Back to Search Start Over

Search for octupole-deformed actinium isotopes using resonance ionization spectroscopy.

Authors :
Verstraelen, E.
Teigelhöfer, A.
Ryssens, W.
Ames, F.
Barzakh, A.
Bender, M.
Ferrer, R.
Goriely, S.
Heenen, P. -H.
Huyse, M.
Kunz, P.
Lassen, J.
Manea, V.
Raeder, S.
Van Duppen, P.
Source :
Physical Review C. Oct2019, Vol. 100 Issue 4, p1-1. 1p.
Publication Year :
2019

Abstract

In-source resonance ionization spectroscopy of the neutron-rich actinium isotopes 225-229Ac has been performed at the ISAC facility in TRIUMF, probing a ²D3/2→4P∘5/2 atomic transition. New data on the magnetic dipole moments and changes in mean-square charge radii δ⟨r²⟩ of 226,228,229Ac have been obtained. The comparison of the measured isotope shifts and magnetic dipole coupling constants a(4P∘5/2) of 225,227Ac with a high-resolution data set is used to identify systematic uncertainties on the deduced δ⟨r²⟩A,215 and magnetic dipole moment values. The charge radii odd-even staggering is evaluated for the odd-N isotopes, showing that 226Ac has an inverted odd-even staggering that might be linked with a reflection-asymmetric shape. Comparison of the magnetic dipole moments of 225,227,229Ac with Nilsson-model estimates supports the assumption of octupole deformation in isotopes 225,227Ac and its gradual decrease toward isotope 229Ac. The changes in mean-square charge radii are compared to self-consistent calculations employing multiple modern energy density functionals: SLy5s1, BSk31, and DD-MEB1. For SLy5s1 in particular, self-consistent time-reversal breaking calculations of odd-odd nuclei incorporating finite octupole deformation are reported for the first time. For these calculations, the overall best agreement is obtained when the octupole degree of freedom is taken into account. [ABSTRACT FROM AUTHOR]

Details

Language :
English
ISSN :
24699985
Volume :
100
Issue :
4
Database :
Academic Search Index
Journal :
Physical Review C
Publication Type :
Academic Journal
Accession number :
139577560
Full Text :
https://doi.org/10.1103/PhysRevC.100.044321