Production of very-low-energy highly charged ions by synchrotron radiation

Details Production of very-low-energy highly charged ions by synchrotron radiation Production of very-low-energy highly charged ions by synchrotron radiation

Jun 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986phrvl..56.2614s&link_type=abstract

Physical Review Letters (ISSN 0031-9007), vol. 56, June 16, 1986, p. 2614-2617. NSF-supported research.

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32

Charged Particles, Photoionization, Recoil Ions, Synchrotron Radiation, Room Temperature, Stellar Radiation, Time Of Flight Spectrometers, Auger Effect And Inner-Shell Excitation Or Ionization

Scientific paper

Very low-energy highly charged ions have been produced by use of white and monochromatic X rays from a wiggler line at the Stanford Synchrotron Radiation Laboratory to generate vacancy cascades following inner-shell photoionization. Recoil-ion energies have been determined and are shown to correspond essentially to room temperatures, even for high charge states. Promising applications to study of the interaction of stellar radiation with cold matter, to high-brightness ion-source development, to precision spectroscopy, and to angle-resolved chemical-physics reactive-scattering studies are discussed.

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