Stepwise ionization of Mo ions in EBIT: The importance of the metastable level
arXiv:2405.00893 · doi:10.1103/physreva.111.042818
Abstract
The visible spectrum of Mo ions was measured using a high-temperature superconducting electron-beam ion trap at the Shanghai EBIT Laboratory, with an electron beam energy =400 eV, significantly lower than the ionization potential (IP=544.0 eV) of Mo ions in the ground state. To expound on the experiment, the energy level structure, radiative transition properties, electron-impact excitation, and electron-impact ionization cross section for both the ground state and low-lying excited state of the Mo ions were calculated using Dirac-Fock-Slater method with a local central potential and distorted wave approximation. The results demonstrated reasonable agreement with both available experimental and theoretical data. Through an analysis of the related atomic processes of Mo ion, a scenario involving the stepwise ionization of the metastable state 3p3d4s was proposed to explain the presence of the Mo ions with a lower energy of the incident electron. Finally, the significance of the metastable levels in ionizing Mo ions is highlighted.
References in corpus (11)
- Highly-charged ions for atomic clocks, quantum information, and search for -variation
- Measurement of the SD transition in hydrogen
- Multipole (E1, M1, E2, M2, E3, M3) transition wavelengths and rates between 3l5l' excited and ground states in nickel-like ions
- Study of highly-charged Ag-like and In-like ions for the development of atomic clocks and search for -variation
- Detection of metastable electronic states by Penning trap mass spectrometry
- Atomic properties of Cd-like and Sn-like ions for the development of frequency standards and search for the variation of the fine-structure constant
- Observation of indirect ionization of W7+ in an electron-beam ion-trap plasma
- Visible spectra of W8+ in an electron-beam ion trap
- Hyperfine-structure-resolved laser spectroscopy of many-electron highly charged ions
- Measurement of the Kr XVIII 3d lifetime at low energy in a unitary Penning trap
- Application of a magnetic-field-induced transition in Fe X to solar and stellar coronal magnetic field measurements