2001
DOI: 10.1006/adnd.2001.0869
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DIRAC–FOCK TRANSITION ENERGIES AND RADIATIVE AND RADIATIONLESS TRANSITION PROBABILITIES FOR Ar9+ TO Ar16+ ION LEVELS WITH K-SHELL HOLES

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Cited by 26 publications
(26 citation statements)
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“…This assessment is based on the assumption that the rate coefficient for inner shell ionization remains quasi-constant (supported by Ref. [8]) during the mixing gas sweep. Combining the results with heavier and lighter gases it is concluded that the most likely explanation fitting both observations is that the gas mixing affects the density of argon (at constant feed rate), thus favoring the ion cooling explanation.…”
Section: -1mentioning
confidence: 99%
“…This assessment is based on the assumption that the rate coefficient for inner shell ionization remains quasi-constant (supported by Ref. [8]) during the mixing gas sweep. Combining the results with heavier and lighter gases it is concluded that the most likely explanation fitting both observations is that the gas mixing affects the density of argon (at constant feed rate), thus favoring the ion cooling explanation.…”
Section: -1mentioning
confidence: 99%
“…A description of the mechanism leading to this spectrum can be found in Refs. Costa et al (2001); Martins et al (2001Martins et al ( , 2009); Santos et al (2010Santos et al ( , 2008Santos et al ( , 2011. The magnetic dipole (M1) transition has a natural width several orders of magnitude smaller than any line ever measured with a DCS until now.…”
Section: Resultsmentioning
confidence: 97%
“…One consequence of the ion creation and excited level population mechanisms described in Refs. Costa et al (2001); Martins et al (2001Martins et al ( , 2009Santos et al (2010Santos et al ( , 2008Santos et al ( , 2011 is that the 1s2s 3 S 1 level in He-like ions is strongly populated. It is created by ionization of the Li-like ion ground state 1s 2 2s.…”
Section: Ecrismentioning
confidence: 97%
“…Continuum-state wave functions were obtained by solving the Dirac-Fock equations with the same atomic potential of the initial state, normalized to represent one ejected electron per unit energy. Radiationless rates were, however, calculated using the correct transition energies obtained in previous independent calculations of initial and final state wave functions and eigenvalues [37][38][39].…”
Section: A Relativistic Calculationsmentioning
confidence: 99%