Exploration on initial structures of extrasolar protoplanets via new explicit RKAHeM(4,4) method

In this paper, a newly proposed embedded Runge–Kutta fourth order with four stages arithmetic Heronian mean method is employed and verified in determining the distribution of thermodynamic variables inside the extra-solar protoplanets formed through gravitational instability at their initial stag...

Full description

Bibliographic Details
Main Authors: Paul, Gour Chandra, SenthilKumar, Sukumar
Format: Article
Published: Elsevier 2015
Subjects:
Online Access:http://eprints.usm.my/39077/
_version_ 1848878645591932928
author Paul, Gour Chandra
SenthilKumar, Sukumar
author_facet Paul, Gour Chandra
SenthilKumar, Sukumar
author_sort Paul, Gour Chandra
building USM Institutional Repository
collection Online Access
description In this paper, a newly proposed embedded Runge–Kutta fourth order with four stages arithmetic Heronian mean method is employed and verified in determining the distribution of thermodynamic variables inside the extra-solar protoplanets formed through gravitational instability at their initial stages. In specific, the case of conduction–radiation is considered regarding the transference of heat inside the protoplanets. A general brief theoretical framework for the proposed numerical method is stated in addition to pseudo code followed by error estimation description. The results based on newly proposed explicit RKAHeM(4,4) method are found to be optimal and efficient in comparison with the ones obtained with classical fourth order Runge–Kutta method.
first_indexed 2025-11-15T17:34:38Z
format Article
id usm-39077
institution Universiti Sains Malaysia
institution_category Local University
last_indexed 2025-11-15T17:34:38Z
publishDate 2015
publisher Elsevier
recordtype eprints
repository_type Digital Repository
spelling usm-390772018-02-21T06:14:50Z http://eprints.usm.my/39077/ Exploration on initial structures of extrasolar protoplanets via new explicit RKAHeM(4,4) method Paul, Gour Chandra SenthilKumar, Sukumar QA1-939 Mathematics In this paper, a newly proposed embedded Runge–Kutta fourth order with four stages arithmetic Heronian mean method is employed and verified in determining the distribution of thermodynamic variables inside the extra-solar protoplanets formed through gravitational instability at their initial stages. In specific, the case of conduction–radiation is considered regarding the transference of heat inside the protoplanets. A general brief theoretical framework for the proposed numerical method is stated in addition to pseudo code followed by error estimation description. The results based on newly proposed explicit RKAHeM(4,4) method are found to be optimal and efficient in comparison with the ones obtained with classical fourth order Runge–Kutta method. Elsevier 2015-06 Article PeerReviewed Paul, Gour Chandra and SenthilKumar, Sukumar (2015) Exploration on initial structures of extrasolar protoplanets via new explicit RKAHeM(4,4) method. Egyptian Journal of Remote Sensing and Space Sciences, 18 (1). pp. 1-8. ISSN 1110-9823 https://doi.org/10.1016/j.ejrs.2015.03.004
spellingShingle QA1-939 Mathematics
Paul, Gour Chandra
SenthilKumar, Sukumar
Exploration on initial structures of extrasolar protoplanets via new explicit RKAHeM(4,4) method
title Exploration on initial structures of extrasolar protoplanets via new explicit RKAHeM(4,4) method
title_full Exploration on initial structures of extrasolar protoplanets via new explicit RKAHeM(4,4) method
title_fullStr Exploration on initial structures of extrasolar protoplanets via new explicit RKAHeM(4,4) method
title_full_unstemmed Exploration on initial structures of extrasolar protoplanets via new explicit RKAHeM(4,4) method
title_short Exploration on initial structures of extrasolar protoplanets via new explicit RKAHeM(4,4) method
title_sort exploration on initial structures of extrasolar protoplanets via new explicit rkahem(4,4) method
topic QA1-939 Mathematics
url http://eprints.usm.my/39077/
http://eprints.usm.my/39077/