Astronomy and Astrophysics · 2010 · 81 citations · 12 references
Natural SciencesPhysicsAstrophysicsNuclear PhysicsPhysical ChemistryMolecular CollisionsStellar StructureInelastic CollisionsIon Pair ProductionNon-lte Stellar AtmospheresPair ProductionReaction Rate CoefficientsScatteringSystematic UncertaintiesTemperature Dependence Of Rate Coefficients
Rate coefficients for inelastic Na+H collisions are calculated for all transitions between the ten levels up to and including the ionic state (ion-pair production), namely Na(3s,3p,4s,3d,4p,5s,4d,4f,5p)+H(1s) and Na<sup>+<sup/>+H<sup>-<sup/>. The calculations are based on recent full quantum scattering cross-section calculations. The data are needed for non-LTE applications in cool astrophysical environments, especially cool stellar atmospheres, and are presented for a temperature range of 500-8000 K. From consideration of the sensitivity of the cross-sections to input quantum chemical data and the results of different methods for the scattering calculations, a measure of the possible uncertainties in the rate coefficients is estimated.
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