TY - JOUR
T1 - Insight into Darcy flow of ternary-hybrid nanofluid on horizontal surfaces
T2 - Exploration of the effects of convective and unsteady acceleration
AU - Animasaun, Isaac Lare
AU - Kumar, T. Kiran
AU - Noah, Fatai Adesegun
AU - Okoya, Samuel Segun
AU - Al-Mdallal, Qasem M.
AU - Bhatti, Muhammad Mubashir
N1 - Publisher Copyright:
© 2022 Wiley-VCH GmbH.
PY - 2023/5
Y1 - 2023/5
N2 - The transport phenomenon of water conveying spherical carbon nanotubes, cylindrical graphene, and platelet aluminum oxide nanoparticles exhibits a linear relationship between the pressure gradient causing the dynamics of ternary-hybrid nanofluid and the velocity. However, it is essential to note that little is known about the computation of roughness at the surface transition zone during the early stages of accretion. The Darcy flow of ternary-hybrid nanofluid was investigated and reported in this paper with the intention to provide insight into the convective and unstable acceleration related to leading-edge accretion. The governing equations roughly represented that the time-dependent fluid flow were nondimensionalized using the Blasius-Rayleigh Stokes variable, and the three-stage Lobatto IIIa integration formula for a finite difference (MATLAB package bvp4c) was used to solve numerically. Based on the analysis of results, it is worth concluding that the velocity decreases significantly due to a growth in the leading-edge accretion (γ) because the convective acceleration increases while the unsteady acceleration decreases for (Formula presented.). As (Formula presented.), convective acceleration increases while the unsteady acceleration decreases. As γ enlarges from 90° to 180°, both forms of the acceleration are decreasing properties, but unsteady deceleration is bound to manifest.
AB - The transport phenomenon of water conveying spherical carbon nanotubes, cylindrical graphene, and platelet aluminum oxide nanoparticles exhibits a linear relationship between the pressure gradient causing the dynamics of ternary-hybrid nanofluid and the velocity. However, it is essential to note that little is known about the computation of roughness at the surface transition zone during the early stages of accretion. The Darcy flow of ternary-hybrid nanofluid was investigated and reported in this paper with the intention to provide insight into the convective and unstable acceleration related to leading-edge accretion. The governing equations roughly represented that the time-dependent fluid flow were nondimensionalized using the Blasius-Rayleigh Stokes variable, and the three-stage Lobatto IIIa integration formula for a finite difference (MATLAB package bvp4c) was used to solve numerically. Based on the analysis of results, it is worth concluding that the velocity decreases significantly due to a growth in the leading-edge accretion (γ) because the convective acceleration increases while the unsteady acceleration decreases for (Formula presented.). As (Formula presented.), convective acceleration increases while the unsteady acceleration decreases. As γ enlarges from 90° to 180°, both forms of the acceleration are decreasing properties, but unsteady deceleration is bound to manifest.
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U2 - 10.1002/zamm.202200197
DO - 10.1002/zamm.202200197
M3 - Article
AN - SCOPUS:85144235706
SN - 0044-2267
VL - 103
JO - ZAMM Zeitschrift fur Angewandte Mathematik und Mechanik
JF - ZAMM Zeitschrift fur Angewandte Mathematik und Mechanik
IS - 5
M1 - e202200197
ER -