Like being inside a star: Simulating high pressures

“We developed this simulation method here at SISSA over the past ten years”, explains Sandro Sorella, a SISSA professor and co-author of the paper. “It’s a highly accurate technique based on the quantum Monte Carlo method – a family of algorithms but usually limited to a small number of particles – that we have developed in order to consider now a large number of atoms, and obtain an almost realistic situation. A great advantage”.

“We used the simulation to verify the Wigner and Huntington prediction”, adds Guglielmo Mazzola, from SISSA and first author of the paper.

In 1935 Eugene Wigner and Hillard Bell Huntington conjectured that at very high pressures, when hydrogen makes the transition from the “molecular” phase to the “atomic” phase (when the atoms are so close to each other that the molecular structures can no longer be distinguished), hydrogen acquires metallic properties.

“In recent years, attempts to verify this hypothesis both theoretically and experimentally have yielded conflicting results with regard to the pressure required to achieve ‘metallization’”, comments Mazzola. “Our simulation, in the liquid phase, showed that we might indeed be very far from being able to observe this transition experimentally. According to our findings, metallization can only take place at pressures approaching 500 gigapascal. This is an enormous value, which only occurs in the innermost layers of gaseous planets and cannot be achieved with currently available experimental equipment”.

“A detailed understanding of the phase diagram of hydrogen”, concludes Sorella, ”is not only important for studies in the field of astrophysics, but also for learning how this element behaves and, for example, under what conditions it becomes a superconductor”.

The research was conducted in collaboration with the advanced research institute AICS-Riken in Tokyo, which provided the computational resources of one of the most powerful supercomputers in the world, the K-computer.