The two rigid body interaction using angular momentum theory formulae-Reference-Cited by-同舟云学术

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The two rigid body interaction using angular momentum theory formulae

Published:2017-01-31 Issue:2-3 Volume:128 Page:261-273
ISSN:0923-2958
Container-title:Celestial Mechanics and Dynamical Astronomy
language:en
Short-container-title:Celest Mech Dyn Astr

Author:

Boué Gwenaël^ORCID

Funder

Université Pierre et Marie Curie

Observatoire de Paris

PSL Research University

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics,Applied Mathematics,Computational Mathematics,Mathematical Physics,Modelling and Simulation

Link

http://link.springer.com/article/10.1007/s10569-017-9751-2/fulltext.html

Reference16 articles.

1. Borderies, N.: Mutual gravitational potential of N solid bodies. Celest. Mech. 18, 295–307 (1978). doi: 10.1007/BF01230170

2. Boué, G., Correia, A.C.M., Laskar, J.: Complete spin and orbital evolution of close-in bodies using a Maxwell viscoelastic rheology. Celest. Mech. Dyn. Astron. 126(1), 31–60 (2016). doi: 10.1007/s10569-016-9708-x

3. Compère, A., Lemaître, A.: The two-body interaction potential in the STF tensor formalism: an application to binary asteroids. Celest. Mech. Dyn. Astron. 119, 313–330 (2014). doi: 10.1007/s10569-014-9568-1

4. Fahnestock, E.G., Scheeres, D.J.: Simulation of the full two rigid body problem using polyhedral mutual potential and potential derivatives approach. Celest. Mech. Dyn. Astron. 96, 317–339 (2006). doi: 10.1007/s10569-006-9045-6

5. Gimbutas, Z., Greengard, L.: A fast and stable method for rotating spherical harmonic expansions. J. Comput. Phys. 228, 5621–5627 (2009)

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