Abstract:N= 3, An=O transitions in Na-like ions have been observed and the resonance level lifetimes have been measured by time-resolved spectroscopy of foil-excited ion beams of Xe (Z = 54) and Au (Z = 79). Other lines in the same wavelength range are identified with n=3, An=O transitions in Ne-, Mg-, and Al-like ions. Wavelengths and transition rates for these new lines are compared to the available theoretical data. A number of experimental problems are discussed.
“…The experimental set-up of the beam-foil work on Xe and Au at the Darmstadt (Germany) GSI UNILAC accelerator has been described elsewhere [7][8][9]. This experimental arrangement has gone through various development stages; most of the experimental effort was directed at the precision spectroscopy of few-electron ions, in particular the determination of QED contributions to the transition energies of n = 2-2 transitions in Li-and Be-like ions [34][35][36][37][38].…”
Section: Experimental Datamentioning
confidence: 99%
“…The Xe experiment [7,8] aimed primarily at spectra from which decay curves of the resonance lines of Na-like Xe ions were to be constructed and then atomic level lifetimes and transition probabilities derived. The wavelengths of the 3s-3p-3d transitions in Na-like ions can be calculated well enough for such purpose.…”
Section: Experimental Datamentioning
confidence: 99%
“…However, a constant dispersion was a reasonable approximation for only two of the three spectral slices, but not for the third. At short wavelengths, the dispersion (wavelength interval divided by distance along the Rowland circle circumference) progressively changes, and it should not have been taken as constant in [8]. Taking the spectrometer geometry into better account (now for all spectral sections covered), changes the dispersion notably, so that-with reference to the same line of Na-like Xe in the short-wavelength spectrum-the probable identifications of several other lines change.…”
Section: Experimental Datamentioning
confidence: 99%
“…The 1995 beam-foil spectra [8] mostly cover three spectral sections within the wavelength range from 50-150 Å. The spectra have been recorded at various foil displacements (up to 28 positions) from the line of sight of the spectrometer, corresponding to observations in a range of delays after excitation.…”
Section: Comparison With Xe Beam-foil Spectramentioning
confidence: 99%
“…We resort to experimental data for atomic systems well beyond the bulk of well-analysed spectra, and thus with some uncertainty in the earlier line classifications. The data are from a series of beam-foil experiments on Xe and Au [7][8][9] that have, about a decade ago, pushed the envelope of such enterprises. (One of us, ET, was the lead author of those three studies, and some of the laboratory notes and other unpublished materials of the time are available to us for a re-investigation.)…”
“…The experimental set-up of the beam-foil work on Xe and Au at the Darmstadt (Germany) GSI UNILAC accelerator has been described elsewhere [7][8][9]. This experimental arrangement has gone through various development stages; most of the experimental effort was directed at the precision spectroscopy of few-electron ions, in particular the determination of QED contributions to the transition energies of n = 2-2 transitions in Li-and Be-like ions [34][35][36][37][38].…”
Section: Experimental Datamentioning
confidence: 99%
“…The Xe experiment [7,8] aimed primarily at spectra from which decay curves of the resonance lines of Na-like Xe ions were to be constructed and then atomic level lifetimes and transition probabilities derived. The wavelengths of the 3s-3p-3d transitions in Na-like ions can be calculated well enough for such purpose.…”
Section: Experimental Datamentioning
confidence: 99%
“…However, a constant dispersion was a reasonable approximation for only two of the three spectral slices, but not for the third. At short wavelengths, the dispersion (wavelength interval divided by distance along the Rowland circle circumference) progressively changes, and it should not have been taken as constant in [8]. Taking the spectrometer geometry into better account (now for all spectral sections covered), changes the dispersion notably, so that-with reference to the same line of Na-like Xe in the short-wavelength spectrum-the probable identifications of several other lines change.…”
Section: Experimental Datamentioning
confidence: 99%
“…The 1995 beam-foil spectra [8] mostly cover three spectral sections within the wavelength range from 50-150 Å. The spectra have been recorded at various foil displacements (up to 28 positions) from the line of sight of the spectrometer, corresponding to observations in a range of delays after excitation.…”
Section: Comparison With Xe Beam-foil Spectramentioning
confidence: 99%
“…We resort to experimental data for atomic systems well beyond the bulk of well-analysed spectra, and thus with some uncertainty in the earlier line classifications. The data are from a series of beam-foil experiments on Xe and Au [7][8][9] that have, about a decade ago, pushed the envelope of such enterprises. (One of us, ET, was the lead author of those three studies, and some of the laboratory notes and other unpublished materials of the time are available to us for a re-investigation.)…”
Als Helium zu Beginn des Jahrhunderts im Labor spektroskopisch untersucht wurde, schien es zwei völlig getrennte Termsysteme aufzuweisen, ein Singulett‐System, in dem die Spins der beiden Elektronen antiparallel stehen (Gesamtspin S = 0) und ein Triplett‐System mit parallel ausgerichteten Elektronenspins (S = 1). Diese beiden Termsysteme lassen sich mit Hilfe des Elektronenspins einfach erklären. Lange Zeit galten aber Übergänge zwischen Systemen mit verschiedenem Gesamtspin — sogenannte Interkombinationsübergänge — oder mit gleicher Parität als spektroskopisch „verboten”︁ oder doch zumindest als exotisch. Heute werden gerade diese Übergänge für die Diagnose von Plasmen auf der Erde und im Weltall genutzt. Nachdem für diese schwachen Linien viele Jahre lang nur grobe Abschätzungen der Übergangswahrscheinlichkeiten möglich waren, gelangen kürzlich präzise Messungen am Schwerionen‐Speicherring und an einer Elektronenstrahl‐Ionenfalle. Diese fordern die Theorie nun zu sehr aufwendigen Strukturrechnungen heraus.
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