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Barrabés Vera, Esther
Cors i Iglesias, Josep M. Vidal, Claudio |
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2020 February 15 | |
We outline some aspects of the dynamics of an infinitesimalmass 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), 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 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 | |
http://hdl.handle.net/2072/372843 | |
eng | |
Springer Verlag | |
Tots els drets reservats | |
Bifurcació, Teoria de la
Bifurcation theory Estabilitat Stability Mecà nica celest Celestial mechanics Dinà mica estel·lar Stellar dynamics Sistemes dinà mics diferenciables Differentiable dynamical systems |
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Spatial collinear restricted four-body problem with repulsive Manev potential | |
info:eu-repo/semantics/article | |
Recercat |