64 citations · 126 across the 13 of their papers we have counts for
13 papers
A New Approach to Modeling Line Shapes with Quasi-H Satellites in Stellar Atmospheres
Jackson R. White, Thomas A. Gomez, Mark C. Zammit +6
Theoretical spectral line shapes describe the distribution of opacity due to bound electronic transitions in hot dense plasmas and are used to fit emergent spectra from many astrop…
Collisional-radiative data for tokamak disruption mitigation modeling
Prashant Sharma, Christopher J. Fontes, Dmitry V. Fursa +6
Effective tokamak disruption mitigation is crucial for ensuring the safety and integrity of fusion power reactors. Accurate collisional-radiative (CR) modeling of a radiative plasm…
Excitation of molecular hydrogen by cosmic-ray protons
Marco Padovani, Daniele Galli, Corey T. Plowman +4
Low-energy cosmic rays ( GeV) are responsible for the ionisation and heating of molecular clouds. While the role of supra-thermal electrons produced in the ionisation…
Pseudoatom Molecular Dynamics Plasma Microfields
J. R. White, C. J. Fontes, M. C. Zammit +2
Spectral line profiles are powerful diagnostic tools for both laboratory and astrophysical plasmas, as their shape is sensitive to the plasma environment. The low-frequency compone…
Experimental Validation of Collision-Radiation Dataset for Molecular Hydrogen in Plasmas
Keisuke Fujii, Keiji Sawada, Kuzmin Arseniy +7
Quantitative spectroscopy of molecular hydrogen has generated substantial demand, leading to the accumulation of diverse elementary-process data encompassing radiative transitions,…
Ultraviolet H luminescence in molecular clouds induced by cosmic rays
Marco Padovani, Daniele Galli, Liam H. Scarlett +5
Galactic cosmic rays (CRs) play a crucial role in ionisation, dissociation, and excitation processes within dense cloud regions where UV radiation is absorbed by dust grains and ga…
ThunderBoltz: An Open-Source DSMC-based Boltzmann Solver for Plasma Transport, Chemical Kinetics, and 0D Plasma Modeling
Ryan Park, Brett S. Scheiner, Mark C. Zammit
Plasma-neutral interactions, including reactive kinetics, are often either studied in 0D using ODE based descriptions, or in multi-dimensional fluid or particle based plasma codes.…
Enhancements of Electron-Atom Collisions due to Pauli Repulsion in Neutron-Star Magnetic Fields
Thomas Gomez, Mark Zammit, Igor Bray +2
Neutron star surfaces and atmospheres are unique environments that sustain the largest-known magnetic fields in the universe. Our knowledge of neutron star material properties, inc…
Photoionization from the ground and excited vibrational states of H+2 and its deuterated isotopologues
Adam Singor, Liam H. Scarlett, Mark C. Zammit +2
Photoionization cross sections and rate coefficients have been calculated for all bound vibrational levels of the 1s state of H, HD, and D…
Cosmic rays in molecular clouds probed by H rovibrational lines -- Perspectives for the James Webb Space Telescope
Marco Padovani, Shmuel Bialy, Daniele Galli +7
Cosmic rays (CRs) at sub-TeV energies play a fundamental role in the chemical and dynamical evolution of molecular clouds, as they control the ionisation, dissociation, and excitat…
Isotopic and vibrational-level dependence of H dissociation by electron impact
Liam H. Scarlett, Dmitry V. Fursa, Jack Knol +2
The low-energy electron-impact dissociation of molecular hydrogen has been a source of disagreement between various calculations and measurements for decades. Excitation of the gro…
Benchmark Calculations of Electron Impact Electronic Excitation of the Hydrogen Molecule
T. Meltzer, J. Tennyson, Z. Mašín +4
We present benchmark integrated and differential cross-sections for electron collisions with H using two different theoretical approaches, namely, the R-matrix and molecular co…
Impact of a minority relativistic electron tail interacting with a thermal plasma containing high-atomic-number impurities
Nathan A. Garland, Hyun-Kyung Chung, Christopher J. Fontes +6
A minority relativistic electron component can arise in both laboratory and naturally-occurring plasmas. In the presence of high-atomic-number ion species, the ion charge state dis…