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Fundamentals of hydrogen storage [Video]

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Fundamentals of hydrogen storage

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Hydrogen storage methods encompass a range of techniques tailored to meet diverse application requirements, from stationary storage for grid-scale energy systems to onboard storage for fuel cell vehicles. These methods can be classified into physical storage, such as compression and liquefaction, and chemical storage, including hydrogen absorption and adsorption in solid materials. Compression involves compressing gaseous hydrogen at high pressures, typically in tanks or cylinders, to increase storage density, while liquefaction involves cooling hydrogen to cryogenic temperatures to store it in liquid form. Chemical storage relies on reversible reactions to bind hydrogen molecules to solid materials, either through absorption into the crystal lattice or adsorption onto the surface. However, hydrogen storage faces several challenges, including low energy density compared to fossil fuels, safety concerns associated with high-pressure or cryogenic storage, and issues related to hydrogen embrittlement. Embrittlement occurs when hydrogen atoms diffuse into the lattice of metals, causing them to become brittle and susceptible to fracture, compromising the structural integrity of storage tanks or components. To mitigate embrittlement, materials with high hydrogen solubility, such as certain metals and alloys, are often avoided in hydrogen storage applications. Instead, materials with low hydrogen solubility, such as carbon-based materials like carbon nanotubes and graphene, or metal hydrides, which form stable compounds with hydrogen, are preferred. These materials offer safe and efficient storage solutions, enabling the widespread adoption of hydrogen as a clean and sustainable energy carrier.

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