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dc.contributor.authorFarrés Basiana, Ariadna
dc.contributor.authorLaskar, Jacques
dc.contributor.authorBlanes, Sergio
dc.contributor.authorCasas, Fernando
dc.contributor.authorMakazaga, Joseba
dc.contributor.authorMurua, Ander
dc.date.accessioned2014-02-18T09:05:11Z
dc.date.available2014-02-18T09:05:11Z
dc.date.issued2013-02
dc.identifier.citationFARRÉS, Ariadna, et al. High precision symplectic integrators for the Solar System. Celestial Mechanics and Dynamical Astronomy, 2013, vol. 116, no 2, p. 141-174ca_CA
dc.identifier.issn0923-2958
dc.identifier.issn1572-9478
dc.identifier.urihttp://hdl.handle.net/10234/83769
dc.description.abstractUsing a Newtonian model of the Solar System with all 8 planets, we perform extensive tests on various symplectic integrators of high orders, searching for the best splitting scheme for long term studies in the Solar System. These com- parisons are made in Jacobi and Heliocentric coordinates and the implementation of the algorithms is fully detailed for practical use. We conclude that high order integrators should be privileged, with a preference for the new (10, 6, 4) method of (Blanes et al, 2012)ca_CA
dc.format.extent33 p.ca_CA
dc.format.mimetypeapplication/pdfca_CA
dc.language.isoengca_CA
dc.publisherSpringer Netherlandsca_CA
dc.relation.isFormatOfVersió preprint del document publicat a http://link.springer.com/article/10.1007/s10569-013-9479-6ca_CA
dc.relation.isPartOfCelestial Mechanics and Dynamical Astronomy, 2013, vol. 116, no. 2ca_CA
dc.rights© Springer Science+Business Media Dordrecht 2013ca_CA
dc.subjectsymplectic integratorsca_CA
dc.subjectHamiltonian systemsca_CA
dc.subjectplanetary motionca_CA
dc.titleHigh precision Symplectic Integrators for the Solar Systemca_CA
dc.typeinfo:eu-repo/semantics/articleca_CA
dc.identifier.doihttp://dx.doi.org/10.1007/s10569-013-9479-6
dc.rights.accessRightsinfo:eu-repo/semantics/openAccessca_CA
dc.relation.publisherVersionhttp://link.springer.com/article/10.1007/s10569-013-9479-6ca_CA


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