Physics
Scientific paper
Feb 1981
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981cemec..23..109d&link_type=abstract
Celestial Mechanics, vol. 23, Feb. 1981, p. 109-117.
Physics
3
Approximation, Charged Particles, Equations Of Motion, Relativistic Particles, Three Body Problem, Euler-Lagrange Equation, Hamiltonian Functions, Newton Theory
Scientific paper
The motions of three charged particles under non-Newtonian assumptions
are shown to be expressed by differential equations of order up to
1/c-squared in relative coordinates. These equations are then shown to
satisfy Lagrange's special solutions, i.e., the equilateral triangle and
the collinear ones.
Antonacopoulos Gr.
Dionysiou Demetrious D.
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