Abstract Rayleigh–Taylor (RT) and Richtmyer–Meshkov (RM) instabilities are well-known
pathways towards turbulent mixing layers, in many cases characterized by significant mass …

White dwarfs are a class of stars with unique physical properties. They present many
challenging problems whose solution requires advanced theories of dense matter, state-of …

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 …

We update the capabilities of the open-knowledge software instrument Modules for
Experiments in Stellar Astrophysics (MESA). The new auto _ diff module implements …

We update the capabilities of the software instrument Modules for Experiments in Stellar
Astrophysics (MESA) and enhance its ease of use and availability. Our new approach to …

In diverse areas of science and technology, including inertial confinement fusion (ICF),
astrophysics, geophysics, and engineering processes, turbulent mixing induced by …

White dwarfs are stellar remnants devoid of a nuclear energy source, gradually cooling over
billions of years, and eventually freezing into a solid state from the inside out,. Recently, it …

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 …

Multi-gigayear White Dwarf Cooling Delays from Clustering-enhanced Gravitational
Sedimentation - IOPscience This site uses cookies. By continuing to use this site you agree …