Nearly a century ago it was recognized that radiation absorption by stellar matter controls
the internal temperature profiles within stars. Laboratory opacity measurements, however …

We present a new, publicly available set of Los Alamos OPLIB opacity tables for the
elements hydrogen through zinc. Our tables are computed using the Los Alamos ATOMIC …

Abstract The Los Alamos suite of relativistic atomic physics codes is a robust, mature
platform that has been used to model highly charged ions in a variety of ways. The suite …

The OPAS opacity model has been used to calculate the radiative opacity of stellar plasmas
in local thermodynamic equilibrium. According to the recent chemical composition revision …

The induced gravitational collapse (IGC) paradigm has been successfully applied to the
explanation of the concomitance of gamma-ray bursts (GRBs) with supernovae (SNe) Ic. The …

We report on the use of the Los Alamos suite of relativistic atomic physics codes to generate
radiative opacities for the modeling of astrophysically relevant plasmas under local …

We determine instability domains on the Hertzsprung–Russell diagram for rotating main
sequence stars with masses of 2–20 M⊙. The effects of the Coriolis force are treated wihin …

Continuum atomic processes initiated by photons and electrons occurring in a plasma are
fundamental in plasma physics, playing a key role in the determination of ionization balance …

At modern laser facilities, energy densities ranging from 1 Mbar to many hundreds of
gigabars can regularly be achieved. These high-energy states of matter last for mere …

Recently developed free-energy density functional theory (DFT)-based methodology for
optical property calculations of warm dense matter has been applied for studying L-shell …