2022
DOI: 10.1103/physreva.105.052804
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X-ray emission associated with radiative recombination for Pb82+ ions at threshold energies

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Cited by 11 publications
(16 citation statements)
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“…In the case of the Balmer series, a multitude of transitions, basically due to the fine-structure splitting of the n = 2 and n = 3 states, are clearly visible in both X-ray detectors. Following the radiative cascade simulation procedure [22], the most populated states 3d 5/2 and 3d 3/2 resulting from Yrast-Cascades chain contribute to the formation of two intense Balmer lines, which are the transitions of 3d 5/2 → 2p 3/2 (Balmer-α 1 ) and 3d 3/2 → 2p 1/2 (Balmer-α 2 ), as observed in this experiment shown in Figure 2. Only small discrepancies are observed in the region of Paschen lines.…”
Section: Data Analysis and Resultsmentioning
confidence: 62%
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“…In the case of the Balmer series, a multitude of transitions, basically due to the fine-structure splitting of the n = 2 and n = 3 states, are clearly visible in both X-ray detectors. Following the radiative cascade simulation procedure [22], the most populated states 3d 5/2 and 3d 3/2 resulting from Yrast-Cascades chain contribute to the formation of two intense Balmer lines, which are the transitions of 3d 5/2 → 2p 3/2 (Balmer-α 1 ) and 3d 3/2 → 2p 1/2 (Balmer-α 2 ), as observed in this experiment shown in Figure 2. Only small discrepancies are observed in the region of Paschen lines.…”
Section: Data Analysis and Resultsmentioning
confidence: 62%
“…In practice, however, one may expect that, apart from the direct recombination, the feeding transitions from high-lying levels will also contribute to the population of the ionic substates. In this way, states with main quantum number n = 1 up to high-Rydberg states such as n = 165 were incorporated in the description of subsequent cascade processes [22] by solving a couple of rate equations [23], written as…”
Section: Data Analysis and Resultsmentioning
confidence: 99%
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“…For each setting of (N photon , ∆E FWHM ), we employed a Monte Carlo method to generate 500 synthetic N, M → L spectra. The N, M → L transition energies were calculated using the Flexible Atomic Code (FAC) [20,21] and the line intensities were predicted using a detailed model of the initial population by the RR process in combination with the subsequent decay cascades [16]. When setting the kinetic energy of the ion beam to 10.225 MeV/u, i.e., identical to the recent measurement, the simulation yields spectra very similar to the experimental data.…”
Section: Resultsmentioning
confidence: 93%
“…Due to the selection rules in combination with the high orbital angular momentum of the initially populated states, most of the recombined electrons pass through a state with the highest orbital angular momentum for a given shell at some point during their cascade. Therefore, the formation of an U 90+ ion in the cooler section typically results in the emission of numerous characteristic photons along a yrast decay pattern [15,16].…”
Section: Resultsmentioning
confidence: 99%