Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
1780548 | NRIAG Journal of Astronomy and Geophysics | 2016 | 8 Pages |
Abstract
Implementation of a novel embedded Runge–Kutta fourth order four stage arithmetic root mean square technique to determine initial configurations of extra-solar protoplanets formed by gravitational instability is the main goal of this present paper. A general mathematical framework for the introduced numerical technique is described in addition to error estimation description. It is noticed that the numerical outputs through the employed novel RKARMS(4,4) method are found to be more effective and efficient in comparison with the results obtained by the classical Runge–Kutta technique.
Keywords
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Astronomy and Astrophysics
Authors
Gour Chandra Paul, Sukumar Senthilkumar,