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Spatial collinear restricted four-body problem with repulsive Manev potential

Autor
Barrabés, E.; Cors, J.; Vidal, C.
Tipus d'activitat
Article en revista
Revista
Celestial mechanics and dynamical astronomy
Data de publicació
2017-09-01
Volum
129
Número
1-2
Pàgina inicial
153
Pàgina final
176
DOI
https://doi.org/10.1007/s10569-017-9771-y Obrir en finestra nova
Repositori
http://hdl.handle.net/2117/108113 Obrir en finestra nova
URL
https://link.springer.com/article/10.1007%2Fs10569-017-9771-y Obrir en finestra nova
Resum
The final publication is available at Springer via http://dx.doi.org/10.1007/s10569-017-9771-y 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/r2-1/r+e/r2), e>0e>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 ßß,...
Citació
Barrabés, E., Cors, J., Vidal, C. Spatial collinear restricted four-body problem with repulsive Manev potential. "Celestial mechanics and dynamical astronomy", 1 Setembre 2017, vol. 129, núm. 1-2, p. 153-176.
Paraules clau
Equilibrium points, Repulsive Manev potential, Restricted four-body problem, Stability

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