DUGiDocsSpatial collinear restricted four-body problem with repulsive Manev potential
dc.contributor.author
dc.date.accessioned
2017-12-15T12:06:14Z
dc.date.available
2021-04-07T08:03:00Z
dc.date.issued
2017-09-01
dc.identifier.issn
0923-2958
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dc.description.abstract
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
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24 p.
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application/pdf
dc.language.iso
eng
dc.publisher
Springer Verlag
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Versió postprint del document publicat a: https://doi.org/10.1007/s10569-017-9771-y
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© Celestial Mechanics & Dynamical Astronomy, 2017, vol. 129 , núm. 1-2, p. 153-176
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Articles publicats (D-IMAE)
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Tots els drets reservats
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Barrabés Vera, Esther Cors i Iglesias, Josep M. Vidal, Claudio 2017 Spatial collinear restricted four-body problem with repulsive Manev potential Celestial Mechanics & Dynamical Astronomy 129 1-2 153 176
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dc.title
Spatial collinear restricted four-body problem with repulsive Manev potential
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info:eu-repo/semantics/article
dc.rights.accessRights
info:eu-repo/semantics/openAccess
dc.embargo.terms
2018-09-01T00:00:00Z
dc.date.embargoEndDate
info:eu-repo/date/embargoEnd/2018-09-01
dc.type.version
info:eu-repo/semantics/acceptedVersion
dc.identifier.doi
dc.identifier.idgrec
027434
dc.identifier.eissn
1572-9478