Energy Reports (Nov 2023)
Thermo-solutal transportation in Reiner Philippoff liquid under influence of non-Fourier’s law on hybrid nanofluid model
Abstract
Current investigation aims for determining the comparative performance of heat transfer and mass diffusion between HMC (Hamilton Crosser)-model and YMO (Yamada Ota)-model in Reiner Philippoff liquid with a magnetic field and heat source towards a vertical plate. Transportation of mass species and temperature carried out by non-Fourier’s law and solar thermal radiation involving chemical reaction and heat sink. HMC-model and YMO model are prepared using hybrid nano-strictures. In comparing points of view, the complex behavior of such hybrid nanofluids utilizing different approaches Ise obtained, such as thermal conductivity, heat transfer, and viscosity. It was investigated that HMC and YMO-hybrid nanofluid models are addressed for obtaining maximum thermal enhancement which is applicable in electronic devices, solar systems, cooling processes, aircraft engines, thermal therapy, etc. The key reason for choosing of HMC-model and YMO-model is based on correlations associated with thermal conductivity improvement in hybrid nanofluids. A non-uniform magnetic force has been placed at the surface of the wall using ethylene glycol. A system related to ODEs is achieved using the concept of similarity variables and the developing flow model is numerically simulated by the finite element method. The analysis reveals that the performance of thermal energy and flow behavior for the case of Yamada Ota hybrid-nanofluid model is higher than the performance of thermal energy and flow behavior for the case of Hamilton Crosser hybrid-nanofluid model. The temperature field increases with large values of time relaxation number, heat source number (Ht), and very small ϵ1. Magnetic parameters have a significant impact on the velocity field. Further, BL (boundary layer)-thickness associated with mass diffusion is addressed as decreasing function Sc,ϵ2, and Kc and increasing function of λ2. The temperature curve enhances with increasing values of solar thermal radiation number (Qs) and magnetic parameter M.
