Nobelium energy levels and hyperfine structure constants
S.G. Porsev, M.S. Safronova, U.I. Safronova, V.A. Dzuba, and V.V., Flambaum

TL;DR
This paper presents high-precision calculations of hyperfine structure constants and energy levels for nobelium, aiding nuclear property extraction and advancing atomic modeling of superheavy elements.
Contribution
The study introduces a hybrid computational approach combining coupled-cluster and configuration interaction methods for nobelium, with extensive energy level analysis including f-shell effects.
Findings
Small mixing of low-lying levels with filled and unfilled f shells.
Calculated HFS constants for key nobelium states.
Support for nuclear property extraction from spectroscopy data.
Abstract
Advances in laser spectroscopy of superheavy () elements enabled determination of the nuclear moments of the heaviest nuclei, which requires high-precision atomic calculations of the relevant hyperfine structure (HFS) constants. Here, we calculated the HFS constants and energy levels for a number of nobelium (Z=102) states using the hybrid approach, combining linearized coupled-cluster and configuration interaction methods. We also carried out an extensive study of the No energies using 16-electron configuration interaction method to determine the position of the (5f^{13}7s^2 6d) and (5f^{13}7s^2 7p) levels with a hole in the 5f shell to evaluate their potential effect on the hyperfine structure calculations of the low-lying (5f^{14}7s6d) and (5f^{14}7s7p) levels. We find that unlike the case of Yb, the mixing of the low-lying levels with filled and unfilled f shell is small and…
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