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論文

Multiple mechanisms in proton-induced nucleon removal at $$sim$$100 MeV/nucleon

Pohl, T.*; Sun, Y. L.*; Obertelli, A.*; Lee, J.*; G$'o$mez-Ramos, M.*; 緒方 一介*; 吉田 数貴; Cai, B. S.*; Yuan, C. X.*; Brown, B. A.*; et al.

Physical Review Letters, 130(17), p.172501_1 - 172501_8, 2023/04

 被引用回数:2 パーセンタイル:90.46(Physics, Multidisciplinary)

大きなフェルミ面非対称性を持つ陽子過剰な$$^{14}$$O原子核からの100MeV/nucleonでの陽子による陽子・中性子除去反応について報告した。この結果は、quasi-freeノックアウト反応、非弾性散乱、核子移行反応を含む複数の反応機構の定量的寄与を初めて示すものである。このようなエネルギー領域では通常無視される非弾性散乱と核子移行の寄与が、弱束縛陽子と強束縛中性子の除去反応断面積にそれぞれ約50%と30%寄与していることが示された。

論文

Chiral restoration of nucleons in neutron star matter; Studies based on a parity doublet model

南川 拓哉*; Gao, B.*; 古城 徹*; 原田 正康*

Symmetry (Internet), 15(3), p.745_1 - 745_30, 2023/03

We review the chiral variant and invariant components of nucleon masses and the con- sequence of their existence on the chiral restoration in extreme conditions, particularly in neutron star matter.

論文

New $$K$$ isomers in $$^{248}$$Cf

Orlandi, R.; 牧井 宏之; 西尾 勝久; 廣瀬 健太郎; 浅井 雅人; 塚田 和明; 佐藤 哲也; 伊藤 由太; 洲嵜 ふみ; 永目 諭一郎*; et al.

Physical Review C, 106(6), p.064301_1 - 064301_11, 2022/12

 被引用回数:0 パーセンタイル:0.02(Physics, Nuclear)

The nuclear structure of $$^{248}$$Cf produced by the $$^{18}$$O+$$^{249}$$Cf multinucleon transfer reaction was investigated using $$gamma$$-ray spectroscopy. Analysis of the $$gamma$$-ray spectrum of $$^{248}$$Cf revealed the presence of multiple long-lived (isomeric) excited states at low excitation energies. The energies and half-lives of the isomers contain information on the proton and neutron orbits in the heavy-element region and the deformation of atomic nuclei, and are important data to predict the properties of nuclei in the "island of stability".

論文

Impacts of the $$U(1)_A$$ anomaly on nuclear and neutron star equation of state based on a parity doublet model

Gao, B.*; 南川 拓哉*; 古城 徹*; 原田 正康*

Physical Review C, 106(6), p.065205_1 - 065205_14, 2022/12

We examine the role of the U(1)$$_{A}$$ anomaly in a parity doublet model of nucleons which include the chiral variant and invariant masses. Our model expresses the U(1)$$_{A}$$ anomaly by the Kobayashi-Maskawa-'t Hooft (KMT) interaction in the mesonic sector. After examining the roles of the KMT term in vacuum, we discuss its impacts on nuclear equations of state (EOS). The U(1)$$_{A}$$ anomaly increases the masses of the $$eta$$' and $$sigma$$ mesons and enhances the chiral symmetry breaking. Also, the U(1)$$_{A}$$ anomaly enlarges the energy difference between chiral symmetric and symmetry broken vacuum; in turn, the chiral restoration at high density adds a larger energy density (often referred as a bag constant) to EOSs than in the case without the anomaly, leading to softer EOSs. Including these U(1)$$_{A}$$ effects, we update the previously constructed unified equations of state that interpolate the nucleonic EOS at $$n$$$$_{B}$$ $$leqq$$ 2$$n$$$$_{0}$$ ($$n$$$$_{0}$$ = 0.16 fm$$^{-3}$$; nuclear saturation density) and quark EOS at $$n$$$$_{B}$$ $$geqq$$ 5 $$n$$$$_{0}$$. The unified EOS is confronted with the observational constraints on the masses and radii of neutron stars. The softening of EOSs associated with the $$U$$(1) anomaly reduces the overall radii, relaxing the previous constraint on the chiral invariant mass $$m$$$$_{0}$$. Including the attractive nonlinear $$rho$$-$$omega$$ coupling for the reduced slope parameter in the symmetry energy, our new estimate is 400 MeV $$leqq$$ $$m$$$$_{0}$$ $$leqq$$ 700 MeV, with $$m$$$$_{0}$$ smaller than our previous estimate by $$approx$$200 MeV.

論文

Anisotropic magnon damping by zero-temperature quantum fluctuations in ferromagnetic CrGeTe$$_{3}$$

Chen, L.*; Mao, C.*; Chung, J.-H.*; Stone, M. B.*; Kolesnikov, A. I.*; Wang, X.*; 村井 直樹; Gao, B.*; Delaire, O.*; Dai, P.*

Nature Communications (Internet), 13, p.4037_1 - 4037_7, 2022/07

 被引用回数:2 パーセンタイル:56.14(Multidisciplinary Sciences)

Spin and lattice are two fundamental degrees of freedom in a solid, and their fluctuations about the equilibrium values in a magnetic ordered crystalline lattice form quasiparticles termed magnons (spin waves) and phonons (lattice waves), respectively. In most materials with strong spin-lattice coupling (SLC), the interaction of spin and lattice induces energy gaps in the spin wave dispersion at the nominal intersections of magnon and phonon modes. Here we use neutron scattering to show that in the two-dimensional (2D) van der Waals honeycomb lattice ferromagnetic CrGeTe$$_{3}$$, spin waves propagating within the 2D plane exhibit an anomalous dispersion, damping, and breakdown of quasiparticle conservation, while magnons along the c axis behave as expected for a local moment ferromagnet. These results indicate the presence of dynamical SLC arising from the zero-temperature quantum fluctuations in CrGeTe$$_{3}$$, suggesting that the observed in-plane spin waves are mixed spin and lattice quasiparticles fundamentally different from pure magnons and phonons.

論文

Status of the uncertainty quantification for severe accident sequences of different NPP-designs in the frame of the H-2020 project MUSA

Brumm, S.*; Gabrielli, F.*; Sanchez-Espinoza, V.*; Groudev, P.*; Ou, P.*; Zhang, W.*; Malkhasyan, A.*; Bocanegra, R.*; Herranz, L. E.*; Berda$"i$, M.*; et al.

Proceedings of 10th European Review Meeting on Severe Accident Research (ERMSAR 2022) (Internet), 13 Pages, 2022/05

The current HORIZON-2020 project on "Management and Uncertainties of Severe Accidents (MUSA)" aims at applying Uncertainty Quantification (UQ) in the modeling of Severe Accidents (SA), particularly in predicting the radiological source term of mitigated and unmitigated accident scenarios. Within its application part, the project is devoted to the uncertainty quantification of different severe accident codes when predicting the radiological source term of selected severe accident sequences of different nuclear power plant designs, e.g. PWR, VVER, and BWR. Key steps for this investigation are, (a) the selection of severe accident sequences for each reactor design, (b) the development of a reference input model for the specific design and SA-code, (c) the selection of a list of uncertain model parameters to be investigated, (d) the choice of an UQ-tool e.g. DAKOTA, SUSA, URANIE, etc., (e) the definition of the figures of merit for the UA-analysis, (f) the performance of the simulations with the SA-codes, and, (g) the statistical evaluation of the results using the capabilities, i.e. methods and tools offered by the UQ-tools. This paper describes the project status of the UQ of different SA codes for the selected SA sequences, and the technical challenges and lessons learnt from the preparatory and exploratory investigations performed.

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

 被引用回数:1 パーセンタイル:9.31(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

ITER test blanket module error field simulation experiments at DIII-D

Schaffer, M. J.*; Snipes, J. A.*; Gohil, P.*; de Vries, P.*; Evans, T. E.*; Fenstermacher, M. E.*; Gao, X.*; Garofalo, A. M.*; Gates, D. A.*; Greenfield, C. M.*; et al.

Nuclear Fusion, 51(10), p.103028_1 - 103028_11, 2011/10

 被引用回数:33 パーセンタイル:80.68(Physics, Fluids & Plasmas)

ITERのテストブランケットモジュールが作ると思われる誤差磁場の影響を調べる実験をDIII-Dにおいて実施した。プラズマ回転とモードロッキング,閉じ込め,LH遷移,ELM安定化,ELMとHモードペデスタル特性,高エネルギー粒子損失等を調べた。実験では、ITERの1つの赤道面ポートを模擬する3つ組のコイルを1セット使用した。その結果、ITERのTBMが作る誤差磁場のためにITERの運転が妨げられるような結果は得られなかった。一番大きな変化はプラズマ回転を減速させるものであり、非共鳴ブレーキング効果によってプラズマ全体の回転が50%程度減少した。密度や閉じ込めへの影響は、回転の影響の1/3程度である。これらの影響は、プラズマ圧力の高いプラズマや回転の低いプラズマで顕著である。それ以外の影響は軽微であった。

論文

PprI: A General switch responsible for extreme radioresistance of ${it Deinococcus radiodurans}$

Hua, Y.*; 鳴海 一成; Gao, G.*; Tian, B.*; 佐藤 勝也; 北山 滋; Shen, B.*

Biochemical and Biophysical Research Communications, 306(2), p.354 - 360, 2003/06

 被引用回数:147 パーセンタイル:95.72(Biochemistry & Molecular Biology)

放射線抵抗性細菌デイノコッカス・ラジオデュランスの放射線高感受性変異株の解析から、DNAの修復と損傷防御機構を担う主要スイッチタンパク質PprIを同定した。放射線高感受性変異株では、この遺伝子がトランスポゾンの挿入によって機能を失っていた。この遺伝子を完全に破壊すると放射線感受性が増大し、野生型遺伝子を導入すると放射線耐性が復帰した。放射線照射に伴い、PprIは${it recA}$遺伝子及び${it pprA}$遺伝子の発現を誘導するとともに、カタラーゼ活性をも助長した。これらの結果は、PprIタンパク質が、放射線応答におけるDNAの修復と防御の調節機構に重要な役割を果たしていることを強く示唆している。

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