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Volume 3, Issue 1, 2024

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This study conducts a numerical investigation into the heat transfer enhancement of $\mathrm{Fe}_3 \mathrm{O}_4$-distilled water nanofluid within a magnetically influenced environment. The research is centered on the analysis of the impact of varying magnetic field strengths on the heat transfer characteristics in a controlled tube setting. The tube, possessing an inner diameter of 25.4 mm and a length of 210 mm, serves as the medium for the flow of nanofluid, initially at 300 K. The influence of magnetism on the nanofluid's thermal boundary layer and the formation of fluid vortices is meticulously examined, leveraging the application of magnetic fields ranging from one to three Teslas. In this context, the study observes the behavior of magnetic particles under these fields, revealing their attraction or repulsion, subsequently inducing turbulence and modifying flow patterns. It is noted that increased flow velocities tend to shield the magnetic field's thermal effects. A key focus is placed on the Nusselt number and $\mathrm{Y}^{+}$ as indicators of heat transfer efficiency, both of which demonstrate significant variations with changes in the magnetic field strength and fluid velocity. The Nusselt number, in particular, escalates to a peak value of 128.7 when exposed to a 0.1 m/s flow velocity and a magnetic field of 3 Teslas. The findings suggest an interrelation between increased magnetic field strengths and the entrance of the fluid into a turbulent state, thereby facilitating an efficient temperature transfer to the fluid. Notably, this research sheds light on the prospect of using ferrofluid-based cooling systems in electrical equipment, highlighting the potential of magnetically manipulated nanofluids to enhance heat transfer capabilities. The investigation delineates how the interplay between magnetic fields, fluid velocity, and nanofluid properties can be optimized for improved thermal management in various applications.

Open Access
Research article
Progress in High-Entropy Alloy Performance Enhancement
xinsheng wang ,
jifeng luo ,
rongbin ma ,
kai wang
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Available online: 02-04-2024

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High-entropy alloy (HEA) is currently regarded as materials with the most superior comprehensive properties, possessing capabilities not found in traditional alloys. This is particularly attributed to the characteristic presence of multiple principal elements, endowing the alloys with exceptional performance across various aspects, thus becoming a focal point of both current and future research endeavors. The performance of HEA is derived from phase transition. This review summarizes the intrinsic phase transition of HEA itself and the enhancement of HEA performance through the addition of particulate phases. Starting from the definition of HEA, the common definitions are introduced, leading to the design principles of HEA and the prediction of solid solution phases. The influence of different elements on the structural changes of HEA solid solution phases is explained through lattice distortion phase transition and segregation phase transition methods. The patterns of phase transition induced by large atomic elements are summarized, and the development process of segregation phase transition by small atomic elements is presented, offering references for future research on HEA. Furthermore, the concept of solubility of elements in HEA is introduced, based on the phase transition caused by large and small atomic elements, providing a more accurate basis for the design and preparation of HEA. The common hard particles used to enhance the performance of HEA are discussed, revealing how direct addition of particles can lead to decomposition and the uncertainty of the effects of elements on HEA performance. The significance of encapsulation techniques in enhancing the performance of high-quality HEA is proposed.

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In this study, an exact solution is developed to elucidate the effects of radially varying temperature-dependent heat sources/sinks (RVTDHS) and magnetic fields on natural convection flow between two vertically oriented concentric cylinders, where heating is administered through both isoflux (constant heat flux) and isothermal (constant wall temperature) conditions. The energy equation incorporates a temperature-dependent heat source/sink term, postulated to vary inversely with the radial coordinate. Through the application of suitable transformations, exact expressions for temperature distributions and fluid velocities as functions of the radial coordinate, the ratio of radii, the heat source/sink parameter, and the Hartmann number (representing magnetic field strength) are derived. Findings indicate that the presence of a radially varying heat source/sink notably influences temperature distribution, velocity profile, skin friction, and mass flux, with the heat source elevating fluid temperature. Consequently, this adjustment shortens the range over which isothermal heating supersedes isoflux heating. Conversely, in the presence of a heat sink, isothermal heating remains predominant over isoflux heating irrespective of the annular gap's size. These results not only provide deeper insights into the dynamics of magnetohydrodynamics (MHD) free-convection flows in engineering and geophysical applications but also enhance the understanding of how magnetic fields and heat sources/sinks can be strategically manipulated to control such flows.
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