Electron impact excitation of Hg+

D. H. Crandall, R. A. Phaneuf, and Gordon H. Dunn
Phys. Rev. A 11, 1223 – Published 1 April 1975
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Abstract

Crossed beams of electrons and Hg+ ions have been employed to measure absolute cross sections for 165.0-nm emission, corresponding to the transition Hg+(6pP3202)Hg+(6sS122). The emission cross section, which is nearly identical to the excitation cross section for Hg+(6pP3202) near threshold, has a value of about 1.2 × 1016 cm2 at the 7.51-eV threshold, rises to a maximum of 2.26 × 1016 cm2 at 13 eV, and falls to 0.64 × 1016 cm2 at 274 eV. The cross section exhibits considerable structure in the energy region from threshold to the onset of the first cascade (7sS122) at 11.9 eV; this structure is likely due to interference from autoionizing states of neutral Hg. The total uncertainty at a "good" confidence level is about 18%, taken as the quadrature sum of random uncertainty (5% at 90% confidence level) with systematic uncertainties (17% at a level equivalent to 90% confidence level). At threshold, the Gaunt-factor formula of Seaton predicts a value of about 3 times that measured, but the two converge to within about 15% for electron energies ranging from 13 to 274 eV. The results are also in reasonable agreement with a semiclassical Gryzinski-type calculation for energies above several times threshold. The data give an emission cross section of (2.8 ± 0.5) × 1016 cm2 at 6.8 eV for 194.2 nm (6pP12026sS122). Analysis of data taken with some metastable 6s2D2 ions in the target beam indicates that the mean cross section for excitation of the 6sP3202 level from the 6s2D2 metastable states is larger than that for excitation from the 6sS122 ground state. Additional measurements of 398.4-nm emission (6pP32026s2D522) yield a cross section of about 6 × 1019 cm2 near threshold, and a branching ratio (P322S122)(P322D522) of 3501.

  • Received 25 November 1974

DOI:https://doi.org/10.1103/PhysRevA.11.1223

©1975 American Physical Society

Authors & Affiliations

D. H. Crandall*, R. A. Phaneuf, and Gordon H. Dunn

  • Joint Institute for Laboratory Astrophysics, University of Colorado and National Bureau of Standards, Boulder, Colorado 80302

  • *Present address: Thermonuclear Division, Oak Ridge National Laboratory, Oak Ridge, Tenn. 37830.
  • National Research Council of Canada Postdoctorate Fellow (1973-1975)
  • Staff Member, Laboratory Astrophysics Division, National Bureau of Standards.

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Vol. 11, Iss. 4 — April 1975

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