In a specific continuum limit at intermediate energy, the Fermi-Pasta-Ulam (FPU)-β chain can be described by a nonlinear partial differential equation whose solutions are shock waves. Proper long-wavelength initial conditions of the discrete model show a time evolution in numerical simulations that agrees with the solution of the continuum model where it is single valued. The breakdown times for the occurrence of the shock, when starting from a smooth initial condition, are shown to be relevant time scales for the transition to equipartition of energy, by an analysis of the time evolution of the spectral entropy. A simple time scale tB∼N2/(βkE) is derived in the continuum limit for mode k initial excitations with energy E and N particles. This time scale is tested numerically in the FPU chain. © 1995 The American Physical Society.

Shock waves and time scales to reach equipartition in the Fermi-Pasta-Ulam model / Poggi, P.; Ruffo, S.; Kantz, H.. - In: PHYSICAL REVIEW E. - ISSN 1063-651X. - 52:1(1995), pp. 307-315. [10.1103/PhysRevE.52.307]

Shock waves and time scales to reach equipartition in the Fermi-Pasta-Ulam model

Ruffo S.;
1995-01-01

Abstract

In a specific continuum limit at intermediate energy, the Fermi-Pasta-Ulam (FPU)-β chain can be described by a nonlinear partial differential equation whose solutions are shock waves. Proper long-wavelength initial conditions of the discrete model show a time evolution in numerical simulations that agrees with the solution of the continuum model where it is single valued. The breakdown times for the occurrence of the shock, when starting from a smooth initial condition, are shown to be relevant time scales for the transition to equipartition of energy, by an analysis of the time evolution of the spectral entropy. A simple time scale tB∼N2/(βkE) is derived in the continuum limit for mode k initial excitations with energy E and N particles. This time scale is tested numerically in the FPU chain. © 1995 The American Physical Society.
1995
52
1
307
315
https://journals.aps.org/pre/abstract/10.1103/PhysRevE.52.307
Poggi, P.; Ruffo, S.; Kantz, H.
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/20.500.11767/116537
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