4.7 Article

Dynamics of ternary-hybrid nanofluid subject to magnetic flux density and heat source or sink on a convectively heated surface

期刊

SURFACES AND INTERFACES
卷 28, 期 -, 页码 -

出版社

ELSEVIER
DOI: 10.1016/j.surfin.2021.101654

关键词

Induced magnetic field; Different shapes of nanoparticle; Ternary-hybrid nanofluid; Convective heating of surface; Silver/aluminium oxide; Aluminium nanoparticles

资金

  1. Basic Science Research Program through the National Research Foundation of Korea (NRF) - Ministry of Science, ICT & Future Planning [2017R1A2B2006927]
  2. King Khalid University, Abha, Saudi Arabia [RGP.2/39/42]

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The size and intensity of the system of delocalized electrons are reflected in the form of the induced magnetic field. However, the significance of different-shaped metal nanoparticles in stagnant water undergoing convective heating is still unclear. Numerical calculations and analysis reveal that an increase in convective heating of the wall can enhance temperature distribution, regardless of whether it is a heat source or heat sink.
The size and intensity of the system of delocalized electrons are reflected in the form of the induced magnetic field. Even though this also affects nearby molecules, nothing is known on the significance of stagnant water conveying silver A(g), aluminum oxide Al2O3, and aluminum Al nanoparticles of different shapes on a horizontal surface experiencing convectively heating as applicable in the industry. Relevant similarity transformations were adopted to non-dimenzionalized the governing equations and solved numerically using the 3-stage Lobatto IIIa integration formula for a finite difference (MATLAB package bvp4c). Based on the analysis of the new results, it is worth concluding that either in the case of heat source or heat sink, an increment in the convective heating of the wall is a factor capable to boost the temperature distribution. Increasing effects of an inclined magnetic field are capable to cause the distance between the turning points of shear stress and that of the gradient of magnetic flux density to be located at the middle of the domain.

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