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Impact of Nuclear Deformation and Pairing on the Charge Radii of Palladium Isotopes

Authors :
Geldhof, S.
Kortelainen, M.
Beliuskina, O.
Campbell, P.
Caceres, L.
Cañete, L.
Cheal, B.
Chrysalidis, K.
Devlin, C. S.
de Groote, R. P.
de Roubin, A.
Eronen, T.
Ge, Z.
Gins, W.
Koszorus, A.
Kujanpää, S.
Nesterenko, D.
Ortiz-Cortes, A.
Pohjalainen, I.
Moore, I. D.
Raggio, A.
Reponen, M.
Romero, J.
Sommer, F.
Grand Accélérateur National d'Ions Lourds (GANIL)
Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)
Source :
Physical Review Letters, Physical Review Letters, 2022, 128 (15), pp.152501. ⟨10.1103/PhysRevLett.128.152501⟩
Publication Year :
2021

Abstract

International audience; The impact of nuclear deformation can been seen in the systematics of nuclear charge radii, with radii generally expanding with increasing deformation. In this Letter, we present a detailed analysis of the precise relationship between nuclear quadrupole deformation and the nuclear size. Our approach combines the first measurements of the changes in the mean-square charge radii of well-deformed palladium isotopes between A=98 and A=118 with nuclear density functional calculations using Fayans functionals, specifically Fy(std) and Fy(Δr,HFB), and the UNEDF2 functional. The changes in mean-square charge radii are extracted from collinear laser spectroscopy measurements on the 4d95s D33→4d95p P23 atomic transition. The analysis of the Fayans functional calculations reveals a clear link between a good reproduction of the charge radii for the neutron-rich Pd isotopes and the overestimated odd-even staggering: Both aspects can be attributed to the strength of the pairing correlations in the particular functional which we employ.

Details

ISSN :
10797114 and 00319007
Volume :
128
Issue :
15
Database :
OpenAIRE
Journal :
Physical review letters
Accession number :
edsair.doi.dedup.....01960d33545212f72a729ff3b3778fe9
Full Text :
https://doi.org/10.1103/PhysRevLett.128.152501⟩