※ 半角英数字
 年 ~ 
検索結果: 23 件中 1件目~20件目を表示


Initialising ...



Initialising ...


Initialising ...


Initialising ...


Initialising ...


Initialising ...


Initialising ...


Initialising ...



Study of the $$N=32$$ and $$N=34$$ shell gap for Ti and V by the first high-precision multireflection time-of-flight mass measurements at BigRIPS-SLOWRI

飯村 俊*; Rosenbusch, M.*; 高峰 愛子*; 角田 佑介*; 和田 道治*; Chen, S.*; Hou, D. S.*; Xian, W.*; 石山 博恒*; Yan, S.*; et al.

Physical Review Letters, 130(1), p.012501_1 - 012501_6, 2023/01

The atomic masses of $$^{55}$$Sc, $$^{56,58}$$Ti, and $$^{56-59}$$V have been determined using the high-precision multireflection time-of-flight technique. The radioisotopes have been produced at RIKEN's Radioactive Isotope Beam Factory (RIBF) and delivered to the novel designed gas cell and multireflection system, which has been recently commissioned downstream of the ZeroDegree spectrometer following the BigRIPS separator. For $$^{56,58}$$Ti and $$^{56-59}$$V, the mass uncertainties have been reduced down to the order of 10 keV, shedding new light on the $$N=34$$ shell effect in Ti and V isotopes by the first high-precision mass measurements of the critical species $$^{58}$$Ti and $$^{59}$$V. With the new precision achieved, we reveal the nonexistence of the $$N=34$$ empirical two-neutron shell gaps for Ti and V, and the enhanced energy gap above the occupied $$nu$$p$$_{3/2}$$ orbit is identified as a feature unique to Ca. We perform new Monte Carlo shell model calculations including the $$nu$$d$$_{5/2}$$ and $$nu$$g$$_{9/2}$$ orbits and compare the results with conventional shell model calculations, which exclude the $$nu$$g$$_{9/2}$$ and the $$nu$$d$$_{5/2}$$ orbits. The comparison indicates that the shell gap reduction in Ti is related to a partial occupation of the higher orbitals for the outer two valence neutrons at $$N = 34$$.


$$alpha$$-clustering in atomic nuclei from first principles with statistical learning and the Hoyle state character

大塚 孝治; 阿部 喬*; 吉田 亨*; 角田 佑介*; 清水 則孝*; 板垣 直之*; 宇都野 穣; Vary, J. P.*; Maris, P.*; 上野 秀樹*

Nature Communications (Internet), 13, p.2234_1 - 2234_10, 2022/04

 被引用回数:1 パーセンタイル:63.35(Multidisciplinary Sciences)



Lifetime measurements of excited states in $$^{55}$$Cr

Kleis, H.*; Seidlitz, M.*; Blazhev, A.*; Kaya, L.*; Reiter, P.*; Arnswald, K.*; Dewald, A.*; Droste, M.*; Fransen, C.*; M$"o$ller, O.*; et al.

Physical Review C, 104(3), p.034310_1 - 034310_9, 2021/09


 被引用回数:1 パーセンタイル:32.08(Physics, Nuclear)

ケルン大学のタンデム加速器にて、$$^{48}$$Ca($$^{11}$$B, $$p3n$$)$$^{55}$$Cr反応によって$$^{55}$$Crの励起状態を生成し、そこから脱励起する励起状態の寿命をドップラーシフト反跳距離法を用いて測定した。$$9/2^-_1$$状態から$$5/2^-_1$$状態へ脱励起する$$E2$$遷移の寿命が6.33(46)ps, $$5/2^-_1$$状態から$$3/2^-_1$$状態へ脱励起する$$M1$$励起の寿命が5.61(28)psであることが決定された。その値から$$B(E2)$$, $$B(M1)$$値を引き出し、これらが殻模型計算の値とよく一致することがわかった。小さな$$B(M1)$$値は、$$5/2^-_1$$状態と$$3/2^-_1$$状態が異なる回転バンドに属しているためであると解釈された。


Variational approach with the superposition of the symmetry-restored quasiparticle vacua for nuclear shell-model calculations

清水 則孝*; 角田 佑介*; 宇都野 穣; 大塚 孝治*

Physical Review C, 103(1), p.014312_1 - 014312_11, 2021/01


 被引用回数:8 パーセンタイル:91.35(Physics, Nuclear)



$$beta$$ decay of $$^{75}$$Ni and the systematics of the low-lying level structure of neutron-rich odd-$$A$$ Cu isotopes

Bello Garrote, F. L.*; Sahin, E.*; 角田 佑介*; 大塚 孝治*; G$"o$rgen, A.*; Orlandi, R.; 他61名*

Physical Review C, 102(3), p.034314_1 - 034314_13, 2020/09

 被引用回数:1 パーセンタイル:18.5(Physics, Nuclear)

Detailed spectroscopy of neutron-rich odd-$$A$$ Cu isotopes is of great importance for studying the shell evolution in the region of $$^{78}$$Ni. Excited states in $$^{75}$$Cu were populated in the $$beta$$ decay of $$^{75}$$Ni isotopes, which were produced by the in-flight fission at RIBF, RIKEN. The $$^{75}$$Ni isotopes were separated, identified, and implanted in a highly segmented Si detector array for the detection of the $$beta$$-decay electrons, while the delayed $$gamma$$ rays were detected by an array of HPGe cluster detectors. A level scheme of $$^{75}$$Cu was built up to $$sim$$4 MeV, from which the location of the two previously known low-lying isomeric states was clarified. The level structure below 2 MeV was interpreted based on the results of the shell-model calculations and the systematics of odd-$$A$$ Cu isotopes, revealing the evolution of single-particle states in this region.


Thick-restart block Lanczos method for large-scale shell-model calculations

清水 則孝*; 水崎 高浩*; 宇都野 穣; 角田 佑介*

Computer Physics Communications, 244, p.372 - 384, 2019/11

 被引用回数:94 パーセンタイル:99.69(Computer Science, Interdisciplinary Applications)



Shape staggering of midshell mercury isotopes from in-source laser spectroscopy compared with density-functional-theory and Monte Carlo shell-model calculations

Sels, S.*; Day Goodacre, T.*; Marsh, B. A.*; Pastore, A.*; Ryssens, W.*; 角田 佑介*; Althubiti, N.*; Andel, B.*; Andreyev, A. N.; 他39名*

Physical Review C, 99(4), p.044306_1 - 044306_17, 2019/04

 被引用回数:29 パーセンタイル:96.22(Physics, Nuclear)

Neutron-deficient $$^{177-185}$$Hg isotopes were studied using in-source laser resonance-ionization spectroscopy at the CERN-ISOLDE radioactive ion-beam facility. The endpoint of the odd-even nuclear shape staggering in mercury was observed directly by measuring the isotope shifts and hyperfine structures of $$^{177-185}$$Hg. Changes in the mean-square charge radii for all mentioned isotopes, magnetic dipole, and electric quadrupole moments of the odd-$$A$$ isotopes and arguments in favor of $$I = 7/2$$ spin assignment for $$^{177,179}$$Hg were deduced. Experimental results are compared with density functional theory (DFT) and Monte Carlo shell model (MCSM) calculations. DFT calculations using Skyrme parametrizations predict a jump in the charge radius around the neutron $$N = 104$$ midshell, with an odd-even staggering pattern related to the coexistence of nearly degenerate oblate and prolate minima. This near-degeneracy is highly sensitive to many aspects of the effective interaction, a fact that renders perfect agreement with experiments out of reach for current functionals. MCSM calculations of states with the experimental spins and parities show good agreement for both electromagnetic moments and the observed charge radii. A clear mechanism for the origin of shape staggering within this context is identified: a substantial change in occupancy of the proton $${pi}h_{9/2}$$ and neutron $${nu}i_{13/2}$$ orbitals.


Characterization of the shape-staggering effect in mercury nuclei

Marsh, B. A.*; Day Goodacre, T.*; 角田 佑介*; Andreyev, A. N.; 他41名*

Nature Physics, 14(12), p.1163 - 1167, 2018/12

 被引用回数:72 パーセンタイル:96.45(Physics, Multidisciplinary)

In rare cases, the removal of a single proton (Z) or neutron (N) from an atomic nucleus leads to a dramatic shape change. These instances are crucial for understanding the components of the nuclear interactions that drive deformation. The mercuryisotopes (Z = 80) are a striking example: their close neighbours, the lead isotopes (Z = 82), are spherical and steadily shrink with decreasing N. The even-mass (A = N + Z) mercury isotopes follow this trend. The odd-mass mercury isotopes $$^{181,183,185}$$Hg, however, exhibit noticeably larger charge radii. Due to the experimental difficulties of probing extremely neutron-deficient systems, and the computational complexity of modelling such heavy nuclides, the microscopic origin of this unique shape staggering has remained unclear. Here, by applying resonance ionization spectroscopy, mass spectrometry and nuclear spectroscopy as far as $$^{177}$$Hg, we determine $$^{181}$$Hg as the shape-staggering endpoint. By combining our experimental measurements with Monte Carlo shell model calculations, we conclude that this phenomenon results from the interplay between monopole and quadrupole interactions driving a quantum phase transition, for which we identify the participating orbitals. Although shape staggering in the mercury isotopes is a unique and localized feature in the nuclear chart, it nicely illustrates the concurrence of single-particle and collective degrees of freedom at play in atomic nuclei.


Monte Carlo shell model studies with massively parallel supercomputers

清水 則孝*; 阿部 喬*; 本間 道雄*; 大塚 孝治*; 富樫 智章*; 角田 佑介*; 宇都野 穣; 吉田 亨*

Physica Scripta, 92(6), p.063001_1 - 063001_19, 2017/06

 被引用回数:24 パーセンタイル:81.96(Physics, Multidisciplinary)



Type II shell evolution in $$A=70$$ isobars from the $$N geq 40$$ island of inversion

Morales, A. I.*; Benzoni, G.*; Watanabe, H.*; 角田 佑介*; Otsuka, T.*; 西村 俊二*; Browne, F.*; Daido, R.*; Doornenbal, P.*; Fang, Y.*; et al.

Physics Letters B, 765, p.328 - 333, 2017/02

 被引用回数:30 パーセンタイル:92.82(Astronomy & Astrophysics)

The level schemes of neutron-rich isotopes $$^{70}$$Co and $$^{70}$$Ni were populated in the $$beta$$ decay of $$^{70}$$Fe and studied using $$beta$$-delayed $$gamma$$-ray spectroscopy of the $$beta$$ decay, at the RIBF in RIKEN, Japan. The experimental results were compared to state-of-the-art shell-model calculations, and indicate a dominance of prolate deformation in the low-lying states, coexisting with spherical states. The $$beta$$ decay of the $$A=70$$ isobars is shown to progress in accordance to a new type of shell evolution, the so-called Type II, which involves many particle-hole excitations across energy gaps.


Are there signatures of harmonic oscillator shells far from stability?; First spectroscopy of $$^{110}$$Zr

Paul, N.*; Corsi, A.*; Obertelli, A.*; Doornenbal, P.*; Authelet, G.*; 馬場 秀忠*; Bally, B.*; Bender, M.*; Calvet, D.*; Ch$^a$teau, F.*; et al.

Physical Review Letters, 118(3), p.032501_1 - 032501_7, 2017/01

 被引用回数:33 パーセンタイル:87.76(Physics, Multidisciplinary)

The first measurement of $$gamma$$ rays emitted by the very neutron rich nuclei $$^{112}$$Mo (Z=42) and $$^{110}$$Zr (Z=40) was carried out at the RIBF facility at RIKEN. These data shine light on the postulated N=70 harmonic oscillator shell. If the spin-orbit splitting which gives rise to the N=82 shell gap is reduced in very neutron-rich nuclei, the harmonic oscillator gap at N=70 should open instead. However, both the measured energy of the first excited state $$^{112}$$Mo and $$^{110}$$Zr, respectively 235(7) keV and 185(11) keV, and their E(4$$^+$$)/E(2$$^+$$) ratio, indicate that these nuclei are good rotors, and exclude the shell stabilization scenario at Z=40 and N=70. These results were compared to state-of-the-art density functional theoretical calculations using Gogny and Skyrme effective interactions.


Large-scale shell-model studies for exotic nuclei; Probing shell evolution

宇都野 穣; 大塚 孝治*; 清水 則孝*; 角田 佑介*; 本間 道雄*; 阿部 喬*; 水崎 高浩*; 富樫 智章*; Brown, B. A.*

Proceedings of International Conference on Nuclear Theory in the Supercomputing Era 2014 (NTSE 2014), p.29 - 34, 2016/00



Recent advances in shell evolution with shell-model calculations

宇都野 穣; 大塚 孝治*; 角田 佑介*; 清水 則孝*; 本間 道雄*; 富樫 智章*; 水崎 高浩*

JPS Conference Proceedings (Internet), 6, p.010007_1 - 010007_8, 2015/06



Identification of deformed intruder states in semi-magic $$^{70}$$Ni

Chiara, C. J.*; Weisshaar, D.*; Janssens, R. V. F.*; 角田 佑介*; 大塚 孝治*; Harker, J. L.*; Walters, W. B.*; Recchia, F.*; Albers, M.*; Alcorta, M.*; et al.

Physical Review C, 91(4), p.044309_1 - 044309_10, 2015/04

 被引用回数:34 パーセンタイル:91.24(Physics, Nuclear)

アルゴンヌ国立研究所にて中性子過剰核$$^{70}$$Niを$$^{70}$$Znの多核子移行反応によって生成し、$$gamma$$線検出器GRETINAを用いて$$gamma$$線分光を行った。その結果、$$2^+_2$$, $$4^+_2$$準位を初めて観測した。これらの準位は小さな模型空間を採用した殻模型計算では再現されないため、陽子の$$f_{7/2}$$軌道からの励起を伴った大きな変形状態であると考えられる。本論文の理論グループが2014年に発表した大規模殻模型計算によって$$^{70}$$Niの励起状態を解析した結果、これらの状態は大きなプロレート変形を持つ状態とよく対応することがわかった。この結果は、中性子過剰ニッケル同位体における変形共存が$$^{68}$$Ni以外にも存在することを実証するとともに、中性子過剰核における大規模殻模型計算の予言能力を確かめるものである。


Nature of isomerism in exotic sulfur isotopes

宇都野 穣; 清水 則孝*; 大塚 孝治*; 吉田 亨*; 角田 佑介*

Physical Review Letters, 114(3), p.032501_1 - 032501_5, 2015/01


 被引用回数:33 パーセンタイル:85.25(Physics, Multidisciplinary)

通常の偶偶核では、$$0^+_1$$, $$2^+_1$$, $$4^+_1cdots$$状態が強い$$E2$$遷移で結ばれていることがよく知られている。最近、中性子過剰核$$^{44}$$Sの$$4^+_1$$状態が観測され、$$4^+_1$$から$$2^+_1$$への$$E2$$遷移が非常に抑制されているという新しい現象が見つかった。この論文では、その起源を理論的に解明した結果を報告する。この強く抑制された$$E2$$遷移は殻模型計算によって得られるが、殻模型の多体波動関数は非常に複雑なため、$$E2$$遷移の抑制が起こる起源がこれまで理解されてこなかった。ここでは、角運動量射影後の変分法によって物体固定座標系における多体波動関数を得るという新規な手法を導入した。その波動関数を解析した結果、$$0^+_1$$, $$2^+_1$$では$$K$$量子数(物体固定座標系における角運動量の第3軸成分)が0となる通常の回転状態が主であるのに対し、$$4^+$$については$$K=4$$が主の状態が$$K=0$$が主の状態よりも低いエネルギーに出現し、それによって$$E2$$遷移が抑制されることがわかった。この解釈は$$^{43}$$Sの励起スペクトルも説明可能なことから妥当性が高い。これは、$$K$$核異性体の一種であり、これまで発見されたもので最も軽い核で出現するものである。


Recent shell-model results for exotic nuclei

宇都野 穣; 大塚 孝治*; 清水 則孝*; 本間 道雄*; 水崎 高浩*; 角田 佑介*; 阿部 喬*

EPJ Web of Conferences, 66, p.02106_1 - 02106_8, 2014/03

 被引用回数:13 パーセンタイル:96.68



Novel shape evolution in exotic Ni isotopes and configuration-dependent shell structure

角田 佑介*; 大塚 孝治*; 清水 則孝*; 本間 道雄*; 宇都野 穣

Physical Review C, 89(3), p.031301_1 - 031301_5, 2014/03


 被引用回数:140 パーセンタイル:99.35(Physics, Nuclear)



Shape coexistence in $$^{68}$$Ni

Suchyta, S.*; Liddick, S. N.*; 角田 佑介*; 大塚 孝治*; Bennett, M. B.*; Chemey, A.*; 本間 道雄*; Larson, N.*; Prokop, C. J.*; Quinn, S. J.*; et al.

Physical Review C, 89(2), p.021301_1 - 021301_5, 2014/02

 被引用回数:74 パーセンタイル:97.59(Physics, Nuclear)



Variational procedure for nuclear shell-model calculations and energy-variance extrapolation

清水 則孝*; 宇都野 穣; 水崎 高浩*; 本間 道雄*; 角田 佑介*; 大塚 孝治*

Physical Review C, 85(5), p.054301_1 - 054301_6, 2012/05


 被引用回数:20 パーセンタイル:72.77(Physics, Nuclear)



New-generation of Monte Carlo shell model for the K computer era

清水 則孝*; 阿部 喬*; 角田 佑介*; 宇都野 穣; 吉田 亨*; 水崎 高浩*; 本間 道雄*; 大塚 孝治*

Progress of Theoretical and Experimental Physics (Internet), 2012(1), p.01A205_1 - 01A205_27, 2012/00


 被引用回数:111 パーセンタイル:96.1(Physics, Multidisciplinary)


23 件中 1件目~20件目を表示