Abstract
We use a formulation of the N-body problem in spaces of constant Gaussian curvature, \({\kappa }\in \mathbb {R}\), as widely used by A. Borisov, F. Diacu and their coworkers. We consider the restricted three-body problem in \(\mathbb {S}^2\) with arbitrary \({\kappa }>0\) (resp. \(\mathbb {H}^2\) with arbitrary \({\kappa }<0\)) in a formulation also valid for the case \({\kappa }=0\). For concreteness when \({\kappa }>0\) we restrict the study to the case of the three bodies at the upper hemisphere, to be denoted as \(\mathbb {S}^2_+\). The main goal is to obtain the totality of relative equilibria as depending on the parameters \({\kappa }\) and the mass ratio \(\mu \). Several general results concerning relative equilibria and its stability properties are proved analytically. The study is completed numerically using continuation from the \({\kappa }=0\) case and from other limit cases. In particular both bifurcations and spectral stability are also studied. The \(\mathbb {H}^2\) case is similar, in some sense, to the planar one, but in the \(\mathbb {S}^2_+\) case many differences have been found. Some surprising phenomena, like the coexistence of many triangular-like solutions for some values \(({\kappa },\mu )\) and many stability changes will be discussed.
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Acknowledgements
This research has been partly supported by grant 2014 SGR 1145 (Catalonia) and grant MTM2013-41168-P (Spain). The authors are indebted to A. Borisov, F. Diacu and E. Pérez-Chavela for helpful discussions, to the referee for helpful suggestions and to the organizers of the conference on Global Dynamics in Hamiltonian Systems for allowing them to present the results on this event.
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Appendix
Appendix
In this Appendix we give reduced formulas for the functions which appear in the equations of the restricted problem.
Let us consider the functions \( \rho _{ij}, f_{ij}, g_{ij} \) defined in (5). It is easy to check that they can be written as
where \( E_i=\sqrt{1- {\kappa }(\xi _i^2 + \eta _i^2)}. \)
If \( \mathbf{U}_1=(\xi _1,\eta _1)^T=(r_1,0)^T,\) \(\mathbf{U}_2=(\xi _2,\eta _2)^T=(-r_2,0)^T, \) \( \mathbf{U}_3= (\xi _3,\eta _3)^T = (x,y)^T, \) then
where \( E_j= \sqrt{1-{\kappa }r_j^2}, \) \( j=1,2\), \(E_3 = \sqrt{1-{\kappa }(x^2 + y^2)} \). Then one has
and, furthermore
Lemma 7.1
Assume \({\kappa }>0\) and \(r_1,r_2\) fixed. Then \( f_{13} \) and \( f_{23} \) are convex functions in \( C_{{\kappa }}:=\{ (x,y)\in \mathbb {R}^2 \,|\,{\kappa }(x^2+y^2) < 1 \} \), such that for any \( (x,y) \in C_{{\kappa }} \)
Moreover \(f_{13}=0 \) along the curve \( \gamma _{13} = \{ (x,y) | x \le 0, {\kappa }(x^2 + E_1^2 y^2 ) = E_1^2 \} \), and \( f_{23}=0 \) on the curve \( \gamma _{23} = \{ (x,y) | x \ge 0, {\kappa }(x^2 + E_2^2 y^2 ) = E_2^2 \} \).
If \({\kappa }<0\), then \(f_{13}>0\) and \(f_{23}>0\) at any point.
Proof
Using
it follows that the Hessian of \(f_{13} \) is negative definite in \(C_{{\kappa }}\). Similar formulas hold for \(f_{23}\) by replacing \(E_1\) by \(E_2\). The maximum for \(f_{13}\) is equal to 1 and it is attained at the point \((x,y)=(r_1,0)\) and the minimum is achieved at the point \((x,y)= (-1/\sqrt{{\kappa }},0).\) Similar for \(f_{23}\). The case \({\kappa }<0\) is obvious from (3). \(\square \)
Let us consider the functions \( {\hat{F}} \), \( {\hat{G}} \) introduced in Sect. 6. We compute the partial derivatives
Lemma 7.2
For any real \({\kappa }\), the following identity holds
Proof
From (59) it follows
Note that from (55), \( \Delta _{13}^{-5/2} (y^2 + S_1^2) = \Delta _{13}^{-3/2}= g_{13} \) and \( \Delta _{23}^{-5/2} (y^2 + S_2^2) = g_{23} \). Using (56) to write
one can easily obtain (60) after some cancellations. \(\square \)
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Martínez, R., Simó, C. Relative equilibria of the restricted three-body problem in curved spaces. Celest Mech Dyn Astr 128, 221–259 (2017). https://doi.org/10.1007/s10569-016-9750-8
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DOI: https://doi.org/10.1007/s10569-016-9750-8
Keywords
- N-body problem in curved spaces
- The restricted three body problem in curved spaces: relative equilibria
- Totality of solutions
- Bifurcations
- Changes of the spectral stability