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首页> 外文期刊>European Physical Journal Plus >Investigation of the entropy generation during natural convection of Newtonian and non-Newtonian fluids inside the L-shaped cavity subjected to magnetic field: application of lattice Boltzmann method
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Investigation of the entropy generation during natural convection of Newtonian and non-Newtonian fluids inside the L-shaped cavity subjected to magnetic field: application of lattice Boltzmann method

机译:对磁场L形腔内牛顿和非牛顿流体自然对流的熵生成的研究:晶格Boltzmann方法的应用

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In the present paper, free heat convection and entropy generation of Newtonian and two types of non-Newtonian fluids, shear-thickening and shear-thinning, inside an L-shaped cavity subjected to a magnetic field have been investigated by the finite difference lattice Boltzmann method. The power-law model was used for modeling the rheology of the fluids. The bottom and left walls of the cavity have been kept at a uniform high temperature. Internal walls are also kept cold. The remaining walls have been insulated against heat and mass transfer. The Boussinesq approximation is used to take the temperature dependency of density into account. The distribution functions of energy and density are modeled through the use of the nine-velocity two-dimensional scheme. The effects of Hartmann number (Ha), aspect ratio, power-law index, and Rayleigh number (Ra), on the flow field, temperature distribution, and entropy distributions are studied. The results show that the magnetic field and the power-law index have an ever-decreasing effect on the heat transfer rate and the entropy generation, while the Ra number has an ever-increasing effect. The maximum heat transfer enhancement of 71% happens at the lowest and the highest values of power-law index and Ra number, respectively, for the case with no magnetic field. The maximum heat transfer deterioration of 77% happens at the highest and lowest values of power-law index and Ra number, respectively, in the presence of the highest magnetic field strength. It is interesting that the sensitivities of heat transfer rate and the entropy generation to the Ha number become significant for shear-thinning fluids. It is found that there is an everlasting interplay between conduction and convection contributions to the irreversibilities, so that, for the Newtonian and shear-thinning fluids, thermal irreversibilities, characterized by Be number, increase with Ha number, reaching to a maximum, and then decline. The heat transfer rate and the total entropy generation for the Newtonian and shear-thinning fluids increase, monotonically, by raising the aspect ratio, while the figure for the shear-thickening case is different. It is decreased first and then increased.
机译:在本文中,通过有限差异格子Boltzmann研究了在经受磁场的L形腔内的牛顿和两种类型的非牛顿流体,剪切增厚和剪切变薄的自由流对流和熵产生。方法。幂律模型用于建模流体的流变学。腔的底部和左壁已经保持在均匀的高温下。内墙也保持冷。剩余的墙壁已经防止了热量和传质。 BoussinesQ近似用于考虑密度的温度依赖性。通过使用九个速度二维方案建模能量和密度的分布函数。研究了Hartmann号(HA),纵横比,幂律指标和瑞利数(RA)的影响,对流场,温度分布和熵分布进行了研究。结果表明,磁场和幂律指数对传热速率和熵产生的效果不断降低,而RA数具有不断增加的效果。对于没有磁场的情况,最大热传递增强71%的最低值分别发生在功率 - 法指数和RA数的最高值。在存在最高磁场强度的情况下,最大传热劣化分别在功率 - 法指数和RA数的最高值下发生77%。有趣的是,传热速率的敏感性和HA编号的熵产生对剪切稀疏流体具有重要意义。发现导通和对流贡献之间存在永恒的相互作用,使得对于牛顿和剪切稀疏的流体,热不缩探,其特征在于Number,随着HA编号的增加,达到最大值,然后衰退。通过提高纵横比,牛顿和剪切稀释液的传热速率和牛剪薄流体的总熵产生,而剪切增厚箱的图形是不同的。首先下降,然后增加。

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