2010
DOI: 10.1103/physreva.81.053416
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Valence-shell photoionization of the chlorinelike Ca3+ion

Abstract: Absolute photoionization measurements were performed for a mixture of 2 P o 3/2 ground-state and 2 P o 1/2 metastable-state Ca 3+ ions over the photon energy range 65.7-104.6 eV by merging an ion beam with a beam of monochromatized synchrotron radiation. The ionization threshold energy of the 2 P o 3/2 ground state was measured to be 67.063 ± 0.015 eV, which is 0.207 eV lower than the value tabulated in the NIST database. Most of the observed resonances associated with multiple Rydberg series of autoionizing s… Show more

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Cited by 19 publications
(14 citation statements)
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“…Initial measurements of photoionization cross sections for O + ions [18] and C 2+ ions [20] using the IPB end station were reported in the literature. The ALS group has recently reported detailed experimental and theoretical studies on the Cl-like calcium (Ca 3+ ) ion [26] in addition to a variety of other singly and multiply charged ions, particularly of astrophysical interest, using this same IPB end station: He-like; Li + [27,28], Li-like; B 2+ [29], Be-like; C 2+ [30], B + [31], C 2+ , N 3+ , and O 4+ [22,32], B-like; C + [33], F-like; Ne + [10], N-like ions; O + [18], F 2+ and Ne 3+ [11]. These high-resolution experimental results enable theoretical studies to be benchmarked, so that the resulting data can be used with confidence in various astrophysical applications that utilize modeling codes such as CLOUDY [34,35] and XSTAR [36].…”
Section: Methodsmentioning
confidence: 99%
“…Initial measurements of photoionization cross sections for O + ions [18] and C 2+ ions [20] using the IPB end station were reported in the literature. The ALS group has recently reported detailed experimental and theoretical studies on the Cl-like calcium (Ca 3+ ) ion [26] in addition to a variety of other singly and multiply charged ions, particularly of astrophysical interest, using this same IPB end station: He-like; Li + [27,28], Li-like; B 2+ [29], Be-like; C 2+ [30], B + [31], C 2+ , N 3+ , and O 4+ [22,32], B-like; C + [33], F-like; Ne + [10], N-like ions; O + [18], F 2+ and Ne 3+ [11]. These high-resolution experimental results enable theoretical studies to be benchmarked, so that the resulting data can be used with confidence in various astrophysical applications that utilize modeling codes such as CLOUDY [34,35] and XSTAR [36].…”
Section: Methodsmentioning
confidence: 99%
“…A detailed description of the IPB apparatus was given by Covington et al [8], with recent modifications described by Alna'Washi et al [9]. Se ions were produced by placing pellets of solid Se within an all-permanent-magnet electron-cyclotron-resonance (ECR) ion source similar to that reported by Broetz et al [10] and Trassl et al [11].…”
Section: Methodsmentioning
confidence: 99%
“…The photoionization measurements were performed using the ion photon beam (IPB) end station on the ALS undulator beamline 10.0.1 [23,24]. A collimated and mass-selected beam of 136 Xe@C + 60 ions was electrostatically guided onto the axis of a counterpropagating beam of monochromatized synchrotron radiation.…”
Section: A Experimentsmentioning
confidence: 99%