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Phase space geometry and stochasticity thresholds in hamiltonian dynamics

Cerruti-Sola1, Pettini, Cohen

  • 1Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, 50125 Firenze, Italy and Istituto Nazionale di Fisica della Materia, UdR di Firenze, Frienze, Italy.

Summary

Numerical computations reveal two thresholds in the Fermi-Pasta-Ulam alpha+beta model. A strong stochasticity threshold (SST) is geometrically characterized by phase space curvature and autocorrelation decay time.

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