L1−L2,3M4,5Coster-Kronig transition thresholds in the region37≤Z≤56
- 1 April 1979
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review A
- Vol. 19 (4), 1433-1438
- https://doi.org/10.1103/physreva.19.1433
Abstract
The and Coster-Kronig transition thresholds in the atomic-number region are determined by bombardment of these elements with 2.5-MeV ions, and detection of the resulting x rays with a curved-crystal spectrometer. The intensities of both the and satellites, along with the total intensities of the , , and x rays which are produced during these collisions, are dependent upon the energetic permissibility of these Coster-Kronig transitions. The discontinuous nature of the intensity ratios as functions of atomic number indicates that the and transitions are energetically allowed for the elements with atomic numbers in the regions and , respectively.
This publication has 25 references indexed in Scilit:
- Wavelength-dispersion analysis of pixe spectraNuclear Instruments and Methods, 1977
- Theoretical L-shell Coster-Kronig energies 11 ≤ Z ≤ 103Atomic Data and Nuclear Data Tables, 1977
- Predictions of inner-shell Coulomb ionization by heavy charged particlesAtomic Data and Nuclear Data Tables, 1975
- X-Ray Fluorescence Yields, Auger, and Coster-Kronig Transition ProbabilitiesReviews of Modern Physics, 1972
- Atomic-Shell Coster-Kronig, Auger, and Radiative Rates, and Fluorescence Yields for Ca-ThPhysical Review A, 1972
- Dependence of fluorescence yield on atomic configurationJournal of Physics B: Atomic and Molecular Physics, 1971
- Range and stopping-power tables for heavy ionsAtomic Data and Nuclear Data Tables, 1970
- Widths of theandX-Ray Lines forPhysical Review B, 1969
- Radiative Decay Rates of Vacancies in theandShellsPhysical Review B, 1969
- New type of auger effect and its influence on the x-ray spectrumPhysica, 1935