Radiative Non-Coaxial Rotating Flow for Viscous Fluid over Accelerated Disk with MHD and Porosity Effects

نویسندگان

چکیده

An analytical solution to analyze the effects of radiation, magnetic, and permeability in an accelerating non-coaxial rotation phenomenon is not yet reported previous studies. Therefore, a radiative mixed convection flow for rotating MHD viscous fluid porous medium past accelerated disk studied. The motion this problem induced by two sources which are buoyancy force. dimensional coupled differential equations subjected initial boundary conditions transformed dimensionless utilizing appropriate variables. Laplace transform technique applied generate closed form problem. impacts Prandtl number, Grashof porosity, parameters on temperature velocity fields illustrated graphically. profiles satisfy both conditions, present results found accordance published work. improved with assistance acceleration, radiation while implementation magnetic field causes opposite effect. Increasing leads growth thermal layer as well reducing heat transmission rate. This result can significantly contribute designing heating systems because imposition able sustain environment specific temperature. obtained be used check correctness from numerical experimental

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ژورنال

عنوان ژورنال: Sains Malaysiana

سال: 2021

ISSN: ['0126-6039', '2735-0118']

DOI: https://doi.org/10.17576/jsm-2022-5108-25