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High precision symplectic integrators for the Solar System

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High precision symplectic integrators for the Solar System

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Nombre: Ariadna;Jaques;Blanes ...
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dc.contributor.author Farrés, Ariadna es_ES
dc.contributor.author Laskar, Jacques es_ES
dc.contributor.author Blanes Zamora, Sergio es_ES
dc.contributor.author Casas Perez, Fernando es_ES
dc.contributor.author Makazaga, Joseba es_ES
dc.contributor.author Murua, Ander es_ES
dc.date.accessioned 2014-06-10T15:50:29Z
dc.date.issued 2013-06
dc.identifier.issn 0923-2958
dc.identifier.uri http://hdl.handle.net/10251/38065
dc.description.abstract Using 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 comparisons 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. (2013). © 2013 Springer Science+Business Media Dordrecht. es_ES
dc.description.sponsorship This work was supported by GTSNext project. The work of SB, FC, JM and AM has been partially supported by Ministerio de Ciencia e Innovacion (Spain) under project MTM2010-18246-C03 (co-financed by FEDER Funds of the European Union). en_EN
dc.language Inglés es_ES
dc.publisher Springer Verlag (Germany) es_ES
dc.relation.ispartof Celestial Mechanics and Dynamical Astronomy es_ES
dc.rights Reserva de todos los derechos es_ES
dc.subject Hamiltonian systems es_ES
dc.subject Heliocentric coordinates es_ES
dc.subject Jacobi coordinates es_ES
dc.subject Planetary motion es_ES
dc.subject Splitting sympletic methods es_ES
dc.subject Symplectic integrators es_ES
dc.subject.classification MATEMATICA APLICADA es_ES
dc.title High precision symplectic integrators for the Solar System es_ES
dc.type Artículo es_ES
dc.embargo.lift 10000-01-01
dc.embargo.terms forever es_ES
dc.identifier.doi 10.1007/s10569-013-9479-6
dc.relation.projectID info:eu-repo/grantAgreement/MICINN//MTM2010-18246-C03-02/ES/METODOS DE ESCISION Y COMPOSICION EN INTEGRACION NUMERICA GEOMETRICA/
dc.relation.projectID info:eu-repo/grantAgreement/EC/FP7/215458/EU/Towards the next generation of the Geological Time Scale for the last 100 million years – the European contribution to EARTHTIME/
dc.relation.projectID info:eu-repo/grantAgreement/MICINN//MTM2010-18246-C03-03/ES/TECNICAS ALGEBRAICAS EN INTEGRACION GEOMETRICA/
dc.rights.accessRights Abierto es_ES
dc.contributor.affiliation Universitat Politècnica de València. Departamento de Matemática Aplicada - Departament de Matemàtica Aplicada es_ES
dc.description.bibliographicCitation Farrés, A.; Laskar, J.; Blanes Zamora, S.; Casas Perez, F.; Makazaga, J.; Murua, A. (2013). High precision symplectic integrators for the Solar System. Celestial Mechanics and Dynamical Astronomy. 116:141-174. https://doi.org/10.1007/s10569-013-9479-6 es_ES
dc.description.accrualMethod S es_ES
dc.relation.publisherversion http://dx.doi.org/10.1007/s10569-013-9479-6 es_ES
dc.description.upvformatpinicio 141 es_ES
dc.description.upvformatpfin 174 es_ES
dc.type.version info:eu-repo/semantics/publishedVersion es_ES
dc.description.volume 116 es_ES
dc.relation.senia 255338
dc.contributor.funder European Regional Development Fund
dc.contributor.funder Ministerio de Ciencia e Innovación
dc.contributor.funder European Commission
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