2012
DOI: 10.1140/epjp/i2012-12004-4
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Hamiltonian structure of classical N-body systems of finite-size particles subject to EM interactions

Abstract: An open issue in classical relativistic mechanics is the consistent treatment of the dynamics of classical N -body systems of mutually-interacting particles. This refers, in particular, to charged particles subject to EM interactions, including both binary and self interactions (EM-interacting N -body systems). The correct solution to the question represents an overriding prerequisite for the consistency between classical and quantum mechanics. In this paper it is shown that such a description can be consisten… Show more

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Cited by 20 publications
(17 citation statements)
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“…72, which permits to establish the adiabatic conservation properties of the relativistic particle magnetic moment, when radiation-reaction effects are ignored. [6][7][8][9][10][11] In the present derivation of gyrokinetics, charged particles are treated as point-like and are assumed to belong to a magnetized plasma, in the sense defined above. For definiteness, the background metric tensor g l r ð Þ is considered a prescribed function of the position 4-vector r l .…”
Section: Non-perturbative Gk Theorymentioning
confidence: 99%
See 1 more Smart Citation
“…72, which permits to establish the adiabatic conservation properties of the relativistic particle magnetic moment, when radiation-reaction effects are ignored. [6][7][8][9][10][11] In the present derivation of gyrokinetics, charged particles are treated as point-like and are assumed to belong to a magnetized plasma, in the sense defined above. For definiteness, the background metric tensor g l r ð Þ is considered a prescribed function of the position 4-vector r l .…”
Section: Non-perturbative Gk Theorymentioning
confidence: 99%
“…[35][36][37][38][39][40][41][42] A qualitative feature of astrophysical magnetized plasmas is related to the occurrence of kinetic plasma regimes, which persist for long times (with respect to the observer and/or plasma characteristic times), despite the presence of macroscopic time-varying phenomena of various origin, such as flows, non-uniform gravitational/EM fields, and EM radiation, 43 possibly including that arising from singleparticle radiation-reaction processes. [4][5][6][7][8][9][10][11] It is argued that, for collisionless plasmas, these states might actually correspond-at least locally and in a suitable asymptotic senseto some kind of kinetic equilibrium, which characterizes the species KDFs. This is realized when the latter distributions are all assumed to be functions only of the single-particle adiabatic invariants.…”
Section: Introductionmentioning
confidence: 99%
“…Ignoring possible weakly dissipative effects (Coulomb collisions and turbulence) and EM radiation effects, [36][37][38][39][40] we shall assume that the KDF and the EM fields associated with the plasma obey the system of Vlasov-Maxwell equations, with Maxwell's equations being considered in the quasistatic approximation. For definiteness, we shall consider here a plasma consisting of s-species of charged particles which are characterized by proper mass M s and total charge Z s e. In particular, given a generic KDF f ¼ f ðr; v; tÞ defined in the phase-space C ¼ C r  C v , with C r and C v being the configuration and velocity space respectively, the Vlasov equation determines the dynamical evolution of f and is given by…”
Section: Basic Assumptions and Definitionsmentioning
confidence: 99%
“…Classical theory was left to (one might say was allowed to) study technically feasible models (charged spheres, capacitors, etc.). Recent researches in this field [2] [3] [4] are worth noticing.…”
Section: Introductionmentioning
confidence: 99%