Abstract

This paper examines discreteness effects in nearly collisionless N-body systems of charged particles interacting via an unscreened r^-2 force, allowing for bulk potentials admitting both regular and chaotic orbits. Both for ensembles and individual orbits, as N increases there is a smooth convergence towards a continuum limit. Discreteness effects are well modeled by Gaussian white noise with relaxation time t_R = const * (N/log L)t_D, with L the Coulomb logarithm and t_D the dynamical time scale. Discreteness effects accelerate emittance growth for initially localised clumps. However, even allowing for discreteness effects one can distinguish between orbits which, in the continuum limit, feel a regular potential, so that emittance grows as a power law in time, and chaotic orbits, where emittance grows exponentially. For sufficiently large N, one can distinguish two different `kinds' of chaos. Short range microchaos, associated with close encounters between charges, is a generic feature, yielding large positive Lyapunov exponents X_N which do not decrease with increasing N even if the bulk potential is integrable. Alternatively, there is the possibility of larger scale macrochaos, characterised by smaller Lyapunov exponents X_S, which is present only if the bulk potential is chaotic. Conventional computations of Lyapunov exponents probe X_N, leading to the oxymoronic conclusion that N-body orbits which look nearly regular and have sharply peaked Fourier spectra are `very chaotic.' However, the `range' of the microchaos, set by the typical interparticle spacing, decreases as N increases, so that, for large N, this microchaos, albeit very strong, is largely irrelevant macroscopically. A more careful numerical analysis allows one to estimate both X_N and X_S.

Highlights

  • A standard, often tacit, assumption in theoretical investigations of charged particle beams is that particle correlations are unimportant

  • If the system is in static equilibrium, the distribution function can be expressed as a function of isolating integrals of particle motion in the mean potential

  • We demonstrate that discreteness effects can be critically important even within just a few dynamical times tD, especially for potentials that support a sizable population of globally chaotic orbits

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Summary

INTRODUCTION

A standard, often tacit, assumption in theoretical investigations of charged particle beams is that particle correlations are unimportant With this assumption, one applies the Vlasov-Poisson equations to calculate the distribution function of the particles in the six-dimensional phase space of a single particle [1,2]. For systems not too far from equilibrium, one can invoke a perturbation theory using Vlasov-Poisson to calculate the evolution of the distribution function [4]. Such techniques are powerful and mature, but the underlying assumption must be questioned [5]. Adequately describe real finite-N systems? A related question is (2) to what extent do predictions derived from a simulation involving N < N macroparticles adequately describe the real N -body system? The present paper is concerned with how discreteness effects, i.e., granularity, influence the answers to both questions

PRELIMINARIES
Frozen N-body models
Methodology for orbital analysis
Modeling N-body orbits and flows by Gaussian white noise
Models considered
Phase mixing and the continuum limit
Individual orbits and the continuum limit
The model
V i1 jr ri j2 e2
Phase mixing of regular orbits
Phase mixing of chaotic orbits
Transitions between regular and chaotic behavior
Findings
DISCUSSION AND CONCLUSIONS

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