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Physics of laser-driven tin plasma sources of EUV radiation for nanolithography
OO Versolato - Plasma Sources Science and Technology, 2019 - iopscience.iop.org
Laser-produced transient tin plasmas are the sources of extreme ultraviolet (EUV) light at
13.5 nm wavelength for next-generation nanolithography, enabling the continued …
13.5 nm wavelength for next-generation nanolithography, enabling the continued …
A new generation of Los Alamos opacity tables
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 …
elements hydrogen through zinc. Our tables are computed using the Los Alamos ATOMIC …
Prominent radiative contributions from multiply-excited states in laser-produced tin plasma for nanolithography
Extreme ultraviolet (EUV) lithography is currently entering high-volume manufacturing to
enable the continued miniaturization of semiconductor devices. The required EUV light, at …
enable the continued miniaturization of semiconductor devices. The required EUV light, at …
A review on ab initio studies of static, transport, and optical properties of polystyrene under extreme conditions for inertial confinement fusion applications
Polystyrene (CH), commonly known as “plastic,” has been one of the widely used ablator
materials for capsule designs in inertial confinement fusion (ICF). Knowing its precise …
materials for capsule designs in inertial confinement fusion (ICF). Knowing its precise …
A line-binned treatment of opacities for the spectra and light curves from neutron star mergers
The electromagnetic observations of GW170817 were able to dramatically increase our
understanding of neutron star mergers beyond what we learned from gravitational waves …
understanding of neutron star mergers beyond what we learned from gravitational waves …
The Los Alamos suite of relativistic atomic physics codes
CJ Fontes, HL Zhang, J Abdallah Jr… - Journal of Physics B …, 2015 - iopscience.iop.org
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 …
platform that has been used to model highly charged ions in a variety of ways. The suite …
Actinide opacities for modelling the spectra and light curves of kilonovae
We extend previous ab initio calculations of lanthanide opacities to include a complete set of
actinide opacities for use in the modelling of kilonova (KN) light curves and spectra …
actinide opacities for use in the modelling of kilonova (KN) light curves and spectra …
Carbon ionization at gigabar pressures: An ab initio perspective on astrophysical high-density plasmas
A realistic description of partially ionized matter in extreme thermodynamic states is critical to
model the interior and evolution of the multiplicity of high-density astrophysical objects …
model the interior and evolution of the multiplicity of high-density astrophysical objects …
An Expanded Set of Los Alamos OPLIB Tables in MESA: Type-1 Rosseland-mean Opacities and Solar Models
We present a set of 1194 Type-1 Rosseland-mean opacity tables for four different metallicity
mixtures. These new Los Alamos OPLIB atomic radiative opacity tables are an order of …
mixtures. These new Los Alamos OPLIB atomic radiative opacity tables are an order of …
Exploring mass loss, low-Z accretion, and convective overshoot in solar models to mitigate the solar abundance problem
JA Guzik, K Mussack - The Astrophysical Journal, 2010 - iopscience.iop.org
Solar models using the new lower abundances of Asplund et al. or Caffau et al. do not agree
as well with helioseismic inferences as models that use the higher Grevesse & Noels or …
as well with helioseismic inferences as models that use the higher Grevesse & Noels or …