140 research outputs found

    Consolidating the concept of low-energy magnetic dipole decay radiation

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    We have made a thorough study of the low-energy behaviour of the γ\gamma-ray strength function within the framework of the shell model. We have performed large-scale calculations spanning isotopic and isotonic chains over several mass regions, with the purpose of studying the systematic behavior of the low-energy enhancement (LEE) for M1M1 transitions. There are clear trends in the calculations: From being all but absent in the lowest mass region, the LEE becomes steeper and more pronounced as the mass number increases, and for a given mass region it further increases towards shell closures. Moreover, the LEE is found to be steeper in regions near doubly-magic nuclei where proton particles couple to neutron holes. These trends enable us to consolidate several previous works on the LEE into a single, consistent concept. We compare the inferred trends to the available experimental data from the Oslo method, and find suppport for the systematic behaviour. Lastly we have compared the calculations to strength functions compiled from discrete, experimental lifetimes, and find excellent agreement; the discrete data are consistent with a LEE, and indicate that the slope varies as function of mass number.Comment: 11 pages, 13 figure

    Observation of large scissors resonance strength in actinides

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    The orbital M1-scissors resonance (SR) has been measured for the first time in the quasi-continuum of actinides. Particle-gamma coincidences are recorded with deuteron and 3He induced reactions on 232Th. The residual nuclei 231,232,233Th and 232,233Pa show an unexpectedly strong integrated strength of BM1=1115μn2B_{M1} = 11-15 \mu_{n}^{2} in the Egamma=1.0 - 3.5 MeV region. The increased gamma-decay probability in actinides due to the SR is important for cross-section calculations for future fuel cycles of fast nuclear reactors and may also have impact on stellar nucleosynthesis.Comment: 5 pages and 4 figure

    Quasicontinuum γ\gamma-decay of 91,92^{91,92}Zr: benchmarking indirect (n,γn,\gamma) cross section measurements for the ss-process

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    Nuclear level densities (NLDs) and γ\gamma-ray strength functions (γ\gammaSFs) have been extracted from particle-γ\gamma coincidences of the 92^{92}Zr(p,pγp,p' \gamma)92^{92}Zr and 92^{92}Zr(p,dγp,d \gamma)91^{91}Zr reactions using the Oslo method. The new 91,92^{91,92}Zr γ\gammaSF data, combined with photonuclear cross sections, cover the whole energy range from Eγ1.5E_{\gamma} \approx 1.5~MeV up to the giant dipole resonance at Eγ17E_{\gamma} \approx 17~MeV. The wide-range γ\gammaSF data display structures at Eγ9.5E_{\gamma} \approx 9.5~MeV, compatible with a superposition of the spin-flip M1M1 resonance and a pygmy E1E1 resonance. Furthermore, the γ\gammaSF shows a minimum at Eγ23E_{\gamma} \approx 2-3~MeV and an increase at lower γ\gamma-ray energies. The experimentally constrained NLDs and γ\gammaSFs are shown to reproduce known (n,γn, \gamma) and Maxwellian-averaged cross sections for 91,92^{91,92}Zr using the {\sf TALYS} reaction code, thus serving as a benchmark for this indirect method of estimating (n,γn, \gamma) cross sections for Zr isotopes.Comment: 10 pages and 9 figure

    Gamma-widths, lifetimes and fluctuations in the nuclear quasi-continuum

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    Statistical γ\gamma-decay from highly excited states is determined by the nuclear level density (NLD) and the γ\gamma-ray strength function (γ\gammaSF). These average quantities have been measured for several nuclei using the Oslo method. For the first time, we exploit the NLD and γ\gammaSF to evaluate the γ\gamma-width in the energy region below the neutron binding energy, often called the quasi-continuum region. The lifetimes of states in the quasi-continuum are important benchmarks for a theoretical description of nuclear structure and dynamics at high temperature. The lifetimes may also have impact on reaction rates for the rapid neutron-capture process, now demonstrated to take place in neutron star mergers.Comment: CGS16, Shanghai 2017, Proceedings, 5 pages, 3 figure

    Level densities and thermodynamical properties of Pt and Au isotopes

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    The nuclear level densities of 194196^{194-196}Pt and 197,198^{197,198}Au below the neutron separation energy have been measured using transfer and scattering reactions. All the level density distributions follow the constant-temperature description. Each group of isotopes is characterized by the same temperature above the energy threshold corresponding to the breaking of the first Cooper pair. A constant entropy excess ΔS=1.9\Delta S=1.9 and 1.11.1 kBk_B is observed in 195^{195}Pt and 198^{198}Au with respect to 196^{196}Pt and 197^{197}Au, respectively, giving information on the available single-particle level space for the last unpaired valence neutron. The breaking of nucleon Cooper pairs is revealed by sequential peaks in the microcanonical caloric curve

    Novel technique for constraining r-process (n,γ\gamma) reaction rates

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    A novel technique has been developed, which will open exciting new opportunities for studying the very neutron-rich nuclei involved in the r-process. As a proof-of-principle, the γ\gamma-spectra from the β\beta-decay of 76^{76}Ga have been measured with the SuN detector at the National Superconducting Cyclotron Laboratory. The nuclear level density and γ\gamma-ray strength function are extracted and used as input to Hauser-Feshbach calculations. The present technique is shown to strongly constrain the 75^{75}Ge(n,γn,\gamma)76^{76}Ge cross section and reaction rate.Comment: 5 pages, 3 figure

    Scissors resonance in the quasi-continuum of Th, Pa and U isotopes

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    The gamma-ray strength function in the quasi-continuum has been measured for 231-233Th, 232,233Pa and 237-239U using the Oslo method. All eight nuclei show a pronounced increase in gamma strength at omega_SR approx 2.4 MeV, which is interpreted as the low-energy M1 scissors resonance (SR). The total strength is found to be B_SR = 9-11 mu_N^2 when integrated over the 1 - 4 MeV gamma-energy region. The SR displays a double-hump structure that is theoretically not understood. Our results are compared with data from (gamma, gamma') experiments and theoretical sum-rule estimates for a nuclear rigid-body moment of inertia.Comment: 11 pages, 9 figure
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