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論文

Shell evolution beyond $$Z$$=28 and $$N$$=50; Spectroscopy of $$^{81,82,83,84}$$Zn

Shand, C. M.*; Podoly$'a$k, Zs.*; G$'o$rska, M.*; Doornenbal, P.*; Obertelli, A.*; Nowacki, F.*; Otsuka, T.*; Sieja, K.*; Tostevin, J. A.*; Tsunoda, T.*; et al.

Physics Letters B, 773, p.492 - 497, 2017/10

 被引用回数:8 パーセンタイル:14.67(Astronomy & Astrophysics)

Low-lying states in neutron-rich $$^{81,82.83.84}$$Zn nuclei were measured for the first time via in-beam $$gamma$$-ray spectroscopy at RIKEN. These include the 4$$_1^+$$ to 2$$_1^+$$ in $$^{82}$$Zn and the 2$$_1^+$$ to 0$$_1^+$$ and 4$$_1^+$$ to 2$$_1^+$$ in $$^{84}$$Zn. The reduced E($$2^+$$) energies and increased E(4$$^+$$)/E(2$$^+$$) ratios at $$N$$=52,54 compared to $$^{80}$$Zn attest that the magicity is confined just on the neutron number $$N$$=50 only. The levels observed in $$^{84}$$Zn suggest the onset of deformation towards heavier Zn isotopes. The data were compared to state-of-the-art shell model calculations.

論文

Single-neutron orbits near $$^{78}$$Ni; Spectroscopy of the N=49 isotope $$^{79}$$Zn

Orlandi, R.; M$"u$cher, 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:15 パーセンタイル:13.65(Astronomy & Astrophysics)

Single-neutron states in $$^{79}$$Zn have been populated using the reaction $$^{78}$$Zn(d,p) at REX-Isolde, CERN. The analysis reveals that the lowest excited states in $$^{79}$$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 $$^{78}$$Ni. These data constitute an important step towards the understanding the magicity of $$^{78}$$Ni and the structure of nuclei in the region.

論文

Yrast 6$$^+$$ seniority isomers of $$^{136,138}$$Sn

Simpson, G. S.*; Gey, G.*; Jungclaus, A.*; Taprogge, J.*; 西村 俊二*; Sieja, K.*; Doornenbal, P.*; Lorusso, G.*; S$"o$derstr$"o$m, P.-A.*; 炭竃 聡之*; et al.

Physical Review Letters, 113(13), p.132502_1 - 132502_6, 2014/09

 被引用回数:39 パーセンタイル:7.38(Physics, Multidisciplinary)

Delayed $$gamma$$-ray cascades, originating from the decay of 6$$^+$$ isomeric states, in the very neutron-rich, semimagic isotopes $$^{136,138}$$Sn were observed following the projectile fission of a $$^{238}$$U beam at RIBF, RIKEN. The wave functions of these isomeric states are proposed to be predominantly a fully aligned pair of f$$_{7/2}$$ neutrons. Shell-model calculations, performed using a realistic effective interaction, reproduce well the energies of the excited states of these nuclei and the measured transition rates, with the exception of the $$B(E$$2;6$$^+ rightarrow 4^+$$) rate of $$^{136}$$Sn, which deviates from a simple seniority scheme. Empirically reducing the $$nu f$$$$_{7/2}^{2}$$ orbit matrix elements produces a 4+1 state with almost equal seniority 2 and 4 components, correctly reproducing the experimental $$B(E$$2;6$$^+ rightarrow 4^+$$) rate of $$^{136}$$Sn. These data provide a key benchmark for shell-model interactions far from stability.

論文

Study of the deformation-driving $$nu$$d$$_{5/2}$$ orbital in $$_{28}^{67}$$Ni$$_{39}$$ using one-neutron transfer reactions

Diriken, J.*; Patronis, N.*; Andreyev, A. N.*; Antalic, S.*; Bildstein, V.*; Blazhev, A.*; Darby, I. G.*; De Witte, H.*; Eberth, J.*; Elseviers, J.*; et al.

Physics Letters B, 736, p.533 - 538, 2014/09

 被引用回数:10 パーセンタイル:28.23(Astronomy & Astrophysics)

The neutron orbits $$g_{9/2}$$, d$$_{5/2}$$ and s$$_{1/2}$$ are assumed to be responsible for the swift onset of collectivity observed in the region below $$^{68}$$Ni. In order to gather information on the single-particle energies and spectroscopic factors of these orbitals, single-particle states in the nucleus $$^{67}$$Ni were populated using the reaction $$^{66}$$Ni(d,p), in inverse kinematics, at REX-ISOLDE, CERN. The new isotope was studied using combined particle-$$gamma$$ spectroscopy. Comparison with DWBA calculations, permitted the identification of positive parity states with a substantial amount of $$nu$$d$$_{9/2}$$ (1007 keV) and $$nu$$d$$_{5/2}$$ (2207 and 3277 keV) single-particle strength. Comparisons with extended Shell-Model calculations was also performed to confirm the single-particle nature of these states, and to deduce general properties around $$^{68}$$Ni.

論文

High spin structure of $$^{34}$$S and the proton-neutron coupling of intruder states

Mason, P.*; M$u{a}$rginean, N.*; Lenzi, S. M.*; Ionescu-Bujor, M.*; Della Vedova, F.*; Napoli, D. R.*; 大塚 孝治*; 宇都野 穣; Nowacki, F.*; Axiotis, M.*; et al.

Physical Review C, 71(1), p.014316_1 - 014316_8, 2005/01

 被引用回数:23 パーセンタイル:17.31(Physics, Nuclear)

Legnaro国立研究所のタンデム加速器で$$^{34}$$Sの高スピン状態を初めて観測し、その結果を原研らのグループによるモンテカルロ殻模型計算と比較した。実験では、$$^{34}$$Sの高スピン状態を$$^{24}$$Mg($$^{16}$$O,$$alpha 2p$$)反応によって生成し、脱励起$$gamma$$線を観測することによって$$^{34}$$Sの準位を組み上げた。その結果、$$10^+$$までの正パリティ状態及び$$8^-$$までの負パリティ状態のイラスト状態に加え、幾つかの非イラスト状態を見つけた。さらに、DSAM法により幾つかの遷移の$$B(E2)$$, $$B(M1)$$を得た。実験結果を殻模型計算と比較したところ、$$5^+$$までの(正パリティ)イラスト状態は$$sd$$殻配位空間内で計算した殻模型計算とよく一致するが、それよりも高いスピンのイラスト状態はN=20の殻ギャップを超えた励起が必要であることがわかった。さらに詳しく調べると、$$6^+$$, $$8^+$$については中性子が2個励起する配位が主であるのに対し、他のスピンでは陽子の励起も重要であることも明らかになった。モンテカルロ殻模型計算はこのような特質を全体としてはよく再現する一方、陽子・中性子励起する状態については実験よりも高い励起エネルギーとなった。この実験及び計算結果は、陽子・中性子間相互作用が多体構造に及ぼす影響について大きな知見を与えている。

口頭

Low-energy states in $$^{79}$$Zn and the structure of $$^{78}$$Ni

Orlandi, R.; M$"u$cher, 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 $$N$$ = 49 isotope $$^{79}$$Zn were populated in the $$^{78}$$Zn(d,p)$$^{79}$$Zn transfer reaction at REX-ISOLDE, CERN. The combined detection of protons ejected in the reaction and of $$gamma$$ rays emitted by $$^{79}$$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 $$nu$$d$$_{5/2}$$ and $$nu$$s$$_{1/2}$$ neutron orbits, which lie above the $$N$$ = 50 neutron shell gap. Comparison with large-scale-shell-model calculations supports a robust $$N$$ = 50 shell-closure for $$^{78}$$Ni. These data constitute a considerable step towards the understanding of the magicity of $$^{78}$$Ni and of the structure of isotopes in the region.

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