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dc.contributor.authorMarco Castillo, Francisco José
dc.contributor.authorMartínez Usó, María José
dc.date.accessioned2012-05-28T14:36:47Z
dc.date.available2012-05-28T14:36:47Z
dc.date.issued2008
dc.identifierhttp://dx.doi.org/10.1016/j.pss.2008.02.028
dc.identifier.citationPlanetary and Space Science, 56, 14, p. 1869-1873
dc.identifier.issn320633
dc.identifier.urihttp://hdl.handle.net/10234/39016
dc.description.abstractThe numerical integration of equations of motion necessarily implies the presence of errors that depend on initial conditions as well as the different physical parameters under consideration. More particularly, dumping or dissipative terms can appear and it is especially interesting to determine its causes. The equivalent differential equation method may allow the errors from a certain numerical scheme to be analyzed and, together with other considerations, can help us to eliminate or reduce them. © 2008 Elsevier Ltd. All rights reserved.
dc.language.isoeng
dc.publisherElsevier
dc.rights.urihttp://rightsstatements.org/vocab/CNE/1.0/*
dc.subjectHarmonical oscillator
dc.subjectKepler problem
dc.subjectModified equations
dc.subjectRunge-Lenz vector
dc.subjectSymplectic integration method
dc.titleIntegration rules from the equivalent differential equation method applied to equations of motion
dc.typeinfo:eu-repo/semantics/article
dc.identifier.doihttp://dx.doi.org/10.1016/j.pss.2008.02.028
dc.rights.accessRightsinfo:eu-repo/semantics/restrictedAccess
dc.type.versioninfo:eu-repo/semantics/publishedVersion


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