classical and quantum chaos

Classical and QuantumChaos

Part I: DeterministicChaos

Predrag Cvitanovic Roberto Artuso Per Dahlqvist RonnieMainieri Gregor Tanner Gabor Vattay Niall Whelan An-dreas Wirzba

-version 10, Aug 26 2003 printed September 1, 2003www.nbi.dk/ChaosBook comments to: [email protected]

Contents

Volume I: Classical chaos

Contributors . . . . . . . . . . . . . . . . . . . . . . . . . . . . . xiAcknowledgements . . . . . . . . . . . . . . . . . . . . . . . . . . xiv

1 Overture 11.1 Why this book? . . . . . . . . . . . . . . . . . . . . . . . . . 21.2 Chaos ahead . . . . . . . . . . . . . . . . . . . . . . . . . . 31.3 The future as in a mirror . . . . . . . . . . . . . . . . . . . 41.4 A game of pinball . . . . . . . . . . . . . . . . . . . . . . . . 91.5 Chaos for cyclists . . . . . . . . . . . . . . . . . . . . . . . . 131.6 Evolution . . . . . . . . . . . . . . . . . . . . . . . . . . . . 191.7 From chaos to statistical mechanics . . . . . . . . . . . . . . 211.8 Guide to literature . . . . . . . . . . . . . . . . . . . . . . . 23guide to exercises 24 - resume 25 - references 27 - exercises 29

2 Flows 312.1 Dynamical systems . . . . . . . . . . . . . . . . . . . . . . . 312.2 Flows . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 352.3 Computing trajectories . . . . . . . . . . . . . . . . . . . . . 382.4 Innite-dimensional ows . . . . . . . . . . . . . . . . . . . 38resume 43 - references 43 - exercises 45

3 Maps 493.1 Poincare sections . . . . . . . . . . . . . . . . . . . . . . . . 493.2 Constructing a Poincare section . . . . . . . . . . . . . . . . 523.3 Do it again . . . . . . . . . . . . . . . . . . . . . . . . . . . 53resume 56 - references 56 - exercises 58

4 Local stability 614.1 Flows transport neighborhoods . . . . . . . . . . . . . . . . 614.2 Linear ows . . . . . . . . . . . . . . . . . . . . . . . . . . . 634.3 Stability of ows . . . . . . . . . . . . . . . . . . . . . . . . 674.4 Stability of maps . . . . . . . . . . . . . . . . . . . . . . . . 704.5 Stability of periodic orbits . . . . . . . . . . . . . . . . . . . 714.6 Neighborhood of a cycle . . . . . . . . . . . . . . . . . . . . 74resume 76 - references 76 - exercises 77

iii

iv CONTENTS

5 Newtonian dynamics 795.1 Hamiltonian ows . . . . . . . . . . . . . . . . . . . . . . . 795.2 Billiards . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 815.3 Stability of billiards . . . . . . . . . . . . . . . . . . . . . . 84resume 87 - exercises 88

6 Get straight 916.1 Changing coordinates . . . . . . . . . . . . . . . . . . . . . 916.2 Rectication of ows . . . . . . . . . . . . . . . . . . . . . . 926.3 Rectication of maps . . . . . . . . . . . . . . . . . . . . . . 946.4 Smooth conjugacies and cycle stability . . . . . . . . . . . . 96resume 97 - references 98 - exercises 99

7 Transporting densities 1017.1 Measures . . . . . . . . . . . . . . . . . . . . . . . . . . . . 1017.2 Perron-Frobenius operator . . . . . . . . . . . . . . . . . . . 1037.3 Invariant measures . . . . . . . . . . . . . . . . . . . . . . . 1057.4 Density evolution for innitesimal times . . . . . . . . . . . 109resume 113 - references 113 - exercises 114

8 Averaging 1198.1 Dynamical averaging . . . . . . . . . . . . . . . . . . . . . . 1198.2 Evolution operators . . . . . . . . . . . . . . . . . . . . . . 1258.3 Lyapunov exponents . . . . . . . . . . . . . . . . . . . . . . 1278.4 Why not just run it on a computer? . . . . . . . . . . . . . 131resume 133 - references 134 - exercises 135

9 Qualitative dynamics, for pedestrians 1379.1 Itineraries . . . . . . . . . . . . . . . . . . . . . . . . . . . . 1379.2 Stretch and fold . . . . . . . . . . . . . . . . . . . . . . . . . 1439.3 Going global: Stable/unstable manifolds . . . . . . . . . . . 1449.4 Temporal ordering: itineraries . . . . . . . . . . . . . . . . . 1469.5 Spatial ordering . . . . . . . . . . . . . . . . . . . . . . . . . 1489.6 Topological dynamics . . . . . . . . . . . . . . . . . . . . . 1509.7 Symbolic dynamics, basic notions . . . . . . . . . . . . . . . 153resume 156 - references 156 - exercises 159

10 Counting, for pedestrians 16110.1 Counting itineraries . . . . . . . . . . . . . . . . . . . . . . 16110.2 Topological trace formula . . . . . . . . . . . . . . . . . . . 16410.3 Determinant of a graph . . . . . . . . . . . . . . . . . . . . 16510.4 Topological zeta function . . . . . . . . . . . . . . . . . . . 17010.5 Counting cycles . . . . . . . . . . . . . . . . . . . . . . . . . 17110.6 Innite partitions . . . . . . . . . . . . . . . . . . . . . . . . 17610.7 Shadowing . . . . . . . . . . . . . . . . . . . . . . . . . . . . 177resume 180 - references 180 - exercises 182

11 Trace formulas 18911.1 Trace of an evolution operator . . . . . . . . . . . . . . . . 18911.2 A trace formula for maps . . . . . . . . . . . . . . . . . . . 19111.3 A trace formula for ows . . . . . . . . . . . . . . . . . . . . 193

CONTENTS v

11.4 An asymptotic trace formula . . . . . . . . . . . . . . . . . 196resume 198 - references 198 - exercises 199

12 Spectral determinants 20112.1 Spectral determinants for maps . . . . . . . . . . . . . . . . 20212.2 Spectral determinant for ows . . . . . . . . . . . . . . . . . 20312.3 Dynamical zeta functions . . . . . . . . . . . . . . . . . . . 20512.4 False zeros . . . . . . . . . . . . . . . . . . . . . . . . . . . . 20812.5 More examples of spectral determinants . . . . . . . . . . . 20912.6 All too many eigenvalues? . . . . . . . . . . . . . . . . . . . 211resume 214 - references 214 - exercises 216

13 Why does it work? 22113.1 The simplest of spectral determinants: A single xed point 22213.2 Analyticity of spectral determinants . . . . . . . . . . . . . 22513.3 Hyperbolic maps . . . . . . . . . . . . . . . . . . . . . . . . 23213.4 Physics of eigenvalues and eigenfunctions . . . . . . . . . . 236resume 241 - references 241 - exercises 243

14 Fixed points, and how to get them 24514.1 Where are the cycles? . . . . . . . . . . . . . . . . . . . . . 24614.2 One-dimensional mappings . . . . . . . . . . . . . . . . . . 24814.3 Multipoint shooting method . . . . . . . . . . . . . . . . . . 24914.4 d-dimensional mappings . . . . . . . . . . . . . . . . . . . . 25114.5 Flows . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 25214.6 Stability of cycles for maps . . . . . . . . . . . . . . . . . . 256resume 257 - references 257 - exercises 259

15 Cycle expansions 26315.1 Pseudocycles and shadowing . . . . . . . . . . . . . . . . . . 26315.2 Cycle formulas for dynamical averages . . . . . . . . . . . . 26915.3 Cycle expansions for nite alphabets . . . . . . . . . . . . . 27315.4 Stability ordering of cycle expansions . . . . . . . . . . . . . 27415.5 Dirichlet series . . . . . . . . . . . . . . . . . . . . . . . . . 277resume 280 - references 281 - exercises 282

16 Why cycle? 28516.1 Escape rates . . . . . . . . . . . . . . . . . . . . . . . . . . . 28516.2 Flow conservation sum rules . . . . . . . . . . . . . . . . . . 28916.3 Correlation functions . . . . . . . . . . . . . . . . . . . . . . 29016.4 Trace formulas vs. level sums . . . . . . . . . . . . . . . . . 291resume 294 - references 295 - exercises 296

17 Thermodynamic formalism 29917.1 Renyi entropies . . . . . . . . . . . . . . . . . . . . . . . . . 29917.2 Fractal dimensions . . . . . . . . . . . . . . . . . . . . . . . 304resume 307 - references 308 - exercises 309

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18 Intermittency 31118.1 Intermittency everywhere . . . . . . . . . . . . . . . . . . . 31218.2 Intermittency for pedestrians . . . . . . . . . . . . . . . . . 31518.3 Intermittency for cyclists . . . . . . . . . . . . . . . . . . . 32718.4 BER zeta functions . . . . . . . . . . . . . . . . . . . . . . . 332resume 336 - references 336 - exercises 338

19 Discrete symmetries 34119.1 Preview . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 34219.2 Discrete symmetries . . . . . . . . . . . . . . . . . . . . . . 34619.3 Dynamics in the fundamental domain . . . . . . . . . . . . 34819.4 Factorizations of dynamical zeta functions . . . . . . . . . . 35219.5 C2 factorization . . . . . . . . . . . . . . . . . . . . . . . . . 35419.6 C3v factorization: 3-disk game of pinball . . . . . . . . . . . 356resume 359 - references 360 - exercises 362

20 Deterministic diusion 36520.1 Diusion in periodic arrays . . . . . . . . . . . . . . . . . . 36620.2 Diusion induced by chains of 1-d maps . . . . . . . . . . . 37020.3 Marginal stability and anomalous diusion . . . . . . . . . . 377resume 382 - references 383 - exercises 385

21 Irrationally winding 38721.1 Mode locking . . . . . . . . . . . . . . . . . . . . . . . . . . 38821.2 Local theory: Golden mean renormalization . . . . . . . . 39421.3 Global theory: Thermodynamic averaging . . . . . . . . . . 39621.4 Hausdor dimension of irrational windings . . . . . . . . . . 39821.5 Thermodynamics of Farey tree: Farey model . . . . . . . . 400resume 405 - references 405 - exercises 407

CONTENTS vii

Volume II: Quantum chaos

22 Prologue 40922.1 Quantum pinball . . . . . . . . . . . . . . . . . . . . . . . . 41022.2 Quantization of helium . . . . . . . . . . . . . . . . . . . . . 412guide to literature 413 - references 413 -

23 Quantum mechanics, briey 415

24 WKB quantization 41924.1 Method of stationary phase . . . . . . . . . . . . . . . . . . 42124.2 WKB quantization . . . . . . . . . . . . . . . . . . . . . . . 422exercises 425

25 Relaxation for cyclists 42725.1 Fictitious time relaxation . . . . . . . . . . . . . . . . . . . 42825.2 Discrete iteration relaxation method . . . . . . . . . . . . . 43325.3 Least action method . . . . . . . . . . . . . . . . . . . . . . 436resume 440 - references 440 - exercises 442

26 Semiclassical evolution 44326.1 Hamilton-Jacobi theory . . . . . . . . . . . . . . . . . . . . 44326.2 Semiclassical propagator . . . . . . . . . . . . . . . . . . . . 45126.3 Semiclassical Greens function . . . . . . . . . . . . . . . . . 455resume 462 - references 463 - exercises 464

27 Semiclassical quantization 46727.1 Trace formula . . . . . . . . . . . . . . . . . . . . . . . . . . 46727.2 Semiclassical spectral determinant . . . . . . . . . . . . . . 47327.3 One-dimensional systems . . . . . . . . . . . . . . . . . . . 47427.4 Two-dimensional systems . . . . . . . . . . . . . . . . . . . 476resume 476 - references 478 - exercises 481

28 Quantum scattering 48328.1 Density of states . . . . . . . . . . . . . . . . . . . . . . . . 48328.2 Quantum mechanical scattering matrix . . . . . . . . . . . . 48728.3 Krein-Friedel-Lloyd formula . . . . . . . . . . . . . . . . . . 48828.4 Wigner time delay . . . . . . . . . . . . . . . . . . . . . . . 491references 493 - exercises 495

29 Helium atom 49729.1 Classical dynamics of collinear helium . . . . . . . . . . . . 49829.2 Semiclassical quantization of collinear helium . . . . . . . . 510resume 519 - references 520 - exercises 521

30 Diraction distraction 52330.1 Quantum eavesdropping . . . . . . . . . . . . . . . . . . . . 52330.2 An application . . . . . . . . . . . . . . . . . . . . . . . . . 529resume 536 - references 536 - exercises 538

viii CONTENTS

Epilogue 539

Index 544

CONTENTS ix

Volume www: Appendices on www.nbi.dk/ChaosBook

A A brief history of chaos 557A.1 Chaos is born . . . . . . . . . . . . . . . . . . . . . . . . . . 557A.2 Chaos grows up . . . . . . . . . . . . . . . . . . . . . . . . . 561A.3 Chaos with us . . . . . . . . . . . . . . . . . . . . . . . . . . 562A.4 Death of the Old Quantum Theory . . . . . . . . . . . . . . 566references 568 -

B Innite-dimensional ows 569

C Stability of Hamiltonian ows 573C.1 Symplectic invariance . . . . . . . . . . . . . . . . . . . . . 573C.2 Monodromy matrix for Hamiltonian ows . . . . . . . . . . 574

D Implementing evolution 579D.1 Material invariants . . . . . . . . . . . . . . . . . . . . . . . 579D.2 Koopmania . . . . . . . . . . . . . . . . . . . . . . . . . . . 580D.3 Implementing evolution . . . . . . . . . . . . . . . . . . . . 582references 586 - exercises 587

E Symbolic dynamics techniques 589E.1 Topological zeta functions for innite subshifts . . . . . . . 589E.2 Prime factorization for dynamical itineraries . . . . . . . . . 597

F Counting itineraries 603F.1 Counting curvatures . . . . . . . . . . . . . . . . . . . . . . 603exercises 605

G Finding cycles 607G.1 Newton-Raphson method . . . . . . . . . . . . . . . . . . . 607G.2 Hybrid Newton-Raphson / relaxation method . . . . . . . . 608

H Applications 611H.1 Evolution operator for Lyapunov exponents . . . . . . . . . 611H.2 Advection of vector elds by chaotic ows . . . . . . . . . . 615references 619 - exercises 621

I Discrete symmetries 623I.1 Preliminaries and denitions . . . . . . . . . . . . . . . . . . 623I.2 C4v factorization . . . . . . . . . . . . . . . . . . . . . . . . 628I.3 C2v factorization . . . . . . . . . . . . . . . . . . . . . . . . 632I.4 Henon map symmetries . . . . . . . . . . . . . . . . . . . . 635I.5 Symmetries of the symbol square . . . . . . . . . . . . . . . 635

J Convergence of spectral determinants 637J.1 Curvature expansions: geometric picture . . . . . . . . . . . 637J.2 On importance of pruning . . . . . . . . . . . . . . . . . . . 640J.3 Ma-the-matical caveats . . . . . . . . . . . . . . . . . . . . . 641J.4 Estimate of the nth cumulant . . . . . . . . . . . . . . . . . 642

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K Innite dimensional operators 645K.1 Matrix-valued functions . . . . . . . . . . . . . . . . . . . . 645K.2 Operator norms . . . . . . . . . . . . . . . . . . . . . . . . . 647K.3 Trace class and Hilbert-Schmidt class . . . . . . . . . . . . . 648K.4 Determinants of trace class operators . . . . . . . . . . . . . 650K.5 Von Koch matrices . . . . . . . . . . . . . . . . . . . . . . . 653K.6 Regularization . . . . . . . . . . . . . . . . . . . . . . . . . 655references 657 -

L Statistical mechanics recycled 659L.1 The thermodynamic limit . . . . . . . . . . . . . . . . . . . 659L.2 Ising models . . . . . . . . . . . . . . . . . . . . . . . . . . . 661L.3 Fisher droplet model . . . . . . . . . . . . . . . . . . . . . . 665L.4 Scaling functions . . . . . . . . . . . . . . . . . . . . . . . . 670L.5 Geometrization . . . . . . . . . . . . . . . . . . . . . . . . . 673resume 681 - references 681 - exercises 684

M Noise/quantum corrections 687M.1 Periodic orbits as integrable systems . . . . . . . . . . . . . 687M.2 The Birkho normal form . . . . . . . . . . . . . . . . . . . 691M.3 Bohr-Sommerfeld quantization of periodic orbits . . . . . . 692M.4 Quantum calculation of corrections . . . . . . . . . . . . . 694references 700 -

N What reviewers say 703N.1 Niels Bohr . . . . . . . . . . . . . . . . . . . . . . . . . . . . 703N.2 Richard P. Feynman . . . . . . . . . . . . . . . . . . . . . . 703N.3 Divakar Viswanath . . . . . . . . . . . . . . . . . . . . . . . 703N.4 Benny Lautrup . . . . . . . . . . . . . . . . . . . . . . . . . 703N.5 Professor Gatto Nero . . . . . . . . . . . . . . . . . . . . . . 704

O Solutions 705

P Projects 729P.1 Deterministic diusion, zig-zag map . . . . . . . . . . . . . 731P.2 Deterministic diusion, sawtooth map . . . . . . . . . . . . 738

CONTENTS xi

Contributors

No man but a blockhead ever wrote except for moneySamuel Johnson

This book is a result of collaborative labors of many people over a spanof several decades. Coauthors of a chapter or a section are indicated inthe byline to the chapter/section title. If you are referring to a speciccoauthored section rather than the entire book, cite it as (for example):

C. Chandre, F.K. Diakonos and P. Schmelcher, section Discrete cy-clist relaxation method, in P. Cvitanovic, R. Artuso, R. Mainieri,G. Tanner and G. Vattay, Chaos: Classical and Quantum (Niels BohrInstitute, Copenhagen 2003); www.nbi.dk/ChaosBook.

Chapters without a byline are written by Predrag Cvitanovic. Friendswhose contributions and ideas were invaluable to us but have not con-tributed written text to this book, are listed in the acknowledgements.

Roberto Artuso

7 Transporting densities . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 10111.3 A trace formula for ows . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 19316.3 Correlation functions . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .29018 Intermittency . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 31120 Deterministic diusion . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 36521 Irrationally winding . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .387

Ronnie Mainieri

2 Flows . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 313.2 The Poincare section of a ow . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 524 Local stability . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 616.1 Understanding ows . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .939.1 Temporal ordering: itineraries . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 137Appendix A: A brief history of chaos . . . . . . . . . . . . . . . . . . . . . . . . . 557Appendix L: Statistical mechanics recycled . . . . . . . . . . . . . . . . . . . 659

Gabor Vattay

17 Thermodynamic formalism . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .29926 Semiclassical evolution . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 44327 Semiclassical trace formula . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .467Appendix M: Noise/quantum corrections . . . . . . . . . . . . . . . . . . . . . 687

Gregor Tanner

18 Intermittency . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 31126 Semiclassical evolution . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 44327 Semiclassical trace formula . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .46729 The helium atom . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 497Appendix C.2: Jacobians of Hamiltonian ows . . . . . . . . . . . . . . . . 574Appendix J.3 Ma-the-matical caveats . . . . . . . . . . . . . . . . . . . . . . . . . 641

xii CONTENTS

Ofer Biham

25.1 Cyclists relaxation method . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 428

Cristel Chandre

25.1 Cyclists relaxation method . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 42825.2 Discrete cyclists relaxation methods . . . . . . . . . . . . . . . . . . . . . . 433G.2 Contraction rates . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .608

Freddy Christiansen

14 Fixed points, and what to do about them . . . . . . . . . . . . . . . . . . 245

Per Dahlqvist

25.3 Orbit length extremization method for billiards . . . . . . . . . . 43618 Intermittency . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 311Appendix E.1.1: Periodic points of unimodal maps . . . . . . . . . . . . 595

Carl P. Dettmann

15.4 Stability ordering of cycle expansions . . . . . . . . . . . . . . . . . . . . .274

Fotis K. Diakonos

25.2 Discrete cyclists relaxation methods . . . . . . . . . . . . . . . . . . . . . . 433

Mitchell J. Feigenbaum

Appendix C.1: Symplectic invariance . . . . . . . . . . . . . . . . . . . . . . . . . 573

Kai T. Hansen

9.4 Unimodal map symbolic dynamics . . . . . . . . . . . . . . . . . . . . . . . . 14610.6 Topological zeta function for an innite partition . . . . . . . . . 176

Rainer Klages

Fig. 20.5

Yueheng Lan

Figs. 9.3 and 19.1

Joachim Mathiesen

8.3 Lyapunov exponents . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 127Rossler system gures, cycles in chapters 2, 3, 4 and 14

Adam Prugel-Bennet

Solutions 1.2, 2.9, 5.1, 12.1, 13.3, 25.1, 15.2

Lamberto Rondoni

7 Transporting densities . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 10116.1.2 Unstable periodic orbits are dense . . . . . . . . . . . . . . . . . . . . . . 288

Juri Rolf

Solution 13.3

Per E. Rosenqvist

exercises, gures throughout the text

Hans Henrik Rugh

CONTENTS xiii

13 Why does it work? . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 221

Peter Schmelcher

25.2 Discrete cyclists relaxation methods . . . . . . . . . . . . . . . . . . . . . . 433

Gabor Simon

Rossler system gures, cycles in chapters 2, 3, 4 and 14

Edward A. Spiegel

2 Flows . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 317 Transporting densities . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 101

Niall Whelan

30 Diraction distraction . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 52328 Semiclassical chaotic scattering . . . . . . . . . . . . . . . . . . . . . . . . . . . . 483

Andreas Wirzba

28 Semiclassical chaotic scattering . . . . . . . . . . . . . . . . . . . . . . . . . . . . 483Appendix K: Innite dimensional operators . . . . . . . . . . . . . . . . . . . 645

xiv CONTENTS

Acknowledgements

I feel I never want to write another book. Whats thegood! I can eke living on stories and little articles,that dont cost a tithe of the output a book costs.Why write novels any more!D.H. Lawrence

This book owes its existence to the Niels Bohr Institutes and Norditashospitable and nurturing environment, and the private, national and cross-national foundations that have supported the collaborators research over aspan of several decades. P.C. thanks M.J. Feigenbaum of Rockefeller Uni-versity; D. Ruelle of I.H.E.S., Bures-sur-Yvette; I. Procaccia of the Weiz-mann Institute; P. Hemmer of University of Trondheim; The Max-PlanckInstitut fur Mathematik, Bonn; J. Lowenstein of New York University; Ed-icio Celi, Milano; and Fundacao de Faca, Porto Seguro, for the hospitalityduring various stages of this work, and the Carlsberg Foundation and GlenP. Robinson for the support.

The authors gratefully acknowledge collaborations and/or stimulatingdiscussions with E. Aurell, V. Baladi, B. Brenner, A. de Carvalho, D.J. Driebe,B. Eckhardt, M.J. Feigenbaum, J. Frjland, P. Gaspar, P. Gaspard, J. Guck-enheimer, G.H. Gunaratne, P. Grassberger, H. Gutowitz, M. Gutzwiller,K.T. Hansen, P.J. Holmes, T. Janssen, R. Klages, Y. Lan, B. Lauritzen,J. Milnor, M. Nordahl, I. Procaccia, J.M. Robbins, P.E. Rosenqvist, D. Ru-elle, G. Russberg, M. Sieber, D. Sullivan, N. Sndergaard, T. Tel, C. Tresser,and D. Wintgen.

We thank Dorte Glass for typing parts of the manuscript; B. Lautrupand D. Viswanath for comments and corrections to the preliminary versionsof this text; M.V. Berry for the quotation on page 557; H. Fogedby for thequotation on page 225; J. Greensite for the quotation on page 5; Ya.B. Pesinfor the remarks quoted on page 565; E.A. Spiegel for quotations on page 1and page 641.

Fritz Haakes heartfelt lament on page 193 was uttered at the end of therst conference presentation of cycle expansions, in 1988. G.P. Morriss ad-vice to students as how to read the introduction to this book, page 4, was of-ferred during a 2002 graduate course in Dresden. Kerson Huangs interviewof C.N. Yang quoted on page 106 is available on www.nbi.dk/ChaosBook/extras.

Who is the 3-legged dog reappearing throughout the book? Long ago,when we were innocent and knew not Borel measurable to sets, P. Cvi-tanovic asked V. Baladi a question about dynamical zeta functions, whothen asked J.-P. Eckmann, who then asked D. Ruelle. The answer wastransmitted back: The master says: It is holomorphic in a strip .Hences His Masters Voice logo, and the 3-legged dog is us, still eagerto fetch the bone. The answer has made it to the book, though not pre-cisely in His Masters words. As a matter of fact, the answer is the book.We are still chewing on it.

Profound thanks to all the unsung heroes - students and colleagues, toonumerous to list here, who have supported this project over many yearsin many ways, by surviving pilot courses based on this book, by providinginvaluable insights, by teaching us, by inspiring us.

Chapter 1

Overture

If I have seen less far than other men it is because Ihave stood behind giants.Edoardo Specchio

Rereading classic theoretical physics textbooks leaves a sense that thereare holes large enough to steam a Eurostar train through them. Herewe learn about harmonic oscillators and Keplerian ellipses - but where isthe chapter on chaotic oscillators, the tumbling Hyperion? We have justquantized hydrogen, where is the chapter on the classical 3-body problemand its implications for quantization of helium? We have learned that aninstanton is a solution of eld-theoretic equations of motion, but shouldnta strongly nonlinear eld theory have turbulent solutions? How are we tothink about systems where things fall apart; the center cannot hold; everytrajectory is unstable?

This chapter oers a quick survey of the main topics covered in thebook. We start out by making promises - we will right wrongs, no longershall you suer the slings and arrows of outrageous Science of Perplexity.We relegate a historical overview of the development of chaotic dynamicsto appendix A, and head straight to the starting line: A pinball game isused to motivate and illustrate most of the concepts to be developed in thisbook.

Throughout the book

indicates that the section requires a hearty stomach and is probablybest skipped on rst reading

fast track points you where to skip to

tells you where to go for more depth on a particular topic

indicates an exercise that might clarify a point in the text1

2 CHAPTER 1. OVERTURE

indicates that a gure is still missing - you are urged to fetch it

This is a textbook, not a research monograph, and you should be able tofollow the thread of the argument without constant excursions to sources.Hence there are no literature references in the text proper, all learned re-marks and bibliographical pointers are relegated to the Commentary sec-tion at the end of each chapter.

1.1 Why this book?

It seems sometimes that through a preoccupationwith science, we acquire a rmer hold over the vi-cissitudes of life and meet them with greater calm,but in reality we have done no more than to nd away to escape from our sorrows.Hermann Minkowski in a letter to David Hilbert

The problem has been with us since Newtons rst frustrating (and unsuc-cessful) crack at the 3-body problem, lunar dynamics. Nature is rich insystems governed by simple deterministic laws whose asymptotic dynam-ics are complex beyond belief, systems which are locally unstable (almost)everywhere but globally recurrent. How do we describe their long termdynamics?

The answer turns out to be that we have to evaluate a determinant,take a logarithm. It would hardly merit a learned treatise, were it not forthe fact that this determinant that we are to compute is fashioned out ofinnitely many innitely small pieces. The feel is of statistical mechanics,and that is how the problem was solved; in 1960s the pieces were counted,and in 1970s they were weighted and assembled together in a fashion that inbeauty and in depth ranks along with thermodynamics, partition functionsand path integrals amongst the crown jewels of theoretical physics.

Then something happened that might be without parallel; this is an areaof science where the advent of cheap computation had actually subtractedfrom our collective understanding. The computer pictures and numericalplots of fractal science of 1980s have overshadowed the deep insights ofthe 1970s, and these pictures have since migrated into textbooks. Frac-tal science posits that certain quantities (Lyapunov exponents, generalizeddimensions, . . . ) can be estimated on a computer. While some of the num-bers so obtained are indeed mathematically sensible characterizations offractals, they are in no sense observable and measurable on the length andtime scales dominated by chaotic dynamics.

Even though the experimental evidence for the fractal geometry of na-ture is circumstantial, in studies of probabilistically assembled fractal ag-gregates we know of nothing better than contemplating such quantities.

intro - 13aug2003 version 10, Aug 26 2003

1.2. CHAOS AHEAD 3

In deterministic systems we can do much better. Chaotic dynamics is gen-erated by interplay of locally unstable motions, and interweaving of theirglobal stable and unstable manifolds. These features are robust and ac-cessible in systems as noisy as slices of rat brains. Poincare, the rst tounderstand deterministic chaos, already said as much (modulo rat brains).Once the topology of chaotic dynamics is understood, a powerful theoryyields the macroscopically measurable consequences of chaotic dynamics,such as atomic spectra, transport coecients, gas pressures.

That is what we will focus on in this book. This book is a self-containedgraduate textbook on classical and quantum chaos. We teach you how toevaluate a determinant, take a logarithm, stu like that. Should take 100pages or so. Well, we fail - so far we have not found a way to traversethis material in less than a semester, or 200-300 page subset of this text.Nothing to be done about that.

1.2 Chaos ahead

Things fall apart; the centre cannot holdW.B. Yeats: The Second Coming

Study of chaotic dynamical systems is no recent fashion. It did not startwith the widespread use of the personal computer. Chaotic systems havebeen studied for over 200 years. During this time many have contributed,and the eld followed no single line of development; rather one sees manyinterwoven strands of progress.

In retrospect many triumphs of both classical and quantum physics seema stroke of luck: a few integrable problems, such as the harmonic oscillatorand the Kepler problem, though non-generic, have gotten us very far.The success has lulled us into a habit of expecting simple solutions to sim-ple equations - an expectation tempered for many by the recently acquiredability to numerically scan the phase space of non-integrable dynamicalsystems. The initial impression might be that all our analytic tools havefailed us, and that the chaotic systems are amenable only to numerical andstatistical investigations. Nevertheless, a beautiful theory of deterministicchaos, of predictive quality comparable to that of the traditional perturba-tion expansions for nearly integrable systems, already exists.

In the traditional approach the integrable motions are used as zeroth-order approximations to physical systems, and weak nonlinearities are thenaccounted for perturbatively. For strongly nonlinear, non-integrable sys-tems such expansions fail completely; the asymptotic time phase space ex-hibits amazingly rich structure which is not at all apparent in the integrableapproximations. However, hidden in this apparent chaos is a rigid skele-ton, a tree of cycles (periodic orbits) of increasing lengths and self-similarstructure. The insight of the modern dynamical systems theory is thatthe zeroth-order approximations to the harshly chaotic dynamics should bevery dierent from those for the nearly integrable systems: a good starting

version 10, Aug 26 2003 intro - 13aug2003


Figure 1.1: A physicists bare bones game ofpinball.

approximation here is the linear stretching and folding of a bakers map,rather than the periodic motion of a harmonic oscillator.

So, what is chaos, and what is to be done about it? To get some feelingfor how and why unstable cycles come about, we start by playing a game ofpinball. The reminder of the chapter is a quick tour through the materialcovered in this book. Do not worry if you do not understand every detail atthe rst reading the intention is to give you a feeling for the main themesof the book, details will be lled out later. If you want to get a particularpoint claried right now, on the margin points at the appropriatesection.

1.3 The future as in a mirror

All you need to know about chaos is contained in theintroduction of the [Cvitanovic et al Chaos: Classi-cal and Quantum] book. However, in order to un-derstand the introduction you will rst have to readthe rest of the book.Gary Morriss

That deterministic dynamics leads to chaos is no surprise to anyone whohas tried pool, billiards or snooker the game is about beating chaos so we start our story about what chaos is, and what to do about it, witha game of pinball. This might seem a trie, but the game of pinball isto chaotic dynamics what a pendulum is to integrable systems: thinkingclearly about what chaos in a game of pinball is will help us tackle moredicult problems, such as computing diusion constants in deterministicgases, or computing the helium spectrum.

We all have an intuitive feeling for what a ball does as it bounces amongthe pinball machines disks, and only high-school level Euclidean geometryis needed to describe its trajectory. A physicists pinball game is the game ofpinball stripped to its bare essentials: three equidistantly placed reectingdisks in a plane, g. 1.1. A physicists pinball is free, frictionless, point-like, spin-less, perfectly elastic, and noiseless. Point-like pinballs are shotat the disks from random starting positions and angles; they spend sometime bouncing between the disks and then escape.


1.3. THE FUTURE AS IN A MIRROR 5

At the beginning of 18th century Baron Gottfried Wilhelm Leibniz wascondent that given the initial conditions one knew all what a deterministicsystem would do far into the future. He wrote [1.1], anticipating by centuryand a half the oft quoted Laplaces Given for one instant an intelligencewhich could comprehend all the forces by which nature is animated...:

That everything is brought forth through an established destiny isjust as certain as that three times three is nine. [. . . ] If, for example,one sphere meets another sphere in free space and if their sizes andtheir paths and directions before collision are known, we can thenforetell and calculate how they will rebound and what course they willtake after the impact. Very simple laws are followed which also apply,no matter how many spheres are taken or whether objects are takenother than spheres. From this one sees then that everything proceedsmathematically that is, infallibly in the whole wide world, so thatif someone could have a sucient insight into the inner parts of things,and in addition had remembrance and intelligence enough to considerall the circumstances and to take them into account, he would be aprophet and would see the future in the present as in a mirror.

Leibniz chose to illustrate his faith in determinism precisely with the typeof physical system that we shall use here as a paradigm of chaos. Hisclaim is wrong in a deep and subtle way: a state of a physical systemcan never be specied to innite precision, there is no way to take all thecircumstances into account, and a single trajectory cannot be tracked, onlya ball of nearby initial points makes physical sense.

1.3.1 What is chaos?

I accept chaos. I am not sure that it accepts me.Bob Dylan, Bringing It All Back Home

A deterministic system is a system whose present state is in principle fullydetermined by its initial conditions, in contra-distinction to a stochasticsystem, for which the initial conditions determine the present state onlypartially, due to noise, or other external circumstances beyond our control.For a stochastic system, the present state reects the past initial conditionsplus the particular realization of the noise encountered along the way.

A deterministic system with suciently complicated dynamics can foolus into regarding it as a stochastic one; disentangling the deterministic fromthe stochastic is the main challenge in many real-life settings, from stockmarket to palpitations of chicken hearts. So, what is chaos?

In a game of pinball, any two trajectories that start out very closeto each other separate exponentially with time, and in a nite (and inpractice, a very small) number of bounces their separation x(t) attainsthe magnitude of L, the characteristic linear extent of the whole system,g. 1.2. This property of sensitivity to initial conditions can be quantied



Figure 1.2: Sensitivity to initial conditions:two pinballs that start out very close to eachother separate exponentially with time.

1

2

3

23132321

2313

as

|x(t)| et|x(0)|

where , the mean rate of separation of trajectories of the system, is calledthe Lyapunov exponent. For any nite accuracy |x(0)| = x of the initial

sect. 8.3 data, the dynamics is predictable only up to a nite Lyapunov time

TLyap 1ln |x/L| , (1.1)

despite the deterministic and, for baron Leibniz, infallible simple laws thatrule the pinball motion.

A positive Lyapunov exponent does not in itself lead to chaos. Onecould try to play 1- or 2-disk pinball game, but it would not be much ofa game; trajectories would only separate, never to meet again. What isalso needed is mixing, the coming together again and again of trajectories.While locally the nearby trajectories separate, the interesting dynamics isconned to a globally nite region of the phase space and thus of necessitythe separated trajectories are folded back and can re-approach each otherarbitrarily closely, innitely many times. In the case at hand there are 2n

topologically distinct n bounce trajectories that originate from a given disk.More generally, the number of distinct trajectories with n bounces can bequantied as

N(n) ehn

sect. 10.1where the topological entropy h (h = ln 2 in the case at hand) is the growthrate of the number of topologically distinct trajectories.

sect. 17.1The appellation chaos is a confusing misnomer, as in deterministic

dynamics there is no chaos in the everyday sense of the word; everythingproceeds mathematically that is, as baron Leibniz would have it, infallibly.When a physicist says that a certain system exhibits chaos, he means thatthe system obeys deterministic laws of evolution, but that the outcome is


1.3. THE FUTURE AS IN A MIRROR 7

(a) (b)

Figure 1.3: Dynamics of a chaotic dynamical system is (a) everywhere locally unsta-ble (positive Lyapunov exponent) and (b) globally mixing (positive entropy). (A. Jo-hansen)

highly sensitive to small uncertainties in the specication of the initial state.The word chaos has in this context taken on a narrow technical meaning.If a deterministic system is locally unstable (positive Lyapunov exponent)and globally mixing (positive entropy) - g. 1.3 - it is said to be chaotic.

While mathematically correct, the denition of chaos as positive Lya-punov + positive entropy is useless in practice, as a measurement of thesequantities is intrinsically asymptotic and beyond reach for systems observedin nature. More powerful is Poincares vision of chaos as the interplay oflocal instability (unstable periodic orbits) and global mixing (intertwiningof their stable and unstable manifolds). In a chaotic system any open ballof initial conditions, no matter how small, will in nite time overlap withany other nite region and in this sense spread over the extent of the entireasymptotically accessible phase space. Once this is grasped, the focus oftheory shifts from attempting precise prediction of individual trajectories(which is impossible) to description of the geometry of the space of pos-sible outcomes, and evaluation of averages over this space. How this isaccomplished is what this book is about.

A denition of turbulence is harder to come by. Intuitively, the wordrefers to irregular behavior of an innite-dimensional dynamical systemdescribed by deterministic equations of motion - say, a bucket of boilingwater described by the Navier-Stokes equations. But in practice the wordturbulence tends to refer to messy dynamics which we understand poorly.As soon as a phenomenon is understood better, it is reclaimed and renamed:

appendix Ba route to chaos, spatiotemporal chaos, and so on.

In this book we shall develop a theory of chaotic dynamics for low dimen-sional attractor visualized as a succession of nearly periodic but unstablemotions. In the same spirit, we shall think of turbulence in spatially ex-tended systems in terms of recurrent spatiotemporal patterns. Pictorially,dynamics drives a given spatially extended system through a repertoire ofunstable patterns; as we watch a turbulent system evolve, every so oftenwe catch a glimpse of a familiar pattern:

= other swirls =



For any nite spatial resolution, the system follows approximately for anite time a pattern belonging to a nite alphabet of admissible patterns,and the long term dynamics can be thought of as a walk through the spaceof such patterns. Recasting this image into mathematics is what this bookis about.

1.3.2 When does chaos matter?

Whether tis nobler in the mind to suerThe slings and arrows of outrageous fortune,Or to take arms against a sea of troubles,And by opposing end them?W. Shakespeare, Hamlet

When should we be mindful of chaos? The solar system is chaotic,yet we have no trouble keeping track of the annual motions of planets. Therule of thumb is this; if the Lyapunov time (1.1) (the time by which a phasespace region initially comparable in size to the observational accuracy ex-tends across the entire accessible phase space) is signicantly shorter thanthe observational time, you need to master the theory that will be devel-oped here. That is why the main successes of the theory are in statisticalmechanics, quantum mechanics, and questions of long term stability in ce-lestial mechanics.

As in science popularizations too much has been made of the impact ofthe chaos theory, a number of caveats are already needed at this point.

At present the theory is in practice applicable only to systems with alow intrinsic dimension the minimum number of degrees of freedom nec-essary to capture its essential dynamics. If the system is very turbulent(description of its long time dynamics requires a space of high intrinsicdimension) we are out of luck. Hence insights that the theory oers to elu-cidation of problems of fully developed turbulence, quantum eld theory ofstrong interactions and early cosmology have been modest at best. Eventhat is a caveat with qualications. There are applications such as spa-

sect. 2.4.1 tially extended systems and statistical mechanics applications where the chapter 20 few important degrees of freedom can be isolated and studied protably by

methods to be described here.

The theory has had limited practical success applied to the very noisysystems so important in life sciences and in economics. Even though weare often interested in phenomena taking place on time scales much longerthan the intrinsic time scale (neuronal interburst intervals, cardiac pulse,etc.), disentangling chaotic motions from the environmental noise hasbeen very hard.


1.4. A GAME OF PINBALL 9

1.4 A game of pinball

Formulas hamper the understanding.S. Smale

We are now going to get down to the brasstacks. But rst, a disclaimer:If you understand most of the rest of this chapter on the rst reading, youeither do not need this book, or you are delusional. If you do not understandit, is not because the people who wrote it are so much smarter than you:the most one can hope for at this stage is to give you a avor of what liesahead. If a statement in this chapter mysties/intrigues, fast forward toa section indicated by on the margin, read only the parts that youfeel you need. Of course, we think that you need to learn ALL of it, orotherwise we would not have written it up in the rst place.

Confronted with a potentially chaotic dynamical system, we analyze itthrough a sequence of three distinct stages; diagnose, count, measure. I.First we determine the intrinsic dimension of the system the minimumnumber of degrees of freedom necessary to capture its essential dynamics. Ifthe system is very turbulent (description of its long time dynamics requires aspace of high intrinsic dimension) we are, at present, out of luck. We knowonly how to deal with the transitional regime between regular motionsand a few chaotic degrees of freedom. That is still something; even aninnite-dimensional system such as a burning ame front can turn out tohave a very few chaotic degrees of freedom. In this regime the chaotic

sect. 2.4.1dynamics is restricted to a space of low dimension, the number of relevantparameters is small, and we can proceed to step II; we count and classify

chapter 9 chapter 10

all possible topologically distinct trajectories of the system into a hierarchywhose successive layers require increased precision and patience on the partof the observer. This we shall do in sects. 1.4 and 1.4.1. If successful, we canproceed with step III of sect. 1.5.1: investigate the weights of the dierentpieces of the system.

We commence our analysis of the pinball game with steps I, II: diagnose,count. We shall return to step III measure in sect. 1.5.1.

chapter 15With the game of pinball we are in luck it is a low dimensional system,

free motion in a plane. The motion of a point particle is such that after acollision with one disk it either continues to another disk or it escapes. Ifwe label the three disks by 1, 2 and 3, we can associate every trajectorywith an itinerary, a sequence of labels which indicates the order in which thedisks are visited; for example, the two trajectories in g. 1.2 have itineraries2313 , 23132321 respectively. The itinerary will be nite for a scatteringtrajectory, coming in from innity and escaping after a nite number ofcollisions, innite for a trapped trajectory, and innitely repeating for aperiodic orbit. Parenthetically, in this subject the words orbit and 1.1

page 29trajectory refer to one and the same thing.

Such labeling is the simplest example of symbolic dynamics. As theparticle cannot collide two times in succession with the same disk, any two



Figure 1.4: Binary labeling of the 3-disk pin-ball trajectories; a bounce in which the trajec-tory returns to the preceding disk is labeled 0,and a bounce which results in continuation tothe third disk is labeled 1.

consecutive symbols must dier. This is an example of pruning, a rulethat forbids certain subsequences of symbols. Deriving pruning rules is ingeneral a dicult problem, but with the game of pinball we are lucky -there are no further pruning rules.

The choice of symbols is in no sense unique. For example, as at eachbounce we can either proceed to the next disk or return to the previous disk,the above 3-letter alphabet can be replaced by a binary {0, 1} alphabet,g. 1.4. A clever choice of an alphabet will incorporate important featuresof the dynamics, such as its symmetries.

sect. 9.7Suppose you wanted to play a good game of pinball, that is, get the

pinball to bounce as many times as you possibly can what would be awinning strategy? The simplest thing would be to try to aim the pinball soit bounces many times between a pair of disks if you managed to shootit so it starts out in the periodic orbit bouncing along the line connectingtwo disk centers, it would stay there forever. Your game would be just asgood if you managed to get it to keep bouncing between the three disksforever, or place it on any periodic orbit. The only rub is that any suchorbit is unstable, so you have to aim very accurately in order to stay closeto it for a while. So it is pretty clear that if one is interested in playingwell, unstable periodic orbits are important they form the skeleton ontowhich all trajectories trapped for long times cling.

sect. 30.2

1.4.1 Partitioning with periodic orbits

A trajectory is periodic if it returns to its starting position and momentum.We shall refer to the set of periodic points that belong to a given periodicorbit as a cycle.

Short periodic orbits are easily drawn and enumerated - some examplesare drawn in g. 1.5 - but it is rather hard to perceive the systematics oforbits from their shapes. In mechanics a trajectory is fully and uniquelyspecied by its position and momentum at a given instant, and no two dis-tinct phase space trajectories can intersect. Their projections on arbitrarysubspaces, however, can and do intersect, in rather unilluminating ways. Inthe pinball example the problem is that we are looking at the projectionsof a 4-dimensional phase space trajectories onto a 2-dimensional subspace,the space coordinates. A clearer picture of the dynamics is obtained byconstructing a phase space Poincare section.

The position of the ball is described by a pair of numbers (the spatialcoordinates on the plane) and its velocity by another pair of numbers (the


1.4. A GAME OF PINBALL 11

Figure 1.5: Some examples of 3-disk cycles:(a) 12123 and 13132 are mapped into eachother by the ip across 1 axis. Similarly (b)123 and 132 are related by ips, and (c) 1213,1232 and 1323 by rotations. (d) The cycles121212313 and 121212323 are related only bytime reversal. These symmetries are discussedin more detail in chapter 19. (from ref. [1.2])

(a)

s11

s2

a

1

(b)

p sin 1

s1

p sin 2

s2

p sin 3

s3

(s1,p1)

(s2,p2)

(s3,p3)

Figure 1.6: (a) The Poincare section coordinates for the 3-disk game of pinball. (b)Collision sequence (s1, p1) (s2, p2) (s3, p3) from the boundary of a disk to theboundary of the next disk presented in the Poincare section coordinates.

components of the velocity vector). As far as baron Leibniz is concerned,this is a complete description.

Suppose that the pinball has just bounced o disk 1. Depending on itsposition and outgoing angle, it could proceed to either disk 2 or 3. Not muchhappens in between the bounces the ball just travels at constant velocityalong a straight line so we can reduce the four-dimensional ow to a two-dimensional map f that takes the coordinates of the pinball from one diskedge to another disk edge. Let us state this more precisely: the trajectoryjust after the moment of impact is dened by marking sn, the arc-lengthposition of the nth bounce along the billiard wall, and pn = p sinn themomentum component parallel to the billiard wall at the point of impact,g. 1.6. Such section of a ow is called a Poincare section, and theparticular choice of coordinates (due to Birkho) is particularly smart, asit conserves the phase-space volume. In terms of the Poincare section, thedynamics is reduced to the return map P : (sn, pn) (sn+1, pn+1) from the



Figure 1.7: (a) A trajectory starting out fromdisk 1 can either hit another disk or escape. (b)Hitting two disks in a sequence requires a muchsharper aim. The cones of initial conditions thathit more and more consecutive disks are nestedwithin each other, as in g. 1.8.

Figure 1.8: Ternary labeled regions of the 3-disk game of pinball phase space Poincaresection which correspond to trajectories that originate on disk 1 and remain connedfor (a) one bounce, (b) two bounces, (c) three bounces. The Poincare sections fortrajectories originating on the other two disks are obtained by the appropriate relabelingof the strips (K.T. Hansen [1.3]).

boundary of a disk to the boundary of the next disk. The explicit form ofthis map is easily written down, but it is of no importance right now.

sect. 5Next, we mark in the Poincare section those initial conditions which

do not escape in one bounce. There are two strips of survivors, as thetrajectories originating from one disk can hit either of the other two disks,or escape without further ado. We label the two stripsM0,M1. Embeddedwithin them there are four stripsM00,M10,M01,M11 of initial conditionsthat survive for two bounces, and so forth, see gs. 1.7 and 1.8. Providedthat the disks are suciently separated, after n bounces the survivors aredivided into 2n distinct strips: the Mith strip consists of all points withitinerary i = s1s2s3 . . . sn, s = {0, 1}. The unstable cycles as a skeletonof chaos are almost visible here: each such patch contains a periodic points1s2s3 . . . sn with the basic block innitely repeated. Periodic points areskeletal in the sense that as we look further and further, the strips shrinkbut the periodic points stay put forever.

We see now why it pays to have a symbolic dynamics; it provides a nav-igation chart through chaotic phase space. There exists a unique trajectoryfor every admissible innite length itinerary, and a unique itinerary labelsevery trapped trajectory. For example, the only trajectory labeled by 12 isthe 2-cycle bouncing along the line connecting the centers of disks 1 and 2;any other trajectory starting out as 12 . . . either eventually escapes or hitsthe 3rd disk.

1.4.2 Escape rate

remark 7.1What is a good physical quantity to compute for the game of pinball? Suchsystem, for which almost any trajectory eventually leaves a nite region


1.5. CHAOS FOR CYCLISTS 13

(the pinball table) never to return, is said to be open, or a repeller. Therepeller escape rate is an eminently measurable quantity. An example ofsuch measurement would be an unstable molecular or nuclear state whichcan be well approximated by a classical potential with possibility of escapein certain directions. In an experiment many projectiles are injected intosuch a non-conning potential and their mean escape rate is measured, asin g. 1.1. The numerical experiment might consist of injecting the pinballbetween the disks in some random direction and asking how many timesthe pinball bounces on the average before it escapes the region between thedisks. 1.2

page 29For a theorist a good game of pinball consists in predicting accuratelythe asymptotic lifetime (or the escape rate) of the pinball. We now showhow the periodic orbit theory accomplishes this for us. Each step will be sosimple that you can follow even at the cursory pace of this overview, andstill the result is surprisingly elegant.

Consider g. 1.8 again. In each bounce the initial conditions get thinnedout, yielding twice as many thin strips as at the previous bounce. The totalarea that remains at a given time is the sum of the areas of the strips, sothat the fraction of survivors after n bounces, or the survival probability isgiven by

1 =|M0||M| +

|M1||M| , 2 =

|M00||M| +

|M10||M| +

|M01||M| +

|M11||M| ,

n =1|M|

(n)i

|Mi| , (1.2)

where i is a label of the ith strip, |M| is the initial area, and |Mi| is thearea of the ith strip of survivors. i = 01, 10, 11, . . . is a label, not a binarynumber. Since at each bounce one routinely loses about the same fractionof trajectories, one expects the sum (1.2) to fall o exponentially with nand tend to the limit

n+1/n = en e . (1.3)

The quantity is called the escape rate from the repeller.

1.5 Chaos for cyclists

We shall now show that the escape rate can be extracted from a highlyconvergent exact expansion by reformulating the sum (1.2) in terms of un-stable periodic orbits.

If, when asked what the 3-disk escape rate is for disk radius 1, center-center separation 6, velocity 1, you answer that the continuous time escaperate is roughly = 0.4103384077693464893384613078192 . . ., you do notneed this book. If you have no clue, hang on.



1.5.1 Size of a partition

Not only do the periodic points keep track of locations and the ordering ofthe strips, but, as we shall now show, they also determine their size.

As a trajectory evolves, it carries along and distorts its innitesimalneighborhood. Let

x(t) = f t(x0)

denote the trajectory of an initial point x0 = x(0). To linear order, theevolution of the distance to a neighboring trajectory xi(t) + xi(t) is givenby the Jacobian matrix

xi(t) =d

j=1

Jt(x0)ijx0j , Jt(x0)ij =xi(t)x0j

.

A trajectory of a pinball moving on a at surface is specied by two positioncoordinates and the direction of motion, so in this case d = 3. Evaluation ofa cycle Jacobian matrix is a longish exercise - here we just state the result.

sect. 5.3 The Jacobian matrix describes the deformation of an innitesimal neigh-borhood of x(t) as it goes with the ow; its the eigenvectors and eigenvaluesgive the directions and the corresponding rates of its expansion or contrac-tion. The trajectories that start out in an innitesimal neighborhood areseparated along the unstable directions (those whose eigenvalues are lessthan unity in magnitude), approach each other along the stable directions(those whose eigenvalues exceed unity in magnitude), and maintain theirdistance along the marginal directions (those whose eigenvalues equal unityin magnitude). In our game of pinball the beam of neighboring trajectoriesis defocused along the unstable eigendirection of the Jacobian matrix J.

As the heights of the strips in g. 1.8 are eectively constant, we canconcentrate on their thickness. If the height is L, then the area of theith strip is Mi Lli for a strip of width li.

Each strip i in g. 1.8 contains a periodic point xi. The ner the inter-vals, the smaller is the variation in ow across them, and the contributionfrom the strip of width li is well approximated by the contraction aroundthe periodic point xi within the interval,

li = ai/|i| , (1.4)

where i is the unstable eigenvalue of the Jacobian matrix Jt(xi) evaluatedat the ith periodic point for t = Tp, the full period (due to the low dimen-sionality, the Jacobian can have at most one unstable eigenvalue). Notethat it is the magnitude of this eigenvalue which is important and we candisregard its sign. The prefactors ai reect the overall size of the system



and the particular distribution of starting values of x. As the asymptotictrajectories are strongly mixed by bouncing chaotically around the repeller,we expect them to be insensitive to smooth variations in the initial distri-bution.

sect. 7.3To proceed with the derivation we need the hyperbolicity assumption: for

large n the prefactors ai O(1) are overwhelmed by the exponential growthof i, so we neglect them. If the hyperbolicity assumption is justied, we

sect. 11.1.1can replace |Mi| Lli in (1.2) by 1/|i| and consider the sum

n =(n)i

1/|i| ,

where the sum goes over all periodic points of period n. We now dene agenerating function for sums over all periodic orbits of all lengths:

(z) =

n=1

nzn . (1.5)

Recall that for large n the nth level sum (1.2) tends to the limit n en ,so the escape rate is determined by the smallest z = e for which (1.5)diverges:

(z)

n=1

(ze)n =ze

1 ze . (1.6)

This is the property of (z) which motivated its denition. We now devisean alternate expression for (1.5) in terms of periodic orbits to make explicitthe connection between the escape rate and the periodic orbits:

(z) =

n=1

zn(n)i

|i|1

=z

|0| +z

|1| +z2

|00| +z2

|01| +z2

|10| +z2

|11|+

z3

|000| +z3

|001| +z3

|010| +z3

|100| + . . . (1.7)

For suciently small z this sum is convergent. The escape rate is now sect. 11.4given by the leading pole of (1.6), rather than a numerical extrapolation of

a sequence of n extracted from (1.3). As any nite truncation n < ntruncof (1.7) is a polynomial in z, convergent for any z, nding this pole requiresthat we know something about n for any n, and that might be a tall order.

We could now proceed to estimate the location of the leading singularityof (z) from nite truncations of (1.7) by methods such as Pade approx-imants. However, as we shall now show, it pays to rst perform a simpleresummation that converts this divergence into a zero of a related function.



1.5.2 Dynamical zeta function

If a trajectory retraces a prime cycle r times, its expanding eigenvalue is rp.A prime cycle p is a single traversal of the orbit; its label is a non-repeatingsymbol string of np symbols. There is only one prime cycle for each cyclicpermutation class. For example, p = 0011 = 1001 = 1100 = 0110 is prime,but 0101 = 01 is not. By the chain rule for derivatives the stability of a 10.5

page 183

sect. 4.4cycle is the same everywhere along the orbit, so each prime cycle of lengthnp contributes np terms to the sum (1.7). Hence (1.7) can be rewritten as

(z) =p

np

r=1

(znp

|p|)r

=p

nptp1 tp , tp =

znp

|p| (1.8)

where the index p runs through all distinct prime cycles. Note that wehave resumed the contribution of the cycle p to all times, so truncating thesummation up to given p is not a nite time n np approximation, butan asymptotic, innite time estimate based by approximating stabilities ofall cycles by a nite number of the shortest cycles and their repeats. Thenpz

np factors in (1.8) suggest rewriting the sum as a derivative

(z) = z ddz

p

ln(1 tp) .

Hence (z) is a logarithmic derivative of the innite product

1/(z) =p

(1 tp) , tp = znp

|p| . (1.9)

This function is called the dynamical zeta function, in analogy to the Rie-mann zeta function, which motivates the choice of zeta in its denition as1/(z). This is the prototype formula of the periodic orbit theory. The zeroof 1/(z) is a pole of (z), and the problem of estimating the asymptoticescape rates from nite n sums such as (1.2) is now reduced to a study ofthe zeros of the dynamical zeta function (1.9). The escape rate is relatedby (1.6) to a divergence of (z), and (z) diverges whenever 1/(z) has azero.

sect. 16.1 sect. 12.4 Easy, you say: Zeros of (1.9) can be read o the formula, a zero zp =

|p|1/np for each term in the product. Whats the problem? Dead wrong!

1.5.3 Cycle expansions

How are formulas such as (1.9) used? We start by computing the lengthsand eigenvalues of the shortest cycles. This usually requires some numericalwork, such as the Newtons method searches for periodic solutions; we shall



assume that the numerics is under control, and that all short cycles up togiven length have been found. In our pinball example this can be done

chapter 14by elementary geometrical optics. It is very important not to miss anyshort cycles, as the calculation is as accurate as the shortest cycle dropped including cycles longer than the shortest omitted does not improve theaccuracy (unless exponentially many more cycles are included). The resultof such numerics is a table of the shortest cycles, their periods and theirstabilities.

sect. 25.3Now expand the innite product (1.9), grouping together the terms of

the same total symbol string length

1/ = (1 t0)(1 t1)(1 t10)(1 t100) = 1 t0 t1 [t10 t1t0] [(t100 t10t0) + (t101 t10t1)]

[(t1000 t0t100) + (t1110 t1t110)+(t1001 t1t001 t101t0 + t10t0t1)] . . . (1.10)

The virtue of the expansion is that the sum of all terms of the same total chapter 15length n (grouped in brackets above) is a number that is exponentially

smaller than a typical term in the sum, for geometrical reasons we explainin the next section.

sect. 15.1The calculation is now straightforward. We substitute a nite set of the

eigenvalues and lengths of the shortest prime cycles into the cycle expansion(1.10), and obtain a polynomial approximation to 1/. We then vary z in(1.9) and determine the escape rate by nding the smallest z = e forwhich (1.10) vanishes.

1.5.4 Shadowing

When you actually start computing this escape rate, you will nd out thatthe convergence is very impressive: only three input numbers (the two xedpoints 0, 1 and the 2-cycle 10) already yield the pinball escape rate to 3-4signicant digits! We have omitted an innity of unstable cycles; so why

sect. 15.1.3does approximating the dynamics by a nite number of the shortest cycleeigenvalues work so well?

The convergence of cycle expansions of dynamical zeta functions is aconsequence of the smoothness and analyticity of the underlying ow.Intuitively, one can understand the convergence in terms of the geometricalpicture sketched in g. 1.9; the key observation is that the long orbits areshadowed by sequences of shorter orbits.

A typical term in (1.10) is a dierence of a long cycle {ab} minus itsshadowing approximation by shorter cycles {a} and {b}

tab tatb = tab(1 tatb/tab) = tab(1

abab) , (1.11)



Figure 1.9: Approximation to (a) a smooth dynamics by (b) the skeleton of periodicpoints, together with their linearized neighborhoods. Indicated are segments of two1-cycles and a 2-cycle that alternates between the neighborhoods of the two 1-cycles,shadowing rst one of the two 1-cycles, and then the other.

where a and b are symbol sequences of the two shorter cycles. If all orbitsare weighted equally (tp = znp), such combinations cancel exactly; if orbitsof similar symbolic dynamics have similar weights, the weights in suchcombinations almost cancel.

This can be understood in the context of the pinball game as follows.Consider orbits 0, 1 and 01. The rst corresponds to bouncing between anytwo disks while the second corresponds to bouncing successively around allthree, tracing out an equilateral triangle. The cycle 01 starts at one disk,say disk 2. It then bounces from disk 3 back to disk 2 then bounces from disk1 back to disk 2 and so on, so its itinerary is 2321. In terms of the bouncetypes shown in g. 1.4, the trajectory is alternating between 0 and 1. Theincoming and outgoing angles when it executes these bounces are very closeto the corresponding angles for 0 and 1 cycles. Also the distances traversedbetween bounces are similar so that the 2-cycle expanding eigenvalue 01is close in magnitude to the product of the 1-cycle eigenvalues 01.

To understand this on a more general level, try to visualize the partitionof a chaotic dynamical systems phase space in terms of cycle neighborhoodsas a tessellation of the dynamical system, with smooth ow approximatedby its periodic orbit skeleton, each face centered on a periodic point, andthe scale of the face determined by the linearization of the ow aroundthe periodic point, g. 1.9.

The orbits that follow the same symbolic dynamics, such as {ab} anda pseudo orbit {a}{b}, lie close to each other in the phase space; longshadowing pairs have to start out exponentially close to beat the expo-nential growth in separation with time. If the weights associated with theorbits are multiplicative along the ow (for example, by the chain rule forproducts of derivatives) and the ow is smooth, the term in parenthesisin (1.11) falls o exponentially with the cycle length, and therefore the


1.6. EVOLUTION 19

curvature expansions are expected to be highly convergent. chapter 13

1.6 Evolution

The above derivation of the dynamical zeta function formula for the escaperate has one shortcoming; it estimates the fraction of survivors as a functionof the number of pinball bounces, but the physically interesting quantity isthe escape rate measured in units of continuous time. For continuous timeows, the escape rate (1.2) is generalized as follows. Dene a nite phasespace region M such that a trajectory that exits M never reenters. Forexample, any pinball that falls of the edge of a pinball table in g. 1.1 is goneforever. Start with a uniform distribution of initial points. The fraction ofinitial x whose trajectories remain within M at time t is expected to decayexponentially

(t) =

M dxdy (y f t(x))

M dx et .

The integral over x starts a trajectory at every x M. The integral overy tests whether this trajectory is still in M at time t. The kernel of thisintegral

Lt(y, x) = (y f t(x)) (1.12)is the Dirac delta function, as for a deterministic ow the initial point xmaps into a unique point y at time t. For discrete time, fn(x) is the nthiterate of the map f . For continuous ows, f t(x) is the trajectory of theinitial point x, and it is appropriate to express the nite time kernel Lt interms of a generator of innitesimal time translations

Lt = etA , sect. 7.4.1 chapter 26very much in the way the quantum evolution is generated by the Hamilto-

nian H, the generator of innitesimal time quantum transformations.

As the kernel L is the key to everything that follows, we shall give it aname, and refer to it and its generalizations as the evolution operator for ad-dimensional map or a d-dimensional ow.

The number of periodic points increases exponentially with the cyclelength (in case at hand, as 2n). As we have already seen, this exponentialproliferation of cycles is not as dangerous as it might seem; as a matter offact, all our computations will be carried out in the n limit. Thougha quick look at chaotic dynamics might reveal it to be complex beyondbelief, it is still generated by a simple deterministic law, and with someluck and insight, our labeling of possible motions will reect this simplicity.



Figure 1.10: The trace of an evolution operator is concentrated in tubes aroundprime cycles, of length Tp and thickness 1/|p|r for rth repeat of the prime cycle p.

If the rule that gets us from one level of the classication hierarchy tothe next does not depend strongly on the level, the resulting hierarchy isapproximately self-similar. We now turn such approximate self-similarity toour advantage, by turning it into an operation, the action of the evolutionoperator, whose iteration encodes the self-similarity.

1.6.1 Trace formula

Recasting dynamics in terms of evolution operators changes everything.So far our formulation has been heuristic, but in the evolution operatorformalism the escape rate and any other dynamical average are given byexact formulas, extracted from the spectra of evolution operators. The keytools are the trace formulas and the spectral determinants.

The trace of an operator is given by the sum of its eigenvalues. Theexplicit expression (1.12) for Lt(x, y) enables us to evaluate the trace. Iden-tify y with x and integrate x over the whole phase space. The result is anexpression for trLt as a sum over neighborhoods of prime cycles p and theirrepetitions

sect. 11.3

trLt =p

Tp

r=1

(t rTp)det (1 Jrp) . (1.13)This formula has a simple geometrical interpretation sketched in g. 1.10.After the rth return to a Poincare section, the initial tube Mp has beenstretched out along the expanding eigendirections, with the overlap withthe initial volume given by 1/

det (1 Jrp) 1/|p|.The spiky sum (1.13) is disquieting in the way reminiscent of the

Poisson resummation formulas of Fourier analysis; the left-hand side is thesmooth eigenvalue sum tr eA =

est, while the right-hand side equals


1.7. FROM CHAOS TO STATISTICAL MECHANICS 21

zero everywhere except for the set t = rTp. A Laplace transform smoothsthe sum over Dirac delta functions in cycle periods and yields the traceformula for the eigenspectrum s0, s1, of the classical evolution operator:

0+

dt est trLt = tr 1sA =

=0

1s s

=p

Tp

r=1

er(ApsTp)det (1 Jrp) . (1.14)The beauty of the trace formulas lies in the fact that everything on the right-

sect. 11.1hand-side prime cycles p, their periods Tp and the stability eigenvaluesof Jp is an invariant property of the ow, independent of any coordinatechoice.

1.6.2 Spectral determinant

The eigenvalues of a linear operator are given by the zeros of the appropriatedeterminant. One way to evaluate determinants is to expand them in termsof traces, using the identities 4.1

page 77

ln det (sA) = tr ln(sA)d

dsln det (sA) = tr 1

sA ,

and integrating over s. In this way the spectral determinant of an evolutionoperator becomes related to the traces that we have just computed:

chapter 12

det (sA) = exp(p

r=1

1r

esTprdet (1 Jrp))

. (1.15)

The s integration leads here to replacement Tp Tp/rTp in the periodicorbit expansion (1.14).

The motivation for recasting the eigenvalue problem in this form issketched in g. 1.11; exponentiation improves analyticity and trades in adivergence of the trace sum for a zero of the spectral determinant. The

sect. 12.5.1computation of the zeros of det (s A) proceeds very much like the com-putations of sect. 1.5.3.

1.7 From chaos to statistical mechanics

While the above replacement of dynamics of individual trajectories by evo-lution operators which propagate densities might feel like just another bit



Figure 1.11: Spectral determinant is prefer-able to the trace as it vanishes smoothly at theleading eigenvalue, while the trace formula di-verges.

of mathematical voodoo, actually something very radical has taken place.Consider a chaotic ow, such as stirring of red and white paint by somedeterministic machine. If we were able to track individual trajectories, theuid would forever remain a striated combination of pure white and purered; there would be no pink. What is more, if we reversed stirring, wewould return back to the perfect white/red separation. However, we knowthat this cannot be true in a very few turns of the stirring stick the thick-ness of the layers goes from centimeters to Angstroms, and the result isirreversibly pink.

Understanding the distinction between evolution of individual trajecto-ries and the evolution of the densities of trajectories is key to understand-ing statistical mechanics this is the conceptual basis of the second law ofthermodynamics, and the origin of irreversibility of the arrow of time fordeterministic systems with time-reversible equations of motion: reversibil-ity is attainable for distributions whose measure in the space of densityfunctions goes exponentially to zero with time.

By going to a description in terms of the asymptotic time evolution oper-ators we give up tracking individual trajectories for long times, but insteadgain a very eective description of the asymptotic trajectory densities. Thiswill enable us, for example, to give exact formulas for transport coecientssuch as the diusion constants without any probabilistic assumptions (such

chapter 20 as the stosszahlansatz of Boltzmann).

A century ago it seemed reasonable to assume that statistical mechanicsapplies only to systems with very many degrees of freedom. More recentis the realization that much of statistical mechanics follows from chaoticdynamics, and already at the level of a few degrees of freedom the evolutionof densities is irreversible. Furthermore, the theory that we shall develophere generalizes notions of measure and averaging to systems far fromequilibrium, and transports us into regions hitherto inaccessible with thetools of the equilibrium statistical mechanics.

The results of the equilibrium statistical mechanics do help us, however,to understand the ways in which the simple-minded periodic orbit theoryfalters. A non-hyperbolicity of the dynamics manifests itself in power-lawcorrelations and even phase transitions.

chapter 18intro - 13aug2003 version 10, Aug 26 2003

1.8. GUIDE TO LITERATURE 23

1.8 Guide to literature

But the power of instruction is seldom of much e-cacy, except in those happy dispositions where it isalmost superuous.Gibbon

This text aims to bridge the gap between the physics and mathematics dy-namical systems literature. The intended audience is the dream graduatestudent, with a theoretical bent. As a complementary presentation we rec-ommend Gaspards monograph [1.4] which covers much of the same groundin a highly readable and scholarly manner.

As far as the prerequisites are concerned - this book is not an intro-duction to nonlinear dynamics. Nonlinear science requires a one semesterbasic course (advanced undergraduate or rst year graduate). A good startis the textbook by Strogatz [1.5], an introduction to ows, xed points,manifolds, bifurcations. It is probably the most accessible introductionto nonlinear dynamics - it starts out with dierential equations, and itsbroadly chosen examples and many exercises make it favorite with stu-dents. It is not strong on chaos. There the textbook of Alligood, Sauer andYorke [1.6] is preferable: an elegant introduction to maps, chaos, perioddoubling, symbolic dynamics, fractals, dimensions - a good companion tothis book. An introduction more comfortable to physicists is the textbookby Ott [1.7], with bakers map used to illustrate many key techniques inanalysis of chaotic systems. It is perhaps harder than the above two as therst book on nonlinear dynamics.

An introductory course should give students skills in qualitative andnumerical analysis of dynamical systems for short times (trajectories, xedpoints, bifurcations) and familiarize them with Cantor sets and symbolicdynamics for chaotic dynamics. With this, and a graduate level exposure tostatistical mechanics, partial dierential equations and quantum mechanics,the stage is set for any of the one-semester advanced courses based on thisbook. The courses taught so far start out with the introductory chapterson qualitative dynamics, symbolic dynamics and ows, and then continuein dierent directions:

Deterministic chaos. Chaotic averaging, evolution operators, traceformulas, zeta functions, cycle expansions, Lyapunov exponents, billiards,transport coecients, thermodynamic formalism, period doubling, renor-malization operators.

Spatiotemporal dynamical systems. Partial dierential equationsfor dissipative systems, weak amplitude expansions, normal forms, symme-tries and bifurcations, pseudospectral methods, spatiotemporal chaos.

Quantum chaology. Semiclassical propagators, density of states,trace formulas, semiclassical spectral determinants, billiards, semiclassicalhelium, diraction, creeping, tunneling, higher corrections.



This book concentrates on the periodic orbit theory. The role of un-stable periodic orbits was already fully appreciated by Poincare [1.8, 1.9],who noted that hidden in the apparent chaos is a rigid skeleton, a tree ofcycles (periodic orbits) of increasing lengths and self-similar structure, andsuggested that the cycles should be the key to chaotic dynamics. Periodicorbits have been at core of much of the mathematical work on the the-ory of the classical and quantum dynamical systems ever since. We referthe reader to the reprint selection [1.10] for an overview of some of thatliterature.

If you nd this book not rigorous enough, you should turn to the math-ematics literature. The most extensive reference is the treatise by Katokand Hasselblatt [1.11], an impressive compendium of modern dynamicalsystems theory. The fundamental papers in this eld, all still valuablereading, are Smale [1.12], Bowen [1.13] and Sinai [1.14]. Sinais paper isprescient and oers a vision and a program that ties together dynamicalsystems and statistical mechanics. It is written for readers versed in statis-tical mechanics. Markov partitions were introduced by Sinai in ref. [1.15].The classical text (though certainly not an easy read) on the subject ofdynamical zeta functions is Ruelles Statistical Mechanics, ThermodynamicFormalism [1.16]. In Ruelles monograph transfer operator technique (orthe Perron-Frobenius theory) and Smales theory of hyperbolic ows areapplied to zeta functions and correlation functions. The status of the the-ory from Ruelles point of view is compactly summarized in his 1995 Pisalectures [1.17]. Further excellent mathematical references on thermody-namic formalism are Parry and Pollicotts monograph [1.18] with emphasison the symbolic dynamics aspects of the formalism, and Baladis clear andcompact reviews of the theory dynamical zeta functions [1.19, 1.20].

A graduate level introduction to statistical mechanics from the dynam-ical point view is given by Dorfman [1.21]; the Gaspard monograph [1.4]covers the same ground in more depth. Driebe monograph [1.22] oers anice introduction to the problem of irreversibility in dynamics. The role ofchaos in statistical mechanics is critically dissected by Bricmont in hishighly readable essay Science of Chaos or Chaos in Science? [1.23].

If you were wandering while reading this introduction whats up withrat brains?, the answer is yes indeed, there is a line of research in studyon neuronal dynamics that focuses on possible unstable periodic states,described for example in ref. [1.25, 1.26, 1.27].

Guide to exercises

God can aord to make mistakes. So can Dada!Dadaist Manifesto

The essence of this subject is incommunicable in print; the only way todevelop intuition about chaotic dynamics is by computing, and the reader isurged to try to work through the essential exercises. Some of the solutions


1.8. GUIDE TO LITERATURE 25

provided might be more illuminating than the main text. So as not tofragment the text, the exercises are indicated by text margin boxes suchas the one on this margin, and collected at the end of each chapter. The 15.2

page 282problems that you should do have underlined titles. The rest (smaller type)are optional. Dicult problems are marked by any number of *** stars.By the end of the course you should have completed at least three projects:(a) compute everything for a one-dimensional repeller, (b) compute escaperate for a 3-disk game of pinball, (c) compute a part of the quantum 3-diskgame of pinball, or the helium spectrum, or if you are interested in statisticalrather than the quantum mechanics, compute a transport coecient. Theessential steps are:

Dynamics1. count prime cycles, exercise 1.1

2. pinball simulator, exercise 5.1, exercise 14.4

3. pinball stability, exercise 5.5, exercise 14.4

4. pinball periodic orbits, exercise 14.6, exercise 14.5

5. helium integrator, exercise 2.9, exercise 14.8

6. helium periodic orbits, exercise 29.4, exercise 14.9

Averaging, numerical1. pinball escape rate, exercise 12.12

2. Lyapunov exponent, exercise 17.2

Averaging, periodic orbits1. cycle expansions, exercise 15.1, exercise 15.2

2. pinball escape rate, exercise 15.4, exercise 15.5

3. cycle expansions for averages, exercise 15.1, exercise 16.3

4. cycle expansions for diusion, exercise 20.1

5. desymmetrization exercise 19.1

6. semiclassical quantization exercise 28.3

7. ortho-, para-helium, lowest eigenenergies exercise 29.7

Solutions for some of the problems are included appendix O. Oftengoing through a solution is more instructive than reading the correspondingchapter.

Resume

The goal of this text is an exposition of the best of all possible theories ofdeterministic chaos, and the strategy is: 1) count, 2) weigh, 3) add up.



In a chaotic system any open ball of initial conditions, no matter howsmall, will spread over the entire accessible phase space. Hence the theoryfocuses on description of the geometry of the space of possible outcomes,and evaluation of averages over this space, rather than attempting theimpossible, precise prediction of individual trajectories. The dynamics ofdistributions of trajectories is described in terms of evolution operators. Inthe evolution operator formalism the dynamical averages are given by exactformulas, extracted from the spectra of evolution operators. The key toolsare the trace formulas and the spectral determinants.

The theory of evaluation of spectra of evolution operators presentedhere is based on the observation that the motion in dynamical systems offew degrees of freedom is often organized around a few fundamental cycles.These short cycles capture the skeletal topology of the motion on a strangeattractor in the sense that any long orbit can approximately be pieced to-gether from the nearby periodic orbits of nite length. This notion is madeprecise by approximating orbits by prime cycles, and evaluating associatedcurvatures. A curvature measures the deviation of a longer cycle from itsapproximation by shorter cycles; smoothness and the local instability ofthe ow implies exponential (or faster) fall-o for (almost) all curvatures.Cycle expansions oer then an ecient method for evaluating classical andquantum observables.

The critical step in the derivation of the dynamical zeta function was thehyperbolicity assumption, that is the assumption of exponential shrinkageof all strips of the pinball repeller. By dropping the ai prefactors in (1.4),we have given up on any possibility of recovering the precise distributionof starting x (which should anyhow be impossible due to the exponentialgrowth of errors), but in exchange we gain an eective description of theasymptotic behavior of the system. The pleasant surprise of cycle expan-sions (1.9) is that the innite time behavior of an unstable system is aseasy to determine as the short time behavior.

To keep exposition simple we have here illustrated the utility of cyclesand their curvatures by a pinball game, but topics covered in this book unstable ows, Poincare sections, Smale horseshoes, symbolic dynamics,pruning, discrete symmetries, periodic orbits, averaging over chaotic sets,evolution operators, dynamical zeta functions, spectral determinants, cycleexpansions, quantum trace formulas and zeta functions, and so on to thesemiclassical quantization of helium should give the reader some con-dence in the general applicability of the theory. The formalism should workfor any average over any chaotic set which satises two conditions:

1. the weight associated with the observable under consideration ismultiplicative along the trajectory,

2. the set is organized in such a way that the nearby points in thesymbolic dynamics have nearby weights.

The theory is applicable to evaluation of a broad class of quantities char-acterizing chaotic systems, such as the escape rates, Lyapunov exponents,


REFERENCES 27

transport coecients and quantum eigenvalues. One of the surprises is thatthe quantum mechanics of classically chaotic systems is very much like theclassical mechanics of chaotic systems; both are described by nearly thesame zeta functions and cycle expansions, with the same dependence onthe topology of the classical ow.

References

[1.1] G.W. Leibniz, Von dem Verhangnisse

[1.2] P. Cvitanovic, B. Eckhardt, P.E. Rosenqvist, G. Russberg and P. Scherer,in G. Casati and B. Chirikov, eds., Quantum Chaos (Cambridge UniversityPress, Cambridge 199

classical and quantum chaos

Documents

stability of ows

stability of maps

topological trace formula

cycle stability

asymptotic trace formula

local stability

trace formulas

stability of billiards84resume