RADIATIVE STABILIZATION FOLLOWING DOUBLE-ELECTRON CAPTURE IN SLOW NE10++HE COLLISIONS

Individual contributions to radiative stabilization in Ne10+ +He colli sions were studied at projectile energies from 1 to 150 keV. In these collisions doubly excited states 3lnl' and 4lnl' (n greater than or eq ual to 4) can be produced by uncorrelated two-electron transitions or by dielectronic processes caused by the electron-electron interaction. Compared to our previous study of stabilization, we extended the proj ectile-energy range down to 1 keV and the present analysis is based en tirely on experimental data. Radiative stabilization was evaluated by combining our recent results for Auger decay cross sections with avail able radiative and nonradiative branching ratios. The total amount of radiative stabilization was found to be nearly constant (approximate t o 0.35) within the studied energy range. However, the individual contr ibutions to stabilization were found to change significantly. At 1 keV the major contribution to stabilization is shown to be due to the dec ay of the nonequivalent electron configurations 3lnl' (n greater than or equal to 6) produced during the collision by the dielectronic proce ss of autoexcitation. [S1050-2947(98)08010-X].