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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Detalles Bibliográficos
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
Descripción
Sumario: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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