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Phys. Rev. A 60, 1187–1198 (1999)

Polarization study of the extreme-ultraviolet emission from helium following electron impact

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H. Merabet, M. Bailey*, and R. Bruch
Department of Physics, University of Nevada Reno, Reno, Nevada 89557

D. V. Fursa and I. Bray
Electronic Structure of Materials Centre, The Flinders, University of South Australia, G.P.O. Box 2100, Adelaide 5001, Australia

J. W. McConkey
Department of Physics, University of Windsor, Windsor, Ontario, Canada N9B 3P4

P. Hammond
Department of Physics, University of Manchester, Manchester M13 9PL, England

Received 11 February 1999; published in the issue dated August 1999

Experimental results are presented on the degree of linear polarization of the extreme-ultraviolet emission of neutral and ionized helium following electron-impact excitation and ionization excitation of helium. The polarization of the photon emission from the decay of He (1snp)1Po states with wavelengths of 517 to 584 Å has been extended to electron-impact energies of 1500 eV, and compared with theory for electron-impact excitation of neutral helium. In addition, the polarization of a number of the He+ decays with wavelengths between 256 and 1640 Å have been measured. Particular attention has been paid to the (2p)2Po→(1s)2S and (3p)2Po→(1s)2S decays with wavelengths of 304 and 256 Å, respectively. These have been measured from threshold (66 and 73 eV, respectively) to 1500 eV using a characterized molybdenum/silicon multilayer mirror polarimeter whose reflection and polarization characteristics have been optimized at 304 Å He+(2p)2Po results are compared with a recent threshold alignment measurement and distorted-wave Born-approximation calculation for the (e-,2e-) reaction of ionization excitation. Very good agreement with the threshold theoretical predictions is obtained. These results indicate that near threshold, partial waves with L>0 contribute substantially to the two-electron wave function of the escaping electrons. Measurements on the unresolved multiplets at 1215 and 1640 Å, made using a more conventional reflection-type polarization analyzer, indicate that relative fine-structure cross sections are quite different than predicted by some theories.

© 1999 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevA.60.1187
DOI:
10.1103/PhysRevA.60.1187
PACS:
34.80.Dp

*Present address: Atmospheric Science Center, Desert Research Institute (DRI), Reno, NV 89506.