2022
DOI: 10.3390/fractalfract6060343
|View full text |Cite
|
Sign up to set email alerts
|

Variable Step Hybrid Block Method for the Approximation of Kepler Problem

Abstract: In this article, a variable step size strategy is adopted in formulating a new variable step hybrid block method (VSHBM) for the solution of the Kepler problem, which is known to be a rigid and stiff differential equation. To derive the VSHBM, the step size ratio r is left the same, halved, or doubled in order to optimize the total number of steps, minimize the number of formulae stored in the code, and ensure that the method is zero-stable. The method is formulated by integrating the Lagrange polynomial with … Show more

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
2
1
1
1

Citation Types

0
16
0

Year Published

2022
2022
2024
2024

Publication Types

Select...
8

Relationship

3
5

Authors

Journals

citations
Cited by 23 publications
(16 citation statements)
references
References 33 publications
0
16
0
Order By: Relevance
“…The values r and s denote output and stage values, respectively. Applying Equati (22) to the linear test equation…”
Section: Regions Of Absolute Stability (Ras) Of the Block Hybrid Methodsmentioning
confidence: 99%
See 1 more Smart Citation
“…The values r and s denote output and stage values, respectively. Applying Equati (22) to the linear test equation…”
Section: Regions Of Absolute Stability (Ras) Of the Block Hybrid Methodsmentioning
confidence: 99%
“…Chan and Tsai [16] considered explicit two-derivative RKMs, which are cheaper to calculate with fewer function evaluations than the standard RKMs. Recently, many authors have worked on methods to obtain better approximate solutions to differential equations or on stability properties to improve the accuracy and efficiency of solution of differential equations (see, for example, [17][18][19][20][21][22][23][24]).…”
Section: Introductionmentioning
confidence: 99%
“…1 241.0492 T (1) 181.4473 T (4) 1 267.6401 T (4) 2 206.5321 T (4) 3 181.4576 T (5) 1 267.6965 T (5) 2 206.5532 T (5) 3 181.4663 T (6) 1 267.1691 T (6) 2 206.3557 T (6) 3 181.3844 T (7) 1 267.6403 T (7) 2 206.5322 T (7) 3 181.4567 T (8) 1 267.4689 T (8) 2 206.468 T (8) 3 181.431 T (9) 1 267.7158 T (9) 2 206.5604 T (9) 3 181.4693 T (10) 1 266.8310 T (10) 2 206.2289 T (10) 3 181.3318 171.5264 T (5) 1 259.3661 T (5) 2 210.6753 T (5) 3 171.5099 T (6) 1…”
Section: Simulation Studymentioning
confidence: 99%
“…Many other researchers have also signifcantly contributed to estimating the fnite population variance. Sunday et al [6] adopted a variable step hybrid block method for the approximation of Kepler Problem by integrating the Lagrange polynomial with limits of integration selected at special points. Juraev et al [7,8] used regularization formula and matrix factorization for explicit form of the approximate solutions of the Cauchy Problem.…”
Section: Introductionmentioning
confidence: 99%
“…Furthermore, Figures 4, 5 and 6 respectively depict the trajectories in the phase plane flow using proposed BHA, BHA developed by [2] and the exact flow N = 160. For more details on Kepler equations, see [29][30][31][32][33][34][35].…”
Section: Numerical Examplesmentioning
confidence: 99%