Influence of host matrices on krypton electron binding energies and KLL Auger transition energies
A. Kh. Inoyatov, L.L. Perevoshchikov, A. Koval\'ik, D.V. Filosofov,, Yu.V. Yushkevich, M. Ry\v{s}av\'y, B.Q. Lee, T. Kib\'edi, A.E. Stuchbery and, V.S. Zhdanov

TL;DR
This study measures how host matrices affect krypton electron binding energies and Auger transition energies, revealing small shifts and providing experimental data alongside theoretical calculations for different host environments.
Contribution
It provides new experimental measurements of krypton electron binding and Auger energies in different host matrices and compares them with multiconfiguration Dirac-Fock calculations.
Findings
Krypton binding energies are slightly lower in evaporated Rb compared to platinum.
Measured Auger transition energies in krypton are around 10.84 keV.
Host matrix influences on electron energies are quantified and modeled.
Abstract
The low-energy electron spectra emitted in the radioactive decay of the Rb and Sr isotopes were measured with a combined electrostatic electron spectrometer. Radioactive sources used were prepared by ion implantation of Sr into a high purity polycrystalline platinum foil at 30 keV and by vacuum-evaporation deposition of Rb on the same type of foil. From the measured conversion electron spectra, the electron binding energies (referenced to the Fermi level) for the K, L , L , L , M , M, and M shell/subshells of krypton in the platinum host were determined to be 14 316.4(12), 1 914.3(9), 1 720.3(9), 1 667.6(9), 281.5(9), 209.6(13), and 201.2(15) eV, respectively, and those for the evaporated layer were observed to be lower by 0.7(1) eV. For both host matrices, values of 2.3(2), 4.6(2), 1.7(2), 1.3(2), and 3.2(3) eV were obtained for…
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