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Impact of nonlinear thermal radiation on three-dimensional unsteady flow of carbon nanotube-suspended nanofluid with different length and radius over a stretching surface

Abdul Hamid Ganie, Zafar Mahmood, Umar Khan and Musawa Yahya Almusawa
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Abdul Hamid Ganie: Basic Science Department, College of Science and Theoretical Studies, Saudi Electronic University, Riyadh-11673, Kingdom of Saudi Arabia
Zafar Mahmood: ��Department of Mathematics and Statistics, Hazara University, Mansehra, Pakistan
Umar Khan: ��Department of Mathematics and Statistics, Hazara University, Mansehra, Pakistan
Musawa Yahya Almusawa: ��Department of Mathematics, Faculty of Science, Jazan University, Jazan 45142, Saudi Arabia

International Journal of Modern Physics C (IJMPC), 2024, vol. 35, issue 02, 1-21

Abstract: Carbon nanotubes (CNTs) influenced nanofluid is gaining popularity in the industry for solar energy and scratch heat exchanger applications. Consequently, this research focuses on evaluating the impact of nonlinear thermal radiation from a CNT-based nanofluid on an unsteady three-dimensional nonasymmetric Homann stagnant flux as a function of length and radius. CNTs have remarkable thermal physical properties that appear to be critical for nonlinear thermal transport. As a result, the nonlinear heat transfer properties of H2O composed of single or multiple wall CNTs are studied. The nanomaterial has a length and radius of approximately 3nm≤L≤70nm and 10nm≤R≤40nm. Partially differential equations with appropriate similarity transformations serve as a mathematical model for the process. The numerical solution of the simplified system of equations is achieved via the use of the well-known Runge–Kutta (RK) method in conjunction with the shooting approach. An effective way to show how a component affects velocity and temperature, skin frictions in both direction and Nusselt number are utilized in graphical representations. Increasing the unsteadiness parameter causes a reduction in the temperature profile and the velocity profile in both directions. As ε grows larger with ϕ, the skin friction in both directions decreases, while the Nusselt number profile grows larger. In addition, the variation in the Nusselt number is included in the tables, along with a comparison of the model without radiation to the model with radiation.

Keywords: Stagnation point; carbon nanotubes; nonlinear thermal radiation; unsteady flow; numerical solutions (search for similar items in EconPapers)
Date: 2024
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DOI: 10.1142/S0129183124400011

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International Journal of Modern Physics C (IJMPC) is currently edited by H. J. Herrmann

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