Excitation and charge transfer in low-energy hydrogen atom collisions with neutral manganese and titanium
arXiv:2003.10029 · doi:10.1051/0004-6361/201937434
Abstract
Data for inelastic processes due to hydrogen atom collisions with manganese and titanium are needed for accurate modeling of the corresponding spectra in late-type stars. In this work excitation and charge transfer in low-energy Mn+H and Ti+H collisions have been studied theoretically using a method based on an asymptotic two-electron linear combination of an atomic orbitals model of ionic-covalent interactions in the neutral atom-hydrogen-atom system, together with the multichannel Landau-Zener model to treat the dynamics. Extensive calculations of charge transfer (mutual neutralization, ion-pair production), excitation and de-excitation processes in the two collisional systems are carried out for all transitions between covalent states dissociating to energies below the first ionic limit and the dominating ionic states. Rate coefficients are determined for temperatures in the range 1000 - 20 000 K in steps of 1000 K. Like for earlier studies of other atomic species, charge transfer processes are found to lead to much larger rate coefficients than excitation processes.
arXiv comment9 pages, 3 figures, 5 tables; accepted for publication in A&A
References in corpus (21)
- Non-LTE calculations for neutral Na in late-type stars using improved atomic data
- Departures from LTE for neutral Li in late-type stars
- NLTE abundances of Mn in a sample of metal-poor stars
- Using chemical tagging to redefine the interface of the Galactic disk and halo
- Observational constraints on the origin of the elements. I. 3D NLTE formation of Mn lines in late-type stars
- Solar abundance of manganese: a case for the existence of near Chandrasekhar-mass Type Ia supernova progenitors
- Inelastic H+Li and H^-+Li^+ collisions and non-LTE Li I line formation in stellar atmospheres
- Ionization balance of Ti in the photospheres of the Sun and four late-type stars
- Accurate abundance analysis of late-type stars: advances in atomic physics
- Mg line formation in late-type stellar atmospheres: I. The model atom
- Excitation and charge transfer in low-energy hydrogen atom collisions with neutral atoms: Theory, comparisons, and application to Ca
- Inelastic Na+H collision data for non-LTE applications in stellar atmospheres
- Inelastic O+H collisions and the OI 777nm solar centre-to-limb variation
- Inelastic Mg+H collision data for non-LTE applications in stellar atmospheres
- Non-LTE analysis of K I in late-type stars
- 3D non-LTE line formation of neutral carbon in the Sun
- Excitation and charge transfer in low-energy hydrogen atom collisions with neutral iron
- Formation of MnI lines in the solar atmosphere
- Ca line formation in late-type stellar atmospheres: I. The model atom
- Excitation and charge transfer in low-energy hydrogen atom collisions with neutral oxygen
- Excitation and charge transfer in low-energy hydrogen atom collisions with neutral carbon and nitrogen
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- Titanium abundances in late-type stars I. 1D non-local thermodynamic equilibrium modelling in benchmark dwarfs and giants
- Revisiting inelastic Cu+H collisions and the non-LTE Galactic evolution of copper