重力驱动对流光学厚纳米流体在磁场和辐射作用下流经振荡垂直板的速度和温度数学模型

Hari R. Kataria , Akhil S. Mittal
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引用次数: 64

摘要

得到了在热辐射和均匀横向磁场作用下,光学厚纳米流体中非定常磁边界层通过振荡垂直板的解析表达式。采用Rosseland扩散通量模型模拟热辐射效应。对动量守恒方程和能量守恒方程进行了无因次化处理,利用拉普拉斯变换得到了解析解。得到了速度和温度的计算结果,并绘制了图形。结果表明,纳米流体的速度随辐射参数Nr、Grashof数Gr和时间的增大而增大,随磁场和普朗特数Pr的增大而减小;纳米流体的温度随时间的增大而增大,随Nr和Pr的增大而减小。
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Mathematical model for velocity and temperature of gravity-driven convective optically thick nanofluid flow past an oscillating vertical plate in presence of magnetic field and radiation

Analytic expression for unsteady hydromagnetic boundary layer flow past an oscillating vertical plate in optically thick nanofluid in presence of thermal radiation and uniform transverse magnetic field is obtained. The Rosseland diffusion flux model is adopted to simulate thermal radiation effects. The momentum and energy conservation equations are made dimensionless and analytic solution is obtained using the Laplace transform. The results for velocity and temperature are obtained and plotted graphically. It is found that the velocity of the nanofluid increases with radiation parameter Nr, Grashof number Gr and time while decreases with increase in magnetic field and Prandtl number Pr. Temperature of nano-fluids increases with time while decrease with increase in Nr and Pr.

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