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Article: A multiple time step symplectic algorithm for integrating close encounters
Title | A multiple time step symplectic algorithm for integrating close encounters |
---|---|
Authors | |
Keywords | Celestial Mechanics, Stellar Dynamics Methods: Numerical Planetary Systems Solar System: General |
Issue Date | 1998 |
Publisher | University of Chicago Press. The Journal's web site is located at http://www.journals.uchicago.edu/AJ/home.html |
Citation | Astronomical Journal, 1998, v. 116 n. 4, p. 2067-2077 How to Cite? |
Abstract | We present a new symplectic algorithm that has the desirable properties of the sophisticated but highly efficient numerical algorithms known as mixed variable symplectic (MVS) methods and that, in addition, can handle close encounters between objects. This technique is based on a variant of the standard MVS methods, but it handles close encounters by employing a multiple time step technique. When the bodies are well separated, the algorithm has the speed of MVS methods, and whenever two bodies suffer a mutual encounter, the time step for the relevant bodies is recursively subdivided to whatever level is required. We demonstrate the power of this method using several tests of the technique. We believe that this algorithm will be a valuable tool for the study of planetesimal dynamics and planet formation. |
Persistent Identifier | http://hdl.handle.net/10722/150930 |
ISSN | 2023 Impact Factor: 5.1 2023 SCImago Journal Rankings: 1.953 |
ISI Accession Number ID | |
References |
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Duncan, MJ | en_US |
dc.contributor.author | Levison, HF | en_US |
dc.contributor.author | Lee, MH | en_US |
dc.date.accessioned | 2012-06-26T06:15:01Z | - |
dc.date.available | 2012-06-26T06:15:01Z | - |
dc.date.issued | 1998 | en_US |
dc.identifier.citation | Astronomical Journal, 1998, v. 116 n. 4, p. 2067-2077 | en_US |
dc.identifier.issn | 0004-6256 | en_US |
dc.identifier.uri | http://hdl.handle.net/10722/150930 | - |
dc.description.abstract | We present a new symplectic algorithm that has the desirable properties of the sophisticated but highly efficient numerical algorithms known as mixed variable symplectic (MVS) methods and that, in addition, can handle close encounters between objects. This technique is based on a variant of the standard MVS methods, but it handles close encounters by employing a multiple time step technique. When the bodies are well separated, the algorithm has the speed of MVS methods, and whenever two bodies suffer a mutual encounter, the time step for the relevant bodies is recursively subdivided to whatever level is required. We demonstrate the power of this method using several tests of the technique. We believe that this algorithm will be a valuable tool for the study of planetesimal dynamics and planet formation. | en_US |
dc.language | eng | en_US |
dc.publisher | University of Chicago Press. The Journal's web site is located at http://www.journals.uchicago.edu/AJ/home.html | en_US |
dc.relation.ispartof | Astronomical Journal | en_US |
dc.subject | Celestial Mechanics, Stellar Dynamics | en_US |
dc.subject | Methods: Numerical | en_US |
dc.subject | Planetary Systems | en_US |
dc.subject | Solar System: General | en_US |
dc.title | A multiple time step symplectic algorithm for integrating close encounters | en_US |
dc.type | Article | en_US |
dc.identifier.email | Lee, MH:mhlee@hku.hk | en_US |
dc.identifier.authority | Lee, MH=rp00724 | en_US |
dc.description.nature | link_to_subscribed_fulltext | en_US |
dc.identifier.scopus | eid_2-s2.0-0001687417 | en_US |
dc.relation.references | http://www.scopus.com/mlt/select.url?eid=2-s2.0-0001687417&selection=ref&src=s&origin=recordpage | en_US |
dc.identifier.volume | 116 | en_US |
dc.identifier.issue | 4 | en_US |
dc.identifier.spage | 2067 | en_US |
dc.identifier.epage | 2077 | en_US |
dc.identifier.isi | WOS:000076413100052 | - |
dc.publisher.place | United States | en_US |
dc.identifier.scopusauthorid | Duncan, MJ=7201431485 | en_US |
dc.identifier.scopusauthorid | Levison, HF=7103193309 | en_US |
dc.identifier.scopusauthorid | Lee, MH=7409119699 | en_US |
dc.identifier.issnl | 0004-6256 | - |