Solving protoplanetary structure equations using Adomian decomposition method

In this paper, the distribution of thermodynamic variables in the protoplanets formed by gravitational instability in the mass range [Formula: see text] ([Formula: see text] Jupiter mass = [Formula: see text] gm) is investigated in their initial state by solving the structure equations via the Adomi...

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Autores principales: Paul, Gour Chandra, Khatun, Shahinur, Nuruzzaman, Md., Kumar, Dipankar, Ali, Md. Emran, Bilkis, Farjana, Barman, Mrinal Chandra
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Elsevier 2021
Materias:
Research Article
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC8566779/
https://www.ncbi.nlm.nih.gov/pubmed/34761131
http://dx.doi.org/10.1016/j.heliyon.2021.e08213
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author Paul, Gour Chandra
Khatun, Shahinur
Nuruzzaman, Md.
Kumar, Dipankar
Ali, Md. Emran
Bilkis, Farjana
Barman, Mrinal Chandra
author_facet Paul, Gour Chandra
Khatun, Shahinur
Nuruzzaman, Md.
Kumar, Dipankar
Ali, Md. Emran
Bilkis, Farjana
Barman, Mrinal Chandra
author_sort Paul, Gour Chandra
collection PubMed
description In this paper, the distribution of thermodynamic variables in the protoplanets formed by gravitational instability in the mass range [Formula: see text] ([Formula: see text] Jupiter mass = [Formula: see text] gm) is investigated in their initial state by solving the structure equations via the Adomian decomposition method. Concerning the heat transfer in the protoplanets, the mode of convection is taken into account. The outcomes indicate that there is a reasonably good agreement between the Adomian semi-analytical solution containing only first 8 terms and the numerical results.
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spelling pubmed-85667792021-11-09 Solving protoplanetary structure equations using Adomian decomposition method Paul, Gour Chandra Khatun, Shahinur Nuruzzaman, Md. Kumar, Dipankar Ali, Md. Emran Bilkis, Farjana Barman, Mrinal Chandra Heliyon Research Article In this paper, the distribution of thermodynamic variables in the protoplanets formed by gravitational instability in the mass range [Formula: see text] ([Formula: see text] Jupiter mass = [Formula: see text] gm) is investigated in their initial state by solving the structure equations via the Adomian decomposition method. Concerning the heat transfer in the protoplanets, the mode of convection is taken into account. The outcomes indicate that there is a reasonably good agreement between the Adomian semi-analytical solution containing only first 8 terms and the numerical results. Elsevier 2021-10-20 /pmc/articles/PMC8566779/ /pubmed/34761131 http://dx.doi.org/10.1016/j.heliyon.2021.e08213 Text en © 2021 The Author(s) https://creativecommons.org/licenses/by-nc-nd/4.0/This is an open access article under the CC BY-NC-ND license (http://creativecommons.org/licenses/by-nc-nd/4.0/).
spellingShingle Research Article
Paul, Gour Chandra
Khatun, Shahinur
Nuruzzaman, Md.
Kumar, Dipankar
Ali, Md. Emran
Bilkis, Farjana
Barman, Mrinal Chandra
Solving protoplanetary structure equations using Adomian decomposition method
title Solving protoplanetary structure equations using Adomian decomposition method
title_full Solving protoplanetary structure equations using Adomian decomposition method
title_fullStr Solving protoplanetary structure equations using Adomian decomposition method
title_full_unstemmed Solving protoplanetary structure equations using Adomian decomposition method
title_short Solving protoplanetary structure equations using Adomian decomposition method
title_sort solving protoplanetary structure equations using adomian decomposition method
topic Research Article
url https://www.ncbi.nlm.nih.gov/pmc/articles/PMC8566779/
https://www.ncbi.nlm.nih.gov/pubmed/34761131
http://dx.doi.org/10.1016/j.heliyon.2021.e08213
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