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Kumar, V.*; Chapman, R.*; O'Donnell, D.*; Ollier, J.*; Orlandi, R.; Smith, J. F.*; Spohr, K.-M.*; Torres, D. A.*; 他13名*
Physical Review C, 108(4), p.044313_1 - 044313_19, 2023/10
被引用回数:0 パーセンタイル:0.02(Physics, Nuclear)The nuclear structure of neutron-rich niobium isotopes Nb were studied at the Legnaro National Laboratories using -ray spectroscopy. The isotopes were produced in two different experiments, either using multi-nucleon transfer reactions of Zr 530-MeV beam onto a Sn target, or via fusion-fission of S on Yb. The level schemes of these isotopes were extended respectively up to excitation energies of 4545, 5409, and 3814 keV. The structure of the low-lying states in these isotopes was interpreted and discussed in the context of shell-model calculations. In particular, for the Nb isotope (=41, =58), the results indicate the presence of shape-coexistence at low-energies, which was observed for the first time in this isotope.
Torres, D. A.*; Chapman, R.*; Kumar, V.*; Hadinia, B.*; Hodsdon, A.*; Labiche, M.*; Liang, X.*; O'Donnell, D.*; Ollier, J.*; Orlandi, R.; et al.
European Physical Journal A, 55(9), p.158_1 - 158_21, 2019/09
被引用回数:0 パーセンタイル:0.02(Physics, Nuclear)Excited states of the rubidium isotopes Rb were studied at the INFN Legnaro National Laboratory. Measurements of the -ray of nuclei produced in binary reactions from the interaction of a beam of 530 MeV Zr ions with a Sn target were complemented by studies of the -rays from nuclei produced in the interaction of a beam of 230 MeV S ions with a thick Yb target. The structure of the yrast states of Rb is discussed within the context of spherical shell-model and cranked Nilsson-Strutinsky calculations.
Orlandi, R.; Pain, S. D.*; Ahn, S.*; Jungclaus, A.*; Schmitt, K. T.*; Bardayan, D. W.*; Catford, W. N.*; Chapman, R.*; Chipps, K. A.*; Cizewski, J. A.*; et al.
Physics Letters B, 785, p.615 - 620, 2018/10
被引用回数:7 パーセンタイル:53.13(Astronomy & Astrophysics)Low-lying neutron-hole states in Sn were populated via the Sn(d,t) reaction at Oak Ridge National Laboratory. The triton angular distributions were compared to DWBA calculations and revealed spectroscopic factors compatible with a single-hole nature of the states populated. The data permit to determine the spin-orbit splitting of the strongly bound and neutron orbits below the shell gap, which was compared to the splitting of the weakly bound 3 and 2 orbits above the gap. The comparison revealed a smaller energy splitting of the 3 orbits. All splittings were reproduced using Woods-Saxon calculations, and the lower splitting of the 3 orbits was explained to arise from the large radial extent of the wavefunction and small value of the amplitude at the surface. This result is important to understand at a fundamental level the spin-orbit interaction, and its effects on neutron-rich nuclei.
西尾 勝久; Andreyev, A. N.*; Chapman, R.*; Derkx, X.*; Dllmann, C. E.*; Ghys, L.*; Heberger, F. P.*; 廣瀬 健太郎; 池添 博*; Khuyagbaatar, J.*; et al.
Physics Letters B, 748, p.89 - 94, 2015/09
被引用回数:44 パーセンタイル:92.84(Astronomy & Astrophysics)Mass distributions of fission fragments from the compound nuclei Hg and Hg formed in fusion reactions Ar+Sm and Ar+Sm, respectively, were measured at initial excitation energies of (Hg)=,3366 MeV and (Hg)=,4871 MeV. In the fission of Hg, the mass spectra were well reproduced by assuming only an asymmetric-mass division, with most probable light and heavy fragment masses /79101. The mass asymmetry for Hg agrees well with that obtained in the low-energy /EC-delayed fission of Tl, from our earlier ISOLDE(CERN) experiment. Fission of Hg is found to proceed in a similar way, delivering the mass asymmetry of /83107, throughout the measured excitation energy range. The persistence as a function of excitation energy of the mass-asymmetric fission for both proton-rich Hg isotopes gives strong evidence for the survival of microscopic effects up to effective excitation energies of compound nuclei as high as 40,MeV. This behavior is different from fission of actinide nuclei and heavier mercury isotope Hg.
Cooper, W. A.*; Brunetti, D.*; Faustin, J. M.*; Graves, J. P.*; Pfefferl, D.*; Raghunathan, M.*; Sauter, O.*; Tran, T. M.*; Chapman, I. T.*; Ham, C. J.*; et al.
Nuclear Fusion, 55(6), p.063032_1 - 063032_8, 2015/05
被引用回数:2 パーセンタイル:9(Physics, Fluids & Plasmas)入れ子の磁気面を持つ一流体三次元MHD平衡にトロイダル回転を適切に考慮するモデルを開発した。このモデルは軸対称系における回転を考慮したMHD平衡を厳密に再現できる。このモデルは三次元的な変化の大きい領域でプラズマ回転のシアが無視できる場合に適用可能である。MAST装置におけるヘリカルコアを持つ平衡において、回転の影響は磁場構造に対しては小さいが圧力分布は大きく変化させることを示した。この圧力の変化は磁気軸付近の圧力の減少であり、回転によってさらなる3次元的な変化を引き起こすものではなかった。また、粒子軌道追跡コードVENUSを用いて3次元トカマクプラズマ中の高エネルギー粒子閉じ込めを調べた。プラズマがトロイダル回転をしている場合、粒子軌道はこの回転が作り出す静電ポテンシャルの影響を受ける。さらに、平衡の3次元性はオーム則に現れる座標に依存した項の影響を受け、これが高エネルギー粒子閉じ込めに大きな影響を与えることを示した。
Orlandi, R.; Mcher, D.*; Raabe, R.*; Jungclaus, A.*; Pain, S. D.*; Bildstein, V.*; Chapman, R.*; De Angelis, G.*; Johansen, J. G.*; Van Duppen, P.*; et al.
Physics Letters B, 740, p.298 - 302, 2015/01
被引用回数:28 パーセンタイル:86.67(Astronomy & Astrophysics)Single-neutron states in Zn have been populated using the reaction Zn(d,p) at REX-Isolde, CERN. The analysis reveals that the lowest excited states in Zn lie at approximately 1 MeV, and involve neutron orbits above the N=50 shell gap. A 5/2 configuration was assigned to the 983-keV state. Comparison with large-scale shell model calculations supports a robust neutron N=50 shell closure for Ni. These data constitute an important step towards the understanding the magicity of Ni and the structure of nuclei in the region.
Cooper, W. A.*; Hirshman, S. P.*; Chapman, I. T.*; Brunetti, D.*; Faustin, J. M.*; Graves, J. P.*; Pfefferl, D.*; Raghunathan, M.*; Sauter, O.*; Tran, T. M.*; et al.
Plasma Physics and Controlled Fusion, 56(9), p.094004_1 - 094004_8, 2014/09
被引用回数:4 パーセンタイル:20.46(Physics, Fluids & Plasmas)入れ子の磁気面を持つ一流体三次元MHD平衡にトロイダル回転を適切に考慮するモデルを開発した。このモデルは軸対称系における回転を考慮したMHD平衡を厳密に再現できる。このモデルは三次元的な変化の大きい領域でプラズマ回転のシアが無視できる場合に適用可能である。MAST装置におけるヘリカルコアを持つ平衡において、回転の影響は磁場構造に対しては小さいが圧力分布は大きく変化させることを示した。この圧力の変化は磁気軸付近の圧力の減少であり、回転によってさらなる3次元的な変化を引き起こすものではなかった。
Chapman, I. T.*; Buttery, R. J.*; Coda, S.*; Gerhardt, S.*; Graves, J. P.*; Howell, D. F.*; 諫山 明彦; La Haye, R. J.*; Liu, Y.*; Maget, P.*; et al.
Nuclear Fusion, 50(10), p.102001_1 - 102001_7, 2010/10
被引用回数:52 パーセンタイル:87.34(Physics, Fluids & Plasmas)本論文では、ASDEX-U, DIII-D, HL-2A, JET, JT-60U, MAST, NSTX, TCV, Tore Supraにおいて鋸歯状振動と新古典テアリングモード(NTM)の発生について調べた結果について記述している。データベース解析の結果、鋸歯状振動がNTMを誘起したときのベータ値は鋸歯状振動の周期とともに低下することがわかった。また、装置間で鋸歯状振動を比較する場合、鋸歯状振動周期を抵抗性拡散時間で規格化し、プラズマ圧力として規格化ベータ値()を用いることがよいことがわかった。今回の結果をITERに外挿した場合、鋸歯状振動周期が10秒の場合はでNTMが誘起されると予想されるのに対し、鋸歯状振動周期が100秒の場合はでNTMが誘起されると予想されることがわかった。
Orlandi, R.; Mcher, D.*; Raabe, R.*; Jungclaus, A.*; Pain, S. D.*; Bildstein, V.*; Chapman, R.*; De Angelis, G.*; Johansen, J. G.*; Van Duppen, P.*; et al.
no journal, ,
Single-neutron states in the = 49 isotope Zn were populated in the Zn(d,p)Zn transfer reaction at REX-ISOLDE, CERN. The combined detection of protons ejected in the reaction and of rays emitted by Zn permitted the identification of the lowest-lying 5/2 and 1/2 excited states. The analysis of proton angular distributions links these states to a significant amount of single-particle strength around 1 MeV, and specifically to the d and s neutron orbits, which lie above the = 50 neutron shell gap. Comparison with large-scale-shell-model calculations supports a robust = 50 shell-closure for Ni. These data constitute a considerable step towards the understanding of the magicity of Ni and of the structure of isotopes in the region.
Orlandi, R.; Pain, S. D.*; Bardayan, D. W.*; Gross, C. J.*; Smith, M. S.*; Jungclaus, A.*; Ahn, S.*; Jones, K. L.*; Pittman, S. T.*; Schmitt, K. T.*; et al.
no journal, ,
Knowledge of single-particle energies in the vicinity of exotic doubly-magic nuclei is of critical importance to understand evolution of nuclear structure. In the present work, the Sn(d,t)Sn reaction (Q=-1.055 MeV) was studied in inverse kinematics at HRIBF of Oak Ridge National Laboratory. The Sn ISOL beam was post-accelerated to an energy of 4.39 MeV/u using the ORNL HRIBF accelerator. The beam (average intensity of 1.2e4 pps) impinged on a 250 g/cm deuterated polyethylene target, for approximately 4 days. Ejected tritons were detected using the Super ORRUBA array of segmented Si telescopes. Low-lying states in Sn were populated in the experiment. Preliminary results will be shown.