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A Review on the Recent Advancements of Ni-Based Sulfides and Mixed Sulfides for Supercapacitors and Electrocatalysis (Oxygen Evolution Reaction)
Published 2025-07-01“…This article summarizes the recent progress of NS and NMS materials in the fields of energy storage (supercapacitors) and conversion (oxygen evolution reactions). …”
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Microstructure evolution of SiCf/TiMoNb heterogeneous core reinforced Ti2AlNb-based composites
Published 2025-05-01Get full text
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High catalytic activity of iron and cobalt-iron oxide nanoparticles synthesized via a green method for the oxygen-evolution reaction
Published 2025-07-01“…Abstract Water oxidation, or the oxygen evolution reaction (OER), is the half-reaction that limits the efficiency of overall water splitting and represents a major bottleneck in the production of sustainable hydrogen fuel. …”
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Mn‐Doped Tuned NiC/NiO Heterostructure for Efficient Electron Transfer in Hydrogen Evolution Reaction
Published 2025-06-01Get full text
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Temperature-dependent microstructural evolution in a compositionally complex solid electrolyte: The role of a grain boundary transition
Published 2025-03-01“…The temperature-dependent grain growth has been examined to investigate the microstructural evolution and the origin of exaggerated (abnormal) grain growth. …”
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Investigation of Mechanical Properties and Microstructural Evolution in Pure Copper with Dual Heterostructures Produced by Surface Mechanical Attrition Treatment
Published 2024-10-01“…Various heterostructured materials have been widely investigated in recent years. …”
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Phase Evolution in La-Alloyed β‑Ga2O3 Nanofibers: Experimental and DFT Simulation Insights
Published 2025-04-01Get full text
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Spectropolarimetry of SN 2023ixf Reveals Both Circumstellar Material and an Aspherical Helium Core
Published 2025-01-01“…In addition, at +14.50 days we see an “inverse P Cygni” profile in the H and He line polarization, which clearly indicates the presence of asymmetrically distributed material overlying the photosphere. The overall temporal evolution of the polarization is typical for Type II SNe, but the high level of polarization during the rising phase has only been observed in SN 2023ixf.…”
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