Lagrangian and Hamiltonian Formalisms for Relativistic Mechanics with Lorentz-Invariant Evolution Parameters in 1 + 1 Dimensions

Author:

Akintsov Nikolai S.12ORCID,Nevecheria Artem P.3,Kopytov Gennadii F.4,Yang Yongjie5ORCID

Affiliation:

1. Research Center for Intelligent Information Technology, Nantong University, Nantong 226019, China

2. College of Physics and Optoelectronic Engineering, Ocean University of China, Qingdao 266100, China

3. Department of Mathematical and Computer Methods, Kuban State University, Krasnodar 350040, Russia

4. Department of Physics, Moscow State University of Technology and Management Named after K.G. Razumovsky, Moscow 109004, Russia

5. School of Information Science and Technology, Nantong University, Nantong 226019, China

Abstract

This article presents alternative Hamiltonian and Lagrangian formalisms for relativistic mechanics using proper time and proper Lagrangian coordinates in 1 + 1 dimensions as parameters of evolution. The Lagrangian and Hamiltonian formalisms for a hypothetical particle with and without charge are considered based on the relativistic equation for the dynamics and integrals of particle motion. A relativistic invariant law for the conservation of energy and momentum in the Lorentz representation is given. To select various generalized coordinates and momenta, it is possible to modify the Lagrange equations of the second kind due to the relativistic laws of conservation of energy and momentum. An action function is obtained with an explicit dependence on the velocity of the relativistic particles. The angular integral of the particle motion is derived from Hamiltonian mechanics, and the displacement Hamiltonian is obtained from the Hamilton–Jacobi equation. The angular integral of the particle motion θ is an invariant form of the conservation law. It appears only at relativistic intensities and is constant only in a specific case. The Hamilton–Jacobi–Lagrange equation is derived from the Hamilton–Jacobi equation and the Lagrange equation of the second kind. Using relativistic Hamiltonian mechanics, the Euler–Hamilton equation is obtained by expressing the energy balance through the angular integral of the particle motion θ. The given conservation laws show that the angular integral of the particle motion reflects the relativistic Doppler effect for particles in 1 + 1 dimensions. The connection between the integrals of the particle motion and the doubly special theory of relativity is shown. As an example of the applicability of the proposed invariant method, analyses of the motion of relativistic particles in circularly polarized, monochromatic, spatially modulated electromagnetic plane waves and plane laser pulses are given, and comparisons are made with calculations based on the Landau and Lifshitz method. To allow for the analysis of the oscillation of a particle in various fields, a phase-plane method is presented.

Funder

Nantong Science and Technology Plan Project

Key Research and Development Program of Jiangsu Province of China

National Natural Science Foundation of Jiangsu Province of China

Natural Science Research Project of Jiangsu Provincial Institutions of Higher Education

Publisher

MDPI AG

Subject

Physics and Astronomy (miscellaneous),General Mathematics,Chemistry (miscellaneous),Computer Science (miscellaneous)

Reference46 articles.

1. Goldstein, H. (1951). Classical Mechanics, Addison-Wesley Reading. [3rd ed.].

2. Jackson, J.D. (1962). Classical Electrodynamics, Wiley.

3. Barut, A.O. (1964). Electrodynamics and Classical Theory of Fields and Particles, Macmollan. Available online: https://inspirehep.net/literature/163207.

4. Doughty, N.A. (1990). Lagrangian Interaction, CRC Press.

5. Remarque à propos de la création de paires de particules en théorie de relativité;Stueckelberg;Helv. Phys. Acta,1941

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