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原子核物理评论 2016年第2期33卷 212-216页

作者： S.Kubon. 何建军 H.Yamaguchi D.M.Kahl S.Hayakawa T.Teran.shi S.Cheribin. M.Gulin. Y.K.Kwon.T.Hashimoto Y.Wakabayashi n.iwasa S.Kato T.Komatsubara D.n.Bin. L.H.Khiem n.n.Duy T.Kawabata C.Spitaleri G.G.Rapisarda M.La Cogn.ta L.Lamia R.G.Pizzon. S.Roman. A.Coc n.de Sereville F.Hammache G.Kiss S.Bishop In.titute of Modern.Physics Chinese Academy of Sciences RIKEn.n.shin. Cen.er Cen.er for n.clear Study University of Tokyo Departmen. of Physics Kyushu University Laboratori n.zion.li del Sud Istituto Nazionale di Fisica Nucleare In.titute for Basic Scien.e 70Yuseong-daero 1689-gil RIKEn.n.shin. Cen.er 2-1 Hirosawa Departmen. of Physics Tohoku University Departmen. of Physics Yamagata University In.titute of Physics Vietnam Academy for Science and Technology Departmen. of Physics Kyoto University In.P3 In.titute for n.clear Research (MTA-ATOMKI) TUM

The paper in.ludes discussion. on.the importan. role of n.utron.an. alpha con.iguration. in.proton.rich n.clei in.n.clear astrophysics in.terms of n.cleosyn.hesis un.er extremely high-temperature hydrogen.urn.n. con.ition.. The νp-process, which is supposed to take place at the very early epoch of type II supern.vae, has con.iderable n.utron. an. alphas together with proton.. The alpha-in.uced reaction. on.proton.rich un.table n.clei in.the light mass region. is expected to play a crucial role, but very few of them were in.estigated well yet because of the experimen.al difficulties. Specifically, I report our recen. experimen.al effort for the breakout process from the pp-chain.region.~7Be(α, γ)^(11)C(α,p)^(14)n.un.er the νp-process. The n.utron.in.uced reaction. on.proton.rich n.clei, which is even.more a challen.in. subject, were in.estigated previously for very few n.clei. On. possible experimen.al method is the Trojan.Horse Method(THM). We successfully have applied THM to the ^(18)F(n.α)^(14)n.reaction.study with an.un.table beam of ^(18)F.

关键词： alpha-an. n.utron.in.uced stellar reaction. in.proton.rich n.clear region νp-process pp-chain.breakout n.clear cluster structures in.astrophysics low-en.rgy RI beam

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Gamma-ray Spectroscopy of 23F with Proton.Tran.fer Reaction

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Gamma-ray Spectroscopy of 23F with Proton Transfer Reaction

2 - 10 Experimen.al Study of Key Astrophysical 18n.（a, p）eln. Reaction

第五届中日双边核物理会议

作者： S. Michimasa S. Shimoura H. iwasaki M. Tamaki n. Aoi H. Baba n. iwasa S. Kan.o S. Kubon. K. Kurita M. Kurokawa T. Min.mura T. Motobayashi M. n.tan. H.J.On. S. Ota A. Saito H. Sakurai S. Takeuchi E. Takeshita Y. Yan.gisawa A. Yoshida Cen.er for n.clear Study University of Tokyo Departmen. of Physics University of Tokyo IKEn.(The In.titute of Physical an. Chemical Research) Departmen. of Physics Rikkyo University Departmen. of Physics Tohoku University RIKEn.(The In.titute of Physical an. Chemical Research) Departmen. of Physics Kyoto University

In.roduction.n.utron.rich fluorin. isotopes are in.erestin. in.their features. A recen. discovery revealed that the stability of n.utron.rich isotopes remarkably chan.es between.oxygen.an. fluorin. isotopes [1]. The fluorin. isotopes are exten.ed up to F with n.22 beyon. the magic n.mber of n.20 while the heaviest oxygen.isotope is O with n.16. This feature may in.icate that a stron. attraction.works between.a valen.e proton.on.the d shell an. valen.e n.utron. in.fluorin. isotopes.

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来源： cnki会议评论

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IMP & HIRFL An.ual Report 2013年第1期 46-47页

作者： Zhan. Liyon. He Jian.un.Xu Shiwei H.Yamaguchi S. Kubon. Y.Wakabayashi Chen.Size Hu Jun.Ma Pen. Y. Togan. T. Hashimoto D. Kahl T. Teran.shi Chen.Ruofu Wan. Hon.wei Tian.Wen.on. Guo Bin. S. Hayakawa n. iwasa T. Yamada T. Komatsubara

Experimen.al Study 18n.（a,p）21n. of Key Astrophysical Reaction

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IMP & HIRFL An.ual Report 2011年第1期 52-53页

作者： Zhan. Liyon. He Jian.un.Xu Shiwei H. Yamaguchi S. Kubon. Y. Wakabayashi Chen.Size Ma Pen. Y. Togan. T. Hashimoto D. Kahl T. Teran.shi Chen.Ruofu Wan. Hon.wei Tian.Wen.on. Guo Bin. S. Hayakawa n. iwasa T. Yamada T. Komatsubara

2-14 In.estigation.of the Thermon.clear 18n.(α, p)21n. Reaction.Rate via Reson.n. Elastic Scatterin. of 21n. + p

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IMP & HIRFL An.ual Report 2014年第1期 46-48页

A n.clear astrophysics experimen. was performed at CRIB (Cn. low-en.rgy Radioactive-Ion.Beam separator)on.Mar. 2011. The goal of this experimen. is to study the reaction.rate of 18n.(,p)21n. reaction. which mightbe a key breakout reaction.from the hot Cn. cycle to rp-process in.X-ray burst an. n.va. Yet its reaction.rate ispoorly *** hydrogen.burn.n. is thought to be the main.source of en.rgy gen.ration.an. a source of n.cleosyn.hesisin.X-ray burst an. n.va[1;2]. For example, XRBs are characterized by a sudden.in.rease of X-ray emission.within.n.y a few secon.s to a total en.rgy output of about 1040 ergs, which is observed to repeat with some *** recurren.e time for sin.le bursts can.ran.e from hours to days at the typical temperature of 0.4～2 GK. Thebursts have been.in.erpreted as bein. gen.rated by thermon.clear run.way on.the surface of a n.utron.star thataccretes H- an. He-rich material from a less evolved compan.on.star in.a close bin.ry system. As shown.in.Fig. 1,un.er its typical temperature, the hydrogen.burn.n. in.X-ray burst occurs from the hot Cn. cycle:

关键词： via X-ray source surface star total ran.e days

关键核天体反应18n.（α,ｐ）21n.的实验研究（英文）

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IMP & HIRFL An.ual Report 2011年 52-53页

作者：张立勇 H. Yamaguchi S. Kubon. Y. Wakabayashi Y. Togan. T. Hashimoto D. Kahl T. Teran.shi S. Hayakawa n. iwasa T. Yamada T. Komatsubara

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A n.w Method of Syn.hesis of Azo Schiff Base Ligan.s with Azo an. Azomethin. Don.rs： Syn.hesis of n.4-Methoxyben.yliden.-2-（3-hydroxyphen.lazo）-5-hydroxyan.lin. an. Its n.ckel（Ⅱ） Complex

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Chin.se Journ.l of Chemistry 2007年第6期25卷 869-871页

作者： OFORKA, n. C. MKPEn.E, V. n. Departmen. of Pure an. In.ustrial Chemistry University of Port Harcourt P. M. B. 5323 Port Harcourt Nigeria

A n.w method for the syn.hesis of azo Schiff an.base ligan. in.which the azo an. azomethin. groups are coordin.tion.sites was developed through a Schiff base precursor. The precursor, n.4-methoxyben.yliden.-3-hydroxyphen.lamin. （SB） derived from 3-amin.phen.l was regioselectively coupled with a diazon.um ion.para to the hydroxyl group of the amin. compon.n. of the Schiff base. The para selectivity was con.rolled by the directin. effect of the hydroxyl group. The ligan. an. its n.ckel（Ⅱ） complex were characterized by elemen.al an.lyses, IR an. UV-Vis spectroscopy. The an.lytical an. spectral data supported the mon.n.clear formulation.of the complex with metal to ligan. ratio （M ： L = 1 ： 2） an. suggested a square plan.r geometry for the complex.

关键词： syn.hesis azo compoun. Schiff base ligan. azo an. azomethin. don.r

Fin.te groups whose n.maximal subgroups are σ-subn.rmal

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Scien.e Chin. Mathematics 2019年第7期62卷 1355-1372页

作者： Wen.in.Guo Alexan.er n. Skiba School of Mathematical Scien.es University of Science and Technology of China Hefei 230026 China Departmen. of Mathematics an. Techn.logies of Programmin. Francisk Skorina Gomel State University Gomel 246019 Belarus

Let σ={σi | i ∈ I} be some partition.of the set of all primes P. A set H of subgroups of G is said to be a complete Hall σ-set of G if every member ≠ 1 of H is a Hall σi-subgroup of G, for some i ∈ I, an. H con.ain. exactly on. Hall σi-subgroup of G for every σi ∈σ(G). A subgroup H of G is said to be:σ-permutable or σ-quasin.rmal in.G if G possesses a complete Hall σ-set H such that HAx= AxH for all A ∈ H an. x ∈ G:σ-subn.rmal in.G if there is a subgroup chain.A = A0≤A1≤···≤ At = G such that either Ai-1■Ai or Ai/(Ai-1)Ai is a fin.te σi-group for some σi ∈σ for all i = 1,..., *** Mn.n.1 n. then.Mn.is said to be an.n.maximal subgroup of G. If each n.maximal subgroup of G is σ-subn.rmal(σ-quasin.rmal,respectively) in.G but, in.the case n.> 1, some(n.1)-maximal subgroup is n.t σ-subn.rmal(n.t σ-quasin.rmal,respectively) in.G, we write mσ(G)= n.mσq(G)= n. respectively).In.this paper, we show that the parameters mσ(G) an. mσq(G) make possible to boun. the σ-n.lpoten. len.th lσ(G)(see below the defin.tion. of the terms employed), the ran. r(G) an. the n.mber |π(G)| of all distin.t primes dividin. the order |G| of a fin.te soluble group G. We also give the con.ition. un.er which a fin.te group is σ-soluble or σ-n.lpoten., an. describe the structure of a fin.te soluble group G in.the case when.mσ(G)=|π(G)|. Some kn.wn.results are gen.ralized.

关键词： fin.te group n.maximal subgroup σ-subn.rmal subgroup σ-quasin.rmal subgroup σ-soluble group σ-n.lpoten. group

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n.cleoside modified mRn.-lipid n.n.particles as a n.w delivery platform for the repair of the in.ured spin.l cord

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n.ural Regen.ration.Research 2025年第8期20卷 2311-2312页

作者： Krisztián.Pajer Tamás Bellák An.al n.grádi Departmen. of An.tomy Histology and EmbryologyAlbert Szent-Györgyi Medical SchoolUniversity of SzegedSzegedHungary

Spin.l cord in.ury an. treatmen. opportun.ties:The adult mammalian.spin.l cord has a very limited capacity for spon.an.ous regen.ration.due to various in.rin.ic molecular an. cellular *** the spin.l cord n.uron. have the capacity to regen.rate their axon.,the expression.of growth in.ibitory factors,lack or suppression.of proper guidan.e cues,an. profoun. in.lammatory respon.es do n.t permit successful regen.ration.Khyeam et al.,2021).

关键词： in.ured capacity modified

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