Element number one, hydrogen, is the simplest and most abundant element in the universe. The relative abundance is reflected in the gas giant Jupiter, where under extreme pressures and temperatures, hydrogen exists in a dense metallic fluid state. It has been long predicted that such a metallic state could also be realised at considerably lower temperatures, whereby the molecular solid would dissociate under compression into an atomic metal. The metallic state of hydrogen is predicted to exhibit a whole host of fascinating properties at high pressure, from room temperature superconductivity, to novel states of matter. If quenchable to ambient conditions, metallic hydrogen could pave the way for a new generation of rocket propellants. As such, the pursuit of reaching these phenomena inspires many from interdisciplinary fields of science.
The overarching aim of MetElOne is to conclusively reach the metallic state of hydrogen and explore the fascinating properties predicted. However, this presents a monumental experimental challenge. The pressure conditions required to reach metallic hydrogen is thought to be in excess of 420 GPa (4.2 million times atmospheric pressure), which far exceeds the pressure at the centre the Earth (3.6 million times atmospheric pressure). To reach these conditions, we use a device called a diamond anvil cell, which harnesses the incredible strength of diamond to exert extreme pressures.
However, the pressures required for metallization are on the limit of conventional diamond anvil cells and hydrogen is light, diffusive and reactive resulting in containment issues and diamond embrittlement. The MetElOne project is exploring novel approaches to high pressure experimentation to overcome the challenges associated with hydrogen. Using a focussed-ion beam, diamonds will be milled into different geometries to optimize and extend current accessible pressure regimes. In parallel, rapid compression techniques are being developed that will be used to compress hydrogen to the metallic state on timescales that will avoid diffusion into the anvils. The combination of these techniques should put metallic hydrogen within reach to investigate with a broad suite of diagnostics. The advances alone will be transformative in the broader field of high pressure research, from recreating planetary interior conditions in the experimental laboratory to the synthesis of novel high-temperature superconductors.