1974
DOI: 10.1007/bf01809718
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A relativistic analogue of the Kepler problem

Abstract: The Poincar~ invariant system of two point particles with an instantaneous interactionat-a-distance originally proposed by Fokker is studied in the Hamittonian formalism. The interaction, which agrees to first order in the coupling constant with the electromagnetic one obtained from the Lienard-Wiechert fields, is described in an advanced-retarded state space. The first particle moves in the advanced field of the second which in turn is subject to the retarded field of the first. The acceleration terms in the … Show more

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Cited by 15 publications
(8 citation statements)
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“…These models are based on the Fokker-type integrals (5.1) with the Fokker potentials U = U v and U = U s , respectively (see (7.3)). Both scalar and vector models were partly considered earlier (the former in the two-dimensional space-time only) [ 44,45,46,26,20,28,47]. Our results obtained by means of both the Lagrangian and especially the Hamiltonian formulations of these models complete the analysis of their classical dynamics.…”
Section: Vector and Scalar Modelsmentioning
confidence: 58%
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“…These models are based on the Fokker-type integrals (5.1) with the Fokker potentials U = U v and U = U s , respectively (see (7.3)). Both scalar and vector models were partly considered earlier (the former in the two-dimensional space-time only) [ 44,45,46,26,20,28,47]. Our results obtained by means of both the Lagrangian and especially the Hamiltonian formulations of these models complete the analysis of their classical dynamics.…”
Section: Vector and Scalar Modelsmentioning
confidence: 58%
“…where ǫ = ±1. Such a description has been developed within the framework of the predictive relativistic mechanics in a series of papers by Künzle [ 27,28,29]. The idea of this definition of simultaneity was formulated in the classic Van Dam-Wigner's work [ 30].…”
Section: Isotropic Forms Of Dynamicsmentioning
confidence: 99%
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“…Rudd and Hill, 27 and studied in more detail in Ref. 28. For NT the corresponding time-asymmetric Fokker-type action can be taken as the classical base for relativistic confinement model.…”
Section: Equations Of Motion and Fokker-type Action Integralsmentioning
confidence: 99%