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arXiv · 1703.04250

Isotope shift and search for metastable superheavy elements in astrophysical data

V. A. Dzuba·V. V. Flambaum·J. K. Webb
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Abstract

Spectral lines belonging to the short-lifetime heavy radioactive elements up to Es ($Z$=99) have been found in the spectra of the Przybylski's star. We suggest that these unstable elements may be decay products of a "magic" metastable nucleus belonging to the the island of stability where the nuclei have a magic number of neutrons $N=184$. The laboratory-produced nuclei have a significantly smaller number of neutrons. To identify spectra of the $N=184$ isotopes of these nuclei and their neutron-reach superheavy decay products in astrophysical data we calculate the isotope shift which should be added to the laboratory - measured wavelenghs. The results for the isotopic shifts in the strongest optical electromagnetic transitions in No, Lr, Nh, Fl,and $Z$=120 elements are presented.

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V. A. Dzuba, V. V. Flambaum, J. K. Webb. 2017-03-13. Isotope shift and search for metastable superheavy elements in astrophysical data. https://doi.org/10.1103/physreva.95.062515

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