bi u ca ion o mul iple local sca e ing maps o o a non global sca e ing map. Di e en c i ical poin s τ∗=τ∗(I, ϕ, s) gi e ise o di e en local sca e ing maps, and pu ing oge he di e en local sca e ing maps, one can some imes ob ain piecewise smoo h global sca e ing maps, which a e e y use ul o design pa hs o ins abili y o he ac ion I, and a e simply called di usion pa hs. Fo ins ance, in Chap e 2 de o ed o he Hamil onian (1.6), i will be p o en ha o 0 < µ =a1/a2<0.625, he e exis wo di e en global sca e ing maps. Among he di e en kinds o associa ed o bi s o hese sca e ing maps, he e will appea wo o hem called highways, whe e he d i o he ac ion Iwas e y as and simple. As will be desc ibed in Sec ion 3.2, such highways do no appea o Hamil onian (1.7). Ne e heless, as will be p o en in Sec ion 3.4, he e exis piecewise smoo h global sca e ing maps, and he possible di usion along he discon inui y se s opens he possibili y o applying he heo y o piecewise smoo h dynamical sys ems [Fil88]. Abou he model chosen and ela ed wo k Hamil onian (1.1) is a s anda d example o an a p io i uns able Hamil onian sys- em [CG94] o med by a pendulum, a o o and a pe u ba ion. I is usual in he li e a u e 8 has a non degene a e c i ical poin τ∗=τ∗(I, ϕ, s), whe e L(I, ϕ, s) = Z+∞ −∞ ( (q0(σ))g(ϕ+Iσ, s +σ; 0) − (0)g(ϕ+Iσ, s +σ; 0)) dσ. Then, o 0<|ε|small enough, he e exis s a unique ans e sal homoclinic poin ˜z o ˜ Λε, which is ε-close o he poin ˜z∗(I, ϕ, s) = (p0(τ∗), q0(τ∗), I, ϕ, s)∈W0(˜ Λ): ˜z= ˜z(I, ϕ, s) = (p0(τ∗) + O(ε), q0(τ∗) + O(ε), I, ϕ, s)∈Wu(˜ Λε) Ws(˜ Λε).(2.7) The unc ion Lis called he Melniko po en ial o Hamil onian (1.1). In ou case, om (2.2) and (2.3) L(I, ϕ, s) = A00 +A10(I) cos ϕ+A01 cos s, (2.8) whe e A00 = 4 a00, A10(I) = 2π I a10 sinh(π I 2)and A01 =2π a01 sinh(π 2).(2.9) Fig. 2.3: The Melniko po en ial, µ=a10/a01 = 0.6 and I= 1. We now look o he c i ical poin s o (2.6) which indeed a e he solu ions o ∂L ∂τ (I, ϕ −Iτ, s −τ) = 0. Equi alen ly, τ∗=τ∗(I, ϕ, s) sa is ies I A10(I) sin(ϕ−I τ∗) + A10 sin(s−τ∗) = 0.(2.10) F om a geome ical iew-poin , o any (I, ϕ, s)∈[−I∗, I∗]×T2, inding τ∗=τ∗(I, ϕ, s) sa is ying (2.10) is equi alen o looking o he ex ema o Lon he NHIM line R(I, ϕ, s) = {(I, ϕ −Iτ, s −τ), τ ∈R},(2.11) 15 which co esponds o he unpe u bed ajec o y o Hamil onian H0 h ough (I, ϕ, s) along he unpe u bed NHIM. Thus we can de ine he sca e ing map as in [DH11]. Le Wbe an open subse o [−I∗, I∗]×T2such ha he map (I, ϕ, s)∈W7→ τ∗(I, ϕ, s), whe e τ∗(I, ϕ, s) is a c i ical poin o (2.6) o , equi alen ly, a solu ion o (2.10), is well de- ined and C2. The e o e, he e exis s a unique ˜zsa is ying (2.7). Le Γ = {˜z(I, ϕ, s;ε),(I, ϕ, s)∈ W}. Fo any ˜z∈Γ he e exis unique ˜x+,−= ˜x+,−(I, ϕ, s;ε)∈˜ Λεsuch ha ˜z∈ Ws ε(˜x−)∩Wu ε(˜x+). Le H+,−=[{˜x+,−(I, ϕ, s;ε),(I, ϕ, s)∈W}. We de ine he sca e ing map associa ed o Γ as he map S:H−−→ H+ ˜x−7−→ S(˜x−) = ˜x+. By he geome ic p ope ies o he sca e ing map (i is an exac symplec ic map [DLS08]) we ha e, see [DH09] and [DH11], ha he sca e ing map has he explici o m S(I, ϕ, s) = I+ε∂L∗ ∂ϕ (I, ϕ, s) + O(ε2), ϕ −ε∂L∗ ∂I (I, ϕ, s) + O(ε2), s,(2.12) whe e L∗(I, ϕ, s) = L(I, ϕ −I τ∗(I, ϕ, s), s −τ∗(I, ϕ, s)).(2.13) The new a iable θ=ϕ−Is No ice ha i τ∗(I, ϕ, s) is a c i ical poin o (2.6), τ∗(I, ϕ, s)−σis a c i ical poin o τ7−→ L(I, ϕ −I(τ+σ), s −(τ+σ)) = L(I, ϕ −Iσ −Iτ, s −σ−τ).(2.14) Since τ∗(I, ϕ −Iσ, s −σ) is a c i ical poin o he igh hand side o (2.14), by he uniqueness in Wwe can conclude ha τ∗(I, ϕ −Iσ, s −σ) = τ∗(I, ϕ, s)−σ. (2.15) Thus, by (2.13), L∗(I, ϕ −Iσ, s −σ) = L(I, ϕ −Iσ −I(τ∗−σ), s −σ−τ∗) =L(I, ϕ −Iτ∗, s −τ∗) = L∗(I, ϕ, s), 16 and, in pa icula o σ=s, L∗(I, ϕ −Is, 0) = L∗(I, ϕ, s). In oducing he new a iable θ=ϕ−Is, we de ine he Reduced Poinca ´e unc ion L∗(I, θ) := L∗(I, ϕ −Is, 0) = L∗(I, ϕ, s).(2.16) We can w i e he sca e ing map on he a iables (I, θ). F om (I0, ϕ0, s0) = S(I, ϕ, s), we ha e ha θ0=ϕ0−I0s0=ϕ−ε∂L∗ ∂I (I, ϕ, s)−I+ε∂L∗ ∂ϕ (I, ϕ, s)s+O(ε2) =θ−ε∂L∗ ∂I (I, ϕ, s) + ∂L∗ ∂ϕ (I, ϕ, s)s+O(ε2). Since ∂L∗ ∂I (I, ϕ, s) = ∂L∗ ∂I (I, θ)−s∂L∗ ∂θ (I, θ) and ∂L∗ ∂ϕ =∂L∗ ∂θ (I, θ), we conclude ha θ0=θ−ε∂L∗ ∂I (I, θ)+O(ε2) and I0=I+ε∂L∗ ∂θ (I, θ)+O(ε2). Then, in he a iables (I, θ), he sca e ing map akes he simple o m S(I, θ) = I+ε∂L∗ ∂θ (I, θ) + O(ε2), θ −ε∂L∗ ∂I (I, θ) + O(ε2),(2.17) so up o O(ε2) e ms, S(I, θ) is he −ε imes low o he au onomous Hamil onian L∗(I, θ). In pa icula , he i e a es unde he sca e ing map ollow he le el cu es o L∗up o O(ε2). Rema k 6. We no ice ha he a iable θis pe iodic in he a iable ϕand quasi-pe iodic in he a iable s. Fixing s, hen θbecomes pe iodic. Rema k 7. No e ha i o some alues o (I, θ) we ha e ha ∇L∗(I, θ) = O(ε), hen ε∂L∗/∂θ(I, θ) = O(ε2) and ε∂L∗/∂I(I, θ) = O(ε2). In his case, he le el cu es o L∗(I, θ) do no p o ide he dominan pa o he sca e ing map S. The e o e, we will be able o desc ibe p ope ly he sca e ing map h ough he le el cu es o he Reduced Poinca ´e unc ion on he se o (I, θ) such ha k∇L∗(I, θ)k  ε. 17 Rema k 8. Using Eq.(2.15) and se ing s=σ, we ha e ha τ∗(I, ϕ−Is, 0) = τ∗(I, ϕ, s)− s. So we can de ine τ∗(I, θ) := τ∗(I, ϕ, s)−s(2.18) and om (2.13) and (2.16) we can w i e L∗as L∗(I, θ) = L(I, θ −Iτ∗(I, θ),−τ∗(I, θ)).(2.19) Rema k 9. In he a iables (I, θ), he a iable sdoes no appea a all in he exp ession (2.17) o he sca e ing map, a leas up o O(ε2). Howe e , sdoes appea in he exp ession (2.12) in he o iginal a iables (I, ϕ), so we ha e in (2.12) a amily o sca e ing maps pa ame e ized by he a iable s. Playing wi h he pa ame e s, we can ha e sca e ing maps wi h di e en p ope ies. See Lemma 14 o an applica ion o his phenomenon. The c es s Fo he compu a ion o he sca e ing maps, we use an impo an geome ical objec in oduced in [DH11], he c es s. De ini ion 10. Fixed I, we de ine by c es s C(I) he cu es on {(I, ϕ, s),(ϕ, s)∈T2}, sa is ying I∂L ∂ϕ(I, ϕ, s) + ∂L ∂s (I, ϕ, s)=0. In ou case I A10(I) sin ϕ+A01 sin s= 0.(2.20) No e ha a poin (I, ϕ, s) belongs o a c es C(I) i i is a minimum o maximum, o mo e gene ally, a c i ical poin o Lalong a NHIM line (2.11), ha is, τ∗(I, ϕ, s) = 0 in (2.10), see Fig. 2.4. Fig. 2.4: Le el cu es o L o µ=a10/a01 = 0.5 and I= 1.2. C es s (dashed) in blue and g een and he NHIM lines in black. 18 Rema k 11. No e ha any c i ical poin o L(I, ·,·) belongs o he c es C(I). In gene al we ha e wo cu es sa is ying Eq.(2.20), he maximum c es CM(I), and he minimum c es Cm(I). The maximum c es con ains he poin (I, ϕ = 0, s = 0), and he minimum c es he poin (I, ϕ =π, s =π). Fo a10 >0, a01 >0, he Melniko unc ion L(I, ·,·) gi en in (2.8) has a maximum poin a he poin (I, ϕ, s)=(I, 0,0), and a minimum a (I, π, π), and he unc ion (2.6) has a maximum on CM(I), and a minimum on Cm(I). Fo o he combina ions o signs o a10, a01, he loca ion o maxima and minima changes, bu o simplici y, we ha e p ese ed he name o maximum and minimum c es . We now p oceed o s udy he c es s. By (2.9) we can ew i e Eq. (2.20) as µα(I) sin ϕ+ sin s= 0,(2.21) whe e α(I) = IA10(I) µA01 =sinh(π 2)I2 sinh(π I 2)and µ=a10 a01 .(2.22) No e ha i |µα(I)|<1 we can w i e sas a unc ion o ϕ o any alue o ϕ. On he o he hand, i |µα(I)|>1 we can w i e ϕas a unc ion o s. So, we ha e wo di e en kinds o c es s: •Fo |α(I)|<1/|µ|, he wo c es s a e ho izon al, see Fig. 2.5(a), wi h CM,m(I) = {(I, ϕ, ξM,m(I, ϕ)) : ϕ∈T}, ξM(I, ϕ) = −a csin(µα(I) sin ϕ) mod 2π(2.23) ξm(I, ϕ) = a csin(µα(I) sin ϕ) + πmod 2π. (a) Ho izon al c es s: µ=a10/a01 = 0.6 and I= 1.2. (b) Ve ical c es s: µ=a10/a01 = 1.2 and I= 1. Fig. 2.5: Types o c es s. •Fo |α(I)|>1/|µ|, he wo c es s a e e ical, see Fig. 2.5(b), wi h CM,m(I) = {(I, ηM,m(I, s), s) : s∈T}, ηM(I, s) = −a csin(sin s/ (µα(I))) mod 2π(2.24) ηm(I, s) = a csin(sin s/ (µα(I))) + πmod 2π. 19 Rema k 12. The case |α(I)|= 1/|µ|is singula , since bo h c es s a e piecewise NHIM lines and hey ouch each o he a he poin s (ϕ, s)=(π/2,3π/2) ,(3π/2, π/2). See Fig. 2.6. Fig. 2.6: Singula case: C es s o I= 1 and µ= 1. We can desc ibe he ela ion be ween he c es s C(I) and he NHIM lines R(I, ϕ, s) h ough he ollowing P oposi ion: P oposi ion 13. Conside he c es C(I)de ined by (2.21) and he NHIM line R(I, ϕ, s) de ined in (2.11). a) Fo |µ|<0.625 he c es s a e ho izon al and he in e sec ions be ween any c es and any NHIM line is ans e sal. b) Fo 0.625 ≤ |µ| ≤ 0.97 he wo c es s C(I)a e s ill ho izon al, bu o some alues o I he e exis wo NHIM lines R(I, ϕ, s)which a e quad a ically angen o he c es s. c) Fo |µ|>0.97, he same p ope ies as s a ed in b) hold, excep ha o |µα(I)|>1, he c es s C(I)a e e ical. P oo . The “ho izon ali y” o a) and b) and he “ e icali y” o c) a e due he uppe bound o |µ|. Since |α(I)|<1/0.97 (see Fig.2.7), o |µ| ≤ 0.97, he c es s a e ho izon al, ha is, hey can be exp essed by equa ions (2.23). The condi ion o ans e sali y is p o ed in [DH11]. Essen ially, he p oo is o ob- se e ha |Iα(I)|<1.6 and ha he e exis s a ϕsuch ha ∂ξ(I, ϕ)/∂ϕ = 1/I i , only i , |Iα(I)|<1/|µ|(we will p o e i in a sligh ly di e en con ex , see he p oo o P oposi- ion 20.) Abou he amoun o NHIM lines angen s o C(I), he p oo is gi en in subsec ion 2.2.2. In Figs. 2.5(a) and 2.5(b) we ha e displayed a segmen o he he NHIM line R(I, ϕ, s), |τ|< π, and we see ha i in e sec s each c es CM(I) and Cm(I) ans e sally, gi ing ise o wo alues τ∗ Mand τ∗ m, he e o e o wo di e en sca e ing maps. We deno e by τ∗ M he τwi h minimum absolu e alue such ha gi en (I, ϕ, s), (I, ϕ −Iτ, s −τ)∈CM(I) and τ∗ m is de ined analogously when (I, ϕ −Iτ, s −τ)∈Cm(I) (see [DH11]). 20 Fig. 2.7: G aph o |α(I)| Sca e ing maps and c es s No e ha τ∗ mand τ∗ Ma e associa ed o di e en homoclinic poin s o he NHIM ˜ Λ, and consequen ly, o di e en homoclinic connec ions. F om his we build di e en sca e ing maps. The mos na u al way is o associa e one sca e ing map o each c es . And we will do his on he a iables (I, ϕ, s) and (I, θ), whe e θ=ϕ−Is. Be o e, we make some conside a ions abou he NHIM lines de ined in (2.11). No e ha θ:= ϕ−Is = (ϕ−Iτ)−I(s−τ), ha is, θis cons an on each NHIM line R(I, ϕ, s), so we will also in oduce ano he no a ion o a NHIM line R(I, ϕ, s), namely Rθ(I) := {(I, ϕ, s) : ϕ−Is =θ}. Since (ϕ, s)∈T2,R(I, ϕ, s) is a closed line i I∈Q, whe eas i is a dense line on T2i I /∈Q. In his case, R(I, ϕ, s) in e sec s he c es s C(I) along an in ini e numbe o poin s. Recall (see Rema k 6) ha θis quasi-pe iodic in he a iable s∈T. To a oid mon- od omy wi h espec o his a iable, we a e going o conside om now on, in his Chap e , sas a eal a iable in an in e al o leng h 2π,−π/2< s ≤3π/2. Unde his es ic ion, he NHIM line R(I, ϕ, s) de ined in (2.11) becomes a NHIM segmen R(I, ϕ, s) = {(I, ϕ −Iτ, s −τ) ; −π/2< s −τ≤3π/2},(2.25) as well as Rθ(I), which can be w i en as Rθ(I) = {(I, ϕ, s) : ϕ−Is =θ, (ϕ, s)∈T×(−π/2,3π/2]}.(2.26) F om now on, when we e e o R(I, ϕ, s) and Rθ(I), hey will be hese line segmen s. No ice ha θ∈T. We begin o conside he p ima y sca e ing map SMassocia ed o he maximum c es CM, ha is, we look only a he in e sec ions be ween he segmen R(I, ϕ, s) gi en in (2.25) and CM(I), pa ame e ized by τ∗ M(I, ϕ, s) = τ∗ M(I, θ) + s(see (2.18)): CM(I)∩R(I, ϕ, s) = {(I, ϕ −Iτ∗ M(I, ϕ, s), ξM(I, ϕ −Iτ∗ M(I, ϕ, s)))}(2.27) ={(I, ϕ −Iτ∗ M(I, ϕ, s), s −τ∗ M(I, ϕ, s))}(2.28) 21 Equa ion (2.27) mo i a es us o in oduce a new a iable ψ=ϕ−Iτ∗ M(I, ϕ, s) ha will be use ul in many con ex s. The a iable ψ: a a iable on he c es . Le C(I) be a c es such ha i can be pa ame e ized by ξ(I, ϕ) as in (2.23). Since τ∗(I, ϕ, s) is he alue o τsuch ha R(I, ϕ, s), gi en in (2.25), in e sec s C(I), we de ine ψ:= ϕ−Iτ∗(I, ϕ, s).(2.29) By (2.18) we can also w i e ψin e ms o he a iable θ: ψ=ϕ−I(τ∗(I, θ) + s) = θ−Iτ∗(I, θ).(2.30) By (2.27) and (2.28), s−τ∗(I, ϕ, s) = ξ(I, ϕ −Iτ∗(I, ϕ, s)) = ξ(I, ψ).(2.31) In pa icula , o s= 0, ξ(I, ψ) = −τ∗(I, ϕ, 0) = −τ∗(I, θ) again by (2.18) and om (2.30) we ha e he exp ession o θin e ms o ψ: θ=ψ−Iξ(I, ψ).(2.32) All he ela ions be ween he a iables (ϕ, s), θand ψa e w i en in Table 2.1 and a e displayed in Fig. 2.8. By he de ini ions o L∗(I, ϕ, s) in (2.13), and L∗(I, θ) in (2.16) and (2.19), we ha e ha L∗(I, θ) = L∗(I, ϕ, s) = L(I, ψ, ξ(I, ψ)),(2.33) So we can de ine he educed Poinca ´e unc ion in e ms o (I, ψ) simply as he es ic ion o he Melniko po en ial L(I, ϕ, s) on he c es C(I) = {(I, ψ, ξ(I, ψ), ψ ∈T)}, i.e., L∗(I, ψ) := L(I, ψ, ξ(I, ψ)),(2.34) which in ou case akes he simple and compu able o m L∗(I, ψ) = A00 +A10(I) cos ψ+A01 cos ξ(I, ψ),(2.35) o a ho izon al c es (3.21). The e o e, as (I, ψ, ξ(I, ψ)) a e poin s on he c es , he domain o L∗(I, ·,·) is a subse o C(I). So, i he e exis di e en subse s whe e L∗(I, ·,·) can be well de ined, we can build di e en sca e ing maps associa ed o C(I). Deno e L∗ i(I, θ) = L(I, ϕ −Iτ∗ i(I, ϕ, s), s −τ∗ i(I, ϕ, s)), i= m,M, and L∗ i(I, ψ) = L(I, ψ, ξi(I, ψ)) om (2.33) and (2.34). We s a e he ollowing lemma Lemma 14. a) The Poinca ´e Reduced unc ions L∗ M(I, ψ)and L∗ M(I, θ)a e e en unc- ions in he a iable I, ha is, L∗ M(I, ψ) = L∗ M(−I, ψ)and L∗ M(I, θ) = L∗ M(−I, θ), and consequen ly SM(I, θ)is symme ic in his a iable I. The same happens o Sm(I, θ), ha is, o he sca e ing map associa ed o Cm(I). 22 0 π/ 2 π 3 π/ 2 - π/ 2 ξ ( I,ψ ) 0 π/ 2 π  ( ϕ − Iτ,s − τ )  − τ ∗ ( I,ϕ,s ) − Iτ ∗ ( I,ϕ,s ) − τ ∗ ( I,θ ) − Iτ ∗ ( I,θ ) θ ψ ( ϕ,s ) Fig. 2.8: The h ee a iables on he plane (ϕ, s): ϕ, θ and ψ. θ=ψ−Iξ(I, ψ)ψ=θ−Iτ∗(I, θ) θ=ϕ−Is ϕ =θ+Is ψ=ϕ−Iτ∗(I, ϕ, s)ϕ=ψ+I(s−ξ(I, ψ)) Table 2.1: Rela ion be ween a iables. b) The sca e ing map o a alue o µand s=π, associa ed o he in e sec ion be ween Rθ(I)and Cm(I)has he same geome ical p ope ies as he sca e ing map o −µ and s= 0, associa ed o he in e sec ion be ween Rθ(I)and CM(I), i.e., Sµ,m(I, ϕ, π) = S−µ,M(I, ϕ, 0) = S−µ,M(I, θ) P oo . a) This is an immedia e consequence o he ac ha unc ion A10(I) is e en and ξM(I, ϕ) is odd in he a iable I, see (2.9) and (2.23). b) Fi s , we look o τ∗ msuch ha he NHIM segmen Rθ(I) in e sec s he c es Cm(I). I we ix s=π, we ha e by (2.13) and (2.8): L∗ µ,m(I, ϕ, π) = A00 +A10(I) cos(ϕ−Iτ∗ m(I, ϕ, π)) + A01 cos(π−τ∗ m(I, ϕ, π)).(2.36) Besides, we ha e by (2.10) IA10(I) sin(ϕ−Iτ∗ m) + A01 sin(π−τ∗ m)=0, which, in oducing µ(2.22), is equi alen o µα(I) sin(ϕ−Iτ∗ m) + sin(π−τ∗ m)=0,(2.37) o −µα(I) sin(ϕ−Iτ∗ m) + sin(−τ∗ m)=0.(2.38) By (2.31) and (2.23) we ha e ha π−τ∗ m=ξm(I, ϕ −Iτ∗ m) o π/2≤ξm≤3π/2 and he e o e −π/2≤ −τ∗ m≤π/2. By looking a (2.37) and (2.38), τ∗ m(I, ϕ, π) o µis solu ion o he same equa ion as τ∗ M(I, ϕ, 0) o −µ, and lies in he same in e al −π/2≤ −τ∗ M≤π/2. The e o e τ∗ m(I, ϕ, π) o µis equal o τ∗ M(I, ϕ, 0) o −µ. F om (2.36), L∗ µ,m(I, ϕ, π) sa is ies L∗ µ,m(I, ϕ, π) = A00 +A10(I) cos(ϕ−τ∗ M(I, ϕ, 0)) + (−A01) cos(−τ∗ M(I, ϕ, 0)) =L∗ −µ,M(I, ϕ, 0). 23 Since L∗ µ,m(·,·, π) and L∗ −µ,M(·,·,0) coincide, hei de i a i es oo and his implies ha Sµ,m(I, ϕ, π) = S−µ,M(I, ϕ, 0) = S−µ,M(I, θ). The impo ance o he pa b) o his lemma is ha , conce ning di usion, he s udy o a posi i e µusing SM(I, θ) is equi alen o he s udy o −µusing Sm(I, ϕ, π), i.e., i we ensu e he di usion o a posi i e µ, we can ensu e i o a nega i e one (jus changing he sca e ing map). Besides, since SM(I, θ) symme ic in he a iable I( om he i s pa o he lemma), om now on we will conside always I≥0, µ > 0 and SM. Now we a e going o desc ibe he in luence o he in e sec ions be ween he c es s and he NHIM segmen s wi h espec o he pa ame e µdesc ibed in P oposi ion 13 on he sca e ing map associa ed o such c es s. Single sca e ing map: µ < 0.625 As in [DH11], assuming µ < 1/1.6 = 0.625, he c es s a e ho izon al and he e is no angency be ween Rθ(I) and CM(I), so ha τ∗ M(I, θ) is well de ined and by (2.19) and (3.11) he educed Poinca ´e unc ion akes he o m L∗ M(I, θ) = A00 +A10(I) cos(θ−Iτ∗ M(I, θ)) + A01 cos(−τ∗ M(I, θ)),(2.39) and he e o e SM(I, θ) akes he o m (2.17). Example To illus a e his cons uc ion, we ix µ= 0.6. In his case he c es s a e ho izon al o all I, and we display CM(I) pa ame ized by ξM(see (3.21)) in Fig.2.9 o I= 1.2. We can see how Rθ(I) in e sec s ans e sally CM(I), as well as he phase space o sca e ing map SMgene a ed by his in e sec ion gi en by he le el cu es o L∗ M(I, θ). Rema k 15. Recall om Rema k 9 ha sdoes no appea in he exp ession (2.17) o S(I, θ) and is a pa ame e in he exp ession (2.12) o S(I, ϕ, s). Compu a ionally, one di e ence is ha in exp ession (2.12), once ixed a alue o s, one h ows om any “ini ial poin ” (ϕ, s) he NHIM segmen R(I, ϕ, s) un il i ouches he c es C(I) a e a ime τ∗(I, ϕ, s), ob aining a alue o L∗(I, ϕ, s) gi en by (2.13), while in exp ession (2.17), sis ixed equal o 0 o , equi alen ly, he ini ial poin o h ow he NHIM segmen Rθ(I) is o he o m (θ, 0) (see Fig. 2.8). Mul iple sca e ing maps: 0.625 ≤µ≤0.97 As said be o e, o µ < 1/1.6 = 0.625 and any alue o I, he wo c es s CM(I) and Cm(I) a e ho izon al, and he NHIM segmen Rθ(I) in e sec s ans e sely each o hem, gi ing ise o a unique sca e ing map SMand Smassocia ed o each c es . We will now explo e la ge alues o µ o de ec angencies be ween C(I) and Rθ(I), ha is, when he e exis s (ϕ, I) such ha ∂ξ ∂ϕ(I, ϕ) = 1/I, 24 •Case 1 |µ|<0.625, ha is, 1/|µ|>1.6. Then, by (2.47) and (2.48), α(I)≤1.03 <1 µand β(I)≤1.6<1 |µ|, o all I, ha is, o I > 0, B= [0,+∞). •Case 2 No e ha o 0.625 ≤ |µ|<0.97 α(I)≤1.03 = 1/0.97 <1 |µ|≤1.6 = β(Iβ), and by (2.47), A= [0,+∞). Bu , now β(Ib)≥1/|µ|. Then he e exis wo alues I∈Asuch ha β(I)=1/|µ|. De ine I+= min {I:β(I) = 1/|µ|} and I++ = max {I:β(I)=1/|µ|}.(2.49) By he cha ac e iza ion (2.46) o he se Bwe ha e B= [0, I+)∪(I++,+∞). Fo 0.97 ≤ |µ| ≤ 1, he e exis Ia< I¯asuch ha α(Ij) = 1/|µ|,j∈ {a, ¯a}and A= [0, Ia)∪(I¯a,+∞). Analogously, he e exis Ib< I¯ bsuch ha β(Ij) = 1/|µ|, j∈ {b,¯ b}. As Ib≤Iaand I¯a< I¯ b, we ha e B= [0, Ib)∪(I¯ b,+∞), see Fig. 2.12. Bu his he equi alen o B= [0, I+)∪(I++,+∞), whe e I+and I++ a e gi en by (2.49). •Case 3 This case is simila o he Case 2 o 0.97 ≤ |µ| ≤ 1. Bu now, as |µ| ≥ 1, we ha e Ia≤Ib. So, in his case we ha e B= [0, Ia)∪(I¯ b,∞), o B= [0, I+)∪(I++,+∞), whe e I+= min {I:α(I) = 1/|µ|} and I++ = max {I:β= 1/|µ|}. Finally, we see ha L∗ M(I, θ) = A00 +A01 is composed by wo cu es in ec angles (θ, I)∈((0, π)∪(π, 2π)) ×B. This is equi alen o p o e ha he de i a i e o his cu e wi h espec o he a iable θis di e en om 0 o all Iin B. Fo any I∈B, we compu e he exp ession o ∂L∗ M/∂θ(I, θ) which using (2.10) and he change o a iables (2.45) akes he o m ∂L∗ M ∂θ (I, θ) = −A10(I) sin(ψ),(2.50) and ne e anishes o ψ∈(0, π)∪(π, 2π), o equi alen ly, o θ∈(0, π)∪(π, 2π). Then L∗ M(I, θ) = A00 +A01 is composed by wo e ical cu es on B. As we ha e seen in Lemma 54, L∗(−I, θ) = L∗(I, θ). Then, he le el cu e L∗ M(I, θ) = A00 +A01 is also de ined o I < 0, which concludes he p oo . Rema k 21. Using he exp essions abo e o I+and I++ one can check ha I+∼π 2|µ|sinh(π/2) and I++ ∼2 πlog(|2 sinh(π/2)µ|),as |µ| → +∞. 31 De ini ion 22. We call highways he wo cu es Hl⊂(0, π)×Tand H ⊂(π, 2π)×Tsuch ha L∗(I, θ) = A00 +A01. By P oposi ion 20, hey exis a leas o I∈(−∞,−I++)∪ (−I+, I+)∪(I++,+∞) o |µ| ≥ 0.615 and o any alue I o |µ|<0.625. I a10 >0, by (2.50), ∂L∗/∂θ is posi i e ( espec i ely nega i e) along he highway H ( esp. Hl). I a10 <0, change Hl o H . P oposi ion 23. Conside he Hamil onian Hε(p, q, I, ϕ, s) = ±p2 2+ cos q−1+I2 2+εcos q(a1cos ϕ+a2cos s), a1a26= 0.The highways ake he o m θh(I) =    a ccos A2(1− (I)) A1(I)+Ia ccos( (I)), I ≤0; a ccos A2(1− (I)) A1(I)−Ia ccos( (I)), I > 0; and θH(I) =   −a ccos A2(1− (I)) A1(I)−Ia ccos( (I)), I ≤0; −a ccos A2(1− (I)) A1(I)+Ia ccos( (I)), I > 0; whe e θh∈(0, π)and θH∈(π, 2π). P oo . F om (2.20), (2.33) and he de ini ion o he highways, we ha e he ollowing wo equa ions A1(I) cos(θ−Iτ∗) + A2cos(−τ∗) = A2(2.51) IA1(I) sin(θ−Iτ∗) + A2sin(−τ∗) = 0. Mul iplying by I he i s equa ion we ob ain IA1(I) cos(θ−Iτ∗) + IA2(cos(−τ∗)−1) = 0 IA1(I) sin(θ−Iτ∗) + A2sin(−τ∗) = 0. o equi alen ly IA1(I) cos(θ−Iτ∗) = −IA2(cos(−τ∗)−1) IA1(I) sin(θ−Iτ∗) = −A2sin(−τ∗). We sum hese wo equa ions squa ed and we ob ain I2A2 1(I)=[IA2(cos(−τ∗)−1)]2+A2 2sin2(−τ∗). A e some a i hme ical manipula ions we ob ain he ollowing equa ion o second de- g ee in cos(−τ∗) (I2−1)A2 2cos2(−τ∗)−2I2A2 2cos(−τ∗) + A2 2(I2+ 1) −I2A2 1(I)=0. 32 Sol ing his equa ion we ha e cos(−τ∗) = 2I2A2 2±p4I4A4 2−4(I2−1)A2 2[A2 2(I2+ 1) −I2A2 1(I)] 2(I2−1)A2 2 . A e mo e a i hme ical manipula ion and conside ing ha −1≤cos(−τ∗)≤1 we ha e cos(−τ∗) = I2A2−pA2 2+ (I2−1)I2A2 1(I) (I2−1)A2 . In o de o simpli y he no a ion we de ine (I) := I2A2−pA2 2+ (I2−1)I2A2 1(I) (I2−1)A2 And he e o e, ⇒ −τ∗(I, θ) = ±a ccos( (I)). Remembe ha we ha e wo highways. This explains why we ha e ound wo di e en alues o he unc ion τ∗. Then we can ew i e he i s equa ion o (2.51) as A1(I) cos(θ±Ia ccos( (I))) + A2 (I) = A2. This immedia ely implies θ=±a ccos A2(1 − (I)) A1(I)∓Ia ccos( (I)). F om he ou possibili ies, by compa ing wi h nume ical esul s we ob ain θh(I) =    a ccos A2(1− (I)) A1(I)+Ia ccos( (I)), I ≤0; a ccos A2(1− (I)) A1(I)−Ia ccos( (I)), I > 0; and θH(I) =   −a ccos A2(1− (I)) A1(I)−Ia ccos( (I)), I ≤0; −a ccos A2(1− (I)) A1(I)+Ia ccos( (I)), I > 0; . 2.3.2 Resul s abou global ins abili y Now we a e going o p o e wo esul s abou exis ence o he di usion phenomenon in ou model. The i s one is a di ec applica ion o he geome ical P oposi ion 20 jus p o ed and desc ibes he di usion ha akes place close o he highways. The second is a mo e gene al ype o di usion, alid also o he alues o he ac ion Iwhe e he e a e no highways. 33 Fig. 2.13: Highways in black o µ= 0.6. Di usion close o highways Theo em 24. Assume ha a10 a01 6= 0 in he Hamil onian (2.1)+(2.3). Then, o any I∗ he e exis s ε∗=ε∗(I∗)>0such ha o 0< ε < ε∗, he e exis s a ajec o y (p( ), q( ), I( ), ϕ( )) such ha o some T > 0 I(0) ≤ −I∗;I(T)≥I∗, whe e he admissible alues o I∗=I∗(µ)sa is y •Fo |µ|<0.625,I∗is a bi a y I∗∈(0,+∞). •Fo 0.625 ≤ |µ| ≤ 1,I∗∈(0, I+), whe e I+= min{I > 0 : I3sinh(π/2)/sinh(πI/2) = 1/|µ|}. •Fo |µ| ≥ 1,I∗∈(0, I+), whe e I+={I > 0 : I2sinh(π/2)/sinh(πI/2) = 1/|µ|}. P oo . Recall ha he educed Poinca ´e unc ion, gi en in (2.39), is L∗ M(I, θ) = A00 +A10(I) cos(θ−Iτ∗ M(I, θ)) + A01 cos(−τ∗ M(I, θ)). Du ing his p oo , we deno e τ∗ M(I, θ) simply by τ∗ M. Fo εsmall enough, he sca e ing map SM(I, θ) akes he o m (2.17) o L∗=L∗ M, so ha o bi s unde he sca e ing map a e con ained in he le el cu es o he educed Poinca ´e unc ion L∗ M, up o e o o O(ε2). P oposi ion 20 ensu es he exis ence o he highways as wo e ical le el cu es L∗ M(I, θ) = A00 +A01 o Iin •(−∞,+∞) o |µ|<0.625. •(−I+, I+),whe e –I+= min{I > 0 : I3sinh(π/2)/sinh(πI/2) = 1/|µ|} o 0.625 ≤ |µ| ≤ 1; –I+= min{I > 0 : I2sinh(π/2)/sinh(πI/2) = 1/|µ|} o |µ| ≥ 1. 34 Take a10 >0. Then gi en I∗>0 (wi h he es ic ion I∗< I+i |µ|>0.625), ∂L∗ M>0 along he highway H . No e ha (I0, θ0) := (0,3π/2) ∈H . Taking any (Ii, θi)∈H ,Ii>0, i s image unde he sca e ing map (e Ii+1,e θi+1) = SM(Ii, θi) sa is ies e Ii+1−Ii=O(ε)>0 and is O(ε2)-close o H . Using he inne map on ˜ Λ, we ind (Ii+1, θi+1) = φ i+1 (e Ii+1,e θi+1)∈H wi h Ii+1 −Ii=O(ε)>0. Con inuing ecu si ely in his way, we ge a pseudo-o bi {(Ii, θi), i = 0, . . . , N} ⊂ H wi h IN≥I∗ o med by applying successi ely he sca e ing map and he inne map. Using he symme y o H , in oducing Ii=−Ii o i < 0, we ha e he pseudo-o bi {(Ii, θi),|i| ≤ N} ⊂ H . Using s anda d shadowing esul s in [FM00, FM03] based on he exis ence o ans e se he e oclinic o bi s be ween non- esonan o i (changing sligh ly Ii o ob ain an i a ional equency o he inne map, i necessa y) o newe esul s like he co olla y 3.5 o [GLS14] whe e he ecu ence p ope y o he inne dynamics is also used, he e exis s a ajec o y o he sys em such ha o some T,I0≤ −I∗and I(T)≥I∗. I a10 <0, changing H o Hlall he p e ious easoning applies. Fig. 2.14: The di usion ajec o y in SM o µ= 0.6. The gene al di usion Now we p esen a heo em ha ensu es he di usion o all alues o he pa ame e a10, a01 (as long as a10a01 6= 0) and o any alue o I∗. Besides, we p o e i using he geome ical p ope ies o he sca e ing map ha we ha e explo ed up o now. Theo em 25. Assume ha a10 a01 6= 0 in he Hamil onian (2.1)+(2.3). Then, o any I∗>0, he e exis s ε∗=ε∗(I∗)>0such ha o any ε,0< ε < ε∗, he e exis s a ajec o y (p( ), q( ), I( ), ϕ( )) such ha o some T > 0 I(0) ≤ −I∗< I∗≤I(T). P oo . Ou p oo consis s on showing he exis ence o adequa e o bi s unde se e al sca e - ing maps, whose o bi s will be gi en app oxima ely by he le el cu es o he co esponding educed Poinca ´e unc ions, in such a way he alue o Iwill be inc easing. La e on, we will combine hem wi h o bi s unde he inne map o p oduce adequa e pseudo-o bi s o shadowing. 35 We begin wi h he simples case. Assume |µ|<0.625. In his case he highways, by P oposi ion 20, a e de ined o any alue o I∈Rand Theo em 24 ensu es he di usion phenomenon. We now assume 0.625 ≤ |µ| ≤ 0.97. In his case o some alue o I he e may exis angencies be ween he c es s CM(I) and he NHIM lines Rθ(I). Again by P oposi ion 20, in his case he highways a e de ined o all I∈(−∞,−I++)∪(−I+, I+)∪(I++,+∞) whe e 0 < I+≤I++. The case I∗∈(0, I+) is con ained in he esul o Theo em 24. So, we a e going o conside I∗∈[I+,+∞). As be o e, we ha e one SM-o bi con ained in one highway whe e Iis inc easing. We ha e o s udy he egion o Iwhe e he highways a e no de ined. Ou s a egy is p o ing he exis ence o a sca e ing map in he side o θwhe e he Iis inc easing, ha is, o θ∈(0, π) o θ∈(π, 2π) ( his depends on sign(a10)) whe e ∂L∗ M/∂θ is posi i e. Then, we will use he inne map (o ano he sca e ing map S0) o changing o pseudo-o bi (le el cu e) o L∗ M. In his way, we con inue he g ow h o I. Fo any I∈(−I++,−I+)∪(I+, I++), he e exis angencies be ween CM(I) and Rθ(I), i.e., he e exis s ψsuch ha ∂ξM/∂ψ = 1/I, and he e o e he e exis h ee di e en sca e ing maps. Conside he case wi h µ > 0. As we ha e seen in Subsec ion 2.2.2, ψ∈T7→ θ∈Tgi en in (2.41) is no longe a change o a iables, bu we ha e h ee bijec ions θi:Di(I)→T, i∈ {A,B,C}(see (2.42)). And o each bijec ion we ha e a sca e ing map associa ed o i . Among hese h ee sca e ing maps, we will chose only one o he di usion. Conside i s he case a10 >0 ( ecall ha he highway H goes om −I+ owa d I+). We chose o ins ance, he sca e ing map associa ed o he educed Poinca ´e unc ion L∗ M,A(I, θ) = L∗ M(I, θA(ψ)), ψ∈DA(I) since ∂L∗ M ∂θ (I, θA(ψ)) = −A10(I) sin(ψ)>0 o ψ∈DA(I)∩(π, 2π) and he e o e he i e a es unde he sca e ing map SM.A(I, θ) (2.17) associa ed o L∗ M,A(I, θ) inc ease he alues o I o θ∈(π, 2π). No ice ha by de ini ion o DA(I) o ψ∈ DA(I)∩(π, 2π) = (ψ2,2π) wi h ψ2∈(π, 3π/2) (see Subsec ion 2.2.2) he e a e no angen- cies be ween he c es and he NHIM segmen . We can now p oceed in he ollowing way. We i s cons uc a pseudo-o bi {(Ii, θi) : i= 0, . . . , N1} ⊂ H wi h I0= 0 and IN=I+, as in he p oo o Theo em 24. No e ha all hese poin s lie in he same le el cu e o L∗ M, ha is, L∗ M(Ii, θi) = A00 +A01,i= 0, . . . , N1. Applying he inne dynamics, we ge (IN1+1, θN1+1) = φ N1(IN1, θN1) wi h θN1+1 ∈ (θA(ψ2(IN1)),2π) and hen we cons uc a pseudo-o bi {(Ii, θi) : i=N1+1, ..., N1+M1} ⊂ L∗ M,A(IN1+1, θN1+1) = lN1+1 wi h θi∈(θN1+1,2π), 2π−θN1+M1=O(ε2). Applying he inne dynamics, we ge (IN1+M1+1, θN1+M1+1) = φ N1+M1(IN1+M1, θN1+M1) wi h θN1+M1+1 ∈ θA(ψ2(IN1+M1),2π)). Recu si ely, we cons uc pseudo-o bi {(Ii, θi) : i= N1+ 1, ..., N2} such ha IN2≥I++.We inally ollow he highway om I++ o I∗cons uc ing a pseudo- o bi {Ii, θi) : i= N2, ..., IN3} ⊂ H wi h IN3=I∗. Using he symme y p ope ies (see Lemma 54) in oducing Ii=−Ii o i < 0 we ha e a pseudo-o bi {(Ii, θi) : |i| ≤ N3}wi h I−N3=−I∗,IN3=I∗. Using now he same 36 shadowing echniques as in he p oo o Theo em 25, he e exis s a di usion ajec o y. I a10 <0, changing H o Hlall he p e ious easoning applies. Rema k 26. Fo he p oo o his heo em we ha e chosen a simple pseudo-o bi , jus choosing he sca e ing map SM,A when i was no unique. O cou se, he e is a lo o eedom in choosing pseudo-o bi s, and we do no claim ha he one chosen he e is he bes one conce ning minimal ime o di usion. (a) SM o µ= 1.5 (b) SMcombined wi h inne map (in ed) Fig. 2.15: Fo µ= 1.5, highways a e no p ese ed. Inne map and sca e ing map can be adequa ely combined Rema k 27. A ough es ima e o ε∗=ε∗(I∗)o Theo em 25 . The sca e ing map S(I, θ) (2.17) is he −ε ime map o he Hamil onian L∗(I, θ) gi en in (2.39), up o o de O(ε2). The e o e, as al eady no iced in Rema k 7, i |∂L∗/∂θ(I, θ)| ≤ εo |∂L∗/∂I(I, θ)| ≤ ε, he le el cu es o L∗(I, θ) a e no use ul enough o desc ibe he o bi s o S. I is easy o check ha ∇L∗(I, θ) only anishes o I= 0, θ= 0, π mod 2πand ha k∇L∗(I, θ)k. 8π|a10I|e−π|I|/2 o |I| → +∞. Thus, in gene al one has o a oid small neighbo hoods o (I, θ) = (0,0),(0, π) and ake ca e in egions whe e |I|is e y la ge. In pa icula , he highways Hl, H a e a om (I, θ) = (0,0),(0, π) and on hem k∇L∗(I, θ)k ≥ A10(I)(1 − O(β(I)µ)) &4π|a10I|e−π|I|/2 o la ge |I|, om which we ge an uppe bound o ε∗(I∗), which is exponen ially small in |I∗| o la ge |I∗|: ε∗(I∗)<4π|a10||I∗|exp(−π|I∗|/2). Fo smalle alues o I∗, one can compu e nume ically he le el cu es o k∇L∗(I, θ)k=ε and ob ain ε∗> ε∗(I∗) such ha k∇L∗(I, θ)k=ε∗implies |I|>|I∗|. See Table 2.2 o some alues o I∗, and µ= 0.9. 2.4 The ime o di usion In his sec ion we will p o ide an es ima e o he di usion ime. Fo simplici y, we a e going o es ima e he ime o a di usion using a highway (see De ini ion 22) as a guide, 37 I∗1 2 3 4 ε∗(I∗) 1.4 0.75 0.25 0.07 Table 2.2: Es ima es o ε∗ o µ= 0.9 ha is, we a e going o cons uc a pseudo-o bi close a he highway. This implies o i e a e he sca e ing map using as ini ial poin a poin on a highway. As we ha e seen be o e, see Subsec ion 2.2.2, one i e a e o SM(I, θ) is app oxima ed by −ε ime map o he Hamil onian L∗ M(I, θ) up o O(ε2). Howe e , i we i e a e he sca e ing map a numbe n o imes, i gene a es a p opaga ed e o wi h espec o he le el cu e o L∗ M(I, θ). So, i s we s udy he e o gene a ed by ni e a es o he sca e ing map. La e , we will es ima e he ime o di usion along he highway combining he sca e ing and he inne maps. 2.4.1 Accu acy o he sca e ing map Equa ion (2.17) o he sca e ing map Sis good enough up o an e o o O(ε2) o unde s anding one i e a e o S. Bu i we conside Sn, ha is, n-i e a es o S, some p oblems appea . These p oblems a e ela ed wi h he lack o p ecision o he equa ion (2.17): •Equa ion (2.17) o he sca e ing map has a ela i e e o o o de O(ε) and an absolu e e o O(ε2). The e o e, o n-i e a es, when nis la ge, he e o is p opaga ed in a such way ha i canno be disca ded. •Highways a e uns able, i.e., he nea by le el cu es o L∗mo e away om highways (see ins ance Fig.2.9.b). Now, ou goal is o show how we can con ol hese e o s along a egion Uin he phase space (I, θ) close o a highway. Basically, he con ol is o choose a good momen and in e al o apply he inne map o come back o he highway and o main ain he e o s small enough. The p opaga ed e o A e i e a ing n imes o mula (2.17) o he sca e ing map, one ge s o (In, θn) = Sn(I0, θ0): In=I0+ε n−1 X j=0 ∂L∗ ∂θ (Ij, θj) + O(nε2),and also θn=θ0−ε n−1 X j=0 ∂L∗ ∂I (Ij, θj) + O(nε2). (2.52) F om now on, in his sec ion, we will use he ollowing no a ion: 38 • S(I, θ) is he sca e ing map, see (2.17). •ST(I, θ) = (I+ε ∂L∗/∂θ(I, θ), θ −ε ∂L∗/∂I(I, θ)) is he unca ed sca e ing map. •S0, (I, θ)=(I( ), θ( )) is he solu ion o he Hamil onian sys em ˙ I( ) = ∂L∗ ∂θ (I( ), θ( )) ˙ θ( ) = −∂L∗ ∂I (I( ), θ( )),(2.53) wi h ini ial condi ion (I(0), θ(0)) = (I, θ). Le (Ih, θh) be a poin in he highway. The e o be ween he sca e ing map and he le el cu e o he educed Poinca ´e unc ion a e n-i e a es is gi en by kSn(Ih+ ∆I, θh+ ∆θ)−S0,nε(Ih, θh)k,(2.54) whe e ∆Iand ∆θa e small. No e ha we can ew i e (2.54) as k(Sn(Ih+ ∆I, θh+ ∆θ)−Sn T(Ih+ ∆I, θh+ ∆θ)) +(Sn T(Ih+ ∆I, θh+ ∆θ)−S0,nε(Ih+ ∆I, θh+ ∆θ)) +S0,nε(Ih+ ∆I, θh+ ∆θ)) −S0,nε(Ih, θh))k. We now p oceed o s udy each sub ac ion. •We begin wi h Sn(Ih+ ∆I, θh+ ∆θ)−Sn T(Ih+ ∆I, θh+ ∆θ). F om (2.52), we can eadily ob ain by induc ion ha Sn(Ih+ ∆I, θh+ ∆θ)−Sn T(Ih+ ∆I, θh+ ∆θ) = O(nε2).(2.55) •Now we conside Sn T(Ih+ ∆I, θh+ ∆θ)−S0,nε(Ih+ ∆I, θh+ ∆θ). By he de ini ion o STwe ha e ha Sn Tis he n-s ep o he Eule me hod wi h s ep size εin each coo dina e o sol ing he sys em (2.53). I is no di icul o check he s anda d bound (see, o ins ance, [SB02]) kSn T(Ih+ ∆I, θh+ ∆θ)−S0,nε(Ih+ ∆I, θh+ ∆θ)k ≤ Lε 2[(1 + εK)n−1] ,(2.56) whe e K:= max(I,θ)∈U JH(I, θ) (J∇L∗(I, θ))T , L = max(I,θ)∈Uk∇L∗(I, θ)kand H(I, θ) is he Hessian ma ix o L∗(I, θ). •Now we look o he las sub ac ion S0,nε(Ih+ ∆I, θh+ ∆θ)) −S0,nε(Ih, θh). Apply- ing G ¨ onwall’s inequali y on he a ia ional equa ion associa ed o he Hamil onian ec o ield −∇L∗(I, θ), one ge s kS0,εn(Ih+ ∆I, θh+ ∆θ)) −S0,εn(Ih, θh)k≤k(∆I, ∆θ)keKεn.(2.57) 39 We can now conclude om (2.55), (2.56) and (2.57), ha he p opaga ed e o is kSn(Ih+ ∆I, θh+ ∆θ)−S0,nε(Ih, θh)k≤O(nε2) + Lε 2[(1 + εK)n−1] + k(∆I, ∆θ)keKεn To a oid la ge p opaga ed e o s, one has o choose nsuch ha nε 1. Fo ins ance, aking n=ε−c,(2.58) wi h 0 < c < 1 (which implies nε 1) and k(∆I, ∆θ)k=εa,a > 0, one ge s kSn(Ih+ ∆I, θh+ ∆θ)−S0,nε(Ih, θh)k=O(ε2−c, εa).(2.59) 2.4.2 Es ima e o he ime o di usion In his sec ion ou goal is o es ima e he ime o di usion along he highway. We ha e h ee di e en ypes o es ima es associa ed o he ime o di usion. •The o al numbe o i e a es Nso he sca e ing map. This is he numbe o i e a es ha sca e ing map spends o co e a piece o a le el cu e o he educed Poinca ´e unc ion L∗. •The ime unde he low along he homoclinic in a ian mani olds o e Λ. This is he ime spen by each applica ion o he sca e ing map ollowing he conc e e homoclinic o bi o e Λ up o a dis ance δo e Λ. This ime is deno ed by Th=Th(δ). •The ime unde he inne map. This ime appea s i we use he inne map be ween i e a es o he sca e ing map (i is some imes called e godiza ion ime) and we deno ed i by Ti. Fo each i e a e o he sca e ing map we ha e o conside he ime Th. Besides, we ha e seen in he p e ious subsec ion ha o con ol he p opaga ed e o , we i e a e successi ely he sca e ing map jus a numbe n=ε−co imes, 0 < c 1. F om now on we deno e his numbe nby Nss. So, a e Nss i e a es o he sca e ing maps we apply he inne dynamics du ing some ime Ti o come back o a dis ance εa o he highway. The e o e, he o al ime spen unde he inne map is bNs/NsscTi. We es ima e ha he di usion ime along he highway is hus Td=NsTh+bNs/NsscTi.(2.60) Theo em 28. The ime o di usion Tdclose o a highway o Hamil onian (2.1)+(2.3) be ween −I∗ o I∗, o any 0< I∗< I+, wi h I+gi en in P oposi ion 20, sa is ies he ollowing asymp o ic exp ession Td=Ts ε2 log C ε+O(εb), o ε→0,whe e 0<b<1, 40 Conside he au onomous ex ended Hamil onian K(I, A, ϕ, s) = I2 2+A+ε(a1cos ϕ+a2cos(ϕ−s)) ,(3.4) wi h associa ed di e en ial equa ions ˙ϕ=I˙ I=ε(a1sin ϕ+a2sin(ϕ−s)) ˙s=1 ˙ A=−εa2sin(ϕ−s). This sys em is equi alen o he sys em ep esen ed by (3.2)+(3.3). We wish o elimina e he dependence on he angle a iables. Conside a change o a iables ε-close o he iden i y (ϕ, s, I, A) = g(φ, σ, J, B)=(φ, σ, J, B) + O(ε) such ha i is he one- ime low o a Hamil onian εG, i.e., g=g =1, whe e g is solu ion o dg d =J2∇εG ◦g ,whe e J2is he symplec ic ma ix 0 1 −1 0. Composing Kwi h gand expanding in a Taylo se ies a ound = 0, one ob ains K◦g=K+K, εG+1 2K, εG, εG+. . . , whe e {·} is he Poisson b acke . Using he expansion (3.4) o K, he equa ion abo e can be w i en as K◦g=J2 2+B+εa1cos φ+a2cos(φ−σ) + J2 2+B, G +ε2 2J2 2+B, G, G+O(ε3). (3.5) We wan o ind Gsuch ha a1cos φ+a2cos(φ−σ) + nJ2 2+B, Go= 0, o equi alen ly, J∂G ∂φ +∂G ∂σ =a1cos φ+a2cos(φ−σ). Gi en a < b < 1, conside any unc ion Ψ ∈C∞(R) sa is ying Ψ(x) = 1 o x∈[−a, a] and Ψ(x) = 0 o |x| ≥ band in oduce G(J, B, φ, σ) := a1 J(1 −Ψ(J)) sin φ+a2 J−1(1 −Ψ(J−1)) sin(φ−σ), Subs i u ing he abo e unc ion G(J, B, φ, σ) in (3.5) we ha e K◦g=J2 2+B+O(ε2),(3.6) 47 o J, J −1/∈[−b, b]. Fo J∈[−a, a], K◦g=J2 2+B+εa1cos φ+O(ε2).(3.7) Finally, o J−1∈[−a, a], K◦g=J2 2+B+εa2cos(φ−σ) + O(ε2).(3.8) F om (3.7) and (3.8), one sees ha on J= 0 and J= 1 he e a e esonances o i s o de in εwi h a pendulum-like beha io . Coming back o he o iginal a iables, h ee kinds o in a ian o i a e ob ained. Fo he i s o de esonance I= 0, he e is a posi i e asuch ha he in a ian o i a e gi en by F0(I, ϕ, s) = cons an wi h F0(I, ϕ, s) = I2 2+εa1cos ϕ+O(ε2).(3.9) o I∈[−a, a]. Analogously, o he i s o de esonance I= 1, wi h F1(I, ϕ, s) = (I−1)2 2+εa2cos(ϕ−s) + O(ε2), o I−1∈[−a, a]. Rema k 32. As commen ed in [DLS06], he e exis s a seconda y esonance in I= 1/2, bu he size o he gap in i s esonan egion is much smalle han he size o gaps in esonan egions associa ed o I= 0 and I= 1. Rema k 33. Fo Hamil onian (1.5) wi h 6= 1, he esonances ake place in I= 0 and I= 1/ . F om (3.6), on he non- esonan egion he in a ian o i has equa ions Fn (I) = cons an wi h Fn (I) = I2 2+O(ε2). An illus a ion o he inne dynamics is displayed in Figu e 3.1. 3.2 Sca e ing map We a e going o explo e he p ope ies o he sca e ing maps o Hamil onian (3.1). The no ion o sca e ing map on a NHIM was in oduced in [DLS00]. Le Wbe an open se o [−I∗, I∗]×T2such ha he in a ian mani olds o he NHIM ˜ Λ in oduced in (1.3) in e sec 48 Fig. 3.1: Plane ϕ×Io inne dynamics o µ= 0.75 and ε= 0.01. ans e sally along a homoclinic mani old Γ = {˜z(I, ϕ, s;ε),(I, ϕ, s)∈W}so ha o any ˜z∈Γ he e exis unique ˜x+,−= ˜x+,−(I, ϕ, s;ε)∈˜ Λ such ha ˜z∈Ws ε(x−)∩Wu ε(˜x+). Le H+,−=[{˜x+,−(I, ϕ, s;ε) : (I, ϕ, s)∈W}. The sca e ing map associa ed o Γ is he map S:H−−→ H+ ˜x−7−→ S(˜x−) = ˜x+. Fo he cha ac e iza ion o he sca e ing maps, i is equi ed o selec he homoclinic mani old Γ and his is done using he Poinca ´e-Melniko heo y. F om [DH11, DLS06], we ha e he ollowing p oposi ion (compa e wi h Chap e 2, P op. 5) P oposi ion 34. Gi en (I, ϕ, s)∈[−I∗, I∗]×T2, assume ha he eal unc ion τ∈R7−→ L(I, ϕ −I τ, s −τ)∈R(3.10) has a non degene a e c i ical poin τ∗=τ∗(I, ϕ, s), whe e L(I, ϕ, s) := Z+∞ −∞ ( (q0(σ)) − (0)) g(ϕ+Iσ, s +σ; 0)dσ. Then, o 0< ε small enough, he e exis s a unique ans e sal homoclinic poin ˜z o ˜ Λε o Hamil onian (1.1), which is ε-close o he poin ˜z∗(I, ϕ, s) = (p0(τ∗), q0(τ∗), I, ϕ, s)∈W0(˜ Λ) : ˜z= ˜z(I, ϕ, s) = (p0(τ∗) + O(ε), q0(τ∗) + O(ε), I, ϕ, s)∈Wu(˜ Λε) Ws(˜ Λε). The unc ion Lis called he Melniko po en ial o Hamil onian (1.1). Fo he conc e e Hamil onian (3.1) i akes he o m L(I, ϕ, s) = A1(I) cos ϕ+A2(I) cos(ϕ−s),(3.11) 49 whe e A1(I) = 2πIa1 sinh(πI/2) and A2(I) = 2π(I−1)a2 sinh(π(I−1)/2). The homoclinic mani old Γ is cha ac e ized by he unc ion τ∗(I, ϕ, s). Once a τ∗(I, ϕ, s) is chosen, which unde he condi ions o P oposi ion 34, is locally smoo hly well de ined, by he geome ic p ope ies o he sca e ing map, see [DH09, DH11, DLS08], he sca e ing map has he explici local o m S(I, ϕ, s) = I+ε∂L∗ ∂ϕ (I, ϕ, s) + O(ε2), ϕ −ε∂L∗ ∂I (I, ϕ, s) + O(ε2), s, whe e L∗(I, ϕ, s) = L(I, ϕ −Iτ∗(I, ϕ, s), s −τ∗(I, ϕ, s)).(3.12) No ice ha he a iable sis ixed unde he sca e ing map. As a consequence, see [DH11], in oducing he a iable θ=ϕ−Is and de ining he educed Poinca ´e unc ion L∗(I, θ) := L∗(I, ϕ −Is, 0) = L∗(I, ϕ, s),(3.13) in he a iables (I, θ), he sca e ing map has he simple o m S(I, θ) = I+ε∂L∗ ∂θ (I, θ) + O(ε2), θ −ε∂L∗ ∂I (I, θ) + O(ε2), so up o O(ε2) e ms, S(I, θ) is he ε imes low o he au onomous Hamil onian −L∗(I, θ). In pa icula , he i e a es unde he sca e ing map ollow he le el cu es o L∗up o O(ε2). 3.2.1 C es s and NHIM lines We ha e seen ha he unc ion τ∗plays a cen al ole in ou s udy. The e o e, we a e in e es ed in inding he c i ical poin s τ∗=τ∗(I, ϕ, s) o unc ion (3.10). Fo ou conc e e case (3.11), τ∗is a solu ion o IA1(I) sin(ϕ−Iτ∗)+(I−1)A2(I) sin(ϕ−s−(I−1)τ∗)=0.(3.14) This equa ion can be iewed om wo equi alen ly geome ical iewpoin s. The i s one is ha o ind τ∗=τ∗(I, ϕ, s) sa is ying (3.14) o any (I, ϕ, s)∈[−I∗, I∗]×T2is he same as o look o he ex ema o Lon he NHIM line R(I, ϕ, s) = {(I, ϕ −Iτ, s −τ) : τ∈R}.(3.15) Rema k 35. Since (ϕ, s)∈T2,R(I, ϕ, s) is a closed line i I∈Qand i is a dense line on {I}×T2i I /∈Q. 50 The o he iewpoin is ha , ixing (I, ϕ, s), a solu ion τ∗o (3.14) is equi alen o inding in e sec ions be ween a NHIM line (3.15) and a cu e de ined by IA1(I) sin ϕ+ (I−1)A2(I) sin(ϕ−s)=0. These cu es a e called c es s, and in a gene al way can be de ined as ollows. De ini ion 36. [DH11] We de ine by C es s C(I) he cu es on (I, ϕ, s), (ϕ, s)∈T2, such ha ∂L ∂τ (I, ϕ −Iτ, s −τ)|τ=0 = 0,(3.16) o equi alen ly, I∂L ∂ϕ(I, ϕ, s) + ∂L ∂s (I, ϕ, s)=0. As in ou case L(I, ϕ −Iτ, s −τ) = A1(I) cos(ϕ−Iτ) + A2(I) cos(ϕ−s−(I−1)τ), equa ion (3.16) akes he o m (3.16). In oducing σ=ϕ−s, (3.17) equa ion (3.16) can be ew i en as µα(I) sin ϕ+ sin σ= 0,(3.18) o I6= 1, whe e µ=a1 a2 and α(I) = I2sinh(π 2(I−1)) (I−1)2sinh(πI 2).(3.19) F om now on, when we e e o c es s C(I) we mean he se o poin s (I, ϕ, σ) sa is ying equa ion (3.18). See an illus a ion in Fig. 3.3. Rema k 37. In Chap e 2 he c es s we e desc ibed on he plane (ϕ, s), whe eas now such cu es lie on he plane (ϕ, σ). Besides, di e en ly om he cases s udied in [DH11] and in Chap e 2, he unc ion α(I) in oduced in (3.19) is no de ined o all I. Mo e p ecisely, i is no de ined o I= 1. Fo his alue o I, equa ion (3.18) is no adequa e, and one has o use (3.16) o check ha o I= 1 he c es s a e jus wo e ical s aigh lines on he plane (ϕ, σ) gi en by ϕ= 0 and ϕ=π. Rema k 38. Fo Hamil onian (1.5) and ∈(0,1), α (I) is no de ined o I= 1/ and is gi en by α (I) = I2sinh π 2( I −1) ( I −1)2sinh πI 2.(3.20) 51 We a e in e es ed in unde s anding he beha io o hese c es s because, as we ha e seen in[DH11] and Chap e 2, hei in e sec ion wi h he NHIM lines de e mine he exis ence and beha io o sca e ing maps. F om (3.18), when |α(I)|<1/|µ|,σcan be w i en as a unc ion o ϕ o all ϕ∈Ton he c es C(I). On he o he hand, i |α(I)|>1/|µ|,ϕcan be w i en as a unc ion o σ o all σ∈T.These wo condi ions gi e us wo kinds o c es s: ho izon al o |α(I)|<1/|µ| and e ical o |α(I)|>1/|µ|. These names a e due o hei o ms on he plane (ϕ, σ). We conside he same cha ac e iza ion used in Chap e 2: •Fo |α(I)|<1/|µ|, he e a e wo ho izon al c es s σ=ξM,m(I, ϕ) CM,m(I) = {(I, ϕ, ξM,m(I, ϕ)) : ϕ∈T}, ξM(I, ϕ) = −a csin(µα(I) sin ϕ) mod 2π(3.21) ξm(I, ϕ) = a csin(µα(I) sin ϕ) + πmod 2π. •Fo |α(I)|>1/|µ|, he e a e wo e ical c es s ϕ=ηM,m(I, σ) CM,m(I) = {(I, ηM,m(I, σ), σ) : σ∈T}, ηM(I, σ) = −a csin(sin σ/ (µα(I))) mod 2π ηm(I, σ) = a csin(sin σ/ (µα(I))) + πmod 2π. Rema k 39. |α(I)|= 1/|µ|is a singula o bi u ca ion case. In his case, he c es s a e s aigh lines and a e no di e en iable in ϕ=π/2 and ϕ= 3π/2. See Fig. 2.6. Rema k 40. The c es con aining he poin (ϕ, σ) = (0,0) will be deno ed by CM(I) and he c es con aining he poin (ϕ, σ) = (π, π) by Cm(I). No e ha he unc ion |α(I)|is no bounded, indeed lim I→1|α(I)|= +∞. This implies ha o any µ he e exis s a neighbo hood Uo I= 1 such ha o all I∈U he c es s a e e ical. On he o he hand, since α(0) = 0 he e exis s a neighbo hood V o I= 0 such ha o all I∈V he c es s a e ho izon al. We no ice he e a ema kable di e ence wi h he Hamil onians s udied in [DH11] and Chap e 2, whe e, o |µ| ≤ 0.97, all he c es s a e ho izon al o all I. Now ake a look a he p ope ies o he unc ion α(I) in oduced in (3.19) o desc ibe unde which condi ions in µ he c es s a e ho izon al o e ical. Fi s o all, obse e ha o I6= 1, α(I) is smoo h and α0(I)6= 0,and o I= 1 α(I) is no bounded, indeed i has a e ical asymp o e lim I→1−α(I) = −∞ and lim I→1+α(I) = +∞. 52 Gi en a µ6= 0, since α(0) = 0, he e exis s a unique Ic∈(0,1) such ha |α(I)|= 1/|µ|. So, he c es s a e ho izon al o I∈[0, Ic) and e ical o I∈(Ic,1). O he s impo an limi s a e lim I→−∞ α(I) = exp(π/2) and lim I→+∞α(I) = exp(−π/2). The i s limi implies ha |α(I)|<exp(π/2) o I∈(−∞,0). Thus, i exp(π/2) ≤1/|µ| he c es s a e ho izon al o I∈(−∞,0). O he wise, i 1/|µ|<exp(π/2), he e exis s a unique Il∈(−∞,0) such ha |α(I)|= 1/|µ|and he c es s a e e ical o I∈(−∞, Il) and ho izon al o I∈(Il,0). The second limi implies ha |α(I)|>exp(−π/2) o I∈(1,+∞). Then, i exp(−π/2) ≥ 1/|µ|, he c es s a e e ical o I∈[1,+∞). i exp(−π/2) <1/|µ|, he e exis s a unique I ∈(1,+∞), such ha he c es s a e e ical o any Iin [1, I ) and ho izon- al o I∈(I ,+∞). Summa izing, o 1/|µ| ≥ exp(π/2), c es s a e ho izon al o I∈(−∞, Ic)∪(I ,+∞) and e ical o I∈(Ic, I ). Fo exp(−π/2) <1/|µ|<exp(π/2), c es s a e ho izon al o I∈(Il, Ic)∪(I ,+∞) and e ical o I∈(−∞, Il)∪(Ic, I ). Finally, i 1/|µ|<exp(−π/2), c es s a e ho izon al o I∈(Il, Ic) and e ical o I∈(−∞, Il)∪(Ic,+∞). Rema k 41. Fo ∈(0,1), α (I) (3.20) is no bounded on a neighbo hood o he esonance I= 1/ , i.e., limI→1/ −α (I) = −∞ and limI→1/ +α (I)=+∞. The same beha io akes place o = 1 and close o I= 1. On he o he hand, o I→ ±∞,α (I) has he same beha io as in he case o = 0, limI→±∞ α (I) = 0. This implies ha o any alue o µ, o Iclose enough o I= 1/ he c es s a e e ical, and o |I|la ge enough he c es s a e ho izon al. Example To illus a e his discussion, we p esen a conc e e example. Taking µ= 0.5, we ha e exp(−π/2) <1/µ = 2 <exp(π/2). In his case we ha e Il≈ −1.807, Ic≈0.701 and I ≈1.367. The c es s a e ho izon al in (−1.807,0.701) ∪(1,367,+∞) and e ical in (−∞,−1.807) ∪(0.701,1.367). We emphasize ha his scena io is e y di e en om he case in Chap e 2. The e, o µ= 0.5 he c es s a e ho izon al o all I. Now, we a e going o ocus on he ans e sali y o he in e sec ion be ween NHIM lines R(I, ϕ, s) and c es s C(I). On he plane (ϕ, σ) he NHIM lines can be w i en as RI(ϕ, σ) = {(ϕ−Iτ, σ −(I−1)τ), τ ∈R},(3.22) so ha i s slope is (I−1)/I in such plane. The e o e, he e exis s an in e sec ion be ween NHIM lines and c es s ha is no ans e sal i , and only i , he e exis s a angen ec o o C(I) a a poin ha is pa allel o (I, I −1), o , using he pa ame e iza ions, ∂ξ ∂ϕ(I, ϕ) = I−1 Io ∂η ∂σ(I, σ) = I I−1. 53 Conside ing a ho izon al pa ame e iza ion o C(I), he angency condi ion is equi alen o ±α(I)µcos ϕ p1−µ2α2(I) sin2ϕ=I−1 I. The e o e, he e exis s a ϕsa is ying he abo e condi ion i , and only i , |β(I)| ≥ 1 |µ|,whe e β(I) = Iα(I) I−1 and ϕ akes he o m ϕ=±a c an sβ(I)2−(1/µ)2 (1/µ)2−α(I)2!. In an analogous way, o a e ical pa ame e iza ion η(I, σ), he e a e angencies i , and only i , |β(I)| ≤ 1 |µ|wi h σ=±a c an  I−1 Is(1/µ)2−β(I)2 α(I)2−(1/µ)2!. Rema k 42. Obse e ha in bo h cases, ho izon al and e ical c es s, he e a e angencies i , and only i , |α(I)|− 1 |µ||β(I)|− 1 |µ|<0. The unc ion |β(I)|is smoo h in R {1}and d|β(I)|/dI = 0 only o I= 0. Besides, we ha e (see Figs. 3.2(a) and 3.2(b)) lim I→1|β(I)|= +∞,lim I→−∞ |β(I)|= exp(π/2) and lim I→+∞|β(I)|= exp(−π/2). The e o e, he e a e h ee possibili ies: • o 1/|µ| ≥ exp(π/2), he e exis I0∈(1/2,1) and I+∈(1,+∞) such ha I0and I+a e solu ions o |β(I)| − 1/|µ|= 0. Besides, |β(I)|<1/|µ| o I∈(−∞, I0)∪ (I+,+∞) and |β(I)|>1/|µ| o I∈(I0,1) ∪(1, I+). • o exp(−π/2) <1/|µ|<exp(π/2), he e exis I−∈(−∞,0), I0∈(0,1) and I+∈(1,+∞) such ha I−,I0and I+a e solu ions o |β(I)|−1/|µ|= 0. Besides, |β(I)|<1/|µ| o I∈(I−, I0)∪(I+,+∞) and |β(I)|>1/|µ| o I∈(−∞, I−)∪ (I0,1) ∪(1, I+). •Fo 1/|µ| ≤ exp(−π/2), he e exis I−∈(−∞,0) and I0∈(0,1/2) such ha I−and I0a e solu ions o |β(I)|− 1/|µ|= 0. Besides, |β(I)|<1/|µ| o I∈(I−, I0) and |β(I)|>1/|µ| o I∈(−∞, I−)∪(I0,1) ∪(1,∞). 54 Pu ing oge he his desc ip ion o |β(I)|wi h he s udy abou e ical and ho izon al c es s and adding ha |β(I)|<|α(I)| ∀I∈(−∞,0) ∪(0,1/2); |β(I)|>|α(I)| ∀I∈(1/2,1) ∪(1,+∞); |β(0)|=|α(0)|= 0 |β(1/2)|=|α(1/2)|= 1 we can s a e he p oposi ion below. P oposi ion 43. Conside he wo c es s C(I)de ined by (3.18) and he NHIM line RI(ϕ, σ)de ined in (3.15) o Hamil onian (3.1). •Fo |µ| ≤ exp(−π/2), he e exis Ib< Ia< IA< IBsuch ha – o I < Ibo IB< I,C(I)a e ho izon al and in e sec ans e sally any RI(ϕ, σ); – o Ib≤I < Iao IA< I ≤IB, he c es s C(I)a e ho izon al, bu now, he e exis angencies be ween C(I)and wo NHIM lines RI(ϕ, σ); – o Ia< I < IA, he c es s C(I)a e e ical and in e sec ans e sally any RI(ϕ, σ). •Fo exp(−π/2) <|µ|<exp(π/2) he e exis Ib< Ia< Ic≤IC< IA< IBsuch ha – o I < Ibo IC< I < IA,C(I)a e e ical and in e sec ans e sally any RI(ϕ, σ); – o Ib≤I < Ia, he c es s C(I)a e e ical and he e exis angencies be ween C(I)and wo NHIM lines RI(ϕ, σ); – o Ia< I < Ico IB< I,C(I)a e ho izon al and in e sec ans e sally any RI(ϕ, σ); – o IA≤I≤IB, he c es s C(I)a e ho izon al and he e exis angencies be ween C(I)and wo NHIM lines RI(ϕ, σ); – o Ic≤I≤IC, i Ic<1/2, he c es s C(I)a e e ical and he e exis an- gencies be ween C(I)and RI(ϕ, σ). I Ic= 1/2, om he p ope ies o α(I)and β(I) his in e al is jus one poin . I Ic>1/2, he c es s C(I)a e ho izon al and he e exis angencies. •Fo |µ| ≥ exp(π/2) he e exis Ib< Ia< IA< IBsuch ha – o I < Ibo IB< I,C(I)a e e ical and in e sec ans e sally any RI(ϕ, σ); – o Ib≤I < Iao IA< I ≤IB, he c es s C(I)a e e ical and he e exis angencies be ween C(I)and wo NHIM lines RI(ϕ, σ); – o Ia< I < IA, he c es s C(I)a e ho izon al and in e sec ans e sally any RI(ϕ, σ). Rema k 44. No e ha we a e no conside ing he singula case |α(I)|= 1/|µ|desc ibed in Rema k 39. 55 Example Again, o illus a e his p oposi ion, we ake he case wi h µ= 0.5, see Fig. 3.2(a). In his case, we ha e |β(I)|= 1/µ o I≈ −2.942,0.595,1.85 and • o I∈(−∞,−2.942) ∪(0.701,1) ∪(1,1.367) ⇒|α(I)|>1/|µ| ⇒ e ical c es s |β(I)|>1/|µ| ⇒ no angencies • o I∈[−2.942,−1.807) ⇒|α(I)|>1/|µ| ⇒ e ical c es s |β(I)| ≤ 1/|µ| ⇒ angencies • o I∈(−1.807,0.595) ∪(1.85,+∞)⇒|α(I)|<1/|µ| ⇒ ho izon al c es s |β(I)|<1/|µ| ⇒ no angencies • o I∈[0.595,0.701) ∪(1.367,1.85] ⇒|α(I)|<1/|µ| ⇒ ho izon al c es s |β(I)| ≥ 1/|µ| ⇒ angencies Once mo e, we compa e wi h he Hamil onian (1.6) s udied in Chap e 2. Fo Hamil o- nian (1.6) and µ= 0.5 he e is no angency, bu o Hamil onian (3.1) we can ind angencies o ho izon al and e ical c es s. Indeed, o Hamil onian (1.6) and any 0 <|µ|<0.625 he e is no angency, whe eas o any µ6= 0 he e a e angencies o Hamil onian (3.1). (a) |α(I)|and |β(I)|:µ= 0.5, Ib≈ −2.942, Ia≈ −1.807, Ic≈0.595, IC≈0.701, IA≈ 1.367 and IB≈1.85 (b) |α (I)|and |β (I)|:µ= 0.5 and = 0.5. Fig. 3.2: |α(I)|and |β(I)|: Beha io o he c es s and angencies. Rema k 45. Fo ∈(0,1) in Hamil onian (1.5), β (I) is de ined by β (I) = Iα (I)/( I − 1). In his case, limI→1/ |β (I)|= +∞and limI→±∞ |β (I)|= 0. In Fig. 3.2(b), a compa - ison be ween he unc ions α (I), β (I) and he s aigh line 1/|µ| o = 1/2 is displayed. Fo each c es , whe e i is well de ined, he e exis s, a leas , a alue τ∗such ha (ϕ−Iτ∗, σ −(I−1)τ∗)=(ϕ−Iτ∗, ξ(I, ϕ −Iτ∗)) o (η(I, σ −(I−1)τ∗), σ −(I−1)τ∗), which means ha RI(ϕ, σ)∩ C(I)6=∅. This in e sec ion is in insically associa ed o a homoclinic o bi o he NHIM. To make a choice abou how o ake such τ∗is o choose in which homoclinic mani old Γ he homoclinic poin s ˜z∗lie. E en mo e, i is o choose wha sca e ing map we a e going o use. 56 c) Fo I > 1, one mo e ime α(I)>0 and sin ξ1(I, ϕ) sin(ϕ)<0, bu now 0 < m = 1−1/I < 1. We i s ix θ= 3π/2 and sea ch o Isuch ha 3π 2−Iτ∗(I, 3π/2) = 0 3π 2−(I−1)τ∗(I, 3π/2) = π. We ob ain I= 3/2, so θ−Iτ∗ 1(I, θ)∈(0, π) o any I≥3/2 and θ∈(π, θ+= 3π/2). Consequen ly, sin(θ−Iτ∗ 1(I, θ)) >0 and ˙ I > 0. Fo he alues o I∈(1,3/2) we change he s a egy. We look o θ∗such ha θ−Iτ∗(I, θ) = 0 θ−(I−1)τ∗(I, θ) = π. We ha e θ∗=πI and θ−Iτ∗ 1(I, θ∗)∈(0, π) o any I∈(1,3/2) and θ∈(π, θ∗), so ˙ I > 0. No e ha θ∗<3π/2 and we can de ine θ+:= θ∗. Obse e ha o I= 1 he c es s a e e ical, and o I= 0, θ=θ−Iτ∗ 1(I, θ), and ˙ I > 0 o θ∈(π, 3π/2). Conside now he case o e ical c es s (|α(I)µ|>1). a) Fo I < 0, sin η1(I, σ) sin σ=−µα(I) sin2σ≤0 and m > 1. We ix θ= 3π/2 and look o Isuch ha 3π/2π−Iτ∗=π 3π/2−(I−1)τ∗(I, 3π/2) = 0. We ob ain I=−1/2 and he e o e, sin(θ−(I−1)τ∗ 1(I, θ)) >0 o I∈(−∞,−1/2) and θ∈(π, 3π/2). Consequen ly, ˙ I > 0 om (3.27). Fo I∈(−1/2,0), we ha e ha θ+= (1 −I)πsa is ies θ−Iτ∗(I, θ+) = π θ+−(I−1)τ∗(I, θ+) = 0. The e o e, sin(θ−(I−1)τ∗ 1)(I, θ)>0 and ˙ I > 0 o any θ∈(π, θ+). b) Fo 0 < I < 1 sin η1(I, σ) sin σ≥0 and m < 0. θ+= (I+ 1)πsa is ies θ−Iτ∗(I, θ+) = π θ+−(I−1)τ∗(I, θ+)=2π. So, sin(θ−(I−1)τ∗ 1(I, θ)) >0 and ˙ I > 0 o any θ∈(π, θ+). No e ha θ+<3π/2 o I∈(0,1/2). c) Finally, o I > 1, sin η1(I, σ) sin σ≤0. We ha e ha θ−(I−1)τ∗ 1(I, θ)∈(π, 2π), so sin(θ−(I−1)τ∗ 1(I, θ)) <0 and ˙ I > 0 o any θ∈(π, 3π/2). 63 Fo I= 0 he c es s a e ho izon al. Fo I= 1, θ=θ−(I−1)τ∗ 1(I, θ), so ˙ I > 0 o θ∈(π, 2π). Rema k 52. I a1<0, we ha e ha he e exis s a θ−such ha ˙ I > 0 o any θ∈(θ−, π). Rema k 53. An analogous p oposi ion holds o S2(I, θ), he sca e ing map associa ed o he g aphs o ξ2and η2o C2(I). In such case, he e is a θ+such ha ˙ I≥0 o any θ∈(θ+,2π) whe e θ≥3π/2 o I∈(1/2,3/2). No e ha his p oposi ion leads us o ensu e he di usion in an analogous way o he one used o p o e Theo em 25. Nex , he di usion mechanism is s a ed and he A nold di usion is p o en. 3.3 A nold Di usion In his sec ion we a e going o comple e ou goal p o ing he exis ence o global ins a- bili y o A nold di usion, ha is, Theo em 1. We begin by p esen ing some gene al geome ical p ope ies o he sca e ing maps ha we ha e o ake in o accoun o p o e he heo em o di usion. The i s one educes he s udy o sca e ing maps o posi i e alues o µ. Mo e p ecisely, we ha e he lemma below Lemma 54. The sca e ing map o a alue o µand s=π, associa ed o he in e sec ion be ween R(I, ϕ, s)and Cm(I)(CM(I)) has he same geome ical p ope ies as he sca e ing map o −µand s= 0, associa ed o he in e sec ion be ween Rθ(I)and CM(I)(Cm(I)), i.e., Sµ m(M)(I, ϕ, π) = S−µ M(m)(I, ϕ, 0) = S−µ M(m)(I, θ) P oo . Fi s , we look o τ∗ msuch ha he NHIM segmen R(I, ϕ, s) in e sec s he c es Cm(I). I we ix s=π, we ha e om (3.11) and (3.12): L∗ µ,m(I, ϕ, π) =A1(I) cos(ϕ−Iτ∗ m(I, ϕ, π)) +A2(I) cos(ϕ−π−(I−1)τ∗ m(I, ϕ, π)).(3.29) Besides, τ∗sa is ies µα(I) sin(ϕ−Iτ∗ m) + sin(ϕ−π−(I−1)τ∗ m) = 0, o −µα(I) sin(ϕ−Iτ∗ m) + sin(ϕ−(I−1)τ∗ m) = 0. We ha e ha ϕ−π−(I−1)τ∗ m(mod 2π) = ξm(I, ϕ −Iτ∗ m) wi h π/2≤ξm≤3π/2. Then, o each τ∗ m he e exis s a K∈Zsuch ha π 2< ϕ −π−(I−1)τ∗ m+ 2πK < 3π 2. 64 This implies 3π 2< ϕ −(I−1)τ∗ m+ 2πK and ϕ−(I−1)τ∗ m+ 2π(K−1) <π 2. The e o e, ϕ−(I−1)τ∗ m(mod 2π)<π 2o ϕ−(I−1)τ∗ m(mod 2π)>3π 2. We can conclude ha ϕ−(I−1)τ∗ m(mod 2π) = ξM(I, ϕ −Iτ∗ m). The e o e τ∗ m(I, ϕ, π) o µis equal o τ∗ M(I, ϕ, 0) o −µ. F om (3.29), L∗ µ,m(I, ϕ, π) sa is ies L∗ µ,m(I, ϕ, π) = A1(I) cos(ϕ−τ∗ M(I, ϕ, 0)) + (−A2(I)) cos(ϕ−(I−1)τ∗ M(I, ϕ, 0)) =L∗ −µ,M(I, ϕ, 0). Since L∗ µ,m(·,·, π) and L∗ −µ,M(·,·,0) coincide, hei de i a i es oo and his implies ha Sµ m(I, ϕ, π) = S−µ M(I, ϕ, 0) = S−µ M(I, θ). F om now on, jus o simpli y he exposi ion, a1and a2a e conside ed posi i e. The same s a egy used in Chap e 2, Sec ion 2.3, is applied o p o e he exis ence he di usion: we combine he sca e ing map in an in e al o θwhe e ˙ I > 0 and he inne map o build a di usion pseudo-o bi . Then we apply shadowing esul s o ge he exis ence o a di usion o bi . Since I= 0 and I= 1 a e esonance alues, he applica ion o he inne map mus be mo e ca e ul, because in hese esonance egions, o some o bi s, he alue o Idec eases in o de O(√ε), i. e., he o i canno be conside ed la . We s udy he ans e sali y be ween he olia ions o in a ian se s o he inne and he sca e ing map in esonan and non- esonan egions and i s image unde he sca e ing map S. Fo mo e de ails and a mo e gene al case, he eade is e e ed o [DH09]. Conside he esonan egion associa ed o I= 0. In such egion, he o i can be app oxima ed by F0(I, ϕ) gi en in (3.9). The an e sali y be ween in a ian se s o he inne and he sca e ing map holds i he g adien ec o s o he le el cu es o F0and L∗ a e no pa allel ec o s, o equi alen ly, F0(I, θ),L∗(I, θ)6= 0, whe e {,}is he Poisson b acke , F0,L∗=∂F0 ∂θ ∂L ∂I −∂F0 ∂I ∂L ∂θ . F om (3.9), he pa ial de i a i es o F0a e ∂F0 ∂I =Iand ∂F0 ∂θ =−εa1sin θ, 65 and since L∗(I, θ) = A1(I) cos(θ−Iτ∗(I, θ)) + A2(I) cos(θ−(I−1)τ∗(I, θ)), we ha e he pa ial de i a i es gi en by ∂L∗ ∂θ =A1(I) sin(θ−Iτ∗) I−1, ∂L∗ ∂I =A0 1(I) cos(θ−Iτ∗) + A0 2(I) cos(θ−(I−1)τ∗) +A1(I)τ∗sin(θ−Iτ∗) + A2(I)τ∗sin(θ−(I−1)τ∗). No e ha i |I|>O(ε), ∂F0/∂I domina es ∂F0/∂θ, so he Poisson b acke abo e can be educed o F0,L∗≃ −∂F0 ∂I ∂L ∂θ =−IA1(I) sin(θ−Iτ∗) I−1 Expanding sin(θ−Iτ∗) in Taylo ’s se ies a ound I= 0, we ha e sin(θ−Iτ∗) = sin θ+O(I), which implies {F0,L∗}= 0 i , and only i , θ≈0, π, assuming ha O(I) is small enough. Now, we conside I=O(ε) and look a he in e sec ions be ween he NHIM lines and he g aph o ξ1. No e ha as he alue o Iis close o 0 we can assume ha he c es s a e ho izon al. Using Taylo ’s se ies we can w i e sin(θ−Iτ∗) = sin θ+O(I) cos(θ−Iτ∗) = cos θ+O(I) sin(θ−(I−1)τ∗) = O(I) cos(θ−(I−1)τ∗) = −1 + O(I). This implies F0,L∗=−IA1(I) sin θ I−1−εa1sin θ(A0 1(I) cos θ−A0 2(I) +A1(I)τ∗sin θ) + O(I2, εI). (3.30) Taylo expanding he unc ions A1(I), A0 1(I) and A0 2(I) a ound I= 0, we ob ain A1(I) = 4a1+O(I2), A0 1(I) = O(I) and A0 2(I) = a2π(πco h π/2−2)csch(π/2) + O(I) Plugging hese exp essions in (3.30), we se F0,L∗=−4a1Isin θ I−1−εa1sin θ[a2π(πco h π/2−2)csch(π/2) +4a1(π−θ) sin θ] + O(I2, Iε). The e o e, F0,L∗= 0 ⇔a1sin θ−4I I−1−εa2ππco h π 2−2csch π 2) +ε4(π−θ) sin θ] = 0. 66 In o he wo ds, we do no ha e ans e sali y i , and only i , θ= 0, π o sa is ies (π−θ) sin θ=I εa1 +π(co h π/2−2)cschπ/2) 4, which is no an ho izon al cu e in he plane (θ, I) and is ans e sal o an in a ian o us o he inne dynamics. Fo he o he esonan egion I= 1, F1is e y simila . Assuming I−1 = O(ε), we ha e F1,L∗=a2sin θ4I−1 I−ε[πa1(2 −πco h(π/2))csch(π/2) + 4a2sin θ]. Applying he same me hodology, we ob ain an analogous esul o he o he esonan egion F1. In sho , we conclude ha he image S(Ti) o an in a ian o us Tio he inne map unde he sca e ing map in e sec s an e sally ano he in a ian o us Ti+1 o he inne map. Finally, in he non- esonan egion, we no ice ha {Fn ,L∗}=−∂Fn ∂I ∂L∗ ∂θ =−IA1(I) sin(θ−Iτ∗) I−1, jus he same exp ession as he one o he esonance I= 0, so he ans e sali y be ween in a ian se s o he inne and he sca e ing map ollows. Now, a cons uc i e p oo o Theo em 1 is p esen ed. This p oo is simila o he p oo p esen ed in Subsec ion 2.3.2 o Chap e 2, bu now, he e is no any piece o “highway” o as e ical lines whe e |I|is la ge. So, he inne map is applied mo e imes. 3.3.1 P oo o Theo em 1 P oo . We conside = 1 in Hamil onian (1.5). Fi s o all we ha e o choose wha sca e ing map we use. This choice depends on he sign o µas explained in Lemma 54. Assuming µ > 0, we ake S1(I, θ), he global sca e ing map associa ed o he g aphs o ξ1 and η1. I a1>0, by P oposi ion 51 o any I he e exis s an in e al θ∈(π, θ+) whe e ˙ I > 0. De ine H he se (ρ, θ+)×[−I∗, I∗], whe e ρ=π+δis such ha π < ρ < θ+ and he ans e sali y be ween NHIM lines and L∗ 1holds. We i s cons uc a pseudo- o bi {(Ii, θi) : i= 0, . . . , N1} ⊂ H wi h I0=−I∗and θN1as close as possible o ρ. No e ha all hese poin s lie in he same le el cu e o L∗ 1, ha is, L∗ 1(I0, θ0) = L∗ 1(Ii, θi), i= 1, . . . , N1. Applying he inne dynamics, we ge (IN1+1, θN1+1) = φ N1(IN1, θN1) wi h θN1+1 ∈(ρ, θ+) and hen we cons uc a pseudo-o bi {(Ii, θi) : i=N1+ 1, . . . , N1+M1} ⊂ L∗ 1(IN1+1, θN1+1) = lN1+1 wi h θi∈(ρ, θN1+1), θ+−θN1+M1=O(ε2). Applying he inne dynamics, we ge (IN1+M1+1, θN1+M1+1) = φ N1+M1(IN1+M1, θN1+M1) wi h θN1+M1+1 ∈(ρ, θ+). Recu si ely, we cons uc a pseudo-o bi {(Ii, θi) : i= N1+ 1,...,N2}such ha IN2≥I∗. In he same way, as in he p oo o Teo em 25, we can apply shadowing echniques o [FM00, FM03, GLS14], due o he ac ha he inne dynamics is simple enough o sa is y 67 he equi ed hypo hesis o hese e e ences, o p o e he exis ence o a di usion ajec o y. I a10 <0, changing H o Hl= (θ+, π) all he p e ious easoning applies. Conside ing Rema k 33, Rema k 38, Rema k 41 and Rema k 45, o any ∈(0,1), an equi alen di usion esul is eadily ob ained. And, inally, he case o = 0 is p o ed in Theo em 25 in Chap e 2. 3.4 Piecewise smoo h global sca e ing maps In his sec ion, he geome ic eedom o he choice o τ∗is explo ed. Un il now, only wo di e en sca e ing maps ha e been used o build a global one, and his was enough o ensu e di usion. Bu , wi h his app oach, inding a di usion pseudo-o bi is no always easy enough and his pseudo-o bi can be also complica ed. This depends simply on he “aspec ” o he sca e ing map ob ained. We now sugges a new c i e ion o choose τ∗: o ake he minimal alue o |τ∗| o any (θ, I). This p o ides us wi h a piecewise smoo h global sca e ing map wi h a good p ope y: he phase space o his sca e ing map which is O(ε2)-close o he le el se s o he educed Poinca ´e unc ion L∗(I, θ) associa ed o he chosen τ∗is simple and“cleane ” han he phase spaces o o he sca e ing maps displayed up o now. By a cleane sca e ing map, we mean ha we can easily iden i y and unde s and he o bi s o he sca e ing maps, excep o a small egion which con ains he angency locus. Besides, he zones whe e he alue o Iis inc eased o dec eased unde he sca e ing map is well beha ed. Idec eases o θ∈(0, π) ( he ed egion on all pic u es in Fig. 3.6) and Iinc eases o θ∈(π, 2π) ( he g een egion on all pic u es in Fig. 3.6). So i is easy o in e ha o inding a di usion pseudo-o bi i is enough o build a combina ion be ween he inne map and his sca e ing map es ic ed o (π, 2π), o example i an inc eased alue o Iis wished. The same idea used in he p oo o Theo em 1. Obse e ha he sca e ing maps we a e now conside ing a e a mix o he sca e ing maps s udied p e iously. As an example, we illus a e he sca e ing map ob ained o µ= 0.9. Such sca e ing map can be di ided in o h ee egions and in each egion, he sca e ing map coincides wi h a sca e ing map s udied be o e. In Fig. 3.7, o egions I (0 < θ < π/2), II (π/2< θ < 3π/2) and III (3π/2< θ < 2π) he sca e ing map has he ollowing co espondence: I Ex ended sca e ing map S0(I, θ) associa ed o he ho izon al CM(I) “unde ” σ=ϕ. II Ex ended sca e ing map S1(I, θ) associa ed o he ho izon al Cm(I). III Ex ended sca e ing map S2(I, θ) associa ed o he ho izon al CM(I) “o e ” σ=ϕ. I ex ended sca e ing maps a e no conside ed and we jus use sca e ing maps associ- a ed o ho izon al and e ical c es s, one can see ha hese sca e ing maps can be di ided in o 6 egions, i.e., hey can be iewed as a combina ion o up o 6 sca e ing maps. 68 (a) Piecewise sca e ing map o µ= 0.3. (b) Piecewise sca e ing map o µ= 0.5. (c) Piecewise sca e ing map o µ= 0.9. (d) Piecewise sca e ing map o µ= 1.5. Fig. 3.6: Examples o piecewise smoo h global sca e ing maps. The o bi s o sca e ing maps a e ep esen ed by he blue lines. In he ed zones he alues o Ion such o bi s dec ease, in he g een one he alues o Iinc ease. Ano he p ope y o hese sca e ing maps is he loss o di e en iabili y on he s aigh lines θ=π/2 and θ= 3π/2. The ec o ield associa ed o he Hamil onian −L∗ ide ined a ound hese discon inui y lines beha es as he ec o ields s udied in non-smoo h dynam- ics heo y. Mo e p ecisely, we can ind egions wi h slide and uns able slide beha io [Fil88]. In a u u e wo k, we en isage o design special pseudo-o bi s along hese discon inui y lines using such heo y. No e ha hese pseudo-o bi s would be e y simila o he “highways” de ined in 2.3 o Chap e 2, so in p inciple, one can expec as and simple di usion along hese discon inui y lines. 69 Fig. 3.7: A piecewise smoo h global sca e ing map di ided in o 3 egions. The e ical black lines a e he bounda ies o he domains o smoo h sca e ing maps. 70 Chap e 4 A case o 3+1/2 deg ees o eedom A e a s udy abou an a p io i uns able Hamil onian sys em wi h 2 + 1/2 deg ees o eedom, a na u al ques ion is wha happens o a simila sys em wi h mo e deg ees o eedom. In his chap e , we y o answe , a leas pa ially, his ques ion. Pa ially because we conside a pa icula case o 3 + 1/2 deg ees o eedom. We a e going o conside a gene aliza ion o he Hamil onian conside ed in Chap e s 2 and 3, which is gi en by he a p io i uns able Hamil onian wi h 3+1/2 deg ees o eedom Hε(p, q, I1, I2, ϕ1, ϕ2, s) = ±p2 2+ cos q−1+h(I1, I2) + ε (q)g(ϕ1, ϕ2, s),(4.1) whe e (q) = cos q,h(I1, I2) = Ω1I2 1/2+Ω2I2 2/2 and g(ϕ1, ϕ2, s) = a1cos ϕ1+a2cos ϕ2+a3cos(k·ϕ−s), wi h k= (k1, k2)∈Z2and (ϕ1, ϕ2)∈T2. Rema k 55. In [DLS16], he au ho s deal wi h k= (1,1) as an example o hei esul s. In his hesis, we es ic ou a en ion o he case wi h k= (0,0). The e a e wo main easons o his es ic ion: Fi s , his sys em is a di ec gene aliza ion o Hamil onian (2.1)+(2.3) in Chap e 2. So, o his Hamil onian, we can expec o ind a simila beha - io o he c es s, he exis ence o global sca e ing maps and, mo eo e , he exis ence o highways. Besides, we ha e a well-known case o compa e wi h he new esul s ob ained. The second eason is ha i is much easie o handle i because we educed he numbe o pa ame e s and i s inne dynamics is simpli ied. The e o e, om now on, we a e always assume g(ϕ1, ϕ2, s) = a1cos ϕ1+a2cos ϕ2+a3cos s. (4.2) Fo a simple no a ion, we deno e I= (I1, I2) and ϕ= (ϕ1, ϕ2). 71 4.1 Unpe u bed case In he unpe u bed case (ε= 0), such sys em is he Hamil onian sys em wi h Hamil o- nian H0(p, q, I, ϕ, s) = ±p2 2+ cos q−1+h(I), and equa ions ˙q=p˙p= sin q ˙ϕ1=ω1˙ I1= 0 ˙ϕ2=ω2˙ I2= 0 ˙s= 1, whe e ωi= ΩiIi,i= 1,2. This sys em consis s o a pendulum plus wo o o s. F om he equa ions abo e, I1and I2a e cons an s and he low has he o m Φ (p, q, I, ϕ)=(p( ), q( ), I, ϕ + ω), whe e ω= (ω1, ω2). And we ha e an in a ian se (on he ex end phase space) TI={(0,0, I, ϕ, s); ϕ, s ∈T3}. In his case, he NHIM is ˜ Λ = {(0,0, I, ϕ, s):(I, ϕ, s)∈R2×T3},(4.3) 4.2 Inne dynamics The inne dynamics is de i ed om he es ic ion o he Hamil onian (4.1) and i s equa ions o ˜ Λ, gi en in (4.3), i.e., Kε(I, ϕ, s) = h(I) + ε(a1cos ϕ1+a2cos ϕ2+a3cos s) and i s equa ions ˙ϕ1=ω1˙ I1=εa1sin ϕ1 ˙ϕ2=ω2˙ I2=εa2sin ϕ2 ˙s= 1. No e ha he inne dynamics is in eg able, wi h i s in eg als F1(I1, ϕ1) = Ω1I2 1 2+a1(cos ϕ1−1) and F2(I2, ϕ2) = Ω2I2 2 2+a2(cos ϕ2−1) in in olu ion. The inne dynamics is jus he p oduc in he spaces (I1, ϕ1), (I2, ϕ2) o he dynamics desc ibed in Fig. 2.2, so he e a e wo esonances cen e ed a I1= 0 and I2= 0. 72 F om (4.6), i is o e i y ha Aiis an e en unc ion, and he e o e, L∗(−I, θ) = A1cos(θ1+ω1τ∗(−I, θ))+A2cos(θ2+ω2τ∗(−I, θ))+A3cos(−τ∗(−I, θ)). (4.17) F om (4.12) and (4.12), τ∗(I, θ) is he solu ion o ω1A1sin(θ1−ω1τ) + ω2A2sin(θ2−ω2τ) + A3sin(−τ)=0.(4.18) Analogously, τ∗(−I, θ) is he solu ion o −ω1A1sin(θ1+ω1τ)−ω2A2sin(θ2+ω2τ) + A3sin(−τ) = 0. No e ha he abo e equa ion can be w i en as ω1A1sin(θ1−ω1(−τ))ω2A2sin(θ2−ω2(−τ)) + A3sin(−(−τ)) = 0.(4.19) F om he local uniqueness o he solu ion o (4.18) and (4.19) we can conclude τ∗ j(I, θ) = −τ∗ −j(−I, θ), so τ∗ 0(I, θ) = −τ∗ 0(−I, θ) Applying his equali y in (4.17), we ob ain L∗ 0(−I, θ) = A1cos(θ1−ω1τ∗ 0(I, θ)) + A2cos(θ2−ω2τ∗ 0(I, θ)) + A3cos(τ∗ 0(I, θ)). The e o e, L∗ 0(I, θ) = L∗ 0(−I, θ). Le (I+, θ+) = S0(I, θ) and (I−, θ−) = S−1 0(−I, θ), whe e S−1 0is he in e se image o he sca e ing map. We a e going o p o e ha I+=−I−and θ+=θ−. F om (4.9) we ha e I+=I+ε∂L∗ 0 ∂θ (I, θ) + O(ε2) and θ+=θ−ε∂L∗ 0 ∂I (I, θ) + O(ε2). On he o he hand, i is easy o e i y ha S−1 0(−I, θ) is I−=−I+ (−ε)∂L∗ 0 ∂θ (−I, θ) + O(ε2) and θ−=θ−(−ε)∂L∗ 0 ∂I (−I, θ) + O(ε2). Now, we use he ac ha L∗ 0(I, θ) = L∗ 0(−I, θ), and so I−=−I+ (−ε)∂L∗ 0 ∂θ (I, θ) + O(ε2) = −I+ θ−=θ−(−ε)−∂L∗ 0 ∂I (I, θ)+O(ε2) = θ+. b) Analogously o he abo e case, τ∗(I, 2π−θ) is he solu ion o ω1A1sin(2π−θ1−ω1τ) + ω2A2sin(2π−θ2−ω2τ) + A3sin(−τ)=0. 79 O , equi alen ly, ω1A1sin(θ1−ω1(−τ)) + ω2A2sin(θ2−ω2(−τ)) + A3sin(−(−τ)) = 0. This implies τ∗(I, θ) = −τ∗(I, 2π−θ). As he ela ed sca e ing map depends on which in e al he unc ion τ∗(I, θ) belongs, we can w i e τ∗ j(I, θ) = −τ∗ −j(I, 2π−θ), j∈Z. The e o e, we ha e τ∗ 0(I, θ) = −τ∗ 0(I, 2π−θ). Using his equali y and he 2πpe iodici y o he cosine, L∗ 0(I, 2π−θ) = A1cos(−θ1+ω1τ∗ 0(I, θ)) + A2cos(−θ2+ω2τ∗ 0(I, θ)) + A3cos(τ∗ 0(I, θ)) =A1cos(θ1−ω1τ∗ 0(I, θ)) + A2cos(θ2−ω2τ∗ 0(I, θ)) + A3cos(−τ∗ 0(I, θ)) =L∗ 0(I, θ). Le (I+, θ+) = S0(I, 2π−θ) and (I−, θ−) = S−1 0(I, θ), whe e S−1 0is he in e se image o he sca e ing map. We wan o p o e I−=I+and θ+= 2π−θ−. F om (4.9) we ha e I+=I+ε∂L∗ 0 ∂θ (I, 2π−θ) + O(ε2) = I+ε−∂L∗ 0 ∂θ (I, θ)+O(ε2) =I+ (−ε)∂L∗ 0 ∂θ (I, θ) + O(ε2) = I−. In he same way, θ+= (2π−θ)−ε∂L∗ 0 ∂I (I, 2π−θ) + O(ε2) = 2π−θ−(−ε)∂L∗ 0 ∂I (I, θ) + O(ε2)= 2π−θ−. Theo em 62 (The gene al di usion).Conside he Hamil onian (4.1)+(4.2). Assume a1a2a36= 0 and |a1/a3|+|a2/a3|<0.625. Then, o e e y δ < 1 he e exis s ε0>0such ha o e e y 0<|ε|< ε0, gi en I±∈ I∗ {(0,0)}, he e exis s an o bi ˜x( )and T > 0, such ha |I(˜x(0)) −I−| ≤ Cδ |I(˜x(T)) −I+| ≤ Cδ P oo . Conside i s he case ha I2−=I2+ so ha I−,I+a e joined by a ho izon al line γ: [0, ∗]→R2such ha γ(0) = I−,γ( ∗) = I+,I1−< I1+ and γ( )6= (0,0) o ∈[0, ∗]. Gi en a posi i e δ, de ine he ini e open co e ing o he image o he cu e γ N [ i=0 Bδ(γ( i)), 80 whe e Bδ(γ( i)) = {p∈R2:kγ( i)−pk∞< δ}. Le Ii∈Bδ(γ( i)) and Ii/∈Bδ(γ( i+1)). This implies Ii 1< γ1( i)< γ1( i+1). We ake he ec o ui=γ( i+1)−Ii. We wan o ind a ec o isa is ying i 1ui 1>0 and i 2ui 2>0. Assume ui 2>0 (ui 1=γ1( i+1)−Ii 1>0 ). In his case we wish j>0, j={1,2}. This implies Ii 2< γ2( i) = γ2( i+1). Since i=˙ I(Ii, θ∗) = −A1(I1) sin(θ∗ 1−ωi 1τ∗(Ii, θ∗),−A2(I2) sin(θ∗ 2−ωi 2τ∗(Ii, θ∗)) and assuming a1, a2>0, j>0 i , and only i , θ∗ j−ωi jτ∗(Ii, θ∗)∈(π, 2π). Since he ini ial alues (Ii, θi), we wan o use he inne dynamics o displace θi o a poin θ∗∈(π, 2π)2. The inne dynamics is e y simple and as Chap e 2 we a e going o assume ha i is ho izon al, i.e., i is desc ibed by he equa ions ˙ Ij= 0 and ˙ϕj=ωj, j = 1,2. And he e o e, ϕ( ) = ω +ϕ(0). So, we wish o p o e he exis ence o a ∗such ha θ( ∗)−ωiτ∗(Ii, θ( ∗)) ∈(π, 2π)2, whe e θ( ) = θi+ωi . De ine ψj( ) = θi j( )−ωi jτ∗(Ii, θ( )). Wi hou loss o gene ali y we can assume ωi 1≥ωi 2, we ha e ψ2=ωi 2 ωi 1 ψ1+¯ ψ, whe e ¯ ψ=θi 2−ωi 2θi 1/ωi 1. Fo ωi 2/ωi 1∈R Q, (ψ1, ψ2(ψ1)) is dense in T2, hen he e exis s a ∗such ha (ψ1( ∗), ψ2( ∗)) ∈(π, 2π). Fo ωi 2/ωi 1=p/q ∈Q,q, p ∈Z, assume wi hou loss o gene ali y q p > 0, his implies 0< p/q ≤1. Now, we look a ψ2(ψ1) = 2πpψ1/q +¯ ψas a o a ion by he angle 2πp/q o Con he S1. So, we w i e l(¯ ψ) = 2πp ql+¯ ψ. We wan o p o e ha o any ¯ ψ he e exis s a l∈Nsuch ha l(¯ ψ)∈(π, 2π], so ha he s aigh lines (ψ1, ψ2(ψ1)) in e sec s (π, 2π)2. Suppose by con adic ion ha l(¯ ψ)∈(0, π], l∈N. No e ha l(¯ ψ) is a q-pe iodic unc ion. This implies ha he e exis s a l0∈N 0 such ha l0(¯ ψ) = ¯ ψ. The e o e, i ¯ ψ∈(π, 2π] we ob ain a con adic ion. So, assume ¯ ψ∈(0, π] and conside he o bi O=0, 1(¯ ψ), . . . , q−1(¯ ψ). Fo q6= 1, i we so he poin s o he o bi we ha e o ob ain qequidis an poin s in S1. Impossible i l(¯ ψ)∈(0, π], l∈ {0, . . . , q −1}. Fo q= 1, ωi 1=ωi 2and i is easy o e i y ha (ψ1, ψ2(ψ1)) does no in e sec (π, 2π]2 only o ¯ ψ=π. We i s p o e he case ha i does no happen. 81 We wan o p o e o any k∈ {0, . . . , N},Ikis δ-close o he cu e γ. We ha e Ii+1 =Ii+ε i+O(ε2).(4.20) So, Ii+1 is δ-close o γi he ollowing condi ions a e sa is ied Ii+1 2< γ2( i) + δand Ii+1 1< γ1( i+1) + δ. F om (4.20) and i we conside only he e ms o he i s o de , hese condi ions a e equi alen o ε < γ2( i)−Ii 2+δ i 2 and ε < γ1( i+1)−Ii 1+δ i 1 . No e ha γ2( i)−Ii 2< δ and γ( i+1)−Ii 1> δ. Besides, i 1, i 2≤ k ik∞. The e o e, i is enough o equi e ε < γ2( i)−Ii 2+δ k ik∞ .(4.21) De ine εi= sup nε:ε < γ2( i)−Ii 2+δ k ik∞o,we ob ain o any 0 <  ≤εi,Ii+1 is δ-close o γ. Fo u2≤0, (4.21) akes he o m ε < Ii 2−γ2( i) + δ k ik∞ . Now we wish o ob ain a simila esul o any i e a e o sca e ing map. Obse e ha k ik∞<4a, o any iand a= max {a1, a2}. The e o e, he esul is hold i we conside ε < δ 4a. Tha is, we ake ε0= sup ε: 0 <ε< δ 4a, and hus o any ε<ε0we ob ain a pseudo-o bi δ-close o γ. Now we come back o he case whe e ωi 1=ωi 2and ¯ ψ=π. In his case (ψ1, ψ2(ψ1)) in e sec s jus ((0, π)×(π, 2π)) S((π, 2π)×(0, π)). Now, we conside a ini e open co e o he image o he s aigh line γgi en by N [ i=0 Bδ/2(γ( i)), whe e Bδ/2(γ( i)) = {p∈R2:kγ( i)−pk∞< δ/2}. As ui 1, ui 2>0, we ake i 1>0 and i 2<0. The image o he sca e ing map in he a iable Iis gi en by Ii+1 1=Ii 1+ε i 1+O(ε2) and Ii+1 2=Ii 2+ε i 2+O(ε2).(4.22) The p oblem is when Ii+1 2< γ2( i)−δ. F om (4.22), Ii+1 2> γ2( i)−δ⇔δ > γ2( i)−Ii 2− i 2εi 2+O(ε2). 82 As Ii∈Bδ(γ( i)), we ha e γ2( i)−Ii 2< δ/2. Besides, k ik∞<4a. The e o e, Ii+1 2> γ2( i)−δ⇔δ/2>4aε. O explici ly, Ii+1 2< γ2( i)−δ o any εsa is ying ε < δ 8a. We p o e now ha his si ua ion is no in a ian , we mean, i is no possible in ou pu pose o ob ain ωi+1 1=ωi+1 2and θi+1 2−θi+1 1=π. We ha e θi+1 2−θi+1 1=θi 2−ε i 2−θi 1+ε i 1+O(ε2) =π−ε i 2− i 1+O(ε2). Then, θi+1 2−θi+1 1= 0 i , and only i , −ε( i 2− i 1) + O(ε2)=2πK,K∈Z. Since i 1 i 2<0, K6= 0. F om he de ini ion o i, we ha e i 1=−A1(I1) sin(θ1−ω1τ∗(Ii, θi)) and i 2=−A2(I2) sin(θ2−ω2τ∗(Ii, θi)) F om ωi 1=ωi 2and θi 2=θi 1+π, we ob ain A2(I1) = a2A1(I1)/a1and i 2− i 1=a2+a1 a1A1(I1) sin(θ1−ω1τ∗(I, θ)). The e o e ε i 2− i 1<δ 8a4(|a1|+|a2|)< δ. So, −ε( i 2− i 1) + O(ε2) = 2πK is sa is ied only o a del a sa is ying δ > 2π+O(ε2). Bu his δis oo big and i is ou ou in e es . Fo e ical lines, he same esul can be s a ed mu a is mu andis. Fo a mo e gene al case, ha is, C1-cu e γ: [0, ∗]→R2such ha γ(0) = I−, γ( ∗) = I+, we ake a s ai s ep cu e γs ep, a combina ion o ho izon al and e ical lines, in a such way ha γs ep is a good enough app oxima ion o γ, whe e “good enough” we mean, he esul is hold o γapplying he abo e esul s ( o ho izon al and e ical lines) o γs ep. Using he shadowing lemmas o [FM00, FM03, GLS14] we ob ain he desi ed o bi . 4.4 Highways In analogy wi h De ini ion 22, in Chap e 2, we de ine a Highway as an in a ian se H={(I, Θ(I))}o he Hamil onian gi en by he educed Poinca ´e unc ion L∗(I, θ) which 83 is con ained in he le el ene gy L∗(I, θ) = A3. I is he e o e a Lag angian mani old, ha is, Θ(I) is g adien unc ion, i.e., he e exis s a unc ion F(I) such ha Θ(I) = ∇F(I). As Θ is a g adien unc ion, i has o sa is y he ollowing condi ion ∂Θ1 ∂I2 =∂Θ2 ∂I1 . This condi ion is equi alen o ∂2F ∂I2∂I1 =∂2F ∂I1∂I2 . P oposi ion 63. Conside he Hamil onian (4.1)+(4.2). Assume a1a2a36= 0 and |a1/a3|+ |a2/a3|<0.625. Fo I1and I2close o in ini y, he unc ion F akes he asymp o ic o m F(I) = 3π 2(I1+I2)−X i=1,2 2aisinh(π/2) π4Ωiπ3ω3 i+ 6π2ω2 i+ 24πωi+ 48e−πωi/2 +O(ω2 1ω2 2eπ(ω1+ω2)/2), (4.23) P oo . Assume a candida e o a unc ion F(I) gi en by (4.23), such ha Θ = ∇F(I). Θ(I) has o sa is y he ene gy le el o highways in he educed Poinca ´e unc ion A1(I1) cos(Θ1−ω1τ∗(I, Θ)) + A2(I2) cos(Θ2−ω2τ∗(I, Θ)) (4.24) +A3(cos(−τ∗(I, Θ)) −1) = 0, and τ∗(I, θ) has o sa is y he equa ion o he c es ω1A1(I1) sin(Θ1−ω1τ∗(I, Θ)) + ω2A2(I2) sin(Θ2−ω2τ∗(I, Θ)) +A3sin(−τ∗(I, θ)) = 0.(4.25) We wan o w i e hei e sion o I1and I2close o in ini y. Using (4.23) we no ice ha Θi= Θi(I) akes he o m Θi= 3π/2−aisinh(π/2)ω3 ie−πωi/2+O(ω2 1ω2 2eπ(ω1+ω2)/2). This implies cos(Θi−ωiτ∗) = −aisinh(π/2)ω3 ie−πωi/2−ωiτ∗ ∞+O(ω2 1ω2 2eπ(ω1+ω2)/2) and sin(Θi−ωiτ∗) = −1 + O(ω6 ie−πωi), Besides, cos(−τ∗(I, Θ)) = 1 −τ∗2 ∞ 2+O(τ∗4 ∞),sin(−τ∗) = −τ∗ ∞+O(τ∗ ∞), whe e τ∗ ∞is an asymp o ic app oxima ion o τ∗ ha we a e going o es ima e below. Fi s , we no ice ha he unc ions A1(I1) and A2(I2) can be app oxima ed by Ai(Ii) = 4πaiωie−πωi/21 + e−2πωi+. . . = 4πaiωie−πωi/2+Oωie−5πωi/2. 84 F om (4.13), he unc ion τ∗(I, Θ) sa is ies −τ∗(I, Θ) = −a csin A1(I1)ω1 A3 sin(Θ1−ω1τ∗(I, Θ)) + A2(I2)ω2 A3 sin(Θ2−ω2τ∗), and he e o e, τ∗ ∞≈X i=1,2 2aisinh(π/2)ω2 ie−πωi/2+Oωie−5πωi/2. Applying hese es ima es in Eq. (4.24) we ob ain ha he le hand o Eq. (4.24) sa is ies X i=1,24πaiωie−πω1/2−aisinh(π/2)ω3 ie−πωi/2−ωi2a1sinh(π/2)ω2 1e−πω1/2 +2a2sinh(π/2)ω2 2e−πω2/2−A3 2 X i=1,2 2aisinh(π/2)ω2 ie−πωi/2!2 +O(ω2 1ω2 2e−π(ω1+ω2)/2) = O(ω2 1ω2 2e−π(ω1+ω2)/2). In he same way, applying in Eq. (4.25) he es ima es ob ained, we ha e ha he le hand o Eq. (4.25) sa is ies −4πa1ω2 1e−πω1/2−4πa2ω2 2e−πω2/2+A3 X i=1,2 2aisinh(π/2)ω2 ie−πωi/2! +O(ω2 1ω2 2e−π(ω1+ω2)/2) = O(ω2 1ω2 2e−π(ω1+ω2)/2). The e o e, up o o de O(ω2 1ω2 2e−π(ω1+ω2)/2), he equa ion o he c es and he ene gy le el o he educed Poinca ´e unc ion a e sa is ied. We inish his chap e wi h an explici equa ion o he highway in a special case. P oposi ion 64. (Highways in a e y special case) Conside he Hamil onian (4.1)+(4.2) and a1=a2=asa is ying 2|a/a3|<0.625 and Ω1= Ω2= Ω. Le O=(I0, θ0),...,(IN, θN)be an o bi in a highway, N∈Nsuch ha I0 1=I0 2and θ0 1=θ0 2. Then, Ii 1=Ii 2=¯ Iiand θi 1=θi 2=¯ θi o any i∈ {0, . . . , N}and can be desc ibed by ¯ θh(¯ I) =    a ccos A3(1− −(¯ I)) A(¯ I)+ ¯ωa ccos( −(¯ I)),¯ I≤0; a ccos A3(1− −(¯ I)) A(¯ I)−¯ωa ccos( −(¯ I)), I > 0; o ¯ θH(I) =   −a ccos A3(1− −(¯ I)) A(¯ I)−¯ωa ccos( −(¯ I)),¯ I≤0; −a ccos A3(1− −(¯ I)) A(¯ I)+ ¯ωa ccos( −(¯ I)),¯ I > 0; , whe e −(¯ I) = ¯ωA3−pA2 3+ (¯ω−1)¯ I2A2(¯ I)/[A3(¯ω2−1)] and ¯ω=¯ IΩ1. 85 P oo . We ha e ha he ajec o ies o he sca e ing map a e gi en by he ε- ime low o he Hamil onian −L∗(I, θ) up o o de O(ε2). And such low is gi en by he ollowing di e en ial equa ions: ˙ Ii=−Ai(Ii) sin(θi−ωiτ∗(I, θ)) (4.26) ˙ θi=−Ωi dAi dωi (Ii) (cos(θi−ωiτ∗) + τ∗(I, θ)Ai(Ii) sin(θi−ωiτ∗(I, θ))) , o i= 1,2. Assuming Ω1= Ω2=: Ω and a1=a2=: aand aking ini ial condi ions sa is ying I(0) = I0and θ(0) = θ0whe e I0 1=I0 2and θ0 1=θ0 2, he solu ion (I( ), θ( )) o (4.26) sa is ies θ1( ) = θ2( ) and I1( ) = I2( ). Le O=(I0, θ0),(I1, θ1),...,(IN, θN)be an o bi o he sca e ing map in a ε- ime low o he Hamil onian −L∗(I, θ) up o o de O(ε2), N∈N. The e o e, Il 1=Il 2and θl 1=θl 2 o any l∈ {0, . . . , N}. We simply deno e I1=I2and θ1=θ2. I he o bi Ois a highway, i has o sa is y wo equa ions: he equa ion o he c es s gi en in (4.12) and L∗(I, θ) = A3. Bu now, as I1=I2=: ¯ I,θ1=θ2=: ¯ θ, Ω1= Ω2and a1=a2, hese equa ions can be ew i en as A(¯ I) cos(¯ θ−¯ωτ∗(¯ I, ¯ θ)) + A3cos(−τ∗(¯ I, ¯ θ)) = A3 ¯ωA(¯ω) sin(¯ θ−¯ωτ∗(¯ I, ¯ θ)) + A3sin(−τ∗(¯ I, ¯ θ)) = 0, whe e ¯ω:= ω1=ω2and A(¯ I)=4π¯ωa/ sinh(π¯ω/2). F om a simila app oach used in P oposi ion 23, we ob ain he c es s a e desc ibed by ¯ θh(¯ I) =    a ccos A3(1− −(¯ I)) A(¯ I)+ ¯ωa ccos( −(¯ I)),¯ I≤0; a ccos A3(1− −(¯ I)) A(¯ I)−¯ωa ccos( −(¯ I)), I > 0; and ¯ θH(I) =   −a ccos A3(1− −(¯ I)) A(¯ I)−¯ωa ccos( −(¯ I)),¯ I≤0; −a ccos A3(1− −(¯ I)) A(¯ I)+ ¯ωa ccos( −(¯ I)),¯ I > 0; , whe e −(¯ I) = ¯ωA3−pA2 3+ (¯ω−1)¯ I2A2(¯ I)/[A3(¯ω2−1)]. 86 Chap e 5 Some open ques ions 5.1 Highways in piecewise smoo h global sca e ing maps As we showed in Sec ion 3.4, in he piecewise smoo h global sca e ing maps he e exis wo lines o discon inui y in he ec o ield o he sca e ing map. I seems ha we can de ine wo special o bi s using he heo y de eloped by [Fil88], such ha hese o bi s lie on he lines o discon inui y and beha e like he highways de ined in Chap e 1. In a u u e wo k we plan o pe o m nume ical expe imen s o e i y whe he i is possible o ind eal o bi s o he Hamil onian beha ing like hese special o bi s in his egion o he phase space. A e ha we wish o exploi hese o bi s o ob ain as and simple di usion. 5.2 Abou he case wi h 3 + 1/2 deg ees o eedom Fo he case s udied in his hesis, i.e., he Hamil onian sys em gi en by (4.1)+(4.2), in P oposi ion 63 we ob ain an asymp o ic app oxima ion o he highways. A nex s ep is o check ha his app oxima ion is good enough in o de o con inue globally hose highways o ob ain a global desc ip ion. Besides, he e we ha e p esen ed esul s o a es ic ed se o alues o a1and a2, mo e p ecisely, o a1and a2sa is ying |a1|+|a2| ≤ 0.625. And we ha e ob ained simila esul s o he pa o he esul s in Chap e 2. The nex s ep is o elimina e his es ic ion o e he alues o a1and a2and o s udy he bi u ca ion o c es s, he bi u ca ion o he sca e ing maps and he exis ence o he highways. Finally, we expec o s udy he case o a complemen a y pe u ba ion wi h espec o (4.2) o co e he comple e amily case, in an analogous way ha we ha e done in Chap e 3. 87 5.3 Abou Shadowing lemmas Taking in o accoun ou nume ical expe imen s, he geome ical mechanisms used in ou p oo and ou es ima es o he ime, we wish o unde s and he eal ole played by he inne map in his mechanism. Ou main ques ion is: Is i eally necessa y o use he inne dynamics in he building o a pseudo-o bi o gua an ee he exis ence o eal o bi o he sys em? In ou heo ems we we e able o use he esul s o [FM00, FM03, GLS14]. In [GLS14] hey p o ed a shadowing lemma o pseudo-o bi s buil by using a numbe o i e a es o sca e ing map. Bu he esul appea s no o be e y p ac ical o as di usion. In he ongoing wo k we plan o use nume ical expe imen s o e i y he exis ence o eal o bi s close o pseudo-o bi s o a sca e ing map (o a combina ion o mul iple sca e ing maps). Besides, in he u u e we wish o ca y ou an analy ic app oach as well. 5.4 Rela ion be ween he o mulas o he sca e ing and sepa a ix maps The sepa a ix map was in oduced by Zasla skii and Filonenko in [ZF68], and has been s udied and de eloped in [T e98, T e02, Pi 06, PT07, GKZ16, DT16]. Unde ce ain condi ions we belie e ha he o mulas ob ained in [T e02] can be imp o ed as I∗=I+ε∂ϕL∗(I∗, ϕ, s)−∂ϕω0 λlog κ ω0 λ+O2 ϕ∗=ϕ+ν−ε∂IL∗(I∗, ϕ, s) + ∂Iω0 λlog κω0 λ+O1 h∗=H0+ε∂sL∗(I∗, ϕ, s)−∂sω0 λlog κω0 λ+O2 s∗=s+¯ ∂hω0 λlog κω0 λ+O1, whe e λ, κ and µa e unc ions o I∗,¯ is an in ege . s+¯ +∂hω0 λlog κω0 λ< c−1 and O1=O(ε1 4)(ε7 8) log2ε,O2=O(ε1 4)(ε5 4) log2εand L∗is a educed Poinca ´e unc ion. Since he Sca e ing map akes he explici o m Sε(I, θ) = I+ε∂ ∂θL∗(I, θ) + O(ε2), θ −ε∂ ∂I L∗(I, θ) + O(ε2). We expec o e i y analy ically and nume ically hese equa ions. 88