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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...
| Autores principales: | , , , , , , |
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| Formato: | Online Artículo Texto |
| Lenguaje: | English |
| Publicado: |
Elsevier
2021
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| Materias: | |
| 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 |