Excitation and charge transfer in low-energy hydrogen atom collisions with neutral atoms: Theory, comparisons, and application to Ca
arXiv:1603.07097 · doi:10.1103/PhysRevA.93.042705
Abstract
A theoretical method for the estimation of cross sections and rates for excitation and charge transfer processes in low-energy hydrogen atom collisions with neutral atoms, based on an asymptotic two-electron model of ionic-covalent interactions in the neutral atom-hydrogen atom system, is presented. The calculation of potentials and non-adiabatic radial couplings using the method is demonstrated. The potentials are used together with the multi-channel Landau-Zener model to calculate cross sections and rate coefficients. The main feature of the method is that it employs asymptotically exact atomic wavefunctions, which can be determined from known atomic parameters. The method is applied to Li+H, Na+H, and Mg+H collisions, and the results compare well with existing detailed full-quantum calculations. The method is applied to the astrophysically important problem of Ca+H collisions, and rate coefficients are calculated for temperatures in the range 1000-20000 K.
Accepted by Phys. Rev. A, small corrections made
References in corpus (1)
Cited by in corpus (39)
- The chemical make-up of the Sun: A 2020 vision
- Non-LTE line formation of Fe in late-type stars - III. 3D non-LTE analysis of metal-poor stars
- Carbon, oxygen, and iron abundances in disk and halo stars. Implications of 3D non-LTE spectral line formation
- Accurate abundance analysis of late-type stars: advances in atomic physics
- High-precision stellar abundances of the elements - methods and applications
- Mg line formation in late-type stellar atmospheres: I. The model atom
- The GALAH Survey: Non-LTE departure coefficients for large spectroscopic surveys
- 3D NLTE analysis of the most iron-deficient star, SMSS0313-6708
- Non-LTE line formation of Fe in late-type stars IV: Modelling of the solar centre-to-limb variation in 3D
- Inelastic O+H collisions and the OI 777nm solar centre-to-limb variation
- The formation of the Milky Way halo and its dwarf satellites, a NLTE-1D abundance analysis. I. Homogeneous set of atmospheric parameters
- Non-LTE analysis of K I in late-type stars
- NLTE for APOGEE: Simultaneous Multi-Element NLTE Radiative Transfer
- Influence of inelastic collisions with hydrogen atoms on the non-LTE modelling of Ca I and Ca II lines in late-type stars
- The GALAH Survey: Verifying abundance trends in the open cluster M67 using non-LTE spectroscopy
- 3D non-LTE line formation of neutral carbon in the Sun
- Atomic transition probabilities for UV and blue lines of Fe II and abundance determinations in the photospheres of the Sun and metal-poor star HD 84937
- Excitation and charge transfer in low-energy hydrogen atom collisions with neutral iron
- Mutual neutralization in Li-D collisions: a combined experimental and theoretical study
- Ca line formation in late-type stellar atmospheres: I. The model atom
- The 3D non-LTE solar nitrogen abundance from atomic lines
- A hydrodynamic study of the escape of metal species and excited hydrogen from the atmosphere of the hot Jupiter WASP-121b
- Influence of inelastic collisions with hydrogen atoms on the non-LTE line formation for Fe I and Fe II in the 1D model atmospheres of late-type stars
- Transition probabilities of Co II, weak lines to the ground and low metastable levels
- Excitation and charge transfer in low-energy hydrogen atom collisions with neutral oxygen
- Mutual neutralisation in Li+H/D and Na+H/D collisions: Implications of experimental results for non-LTE modelling of stellar spectra
- Titanium abundances in late-type stars I. 1D non-local thermodynamic equilibrium modelling in benchmark dwarfs and giants
- 3D NLTE modelling of Y and Eu. Centre-to-limb variation and solar abundances
- An empirical recipe for inelastic hydrogen-atom collisions in non-LTE calculations
- Influence of Inelastic Collisions with Hydrogen Atoms on Non-LTE Oxygen Abundance Determination in the Sun and late-type stars
- Excitation and charge transfer in low-energy hydrogen atom collisions with neutral carbon and nitrogen
- Atomic line radiative transfer with MCFOST I. Code description and benchmarking
- The influence of photo-induced processes and charge transfer on carbon and oxygen in the lower solar atmosphere
- Revisiting inelastic Cu+H collisions and the non-LTE Galactic evolution of copper
- A distinct halo population revealed from 3D non-LTE magnesium abundances
- Excitation and charge transfer in low-energy hydrogen atom collisions with neutral manganese and titanium
- Accurate Metallicities for Very Metal-Poor Stars from the Ca~II Infrared Triplet
- Solar off-limb emission of the OI 7772 Å line
- A Sequoia stellar candidate with very high 7Li and 9Be