6533b858fe1ef96bd12b5779

RESEARCH PRODUCT

Decay properties of exoticN≃28 S and Cl nuclei and theCa48/46Ca abundance ratio

M. LewitowiczFriedrich-karl ThielemannKarl KratzWolfgang HillebrandtO. SorlinS. M. LukyanovC. BorceaYu. E. PenionzhkevichR. AnneW. ZiegertS. DognyM. G. Saint-laurentV. S. SalamatinA. WöhrA.c. MuellerL.k. FifieldV. BorrelB. PfeifferD. Guillemaud-muellerH. GabelmannD. BazinF. PougheonC. Détraz

subject

Nuclear physicsBaryonPhysicsNuclear reactionNuclear and High Energy PhysicsHadronNuclear structureIsotopes of chlorineNeutronAtomic physicsNuclear ExperimentNucleonRadioactive decay

description

Beta-decay half-lives and \ensuremath{\beta}-delayed neutron-emission probabilities of the very neutron-rich nuclei $^{44}\mathrm{S}$ and $^{45--47}\mathrm{Cl}$ have been measured. These isotopes, which lie at or close to the N=28 magic shell, were produced in interactions of a 60 MeV/u $^{48}\mathrm{Ca}$ beam from GANIL (Grand Acc\'el\'erateur National d'Ions Lourds) with a $^{64}\mathrm{Ni}$ target, and were separated by the doubly achromatic spectrometer LISE (Ligne d'Ions Super Epluch\'es). Their decay was studied by a \ensuremath{\beta}-n time correlation measurement. The results are compared to recent model predictions and indicate a rapid weakening of the N=28 shell effect below $_{20}^{48}\mathrm{Ca}_{28}$. The nuclear structure effects reflected in the decay properties of the exotic S and Cl isotopes may be the clue for the astrophysical understanding of the unusual $^{48}\mathrm{Ca}$${/}^{46}$Ca abundance ratio measured in the solar system as well as the Ca-Ti-Cr anomalies observed in E. King inclusions of the Allende meteorite.

https://doi.org/10.1103/physrevc.47.2941