2010
DOI: 10.1088/1742-5468/2010/04/p04021
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Thermostatistics in the neighbourhood of the π-mode solution for the Fermi–Pasta–Ulam β system: from weak to strong chaos

Abstract: Abstract. We consider a π-mode solution of the Fermi-Pasta-Ulam β system. By perturbing it, we study the system as a function of the energy density from a regime where the solution is stable to a regime, where is unstable, first weakly and then strongly chaotic. We introduce, as indicator of stochasticity, the ratio ρ (when is defined) between the second and the first moment of a given probability distribution. We will show numerically that the transition between weak and strong chaos can be interpreted as the… Show more

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Cited by 18 publications
(27 citation statements)
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References 35 publications
(49 reference statements)
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“…Such is the case for the Fermi-Pasta-Ulam β model for finite N , as recently shown [95,96]: Gaussian distributions of momenta are observed for time averages far from its π-orbit (consistently with the CLT), whereas (strict or approximate) q-Gaussians emerge very close to it. See Figure 13.…”
Section: Remarks On Paradigmatic Long-range-interacting Many-body Clasupporting
confidence: 55%
“…Such is the case for the Fermi-Pasta-Ulam β model for finite N , as recently shown [95,96]: Gaussian distributions of momenta are observed for time averages far from its π-orbit (consistently with the CLT), whereas (strict or approximate) q-Gaussians emerge very close to it. See Figure 13.…”
Section: Remarks On Paradigmatic Long-range-interacting Many-body Clasupporting
confidence: 55%
“…(18) therein]. We also note that our results do not exclude the possibility of Tsallis distributions in nonergodic systems such as those composed of classical longrange interacting particles or in some regions of weak chaos [27][28][29][30] since the ergodicity of the total system is assumed in the present work.…”
Section: Discussionmentioning
confidence: 73%
“…Following the approach of [34], we verify that the pdfs of chaotic orbits starting very close to the unstable π-mode are well approximated by a q-Gaussian over time intervals of the order of t ≈ 10 6 . These trajectories, however, represent a QSS: Their distributions for longer times deviate from a q-Gaussian and show a tendency to converge to a Gaussian as q → 1.…”
Section: Introductionmentioning
confidence: 72%