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Phys. Rev. E 54, 5969–5984 (1996)

Riemannian theory of Hamiltonian chaos and Lyapunov exponents

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Lapo Casetti*
Scuola Normale Superiore, Piazza dei Cavalieri 7, 56126 Pisa, Italy

Cecilia Clementi
International School for Advanced Studies (SISSA/ISAS), via Beirut 2-4, 34014 Trieste, Italy

Marco Pettini
Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, 50125 Firenze, Italy

Received 19 July 1996; published in the issue dated December 1996

A nonvanishing Lyapunov exponent λ1 provides the very definition of deterministic chaos in the solutions of a dynamical system; however, no theoretical mean of predicting its value exists. This paper copes with the problem of analytically computing the largest Lyapunov exponent λ1 for many degrees of freedom Hamiltonian systems as a function of ɛ=E/N, the energy per degree of freedom. The functional dependence λ1(ɛ) is of great interest because, among other reasons, it detects the existence of weakly and strongly chaotic regimes. This aim, the analytic computation of λ1(ɛ), is successfully reached within a theoretical framework that makes use of a geometrization of Newtonian dynamics in the language of Riemannian differential geometry. An alternative point of view about the origin of chaos in these systems is obtained independently of the standard explanation based on homoclinic intersections. Dynamical instability (chaos) is here related to curvature fluctuations of the manifolds whose geodesics are natural motions and is described by means of the Jacobi-Levi-Civita equation (JLCE) for geodesic spread. In this paper it is shown how to derive from the JLCE an effective stability equation. Under general conditions, this effective equation formally describes a stochastic oscillator; an analytic formula for the instability growth rate of its solutions is worked out and applied to the Fermi-Pasta-Ulam β model and to a chain of coupled rotators. Excellent agreement is found between the theoretical prediction and numeric values of λ1(ɛ) for both models.

© 1996 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevE.54.5969
DOI:
10.1103/PhysRevE.54.5969
PACS:
05.45.+b, 02.40.-k, 05.20.-y

*Also at INFN, Sezione di Firenze, Italy. Electronic address: casetti@sns.it

Also at INFM, Unità di Trieste, and INFN, Sezione di Trieste, Italy. Electronic address: clementi@sissa.it

Also at INFM, Unità di Firenze, and INFN, Sezione di Firenze, Italy. Electronic address: pettini@arcetri.astro.it