Depolarizing collisions with hydrogen: neutral and singly ionized alkaline earths
arXiv:1404.6339 · doi:10.1088/0004-637X/788/2/118
Abstract
Depolarizing collisions are elastic or quasielastic collisions that equalize the populations and destroy the coherence between the magnetic sublevels of atomic levels. In astrophysical plasmas, the main depolarizing collider is neutral hydrogen. We consider depolarizing rates on the lowest levels of neutral and singly ionized alkaly-earths Mg I, Sr I, Ba I, Mg II, Ca II, and Ba II, due to collisions with H. We compute ab initio potential curves of the atom-H system and solve the quantum mechanical dynamics. From the scattering amplitudes we calculate the depolarizing rates for Maxwellian distributions of colliders at temperatures T <10000 K. A comparative analysis of our results and previous calculations in the literature is done. We discuss the effect of these rates on the formation of scattering polarization patterns of resonant lines of alkali-earths in the solar atmosphere, and their effect on Hanle effect diagnostics of solar magnetic fields.
arXiv comment18 pages, 3 figures. Summitted to ApJ (2014)
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- The transfer of polarized radiation in resonance lines with partial frequency redistribution, J-state interference, and arbitrary magnetic fields. A radiative transfer code and useful approximations
- The magnetic sensitivity of the Ca II resonance and subordinate lines in the solar atmosphere
- On the (mis)interpretation of the scattering polarization signatures in the Ca II 8542 A line through spectral line inversions