Abstract

Photoelectron angular distributions should show pronounced variations with energy across autoionization resonances. This prediction applies quite generally to both atomic and molecular autoionization. Examples illustrate both the magnitude of the spectral variation and the inability of the Cooper-Zare model to account for the phenomenon. Calculations are reported for autoionization in xenon between the fine-structure levels $5{p}^{5} ^{2}P_{\frac{3}{2}}^{\ensuremath{\circ}}$ and $5{p}^{5} ^{2}P_{\frac{1}{2}}^{\ensuremath{\circ}}$ of the ion ground-state doublet. An analysis is given of the recent measurements by Niehaus and Ruf on autoionizing levels of the mercury Rydberg series $5{d}^{9}6{s}^{2}(^{2}D)np$ and $5{d}^{9}6{s}^{2}(^{2}D){n}^{\ensuremath{'}}f$ below the ${\mathrm{Hg}}^{+}$ $5{d}^{9}6{s}^{2} ^{2}D_{\frac{5}{2}}$ threshold.

Full Text
Paper version not known

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call

Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.