Ítem
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Barrabés Vera, Esther
Cors Iglesias, Josep Maria Vidal, Claudio |
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| 1 setembre 2017 | |
| 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 | |
| application/pdf | |
| http://hdl.handle.net/10256/14759 | |
| eng | |
| Springer | |
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info:eu-repo/semantics/altIdentifier/doi/10.1007/s10569-017-9771-y info:eu-repo/semantics/altIdentifier/issn/0923-2958 info:eu-repo/semantics/altIdentifier/eissn/1572-9478 |
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| Tots els drets reservats | |
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Bifurcació, Teoria de la
Bifurcation theory Estabilitat Stability Mecànica celest Celestial mechanics Dinàmica estel·lar Stellar dynamics Sistemes dinàmics diferenciables Differentiable dynamical systems |
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| Spatial collinear restricted four-body problem with repulsive Manev potential | |
| info:eu-repo/semantics/article | |
| DUGiDocs |
