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Numerical treatment of squeezed MHD Jeffrey fluid flow with Cattaneo Chrisstov heat flux in a rotating frame using Levnberg-Marquard method

Hakeem UllahDepartment of Mathematics, Abdul Wali Khan University, Mardan 23200, KP, PakistanKashif UllahDepartment of Mathematics, Abdul Wali Khan University, Mardan 23200, KP, PakistanMuhammad Asif Zahoor RajaFuture Technology Research Center, National Yunlin University of Science and Technology, 123 University Road, Section 3, Douliou, Yunlin 64002, TaiwanMuhammad ShoaibYuan Ze University, AI Center, Taoyuan 320, TaiwanKottakkaran Sooppy NisarDepartment of Mathematics, College of Arts & Sciences, Wadi Aldawaser, Prince Sattam bin Abdulaziz University, Saudi ArabiaSaeed IslamDepartment of Mathematics, Abdul Wali Khan University, Mardan 23200, KP, PakistanWajaree WeeraDepartment of Mathematics, Faculty of Science, Khon Kaen University, Khon Kaen 40002, ThailandNuha Al‐HarbiDepartment of Physics, Faculty of Applied Sciences, Umm Al-Qura University, Makkah, Saudi Arabia
2022en
ABI

Аннотация

The present communication examines the unsteady-two-dimensional (2-D) squeezing flow of magnetohydrodynamic (MHD) Jeffrey fluid between two parallel plates (HT2DUSMHDJF). In its own plane, the bottom channel plate is extended while the upper plate squeezes towards the lower plate. The complete structure is takan is a rotating frame. Cattaneo-Christov heat flux model (CCHFM) is forced to explore the features of heat transfer. Distinct the conventional position, Instead of the Fourier heat conduction law, the heat flux is implemented by the Cattaneo-Christov theory. The resultant systems are computed through Artificial Neural Network (ANN). The behaviors of a number of relevant parameters are analyzed through graphs and numerical data. The velocity profile increases for Deborah number β and squeezing parameter sq and decreases for rotation, magnetic and relaxation time parameter ω, M, and λ1 respectively. Also the Skin friction coefficient decreases for λ1 and Sq and increases for high value of Deborah numbers β, ω and M.

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