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

Internet

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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