dc.contributor.author |
Tsitouras, Ch |
en |
dc.date.accessioned |
2014-03-01T01:14:22Z |
|
dc.date.available |
2014-03-01T01:14:22Z |
|
dc.date.issued |
1999 |
en |
dc.identifier.issn |
0923-2958 |
en |
dc.identifier.uri |
https://dspace.lib.ntua.gr/xmlui/handle/123456789/13021 |
|
dc.subject |
Hamiltonian problems |
en |
dc.subject |
Runge-Kutta-Nyström methods |
en |
dc.subject |
Symplectic methods |
en |
dc.subject.classification |
Astronomy & Astrophysics |
en |
dc.subject.classification |
Mathematics, Interdisciplinary Applications |
en |
dc.subject.other |
INTEGRATORS |
en |
dc.subject.other |
SYSTEMS |
en |
dc.title |
A tenth order symplectic Runge-Kutta-Nyström method |
en |
heal.type |
journalArticle |
en |
heal.identifier.primary |
10.1023/A:1008346516048 |
en |
heal.identifier.secondary |
http://dx.doi.org/10.1023/A:1008346516048 |
en |
heal.language |
English |
en |
heal.publicationDate |
1999 |
en |
heal.abstract |
A tenth order explicit symmetric and in consequence symplectic Runge-Kutta-Nyström method is presented here. We derive the order conditions needed and solve them for the parameters of the method. Numerical results indicate the superiority of the new method compared to the other high order symplectic methods appeared in the literature until now. |
en |
heal.publisher |
KLUWER ACADEMIC PUBL |
en |
heal.journalName |
Celestial Mechanics and Dynamical Astronomy |
en |
dc.identifier.doi |
10.1023/A:1008346516048 |
en |
dc.identifier.isi |
ISI:000083815000001 |
en |
dc.identifier.volume |
74 |
en |
dc.identifier.issue |
4 |
en |
dc.identifier.spage |
223 |
en |
dc.identifier.epage |
230 |
en |