Motion Of Bodies And Its Stability In The General Relativity Theory

Details Motion Of Bodies And Its Stability In The General Relativity Theory Motion Of Bodies And Its Stability In The General Relativity Theory

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1205..148r&link_type=abstract

THE SUN, THE STARS, THE UNIVERSE AND GENERAL RELATIVITY: International Conference in Honor of Ya.B. Zeldovich's 95th Anniversary

Astronomy and Astrophysics

Astronomy

General Relativity, Conservation Laws, Newton Method, Rotational States, Fundamental Problems And General Formalism, Nonlinear And Dynamical Symmetries, Newtonian Mechanics, Velocity, Acceleration, And Rotation

Scientific paper

This paper reviews the works by the Belarusian school investigators on relativistic motion and its stability for a system of bodies, each of which may have its own rotation, charge, and magnetic field of the dipole type. The corresponding Lagrangian and conservation laws are derived, several secular effects are predicted. For motion of bodies in the medium the secular effect of the periastron reverse shift is predicted as compared to the Mercury perihelion shift. The cause for the Pioneer anomaly is explained.

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