360 research outputs found

    In-beam spectroscopic studies of 44^{44}S nucleus

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    The structure of the 44^{44}S nucleus has been studied at GANIL through the one proton knock-out reaction from a 45^{45}Cl secondary beam at 42 A\cdotMeV. The γ\gamma rays following the de-excitation of 44^{44}S were detected in flight using the 70 BaF2{_2} detectors of the Ch\^{a}teau de Cristal array. An exhaustive γγ\gamma\gamma-coincidence analysis allowed an unambiguous construction of the level scheme up to an excitation energy of 3301 keV. The existence of the spherical 22+^+_2 state is confirmed and three new γ\gamma-ray transitions connecting the prolate deformed 21+^+_1 level were observed. Comparison of the experimental results to shell model calculations further supports a prolate and spherical shape coexistence with a large mixing of states built on the ground state band in 44^{44}S.Comment: 6 pages, 5 figures, accepted for publication in Physical Review

    First application of mass measurement with the Rare-RI Ring reveals the solar r-process abundance trend at A=122 and A=123

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    The Rare-RI Ring (R3) is a recently commissioned cyclotron-like storage ring mass spectrometer dedicated to mass measurements of exotic nuclei far from stability at Radioactive Isotope Beam Factory (RIBF) in RIKEN. The first application of mass measurement using the R3 mass spectrometer at RIBF is reported. Rare isotopes produced at RIBF, 127^{127}Sn, 126^{126}In, 125^{125}Cd, 124^{124}Ag, 123^{123}Pd, were injected in R3. Masses of 126^{126}In, 125^{125}Cd, and 123^{123}Pd were measured whereby the mass uncertainty of 123^{123}Pd was improved. This is the first reported measurement with a new storage ring mass spectrometery technique realized at a heavy-ion cyclotron and employing individual injection of the pre-identified rare nuclei. The latter is essential for the future mass measurements of the rarest isotopes produced at RIBF. The impact of the new 123^{123}Pd result on the solar rr-process abundances in a neutron star merger event is investigated by performing reaction network calculations of 20 trajectories with varying electron fraction YeY_e. It is found that the neutron capture cross section on 123^{123}Pd increases by a factor of 2.2 and β\beta-delayed neutron emission probability, P1nP_\mathrm{1n}, of 123^{123}Rh increases by 14\%. The neutron capture cross section on 122^{122}Pd decreases by a factor of 2.6 leading to pileup of material at A=122A=122, thus reproducing the trend of the solar rr-process abundances. The trend of the two-neutron separation energies (S2n_\mathrm{2n}) was investigated for the Pd isotopic chain. The new mass measurement with improved uncertainty excludes large changes of the S2n_\mathrm{2n} value at N=77N=77. Such large increase of the S2n_\mathrm{2n} values before N=82N=82 was proposed as an alternative to the quenching of the N=82N=82 shell gap to reproduce rr-process abundances in the mass region of A=112124A=112-124

    Spectroscopic factor and proton formation probability for the d3/2 proton emitter 151mLu

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    The quenching of the experimental spectroscopic factor for proton emission from the short-lived d3/2 isomeric state in 151mLu was a long-standing problem. In the present work, proton emission from this isomer has been reinvestigated in an experiment at the Accelerator Laboratory of the University of Jyväskylä. The proton-decay energy and half-life of this isomer were measured to be 1295(5) keV and 15.4(8) μs, respectively, in agreement with another recent study. These new experimental data can resolve the discrepancy in the spectroscopic factor calculated using the spherical WKB approximation. Using the R-matrix approach it is found that the proton formation probability indicates no significant hindrance for the proton decay of 151mLu
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