Shape factor and thermal radiation effects on convective MHD flow of Casson blood ternary hybrid nano-fluid through a stretched rotating rigid disk

DOI10.1002/zamm.202300911MaRDI QIDQ6669188

Ilyas Khan, Abdelaziz Nehal, Naveen Dwivedi, Sultan Alshehery, Ismail Tabet, Mounir Gahgah, Mohamed Kezzar, Abdulrahman Aljohani, Mohamed Rafik Sari

Publication date: 22 January 2025

Published in: ZAMM. Zeitschrift für Angewandte Mathematik und Mechanik (Search for Journal in Brave)

Mathematics Subject Classification ID

Basic methods in fluid mechanics (76Mxx) Multiphase and multicomponent flows (76Txx) Thermodynamics and heat transfer (80Axx)

Cites Work

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• Revisit on partial solutions in the Adomian decomposition method: solving heat and wave equations
• On the heat transfer between two rotating disks
• The flow due to a rotating disc.
• Numerical simulation of a nonlinear coupled differential system describing a convective flow of Casson gold–blood nanofluid through a stretched rotating rigid disk in the presence of Lorentz forces and nonlinear thermal radiation

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