Sakiadis flow of Maxwell fluid considering magnetic field and convective boundary conditions
Source abstract
Abstract
In this paper we address the flow of Maxwell fluid due to constantly moving flat radiative surface with convective condition. The flow is under the influence of non-uniform transverse magnetic field. The velocity and temperature distributions have been evaluated numerically by shooting approach. The solution depends on various interesting parameters including local Deborah number De, magnetic field parameter M, Prandtl number Pr and Biot number Bi. We found that variation in velocity with an increase in local Deborah number De is non-monotonic. However temperature is a decreasing function of local Deborah number De.
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Research context
OpenAlex topics: Nanofluid Flow and Heat Transfer · Fluid Dynamics and Turbulent Flows · Heat Transfer Mechanisms
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
Affiliations
School of Natural Sciences (SNS), National University of Sciences and Technology (NUST) 1 , Islamabad 44000, Pakistan
Research Centre for Modeling and Simulation (RCMS), National University of Sciences and Technology (NUST) 2 , Islamabad 44000, Pakistan
Quaid-I-Azam University 45320 3 Department of Mathematics, , Islamabad 44000, Pakistan
Nonlinear Analysis and Applied Mathematics (NAAM) Research Group, King Abdulaziz University 4 , P. O. Box 80257, Jeddah 21589, Saudi Arabia
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Show source-provided references
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