Scientists create tiny piece of matter similar to dwarf stars in laboratory

Groundbreaking laboratory experiments conducted at the Lawrence Livermore National Laboratory (LLNL) have yielded significant insights into the intricate process of pressure-driven ionization in stars and giant planets. Published in the prestigious journal Nature, the research sheds light on the behavior and material properties of matter under extreme compression, holding great implications for both astrophysics and nuclear fusion studies.

According to Siegfried Glenzer, the director of the High Energy Density Division at the Department of Energy’s SLAC National Accelerator Laboratory and a collaborator on the project, replicating stellar conditions enables scientists to unravel the inner workings of celestial bodies. He likened it to placing a thermometer inside a star, allowing for precise measurements of temperature and the impact of these conditions on atomic structures. This knowledge can pave the way for innovative techniques to manipulate matter for the advancement of fusion energy sources.

To create the necessary conditions for pressure-driven ionization, the international research team utilized the National Ignition Facility (NIF), the world’s largest and most energetic laser. By employing a staggering 184 laser beams, the team focused the energy to heat a cavity’s interior, converting it into X-rays. These X-rays then heated a 2 mm diameter beryllium shell positioned at the cavity’s center. As a result, the outer layer of the shell rapidly expanded due to the intense heat, while the inner portion moved inward, reaching temperatures of approximately two million kelvins and pressures up to three billion atmospheres. This process emulated the formation of matter found in dwarf stars, generating a miniature version of stellar material in the laboratory for a fleeting few nanoseconds.

Radiation hydrodynamic simulations. Results of one-dimensional radiation-hydrodynamic simulations using the HYDRA code illustrating the implosion dynamics of the beryllium shell. These simulations are tuned to reproduce the observed timing of radiography experiment N160801-001-999. (a) Simulation results for the evolution of the mass density and (b) a zoom-in for the behaviour close to stagnation. Panels (c) and (d) show radial profiles of mass density and temperature for different times near stagnation, respectively. Credit: Nature (2023). DOI: 10.1038/s41586-023-05996-8

In groundbreaking laboratory experiments, scientists at Lawrence Livermore National Laboratory (LLNL) delved into the intricate process of pressure-driven ionization in stars and giant planets. By subjecting a beryllium sample to extreme compression, researchers probed its density, temperature, and electron structure using X-rays. The study yielded remarkable findings, indicating that a substantial portion of electrons in beryllium transitioned into conducting states under strong heating and compression. Surprisingly, weak elastic scattering was observed, suggesting increased mobility of the remaining electrons.

The compression of matter in the cores of giant planets and certain cooler stars, caused by the immense weight of the layers above, leads to high pressures. At such pressures, interactions between the bound states of neighboring ions result in their complete ionization. While temperature primarily governs ionization in burning stars, pressure-driven ionization dominates in cooler celestial objects.

Theoretical understanding of pressure ionization as a pathway to highly ionized matter is limited, and the extreme states of matter required for study are challenging to create and examine in the laboratory, emphasized LLNL physicist Tilo Döppner, who spearheaded the project.

By replicating conditions akin to those inside giant planets and stars, the research team observed changes in material properties and electron structure that existing models fail to capture. Döppner highlighted the new possibilities opened for studying and modeling matter under extreme compression. Ionization in dense plasmas plays a crucial role as it affects the equation of state, thermodynamic properties, and the transport of radiation through opacity.

The implications of this research extend to inertial confinement fusion experiments conducted at the National Ignition Facility (NIF), where parameters such as X-ray absorption and compressibility are vital for optimizing high-performance fusion endeavors. A comprehensive comprehension of pressure- and temperature-driven ionization is pivotal for modeling compressed materials and ultimately developing a sustainable, carbon-free energy source through laser-driven nuclear fusion, added Döppner.

Bruce Remington, NIF Discovery Science program leader, emphasized the unparalleled capabilities of the National Ignition Facility in creating extreme compressions akin to planetary cores and stellar interiors. It remains the sole location on Earth where these conditions can be replicated, studied, and observed using the world’s largest and most energetic laser. This research builds upon previous studies at NIF, pushing the boundaries of laboratory astrophysics forward.

Source: SLAC National Accelerator Laboratory

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