Dissipative trigonometrically fitted methods for the numerical solution of orbital problems

Details Dissipative trigonometrically fitted methods for the numerical solution of orbital problems Dissipative trigonometrically fitted methods for the numerical solution of orbital problems

Jan 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004newa....9...59s&link_type=abstract

New Astronomy, Volume 9, Issue 1, p. 59-68.

Astronomy and Astrophysics

Astronomy

3

Methods: Numerical

Scientific paper

In this paper a new approach for the numerical solution of orbital problems is introduced. This approach is based on the dissipative multistep methods (i.e., methods which are not symmetric). We show that the trigonometrical fitting property produces efficient methods of this category. For comparison purposes we use well-known symmetric multistep methods.
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