Spatial collinear restricted four-body problem with repulsive Manev potential

Spatial collinear restricted four-body problem with repulsive Manev potential We outline some aspects of the dynamics of an infinitesimal mass under the Newtonian attraction of three point masses in a symmetric collinear relative equilibria configuration when a repulsive Manev potential ( $$-1/r +e/r^{2}$$ - 1 / r + e / r 2 ), $$e>0$$ e > 0 , is applied to the central mass. We investigate the relative equilibria of the infinitesimal mass and their linear stability as a function of the mass parameter $$\beta $$ β , the ratio of mass of the central body to the mass of one of two remaining bodies, and e. We also prove the nonexistence of binary collisions between the central body and the infinitesimal mass. Celestial Mechanics and Dynamical Astronomy Springer Journals

Spatial collinear restricted four-body problem with repulsive Manev potential

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Springer Netherlands
Copyright © 2017 by Springer Science+Business Media B.V.
Physics; Astrophysics and Astroparticles; Dynamical Systems and Ergodic Theory; Aerospace Technology and Astronautics; Geophysics/Geodesy; Classical Mechanics
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