460 research outputs found

    Spectroscopy of 35^{35}P using the one-proton knockout reaction

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    The structure of 35^{35}P was studied with a one-proton knockout reaction at88~MeV/u from a 36^{36}S projectile beam at NSCL. The γ\gamma rays from thedepopulation of excited states in 35^{35}P were detected with GRETINA, whilethe 35^{35}P nuclei were identified event-by-event in the focal plane of theS800 spectrograph. The level scheme of 35^{35}P was deduced up to 7.5 MeV usingγγ\gamma-\gamma coincidences. The observed levels were attributed to protonremovals from the sdsd-shell and also from the deeply-bound p_1/2p\_{1/2} orbital.The orbital angular momentum of each state was derived from the comparisonbetween experimental and calculated shapes of individual (γ\gamma-gated)parallel momentum distributions. Despite the use of different reactions andtheir associate models, spectroscopic factors, C2SC^2S, derived from the36^{36}S (1p)(-1p) knockout reaction agree with those obtained earlier from36^{36}S(dd,\nuc{3}{He}) transfer, if a reduction factor R_sR\_s, as deducedfrom inclusive one-nucleon removal cross sections, is applied to the knockout transitions.In addition to the expected proton-hole configurations, other states were observedwith individual cross sections of the order of 0.5~mb. Based on their shiftedparallel momentum distributions, their decay modes to negative parity states,their high excitation energy (around 4.7~MeV) and the fact that they were notobserved in the (dd,\nuc{3}{He}) reaction, we propose that they may resultfrom a two-step mechanism or a nucleon-exchange reaction with subsequent neutronevaporation. Regardless of the mechanism, that could not yet be clarified, thesestates likely correspond to neutron core excitations in \nuc{35}{P}. Thisnewly-identified pathway, although weak, offers the possibility to selectivelypopulate certain intruder configurations that are otherwise hard to produceand identify.Comment: 5 figures, 1 table, accepted for publication in Physical Review

    Single-Proton Removal Reaction Study of 16B

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    The low-lying level structure of the unbound system 16^{16}B has been investigated via single-proton removal from a 35 MeV/nucleon 17^{17}C beam. The coincident detection of the beam velocity 15^{15}B fragment and neutron allowed the relative energy of the in-flight decay of 16^{16}B to be reconstructed. The resulting spectrum exhibited a narrow peak some 85 keV above threshold. It is argued that this feature corresponds to a very narrow (Γ\Gamma \ll 100 keV) resonance, or an unresolved multiplet, with a dominant π(p3/2)1ν(d5/23)J=3/2+\pi (p_{3/2})^{-1} \otimes \nu (d_{5/2}^3)_{J=3/2^+} + π(p3/2)1ν(d5/22,s1/2)J=3/2+\pi (p_{3/2})^{-1} \otimes \nu (d_{5/2}^2,s_{1/2})_{J=3/2^+} configuration which decays by d-wave neutron emission.Comment: 16 pages, 5 figures, 1 table, submitted to Phys. Lett.

    Unveiling the intruder deformed 02+^+_2 state in 34^{34}Si

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    The 02+^+_2 state in 34^{34}Si has been populated at the {\sc Ganil/Lise3} facility through the β\beta-decay of a newly discovered 1+^+ isomer in 34^{34}Al of 26(1) ms half-life. The simultaneous detection of e+ee^+e^- pairs allowed the determination of the excitation energy E(02+^+_2)=2719(3) keV and the half-life T1/2_{1/2}=19.4(7) ns, from which an electric monopole strength of ρ2\rho^2(E0)=13.0(0.9)×103\times10^{-3} was deduced. The 21+^+_1 state is observed to decay both to the 01+^+_1 ground state and to the newly observed 02+^+_2 state (via a 607(2) keV transition) with a ratio R(21+^+_101+/21+\rightarrow0^+_1/2^+_102+\rightarrow0^+_2)=1380(717). Gathering all information, a weak mixing with the 01+^+_1 and a large deformation parameter of β\beta=0.29(4) are found for the 02+^+_2 state, in good agreement with shell model calculations using a new {\sc sdpf-u-mix} interaction allowing \textit{np-nh} excitations across the N=20 shell gap.Comment: 5 pages, 3 figures, accepted for publication in Physical Review Letter

    First observation of 54Zn and its decay by two-proton emission

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    The nucleus 54Zn has been observed for the first time in an experiment at the SISSI/LISE3 facility of GANIL in the quasi-fragmentation of a 58Ni beam at 74.5 MeV/nucleon in a natNi target. The fragments were analysed by means of the ALPHA-LISE3 separator and implanted in a silicon-strip detector where correlations in space and time between implantation and subsequent decay events allowed us to generate almost background free decay spectra for about 25 different nuclei at the same time. Eight 54Zn implantation events were observed. From the correlated decay events, the half-life of 54Zn is determined to be 3.2 +1.8/-0.8 ms. Seven of the eight implantations are followed by two-proton emission with a decay energy of 1.48(2) MeV. The decay energy and the partial half-life are compared to model predictions and allow for a test of these two-proton decay models.Comment: 4 pages, 4 figures, accepted for publication in PR

    Prolate-Spherical Shape Coexistence at N=28 in 44^{44}S

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    The structure of 44^{44}S has been studied using delayed γ\gamma and electron spectroscopy at \textsc{ganil}. The decay rates of the 02+^+_2 isomeric state to the 21+^+_1 and 01+^+_1 states have been measured for the first time, leading to a reduced transition probability B(E2~:~21+^{+}_1\rightarrow02+)^{+}_2)= 8.4(26)~e2^2fm4^4 and a monopole strength ρ2\rho^2(E0~:~02+^{+}_2\rightarrow01+)^{+}_1) =~8.7(7)×\times103^{-3}. Comparisons to shell model calculations point towards prolate-spherical shape coexistence and a phenomenological two level mixing model is used to extract a weak mixing between the two configurations.Comment: 5 pages, 3 figures, accepted for publication in Physical Review Letter

    Spectroscopy of 26^{26}F

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    The structure of the weakly-bound     926^{26}_{\;\;9}F17_{17} odd-odd nucleus, produced from 27,28^{27,28}Na nuclei, has been investigated at GANIL by means of the in-beam γ\gamma-ray spectroscopy technique. A single γ\gamma-line is observed at 657(7) keV in 926^{26}_{9}F which has been ascribed to the decay of the excited J=2+2^+ state to the J=1+^+ ground state. The possible presence of intruder negative parity states in 26^{26}F is also discussed.Comment: 3 pages, 1 figure, accepted for publication in Physical Review

    Probing Nuclear forces beyond the drip-line using the mirror nuclei 16^{16}N and 16^{16}F

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    Radioactive beams of 14^{14}O and 15^{15}O were used to populate the resonant states 1/2+^+, 5/2+^+ and 0,1,20^-,1^-,2^- in the unbound 15^{15}F and 16^{16}F nuclei respectively by means of proton elastic scattering reactions in inverse kinematics. Based on their large proton spectroscopic factor values, the resonant states in 16^{16}F can be viewed as a core of 14^{14}O plus a proton in the 2s1/2_{1/2} or 1d5/2_{5/2} shell and a neutron in 1p1/2_{1/2}. Experimental energies were used to derive the strength of the 2s1/2_{1/2}-1p1/2_{1/2} and 1d5/2_{5/2}-1p1/2_{1/2} proton-neutron interactions. It is found that the former changes by 40% compared with the mirror nucleus 16^{16}N, and the second by 10%. This apparent symmetry breaking of the nuclear force between mirror nuclei finds explanation in the role of the large coupling to the continuum for the states built on an =0\ell=0 proton configuration.Comment: 6 pages, 3 figures, 2 tables, accepted for publication as a regular article in Physical Review

    New pathway to bypass the 15O waiting point

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    We propose the sequential reaction process 15^{15}O(pp,γ)(β+\gamma)(\beta^{+})16^{16}O as a new pathway to bypass of the 15^{15}O waiting point. This exotic reaction is found to have a surprisingly high cross section, approximately 1010^{10} times higher than the 15^{15}O(pp,β+\beta^{+})16^{16}O. These cross sections were calculated after precise measurements of energies and widths of the proton-unbound 16^{16}F low lying states, obtained using the H(15^{15}O,p)15^{15}O reaction. The large (p,γ)(β+)(p,\gamma)(\beta^{+}) cross section can be understood to arise from the more efficient feeding of the low energy wing of the ground state resonance by the gamma decay. The implications of the new reaction in novae explosions and X-ray bursts are discussed.Comment: submitte
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