Shape factor and thermal radiation effects on convective MHD flow of Casson blood ternary hybrid nano-fluid through a stretched rotating rigid disk
From MaRDI portal
Publication:6669188
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)
Basic methods in fluid mechanics (76Mxx) Multiphase and multicomponent flows (76Txx) Thermodynamics and heat transfer (80Axx)
Cites Work
- Unsteady two-layer film flow on a non-uniform rotating disk in presence of uniform transverse magnetic field
- A critical synthesis of thermophysical characteristics of nanofluids
- Magnetohydrodynamic flow between a solid rotating disk and a porous stationary disk
- Solving frontier problems of physics: the decomposition method
- Buoyancy-driven heat transfer enhancement in a two-dimensional enclosure utilizing nanofluids.
- Colours in metal glasses and in metallic films.
- Series solution of nanofluid flow and heat transfer between stretchable/shrinkable inclined walls
- Numerical solution of non-Newtonian fluid flow due to rotatory rigid disk
- 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
This page was built for publication: Shape factor and thermal radiation effects on convective MHD flow of Casson blood ternary hybrid nano-fluid through a stretched rotating rigid disk
