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Pulsatile flow of power-law fluids over a sphere: Momentum and heat transfer characteristics

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dc.contributor.author Mishra, G.
dc.contributor.author Patel, S. A.
dc.contributor.author Chhabra, R. P.
dc.date.accessioned 2021-07-12T09:12:12Z
dc.date.available 2021-07-12T09:12:12Z
dc.date.issued 2021-07-12
dc.identifier.uri http://localhost:8080/xmlui/handle/123456789/2078
dc.description.abstract The effect of pulsatile flow on the momentum and heat transfer characteristics for a sphere in power-law fluids is investigated numerically otherwise in the steady regime. Extensive results are presented in terms of streamlines, isotherms, pressure coefficient and local Nusselt number, drag coefficient and Nusselt number over the range of conditions as: Reynolds number (5 ≤ Re ≤ 120), Prandtl number (0.7 ≤ Pr ≤ 100), power-law index (0.3 ≤ n ≤ 1.5), frequency (π/4 ≤ ω* ≤ π) and amplitude of pulsations (0 ≤ A ≤ 0.8). The vortex grows during the deceleration phase of the pulsatile cycle and vice-versa. The pulsatile flow enhances heat transfer in shear-thinning fluids by 30% (at Re = 120, Pr = 100) over that of uniform flow conditions whereas the corresponding improvement is smaller than this value for shear-thickening fluids, i.e., n N 1. This is accompanied by a marginal increase in drag en_US
dc.language.iso en_US en_US
dc.subject Sphere en_US
dc.subject Pulsatile flow en_US
dc.subject Frequency of pulsation en_US
dc.subject Power-law fluid en_US
dc.subject Nusselt number en_US
dc.subject Drag coefficient en_US
dc.title Pulsatile flow of power-law fluids over a sphere: Momentum and heat transfer characteristics en_US
dc.type Article en_US


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