6533b871fe1ef96bd12d2272
RESEARCH PRODUCT
Neutron Skin Effects in Mirror Energy Differences: The Case of Mg23−Na23
F. Ghazi-moradiK JuhászBo CederwallA. BosoIstván KutiV. ModamioP. R. JohnA. GadeaD. R. NapoliT. HüyükM. A. BentleyJohan NybergS. M. LenziT. W. HenryB. M. NyakóEric ClémentB. MelonA. DijonSibel Zehra AydinA. GottardoJános TimárJ. BonnardMaria DoncelG. JaworskiM. PalaczD. MengoniC. MichelagnoliJ. J. Valiente-dobónA. Di NittoA. P. ZukerA. P. ZukerF. Recchiasubject
PhysicsProton010308 nuclear & particles physicsYrastNuclear TheoryShell (structure)General Physics and Astronomy01 natural sciences0103 physical sciencesOrbit (dynamics)NeutronHaloMirror nucleiAtomic physicsNuclear Experiment010306 general physicsEnergy (signal processing)description
Energy differences between analogue states in the T=1/2 Mg23-Na23 mirror nuclei have been measured along the rotational yrast bands. This allows us to search for effects arising from isospin-symmetry-breaking interactions (ISB) and/or shape changes. Data are interpreted in the shell model framework following the method successfully applied to nuclei in the f7/2 shell. It is shown that the introduction of a schematic ISB interaction of the same type of that used in the f7/2 shell is needed to reproduce the data. An alternative novel description, applied here for the first time, relies on the use of an effective interaction deduced from a realistic charge-dependent chiral nucleon-nucleon potential. This analysis provides two important results: (i) The mirror energy differences give direct insight into the nuclear skin; (ii) the skin changes along the rotational bands are strongly correlated with the difference between the neutron and proton occupations of the s1/2 "halo" orbit.
year | journal | country | edition | language |
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2018-07-19 | Physical Review Letters |