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 |
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| Hlavní autori: | , , |
| Médium: | Journal Article Publikácia |
| Jazyk: | English |
| Vydavateľské údaje: |
Dordrecht
Springer Netherlands
01.09.2017
Springer Nature B.V |
| Predmet: | |
| ISSN: | 0923-2958, 1572-9478 |
| On-line prístup: | Získať plný text |
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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. |
|---|---|
| Bibliografia: | ObjectType-Article-1 SourceType-Scholarly Journals-1 ObjectType-Feature-2 content type line 14 |
| ISSN: | 0923-2958 1572-9478 |
| DOI: | 10.1007/s10569-017-9771-y |