dc.contributor.author | Φαμέλης, Ιωάννης Θ. | el |
dc.date.accessioned | 2015-02-14T11:21:49Z | |
dc.date.issued | 2015-02-14 | |
dc.identifier.uri | http://hdl.handle.net/11400/6226 | |
dc.rights | Αναφορά Δημιουργού-Μη Εμπορική Χρήση-Όχι Παράγωγα Έργα 3.0 Ηνωμένες Πολιτείες | * |
dc.rights.uri | http://creativecommons.org/licenses/by-nc-nd/3.0/us/ | * |
dc.source | http://www.worldscientific.com/ | en |
dc.subject | Kepler problem | |
dc.subject | Neural networks | |
dc.subject | Πρόβλημα κέπλερ | |
dc.subject | Νευρωνικό δίκτυο | |
dc.title | Neural network based derivation of efficient high order runge-kutta-nystrom pairs for the integration of orbits | en |
heal.type | journalArticle | |
heal.classification | Physics | |
heal.classification | Mathematical physics | |
heal.classification | Φυσική | |
heal.classification | Μαθηματική φυσική | |
heal.classificationURI | http://skos.um.es/unescothes/C02994 | |
heal.classificationURI | http://id.loc.gov/authorities/subjects/sh85082129 | |
heal.classificationURI | **N/A**-Φυσική | |
heal.classificationURI | **N/A**-Μαθηματική φυσική | |
heal.keywordURI | http://zbw.eu/stw/descriptor/19808-6 | |
heal.identifier.secondary | DOI: 10.1142/S0129183111016919 | |
heal.dateAvailable | 10000-01-01 | |
heal.language | en | |
heal.access | forever | |
heal.recordProvider | Τ.Ε.Ι. Αθήνας. Σχολή Τεχνολογικών Εφαρμογών. Τμήμα Ηλεκτρονικών Μηχανικών Τ.Ε. | el |
heal.publicationDate | 2011 | |
heal.bibliographicCitation | Famelis, I. 9December 2011). Neural network based derivation of efficient high order runge-kutta-nystrom pairs for the integration of orbits. International Journal of Modern Physics C. 22(12). pp. 469–473. World Scientific Publishing Company: 2011. | en |
heal.abstract | We use Neural Network approach to derive a Runge{Kutta{Nystr om pair of orders 8(6) for the integration of orbital problems. We use an di erential evolution optimization technique to choose the free parameters of the method's family. We train the method to perform optimally in a speci c test orbit from the Kepler problem for a speci c tolerance. Our measure of e ciency involves the global error and the number of function evaluations. Other orbital problems are solved to test the new pair. | en |
heal.publisher | World Scienti c Publishing Company | en |
heal.journalName | International Journal of Modern Physics C | en |
heal.journalType | peer-reviewed | |
heal.fullTextAvailability | true |
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