Theoretical treatment of charge transfer processes of relevance to astrophysics

Details Theoretical treatment of charge transfer processes of relevance to astrophysics Theoretical treatment of charge transfer processes of relevance to astrophysics

Dec 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997stin...9928789k&link_type=abstract

Technical Report, Atomic and Nuclear Astrophysics Office of Energy Research

Computer Science

Numerical Analysis

Astrophysics, Numerical Analysis, Charge Exchange, Charge Transfer, Charged Particles, Ion Atom Interactions, Electron Capture, Magnesium, Calcium, Iron, Cobalt, Nickel, Zinc, Hydrogen, Helium, Atmospheric Composition, Collisions, Ions, Metals, Molecules, Targets

Scientific paper

Charge transfer is an important process in many astrophysical and atmospheric environments. While numerous experimental and theoretical studies exist for H and He targets, data on other targets, particularly metals and molecules, are sparse. Using a variety of theoretical methods and computational techniques the authors are developing methods to estimate the cross sections for electron capture (charge transfer) in slow collisions of low charge state ions with heavy (Mg, Ca, Fe, Co, Ni and Zn) neutrals. In this ongoing work particular attention is paid to ascertaining the importance of double electron capture.

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