Radiative MHD Non-Newtonian Chemically Reactive Nanofluid Flow with Heat Source Induced by Non-linear Stretching Cylinder
نویسندگان
چکیده
Magnetohydrodynamic (MHD) chemically reacting flow by Casson nanofluid bounded a stretched surface is analyzed. Convective conditions of transport phenomena, radiation and heat generation /absorption effects are discussed. Influence Brownian motion thermophoresis has been taken into account. This manuscript investigates the outcomes yield stress, thermophoresis, motion, magnetic parameter, Prandtl number, parameter thermal conductivity on velocity, temperature nanoparticle concentration profiles. To solve transformed equations, well designed numerical technique (Runge Kutta Fehlberg) implemented following Shooting procedure. MATLAB programming with ODE45 solver used to calculate results compare for local Nusselt number (-qa¢(0)) extant in absence parameters via table bar graphs pertinent values non linear stretching parameter. An excellent agreement noted non-linear cylinder. The impact controlling fluid represented graphically. Additionally, physical quantities interest tabulated explained graphs.
 GRAPHICAL ABSTRACT
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ژورنال
عنوان ژورنال: Trends in Sciences
سال: 2022
ISSN: ['2774-0226']
DOI: https://doi.org/10.48048/tis.2022.6314