9 research outputs found

    The electric dipole response of 76^{76}Se above 4 MeV

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    The dipole response of 3476^{76}_{34}Se in the energy range 4 to 9 MeV has been analyzed using a (γ,γ)(\vec\gamma,{\gamma}') polarized photon scattering technique, performed at the High Intensity γ\gamma-Ray Source facility, to complement previous work performed using unpolarized photons. The results of this work offer both an enhanced sensitivity scan of the dipole response and an unambiguous determination of the parities of the observed J=1 states. The dipole response is found to be dominated by E1E1 excitations, and can reasonably be attributed to a pygmy dipole resonance. Evidence is presented to suggest that a significant amount of directly unobserved excitation strength is present in the region, due to unobserved branching transitions in the decays of resonantly excited states. The dipole response of the region is underestimated when considering only ground state decay branches. We investigate the electric dipole response theoretically, performing calculations in a 3D cartesian-basis time-dependent Skyrme-Hartree-Fock framework.Comment: 20 pages, 18 figures, to be submitted to PR

    Structure of high-lying levels populated in the Y-96 -> Zr-96 beta decay

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    The nature of Jπ=1J^{\pi}=1^- levels of 96^{96}Zr below the β\beta-decay QβQ_{\beta} value of 96^{96}Y has been investigated in high-resolution γ\gamma-ray spectroscopy following the β\beta decay as well as in a campaign of inelastic photon scattering experiments. Branching ratios extracted from β\beta decay allow the absolute E1E1 excitation strength to be determined for levels populated in both reactions. The combined data represents a comprehensive approach to the wavefunction of 11^- levels below the QβQ_{\beta} value, which are investigated in the theoretical approach of the Quasiparticle Phonon Model. This study clarifies the nuclear structure properties associated with the enhanced population of high-lying levels in the 96^{96}Ygs_{gs} β\beta decay, one of the three most important contributors to the high-energy reactor antineutrino spectrum

    Brain homeostasis: VEGF receptor 1 and 2—two unequal brothers in mind

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    The B-10((p)over-right-arrow, gamma)C-11 reaction at astrophysically relevant energies

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    The B-10(, gamma)C-11 reaction was studied by detecting the gamma-rays produced when 100, 130-, and 160-keV polarized protons were stopped in a thick B-10 target. Polarized and unpolarized incident beams were used to measure the cross section and vector analyzing power as a function of angle and energy for capture to the ground (J(pi)=3/2(-)), the second (E=4319 keV, J(pi)=5/2(-)), and the fifth (E=6478 keV, J(pi)=7/2(-)) excited states of C-11. The data were analyzed to obtain the amplitudes and phases of the contributing transition-matrix elements at each measured energy for all three transitions. Values of the astrophysical S factors were obtained from the cross section data and are compared to previous results. A direct capture plus resonance model calculation was performed in an attempt to account for all measured quantities. It was found that the large (similar to32%) value of A(y)(90degrees) observed in the case of capture to the ground state could be accounted for by including the subthreshold resonance at 8420 keV

    Two-body photodisintegration of (3)He between 7 and 16 MeV

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    A comprehensive data set is reported for the two-body photodisintegration cross section of (3)He using mono-energetic photon beams at eleven energies between 7.0 and 16.0 MeV. A (3)He + Xe high-pressure gas scintillator served as target and detector. Although our data are in much better agreement with our state-of-the-art theoretical calculations than the majority of the previous data, these calculations underpredict the new data by about 10%. This disagreement suggests an incomplete understanding of the dynamics of the three-nucleon system and its response to electromagnetic probes. (C) 2011 Elsevier B.V. All rights reserved
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