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 ), e > 0 , is applied to the central mass. We investigate the relat...

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Vydané v:Celestial mechanics and dynamical astronomy Ročník 129; číslo 1-2; s. 153 - 176
Hlavní autori: Barrabés, Esther, Cors, Josep M., Vidal, Claudio
Médium: Journal Article Publikácia
Jazyk:English
Vydavateľské údaje: Dordrecht Springer Netherlands 01.09.2017
Springer Nature B.V
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ISSN:0923-2958, 1572-9478
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Shrnutí: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 ), 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.
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ISSN:0923-2958
1572-9478
DOI:10.1007/s10569-017-9771-y