For more than half a century, researchers around the world have been engaged in attempts
to achieve fusion ignition as a proof of principle of various fusion concepts. Following the …

White dwarfs represent the final state of evolution for most stars,–. Certain classes of white
dwarfs pulsate,, leading to observable brightness variations, and analysis of these variations …

We put together a first-principles equation of state (FPEOS) database for matter at extreme
conditions by combining results from path integral Monte Carlo and density functional …

In this work we present the design of the first controlled fusion laboratory experiment to
reach target gain G> 1 N221204 (5 December 2022)[Phys. Rev. Lett. 132, 065102 (2024) …

We present the design of the first igniting fusion plasma in the laboratory by Lawson's
criterion that produced 1.37 MJ of fusion energy, Hybrid-E experiment N210808 (August 8 …

We present the results of the first Charged-Particle Transport Coefficient Code Comparison
Workshop, which was held in Albuquerque, NM October 4–6, 2016. In this first workshop …

Strong interest in the modeling of planetary interiors, dwarf stars, and the physical conditions
necessary to achieve inertial confinement fusion (ICF) have driven attention to the properties …

We review the results of the 1 st Extreme Ultraviolet (EUV) Light Sources Code Comparison
Workshop. The goal of this workshop was to provide a platform for specialists in EUV light …

In high-temperature density functional theory simulations (from tens of eV to keV), the total
number of Kohn–Sham orbitals is a critical quantity to get accurate results. To establish the …

We have developed an experimental platform at the National Ignition Facility that employs
colliding planar shocks to produce warm dense matter with uniform conditions and enable …