2,241 research outputs found

    Solar Neutrinos from CNO Electron Capture

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    The neutrino flux from the sun is predicted to have a CNO-cycle contribution as well as the known pp-chain component. Previously, only the fluxes from beta+ decays of 13N, 15O, and 17F have been calculated in detail. Another neutrino component that has not been widely considered is electron capture on these nuclei. We calculate the number of interactions in several solar neutrino detectors due to neutrinos from electron capture on 13N, 15O, and 17F, within the context of the Standard Solar Model. We also discuss possible non-standard models where the CNO flux is increased.Comment: 4 pages, 1 figure, submitted to Phys. Rev. C; v2 has minor changes including integration over solar volume and addition of missing reference to previous continuum electron capture calculation; v3 has minor changes including addition of references and the correction of a small (about 1%) numerical error in the table

    Level densities and γ\gamma-ray strength functions in 170,171,172^{170,171,172}Yb

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    Level densities and radiative strength functions in 171^{171}Yb and 170^{170}Yb nuclei have been measured using the 171^{171}Yb(3^3He,3^3Heγ^\prime\gamma)171^{171}Yb and 171^{171}Yb(3^3He,αγ\alpha\gamma)170^{170}Yb reactions. New data on 171^{171}Yb are compared to a previous measurement for 171^{171}Yb from the 172^{172}Yb(3^3He,αγ\alpha\gamma)171^{171}Yb reaction. Systematics of level densities and radiative strength functions in 170,171,172^{170,171,172}Yb are established. The entropy excess in 171^{171}Yb relative to the even-even nuclei 170,172^{170,172}Yb due to the unpaired neutron quasiparticle is found to be approximately 2kBk_B. Results for the radiative strength function from the two reactions lead to consistent parameters characterizing the ``pygmy'' resonances. Pygmy resonances in the 170,172^{170,172}Yb populated by the (3^3He,α\alpha) reaction appear to be split into two components for both of which a complete set of resonance parameters are obtained.Comment: 8 pages, 7 figure

    First decay study of the very neutron-rich isotope Br-93

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    The decay of the mass-separated, very neutron-rich isotope Br-93 has been studied by gamma-spectroscopy. A level scheme of its daughter Kr-93 has been constructed. Level energies, gamma-ray branching ratios and multipolarities suggest spins and parities which are in accord with a smooth systematics of the N=57 isotones for Z less-equal 40, suggesting the N=56 shell closure still to be effective in Kr isotopes. So far, there is no indication of a progressive onset of deformation in neutron-rich Kr isotopes.Comment: 17 pages, 3 figures, Phys. Rev. C, in prin

    Existence of long-lived isotopes of a superheavy element in natural Au

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    Evidence for the existence of long-lived isotopes with atomic mass numbers 261 and 265 and abundance of (1-10)x1010^{-10} relative to Au has been found in a study of natural Au using an inductively coupled plasma - sector field mass spectrometer. The measured masses fit the predictions made for the masses of 261^{261}Rg and 265^{265}Rg (Z=111) and for some isotopes of nearby elements. The possibility that these isotopes belong to the recently discovered class of long-lived high spin super- and hyperdeformed isomeric states is discussed.Comment: 4 pages, 3 figures, 2 table

    The beta-decay of 22Al

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    In an experiment performed at the LISE3 facility of GANIL, we studied the decay of 22Al produced by the fragmentation of a 36Ar primary beam. A beta-decay half-life of 91.1 +- 0.5 ms was measured. The beta-delayed one- and two-proton emission as well as beta-alpha and beta-delayed gamma decays were measured and allowed us to establish a partial decay scheme for this nucleus. New levels were determined in the daughter nucleus 22Mg. The comparison with model calculations strongly favours a spin-parity of 4+ for the ground state of 22Al

    A New Approach to Background Subtraction in Low-Energy Neutrino Experiments

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    We discuss a new method to extract neutrino signals in low energy experiments. In this scheme the symmetric nature of most backgrounds allows for direct cancellation from data. The application of this technique to the Palo Verde reactor neutrino oscillation experiment allowed us to reduce the measurement errors on the anti-neutrino flux from 20\sim 20% to 10\sim 10%. We expect this method to substantially improve the data quality in future low background experiments such as KamLAND and LENS.Comment: 7 pages, 2 figure

    Evolution of level density step structures from 56,57-Fe to 96,97-Mo

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    Level densities have been extracted from primary gamma spectra for 56,57-Fe and 96,97-Mo nuclei using (3-He,alpha gamma) and (3-He,3-He') reactions on 57-Fe and 97-Mo targets. The level density curves reveal step structures above the pairing gap due to the breaking of nucleon Cooper pairs. The location of the step structures in energy and their shapes arise from the interplay between single-particle energies and seniority-conserving and seniority-non-conserving interactions.Comment: 9 pages, including 5 figure

    Negative-Parity States and beta-decays in odd Ho and Dy Nuclei with A=151,153

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    We have investigated the negative-parity states and electromagnetic transitions in 151,153^{151,153}Ho and 151,153^{151,153}Dy within the framework of the interacting boson fermion model 2 (IBFM-2). Spin assignments for some states with uncertain spin are made based on this calculation. Calculated excitation energies, electromagnetic transitions and branching ratios are compared with available experimental data and a good agreement is obtained. The model wave functions have been used to study β\beta-decays from Ho to Dy isotones, and the calculated logft\log ft values are close to the experimental data.Comment: 23 pages and 8 figures. accepted by Physical Review
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