Equipartition threshold in nonlinear large Hamiltonian systems: The Fermi-Pasta-Ulam model

Roberto Livi, Marco Pettini, Stefano Ruffo, Massimo Sparpaglione, and Angelo Vulpiani
Phys. Rev. A 31, 1039 – Published 1 February 1985
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Abstract

The Fermi-Pasta-Ulam β model has been studied by integrating numerically the equations of motion for a system of N nonlinearly coupled oscillators with N ranging from 64 to 512. Multimode excitations have been considered as initial conditions; the number Δn of initially excited modes is such that the ratio Δn/N is kept constant. We can consider the system as a gas of weakly coupled phonons (normal modes), so that if we keep the ratio Δn/N constant we find an analogy with the thermodynamical limit of statistical mechanics where the ratio M/V is constant when both the volume V and the number of particles M are increased up to infinity. The relaxation towards stationary states is followed through the time evolution of a suitably defined ‘‘spectral entropy’’ which depends on the shape of the space Fourier spectrum; this spectral entropy is a good equipartition indicator: Strong evidence is reported in favor of the existence of an equipartition threshold. Its persistence at very different values of N is also clearly shown. The main result concerns the occurrence of the threshold at the same value of the energy density (i.e., of the ‘‘control parameter’’) when the number of degrees of freedom is changed. More general initial conditions are also considered and the same result is found using as a control parameter a pseudo-Reynolds-number R: The threshold occurs at the same critical value Rc when N is varied. It turns out that a fully chaotic regime (equipartition) is obtained with an ‘‘average nonlinearity’’ of the system of about 3%.

  • Received 30 January 1984

DOI:https://doi.org/10.1103/PhysRevA.31.1039

©1985 American Physical Society

Authors & Affiliations

Roberto Livi

  • Dipartimento di Fisica dell’Università degli Studi di Firenze, Largo Enrico Fermi 2, I-50125 Firenze, Italy and Istituto Nazionale di Fisica Nucleare, Sezione di Firenze, I-50125 Firenze, Italy

Marco Pettini

  • Osservatorio Astrofisico di Arcetri, Largo Enrico Fermi 5, I-50125 Firenze, Italy and Gruppo Nazionale di Astronomia del Consiglio Nazionale delle Ricerche, I-50125 Firenze, Italy

Stefano Ruffo

  • Dipartimento di Fisica dell’Università degli Studi di Firenze, Largo Enrico Fermi 2, I-50125 Firenze, Italy and Istituto Nazionale di Fisica Nucleare, Sezione di Firenze, I-50125 Firenze, Italy

Massimo Sparpaglione

  • Department of Chemistry, University of Rochester, Hutchison 419, Rochester, New York 14627

Angelo Vulpiani

  • Dipartimento di Fisica, Università ‘‘La Sapienza,’’ Piazzale Aldo Moro 2, I-00185 Roma, Italy and Gruppo Nazionale di Struttura della Materia del Consiglio Nazionale delle Ricerche, I-00185 Roma, Italy

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Vol. 31, Iss. 2 — February 1985

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