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論文

Quantum spin wave excited from a Cr-Dy single-molecule magnet

Ling, B.-K.*; Chang, M.*; Zhai, Y.-Q.*; Deng, J.*; 古府 麻衣子*; Guo, H.*; Zhao, J.*; Fu, Z.*; Zheng, Y.-Z.*

Journal of the American Chemical Society, 147(13), p.10935 - 10942, 2025/03

https://doi.org/10.1021/jacs.4c13628
 被引用回数：0 パーセンタイル：0.00(Chemistry, Multidisciplinary)

The efficient excitation and controlled propagation of nanoscale spin waves remain significant challenges, as their intrinsic dispersion relations are primarily determined by magnetic dipole and exchange interactions. Here we report the first observed coexistence of quantum spin wave excitation and single-molecule magnet behavior in a mixed chromium(III) and dysprosium(III) complex, namely Dy$$_{4}$$Cr$$_{2}$$($$mu_{3}$$-F)$$_{2}$$(mdea)$$_{3}$$(piv)$$_{10}$$, which shows a large ferrimagnetic ground moment with a restricted quantum tunneling gap ($$<$$ 3.8 $$times$$ 10$$^{-7}$$cm$$^{-1}$$) up to nine levels, leading to an axial anisotropic energy barrier of 12 cm$$^{-1}$$ and opened hysteresis loop at 0.4 K.

論文

First observation of the decay of the 13/2$$^+$$ isomer in $$^{183}$$Hg and $$B$$(${it M}$2) systematics of neutron transitions across the nuclear chart

Huang, H.*; Zhang, W. Q.*; Andreyev, A. N.; Liu, Z.*; Seweryniak, D.*; Li, Z. H.*; Guo, C. Y.*; Barzakh, A. E.*; Van Duppen, P.*; Andel, B.*; et al.

Physics Letters B, 833, p.137345_1 - 137345_8, 2022/10

https://doi.org/10.1016/j.physletb.2022.137345
 被引用回数：1 パーセンタイル：18.70(Astronomy & Astrophysics)

The decay of the 13/2$$^+$$ isomeric state in $$^{183}$$Hg was observed for the first time following the $$alpha$$ decay of the 13/2$$^+$$ isomer in $$^{187}$$Pb produced in the $$^{142}$$Nd$$(^{50}$$Cr$$, 2p3n)$$ reaction. Using $$alpha$$-$$gamma$$ delayed coincidence measurements, the half-life of this isomer was measured to be 290(30) $$mu$$s. This isomer is proposed to deexcite by an unobserved low-energy $$M$$2 transition to the known 9/2$$^-$$ member of a strongly prolate-deformed 7/2$$^-$$[514] band, followed by a 105-keV $$M$$1 transition to the bandhead. A lower limit of B($$M$$2)$$geq$$0.018 W.u. was deduced for the unobserved transition. The presumed retardation is proposed to be due to the notable shape change between the initial, nearly spherical, and the final, strongly deformed, states. A similar scenario is also considered for the 13/2$$^+$$ isomer in $$^{181}$$Hg, suggesting both are cases of shape isomers. The B($$M$$2) systematics of neutron transitions across the nuclear chart is discussed.

論文

Two-step Mott transition in Ni(S,Se)$$_2$$; $$mu$$SR studies and charge-spin percolation model

Sheng, Q.*; 金子 竜也*; Yamakawa, Kohtaro*; Guguchia, Z.*; Gong, Z.*; Zhao, G.*; Dai, G.*; Jin, C.*; Guo, S.*; Fu, L.*; et al.

Physical Review Research (Internet), 4(3), p.033172_1 - 033172_14, 2022/09

https://doi.org/10.1103/PhysRevResearch.4.033172

A pyrite system NiS$$_{2-x}$$Se$$_x$$ exhibits a bandwidth controlled Mott transition via (S,Se) substitutions in a two-step process: the antiferromagnetic insulator (AFI) to antiferromagnetic metal (AFM) transition at $$xsim$$0.45 followed by the AFM to paramagnetic metal (PMM) transition at $$xsim$$1.0. Among a few other Mott systems which exhibit similar two-step transitions, Ni(S,Se)$$_2$$ is of particular interest because a large intermediate AFM region in the phase diagram would provide unique opportunities to study the interplay between the spin and charge order. By comparing and combining our muon spin relaxation studies and previous neutron scattering studies, here we propose a picture where the spin order is maintained by the percolation of "nonmetallic" localized and dangling Ni moments surrounded by S, while the charge transition from AFI to AFM is caused by the percolation of the conducting paths generated by the Ni-Se-Ni bonds.

論文

First observation of a shape isomer and a low-lying strongly-coupled prolate band in neutron-deficient semi-magic $$^{187}$$Pb

Zhang, W. Q.*; Andreyev, A. N.; Liu, Z.*; Seweryniak, D.*; Huang, H.*; Li, Z. H.*; Li, J. G.*; Guo, C. Y.*; 他34名*

Physics Letters B, 829, p.137129_1 - 137129_7, 2022/06

https://doi.org/10.1016/j.physletb.2022.137129
 被引用回数：6 パーセンタイル：68.58(Astronomy & Astrophysics)

Prompt and delayed $$gamma$$-ray spectroscopy of the neutron-deficient, semi-magic isotope $$^{187}$$Pb has been performed at the Argonne Gas-Filled Analyzer. A new 5.15(15)-$$mu$$s isomeric state at only 308 keV above the spherical 3/2$$^{-}$$ ground state is identified and classified as a shape isomer. A strongly-coupled band is observed on top of the isomer, which is nearly identical to the one built on the prolate 7/2$$^{-}$$[514] Nilsson state in the isotone $$^{185}$$Hg. Based on this similarity and on the result of the potential-energy surface calculations, the new isomer in $$^{187}$$Pb is proposed to originate from the same configuration. The retarded character of the 308-keV transition can be well explained by the significant difference between the prolate parent and spherical daughter configurations, leading to the shape isomerism. The combined results of the present work and the previous $$alpha$$-decay and laser spectroscopy studies present evidence for triple shape coexistence at low energy in the negative-parity configurations of $$^{187}$$Pb, which is well reproduced by the potential-energy surface calculations.

論文

The $$^{59}$$Fe(n,$$gamma$$)$$^{60}$$Fe cross section from the surrogate ratio method and its effect on the $$^{60}$$Fe nucleosynthesis

Yan, S. Q.*; Li, X. Y.*; 西尾 勝久; Lugaro, M.*; Li, Z. H.*; 牧井 宏之; Pignatari, M.*; Wang, Y. B.*; Orlandi, R.; 廣瀬 健太郎; et al.

Astrophysical Journal, 919(2), p.84_1 - 84_7, 2021/10

https://doi.org/10.3847/1538-4357/ac12ce
 被引用回数：6 パーセンタイル：23.59(Astronomy & Astrophysics)

The long-lived $$^{60}$$Fe (with a half-life of 2.62 Myr) is a crucial diagnostic of active nucleosynthesis in the Milky Way galaxy and in supernovae near the solar system. The neutron-capture reaction $$^{59}$$Fe(n,$$gamma$$)$$^{60}$$Fe on $$^{59}$$Fe (half-life=44.5 days) is the key reaction for the production of $$^{60}$$Fe in massive stars. This reaction cross section has been previously constrained by the Coulomb dissociation experiment, which offered partial constraint on the E1 $$gamma$$-ray strength function but a negligible constraint on the M1 and E2 components. In this work, for the first time, we use the surrogate ratio method to experimentally determine the $$^{59}$$Fe(n,$$gamma$$)$$^{60}$$Fe cross sections in which all the components are included. We derived a Maxwellian-averaged cross section of 27.5$$pm$$3.5 mb at $$kT$$ = 30 keV and 13.4$$pm$$1.7 mb at $$kT$$ = 90 keV, roughly 10%-20% higher than previous estimates. We analyzed the impact of our new reaction rates in nucleosynthesis models of massive stars and found that uncertainties in the production of $$^{60}$$Fe from the $$^{59}$$Fe(n,$$gamma$$)$$^{60}$$Fe rate are at most 25$$%$$. We conclude that stellar physics uncertainties now play a major role in the accurate evaluation of the stellar production of $$^{60}$$Fe.

論文

The $$^{95}$$Zr($$n, gamma$$)$$^{96}$$Zr cross section from the surrogate ratio method and its effect on $$s$$-process nucleosynthesis

Yan, S. Q.*; Li, Z. H.*; Wang, Y. B.*; 西尾 勝久; Lugaro, M.*; Karakas, A. I.*; 牧井 宏之; Mohr, P.*; Su, J.*; Li, Y. J.*; et al.

Astrophysical Journal, 848(2), p.98_1 - 98_8, 2017/10

https://doi.org/10.3847/1538-4357/aa8c74
 被引用回数：8 パーセンタイル：26.01(Astronomy & Astrophysics)

The $$^{95}$$Zr($$n, gamma$$)$$^{96}$$Zr reaction cross section is crucial in the modelling of $$s$$-process nucleosynthesis in asymptotic giant branch stars because it controls the operation of the branching point at the unstable $$^{95}$$Zr and the subsequent production of $$^{96}$$Zr. We have carried out the measurement of the $$^{90}$$Zr($$^{18}$$O,$$^{16}$$O) and $$^{94}$$Zr($$^{18}$$O,$$^{16}$$O) reactions and obtained the $$gamma$$-decay probability ratio of $$^{92}$$Zr$$^{*}$$ and $$^{96}$$Zr$$^{*}$$ to determine the $$^{95}$$Zr($$n, gamma$$)$$^{96}$$Zr reaction cross sections with the surrogate ratio method. We tested our deduced maxwellian-averaged cross section in stellar models with masses between 2 and 6 $$M_{odot}$$ and metallicities 0.014 and 0.03. The largest changes - up 80 % variations in $$^{96}$$Zr - are seen in the models of 3-4 $$M_{odot}$$, where the $$^{22}$$Ne neutron source is mildly activated. The new rate can still provide a match to data from meteoritic stardust silicon carbide grains, provided the maximum mass of the parent stars is below 4 $$M_{odot}$$, for a metallicity of 0.03.

論文

Examination of the surrogate ratio method for the determination of the $$^{93}$$Zr(n,$$gamma$$)$$^{94}$$Zr cross section with $$^{90,92}$$Zr($$^{18}$$O,$$^{16}$$O)$$^{92,94}$$Zr reactions

Yan, S. Q.*; Li, Z. H.*; Wang, Y. B.*; 西尾 勝久; 牧井 宏之; Su, J.*; Li, Y. J.*; 西中 一朗; 廣瀬 健太郎; Han, Y. L.*; et al.

Physical Review C, 94(1), p.015804_1 - 015804_5, 2016/07

https://doi.org/10.1103/PhysRevC.94.015804
 被引用回数：7 パーセンタイル：46.65(Physics, Nuclear)

The relative $$gamma$$-decay probability ratios of the neutron resonance states in $$^{94}$$Zr and $$^{92}$$Zr populated via two neutron transfer reactions, $$^{92}$$Zr($$^{18}$$O,$$^{16}$$O)$$^{94}$$Zr and $$^{90}$$Zr($$^{18}$$O,$$^{16}$$O)$$^{92}$$Zr, have been measured to test the validity of the surrogate ratio method (SRM) in determining the (n,$$gamma$$) reaction cross section. The cross sections of the $$^{93}$$Zr(n,$$gamma$$)$$^{94}$$Zr reaction are derived from the experimentally obtained ratios and the cross sections of the $$^{91}$$Zr(n,$$gamma$$)$$^{92}$$Zr reaction in the equivalent neutron energy range of $$E_{rm n}$$ = 0 - 8 MeV. The deduced cross sections of $$^{93}$$Zr(n,$$gamma$$)$$^{94}$$Zr reaction agree with the directly measured ones in the low-energy region, and with the evaluated ENDF/B-VII.1 data at higher energies of $$E_{rm n} >$$ 3 MeV. The agreement supports the concept of the SRM method to indirectly determine the (n,$$gamma$$) reaction cross sections.

論文

Monitoring network of atmospheric Radon-222 concentration in East Asia and backward trajectory analysis of Radon-222 concentration trend at a small solitary island on Pacific Ocean

大倉 毅史; 山澤 弘実*; 森泉 純*; 平尾 茂一*; Guo, Q.*; 遠嶋 康徳*; 飯田 孝夫*

Proceedings of 3rd Asian and Oceanic Congress on Radiation Protection (AOCRP-3) (CD-ROM), 3 Pages, 2010/05

大気中$$^{222}$$Rnを大気の広域輸送の諸現象を解明するためのトレーサーとするため、東アジア域において大気中$$^{222}$$Rn濃度の連続測定ネットワークを構築した。北京,名古屋,舳倉島,八丈島,波照間島などにおいて測定した。陸域に位置する北京,名古屋において高い濃度の$$^{222}$$Rnが観測され、海域に位置する八丈島,波照間島においては、低い濃度の$$^{222}$$Rnが観測された。大気中$$^{222}$$Rn濃度の季節変動では、夏季に最も低く冬季に最も高い傾向が見られる。短周期の変動トレンドは、北京,名古屋では、1日周期の変動が見られ、八丈島,波照間島においては、1日周期の変動は観測されず、数日周期の変動が観測された。八丈島での大気中$$^{222}$$Rn濃度の数日周期変動は、総観規模の大気擾乱に依存していることが確認された。後方流跡線を用いて、八丈島における大気中$$^{222}$$Rn濃度と大気の輸送経路の関係を解析したところ、八丈島における大気中$$^{222}$$Rn濃度は大気の輸送経路に密接に関係しており、八丈島で観測される$$^{222}$$Rnは、おもに中国大陸北部からシベリアや日本列島を起源とした$$^{222}$$Rnの長距離輸送成分に強く依存することが明らかになった。

論文

東アジア域における大気中$$^{222}$$Rn濃度連続測定ネットワークと洋上の孤島における大気中$$^{222}$$Rn濃度の後方流跡線解析

大倉 毅史; 山澤 弘実*; 森泉 純*; 平尾 茂一*; Guo, Q.*; 遠嶋 康徳*; 飯田 孝夫*

大気環境学会誌, 44(1), p.42 - 51, 2009/01

http://ci.nii.ac.jp/naid/110007029877

大気中$$^{222}$$Rnを大気の広域輸送の諸現象を解明するためのトレーサーとするため、東アジア域において大気中$$^{222}$$Rn濃度の連続測定ネットワークを構築した。測定点は、北京,名古屋,舳倉島,八丈島,波照間島などである。陸域に位置する北京,名古屋において高い濃度の$$^{222}$$Rnが観測され、海域に位置する八丈島,波照間島においては、低い濃度の$$^{222}$$Rnが観測された。大気中$$^{222}$$Rn濃度の季節変動では、夏季に最も低く冬季に最も高い傾向が見られる。短周期の変動トレンドについては、北京,名古屋では、1日周期の変動が見られ、八丈島,波照間島においては、1日周期の変動は観測されず、数日周期の変動が観測された。八丈島での大気中$$^{222}$$Rn濃度の数日周期変動は、総観規模の大気擾乱に依存していることが確認された。後方流跡線を用いて、八丈島における大気中$$^{222}$$Rn濃度と大気の輸送経路の関係を解析したところ、八丈島における大気中$$^{222}$$Rn濃度は大気の輸送経路に密接に関係しており、八丈島で観測される$$^{222}$$Rnは、おもに中国大陸北部からシベリアや日本列島を起源とした$$^{222}$$Rnの長距離輸送成分に強く依存することが明らかになった。

論文

Self-guiding of 100 TW femtosecond laser pulses in centimeter-scale underdense plasma

Chen, L.-M.; 小瀧 秀行; 中島 一久*; Koga, J. K.; Bulanov, S. V.; 田島 俊樹; Gu, Y. Q.*; Peng, H. S.*; Wang, X. X.*; Wen, T. S.*; et al.

Physics of Plasmas, 14(4), p.040703_1 - 040703_4, 2007/04

https://doi.org/10.1063/1.2720374
 被引用回数：37 パーセンタイル：74.88(Physics, Fluids & Plasmas)

レーザーの自己導波の調査のため、長いunderdenseのプラズマと100TWレーザーパルスの相互作用実験を行い、レイリー長の約20倍の10mmという非常に長いプラズマチャネルを観測した。レーザーパルスがチャネル中で曲がること、及び電子キャビティ形成が実験的に初めて観測された。

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