Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
1779390 | New Astronomy | 2010 | 10 Pages |
Abstract
Results from the unified method for photoionization and electron-ion recombination of (HeI+hνâHeII+e) are presented. He I wave function is represented by an expansion that includes 10 core states for excitations to n = 2, 3, and 4 states. A total of 99 bound LS states with n⩽10 are obtained. They all, except two, agree with the observed energies in less than 1%. Photoionization cross sections ÏPI for the total ionization, leaving the residual ion in all excited states, and the partial ionization, leaving the ion in the ground state, are presented for all 99 bound states. Calculated ÏPI agree very well with the measured ground state cross section. Detailed resonant features of ÏPI and coupling effects on the background cross sections are illustrated. For the recombination process, state-specific and total recombination rate coefficients are presented. These include both the radiative and dielectronic recombination processes. In addition, the total recombination spectrum with electron energy is presented and exhibits the resonant features that were observed experimentally. Recombination rates for hydrogenic He II is also presented. The present results obtained in LS coupling approximation provide a unified and self-consistent sets of results for astrophysical modelings of the two inverse radiative processes until highly accurate and precise results will be available through comprehensive relativistic calculations.
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Astronomy and Astrophysics
Authors
Sultana N. Nahar,