We investigate the dynamics of the Fermi-Pasta-Ulam-Tsingou chain with long-wavelength random initial data. When the energy per particle is small, thermal equilibrium is not reached on a fast timescale, and the system enters prethermalization. The formation of the prethermal state is characterized by the development of a Burgers-type shock and the onset of a turbulentlike spectrum with a time dependent exponent zeta(t) in the inertial range. We perform a significant step forward by demonstrating that these features are robust under generic long-wavelength random initial conditions. By employing advanced probabilistic techniques inspired by the works of Dudley and Talagrand, we derive a sharp asymptotic expression for the average shock time in the thermodynamic limit. For large p, this time scales as (p√log p)⁻¹, where p is the number of excited modes, proving that it is an intensive quantity up to a logarithmic correction in the size of the system.
Random Initial Data and Average Shock Time in the Fermi-Pasta-Ulam-Tsingou Chain / M. Gallone, R.G.. - In: PHYSICAL REVIEW LETTERS. - ISSN 0031-9007. - 136:21(2026 May 27), pp. 1-7. [10.1103/qxzs-1t1l]
Random Initial Data and Average Shock Time in the Fermi-Pasta-Ulam-Tsingou Chain
M. Gallone
Primo
;A. Ponno;
2026
Abstract
We investigate the dynamics of the Fermi-Pasta-Ulam-Tsingou chain with long-wavelength random initial data. When the energy per particle is small, thermal equilibrium is not reached on a fast timescale, and the system enters prethermalization. The formation of the prethermal state is characterized by the development of a Burgers-type shock and the onset of a turbulentlike spectrum with a time dependent exponent zeta(t) in the inertial range. We perform a significant step forward by demonstrating that these features are robust under generic long-wavelength random initial conditions. By employing advanced probabilistic techniques inspired by the works of Dudley and Talagrand, we derive a sharp asymptotic expression for the average shock time in the thermodynamic limit. For large p, this time scales as (p√log p)⁻¹, where p is the number of excited modes, proving that it is an intensive quantity up to a logarithmic correction in the size of the system.| File | Dimensione | Formato | |
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