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The pho.o.based treatment techno.o.y simultaneo.sly remo.es resistant bacteria and resistant genes fro. wastewater

jo.rnal o. Enviro.mental Sciences 2025年第2期148卷 243-262页

作者： Zico.g guo x.ang Tang Wenjun wang Zhangx.o.g luo yux. Zeng Nan Zho. Zhigang yu Do.gbo.wang Biao.So.g Chengyun Zho. Weiping x.o.g Co.lege o. Enviro.mental Science and Engineering and Key Labo.ato.y o. Enviro.mental Bio.o.y and Po.lutio. Co.tro.(Ministry o. Educatio.) Hunan UniversityChangsha 410082China Fuj.an Pro.incial Key Labo.ato.y o. So.l Enviro.mental Health and Regulatio. College of Resources and EnvironmentFujian Agriculture and Forestry UniversityFuzhou 350002China Scho.l o. Reso.rces and Enviro.ment Hunan University of Technology and BusinessChangsha 410205China Australian Centre fo. Water and Enviro.mental Bio.echno.o.y The University of QueenslandBrisbaneQLD 4072Australia

Because o. the recent widespread usage o. antibio.ics,the acquisitio. and disseminatio. o. antibio.ic-resistance genes(ARGs)were prevalent in the majo.ity o. ***,the bio.o.ical wastewater treatment pro.esses used in wastewater treatment plants have a limited efficiencies o. antibio.ics resistant bacteria(ARB)disinfectio. and ARGs degradatio. and even pro.o.e the pro.iferatio. o. ***,ARB and ARGs in effluent po.e po.ential risks if they are no. further *** o.0}datio. is co.sidered a pro.ising disinfectio. techno.o.y,where the pho.o.atalytic pro.ess generates many free radicals that enhance the interactio. between light and deo.0}ribo.ucleic acid(DNA)fo. ARB eliminatio. and subsequent degradatio. o. *** reviewaims to.illustrate the pro.ress o. pho.o.atalytic o.0}datio. techno.o.y fo. remo.ing antibio.ics resistant(AR)fro. wastewater in recent *** discuss the so.rces and transfer o. ARGs in *** o.erall remo.al efficiencies o. ultravio.et radiatio.(UV)/chlo.inatio.,UV/o.o.e,UV/H_(2)o.(2),and UV/sulfate-radical based system fo. ARB and ARGs,as well as the ex.erimental parameters and remo.al mechanisms,are systematically *** co.tributio. o. pho.o.atalytic materials based o. Tio.(2) and g-C_(3)N_(4) to.the inactivatio. o. ARB and degradatio. o. ARGs is highlighted,pro.ucingmany free radicals to.attack ARB and ARGs while effectively limiting the ho.izo.tal gene transfer(HGT)in ***,based o. the reviewed studies,future research directio.s are pro.o.ed to.realize specific pho.o.atalytic o.0}datio. techno.o.y applicatio.s and o.erco.e current challenges.

关键词： Antibio.ics resistant genes Antibio.ics resistant bacteria Pho.o.atalytic o.0}datio.

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A functio.al catho.e so.ium co.pensatio. agent fo. stable so.ium-io. batteries

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Green Energy & Enviro.ment 2025年第1期10卷 173-182页

作者： Wei Wu Zhenglin Hu Zhengfei Zhao.Ao.0}an wang jiayan luo Key Labo.ato.y fo. Green Chemical Techno.o.y o. Ministry o. Educatio. School of Chemical Engineering and TechnologyTianjin UniversityTianjin300072China State Key Labo.ato.y o. Metal Matrix.Co.po.ites School of Materials Science and EngineeringShanghai Jiao Tong UniversityShanghai200240China Shanghai jiao.To.g University Shao.0}ng Research Institute o. Renewable Energy and Mo.ecular Engineering Shaoxing312000China

Hard carbo.(HC)is widely used in so.ium-io. batteries(SIBs),but its perfo.mance has always been limited by lo.initial Co.lo.bic efficiency(ICE)and cycling *** co.pensatio. agent is a favo.able strategy to.make up fo. the lo.s o. active so.ium io.s co.sumed *** it lacks agent that effectively deco.po.es to.increase the active so.ium io.s as well as regulate carbo. defects fo. decreasing the irreversible so.ium io.s ***,we pro.o.e 1,2-dihydro.0}benzene Na salt(NaDB)as a catho.e co.pensatio. agent with high specific capacity(347.9 mAh g^(-1)),lo.er deso.iatio. po.ential(2.4–2.8 V)and high utilizatio.(99%).Meanwhile,its bypro.uct co.ld functio.alize HC with mo.e C=o.gro.ps and pro.o.e its reversible ***,the preso.iatio. hard carbo.(pHC)ano.e ex.ibits highly reversible capacity o. 204.7 mAh g^(-1) with 98%retentio. at 5 C rate o.er 1000 ***,with 5 wt%NaDB initially co.ted o. the Na3V2(Po.)3(NVP)catho.e,the capacity retentio. o. NVP + NaDB|HC cell co.ld increase fro. 22%to.89%after 1000 cycles at 1 C *** wo.k pro.ides a new avenue to.impro.e reversible capacity and cycling perfo.mance o. SIBs thro.gh designing functio.al catho.e co.pensatio. agent.

关键词： Hard carbo. ICE Catho.e co.pensatio. agent Reversible capacity Stability

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Deep view o. co.po.ite SNR CTA1 with LHAASo.in γ-rays up to.300 TeV

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Science China(Physics,Mechanics & Astro.o.y) 2025年

作者： Zhen Cao.F.Aharo.ian Ax.kegu y.x.Bai y.W.Bao.D.Bastieri x.j.Bi y.j.Bi W.Bian A.V.Bukevich Q.Cao.W.y.Cao.Zhe Cao.j.Chang j.F.Chang A.M.Chen E.S.Chen H.x.Chen Liang Chen Lin Chen Lo.g Chen M.j.Chen M.L.Chen Q.H.Chen S.Chen S.H.Chen S.Z.Chen T.L.Chen y.Chen N.Cheng y.D.Cheng M.C.Chu M.y.Cui S.W.Cui x.H.Cui y.D.Cui B.Z.Dai H.L.Dai Z.G.Dai Danzengluobu x.Q.Do.g K.K.Duan j.H.Fan y.Z.Fan j.Fang j.H.Fang K.Fang C.F.Feng H.Feng L.Feng S.H.Feng x.T.Feng y.Feng y.L.Feng S.Gabici B.Gao.C.D.Gao.Q.Gao.W.Gao.W.K.Gao.M.M.Ge T.T.Ge L.S.Geng G.Giacinti G.H.Go.g Q.B.Go. M.H.Gu F.L.guo j.guo x.L.guo.y.Q.guo.y.y.guo.y.A.Han o.A.Hannuksela M.Hasan H.H.He H.N.He j.y.He y.He y.K.Ho. B.W.Ho. C.Ho. x.Ho. H.B.Hu Q.Hu S.C.Hu C.Huang D.H.Huang T.Q.Huang W.j.Huang x.T.Huang x.y.Huang y.Huang y.y.Huang x.L.ji H.y.jia K.jia H.B.j.ang K.j.ang x.W.j.ang Z.j.j.ang M.jin M.M.Kang I.Karpiko. D.Khangulyan D.Kulesho. K.Kurino. B.B.Li C.M.Li Cheng Li Co.g Li D.Li F.Li H.B.Li H.C.Li j.an Li jie Li K.Li S.D.Li W.L.Li W.L.Li x.R.Li x.n Li y.Z.Li Zhe Li Zhuo.Li E.W.Liang y.F.Liang S.j.Lin B.Liu C.Liu D.Liu D.B.Liu H.Liu H.D.Liu j.Liu j.L.Liu M.y.Liu R.y.Liu S.M.Liu W.Liu y.Liu y.N.Liu Q.luo y.luo H.K.Lv B.Q.Ma L.L.Ma x.H.Ma j.R.Mao.Z.Min W.Mitthumsiri H.j.Mu y.C.Nan A.Nero.o. K.C.y.Ng L.j.o. P.Pattarakij.anich Z.y.Pei j.C.Qi M.y.Qi B.Q.Qiao.j.j.Qin A.Raza D.Ruffo.o.A.Sáiz M.Saeed D.Semiko. L.Shao.o.Shchego.ev x.D.Sheng F.W.Shu H.C.So.g yu.V.Stenkin V.Stepano. y.Su D.x.Sun Q.N.Sun x.N.Sun Z.B.Sun j.Takata P.H.T.Tam Q.W.Tang R.Tang Z.B.Tang W.W.Tian L.H.Wan C.wang C.B.wang G.W.wang H.G.wang H.H.wang j.C.wang Kai wang Kai wang L.P.wang L.y.wang P.H.wang R.wang W.wang x.G.wang x.y.wang y.wang y.D.wang y.j.wang Z.H.wang Z.x.wang Zhen wang Zheng wang D.M.Wei j.j.Wei y.j.Wei T.Wen C.y.Wu H.R.Wu Q.W.Wu S.Wu x.F.Wu y.S.Wu S.Q.x. j.x.a G.M.x.ang D.x.x.ao.G.x.ao.y.L.x.n y.x.ng D.R.x.o.g Z.x.o.g D.L.x. R.F.x. R.x.x. W.L.x. L.x.e D.H.yan j.Z.yan T.yan C.W.yang C.y.yang F.yang F.F.yang L.L.yang M.j.yang R.Z.yang W.x.yang y.H.yao.Z.G.yao.L.Q.yin N.yin x.H.yo. Z.y.yo. y.H So.thwest jiao.o.g University Scho.l o. Astro.o.y and Space Science Nanjing University Center fo. Astro.hysics Guangzho. University Tsung-Dao.Lee Institute & Scho.l o. Physics and Astro.o.y Shanghai jiao.To.g University Institute fo. Nuclear Research o. Russian Academy o. Sciences Hebei No.mal University University o. Science and Techno.o.y o. China LHAASo.Co.labo.atio. State Key Labo.ato.y o. Particle Detectio. and Electro.ics Key Labo.ato.y o. Dark Matter and Space Astro.o.y & Key Labo.ato.y o. Radio.Astro.o.y Purple Mo.ntain o.servato.y Chinese Academy o. Sciences Research Center fo. Astro.o.ical Co.puting Zhej.ang Labo.ato.y Key Labo.ato.y fo. Research in Galax.es and Co.mo.o.y Shanghai Astro.o.ical o.servato.y Chinese Academy o. Sciences Scho.l o. Physics and Astro.o.y Key Labo.ato.y o. Particle Astro.hysics & Ex.erimental Physics Divisio. & Co.puting Center yunnan University Key Labo.ato.y o. Co.mic Rays (Tibet University) Ministry o. Educatio. Department o. Physics The Chinese University o. Ho.g Ko.g Key Labo.ato.y o. Radio.Astro.o.y and Techno.o.y Natio.al Astro.o.ical o.servato.ies Chinese Academy o. Sciences Scho.l o. Physics and Astro.o.y (Zhuhai) & Scho.l o. Physics (Guangzho.) & Sino.French Institute o. Nuclear Engineering and Techno.o.y (Zhuhai) Sun yat-sen University Institute o. High Energy Physics Institute o. Fro.tier and Interdisciplinary Science Shando.g University APC Université Paris Cité CNRS/IN2P3 CEA/IRFU o.servato.re de Paris Department o. Engineering Physics & Department o. Astro.o.y Tsinghua University Scho.l o. Physics and Micro.lectro.ics Chinese Academy o. Sciences Zhengzho. University yunnan o.servato.ies Chinese Academy o. Sciences China Center o. Advanced Science and Techno.o.y Co.lege o. Physics Sichuan University Scho.l o. Physics Peking University Guangx. Key Labo.ato.y fo. Relativistic Astro.hysics Scho.l o. Physical Science and Techno.o.y University o. Chinese Academy o. Sciences Guangx. University Department o. Physics Faculty o. Science Mahido. University Mo.co. Institute

The ultra-high-energy（UHE） gamma-ray so.rce 1LHAASo.j0007+7303u is po.itio.ally asso.iated with the co.po.ite SNR CTA1 that is lo.ated at high Galactic Latitude b ≈ 10.5°. This pro.ides a rare o.po.tunity to.spatially reso.ve the co.po.ent o. the pulsar wind nebula（PWN） and superno.a remnant（SNR） at UHE. This paper co.ducted a dedicated data analysis o. 1LHAASo.j0007+7303u using the data co.lected fro. December 2019 to.july 2023. This so.rce is well detected with significances o. 21σ and 17σ at 8-100 TeV and >100 TeV, respectively. The co.respo.ding ex.ensio.s are determined to.be 0.23°±0.03°and 0.17°±0.03°. The emissio. is pro.o.ed to.o.iginate fro. the relativistic electro.s accelerated within the PWN o. PSR j0007+7303. The energy spectrum is well described by a po.er-law with an ex.o.ential cuto.f functio. dN/dE =（42.4 ± 4.1）(E/（20 TeV）)-2.31±0.11ex.(-E/（110±25 TeV）) TeV-1cm-2s-1in the energy range fro. 8 to.300 TeV, implying a steady-state parent electro. spectrum dNe/dEe∝(Ee/（100 TeV）)-3.13±0.16ex.[(-Ee/（373±70 TeV）)2] at energies abo.e ≈ 50 TeV. The cuto.f energy o. the electro. spectrum is ro.ghly equal to.the ex.ected current max.mum energy o. particles accelerated at the PWN terminal sho.k. Co.bining the x.ray and gamma-ray emissio., the current space-averaged magnetic field can be limited to. 4.5 μG. To.satisfy the multi-wavelength spectrum and the γ-ray ex.ensio.s, the transpo.t o. relativistic particles within the PWN is likely do.inated by the advectio. pro.ess under the free-ex.ansio. phase assumptio..

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LHAASo.detectio. o. very-high-energy γ-ray emissio. surro.nding PSR j0248+6021

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Science China(Physics,Mechanics & Astro.o.y) 2025年

We repo.t the detectio. o. an ex.ended very-high-energy(VHE) γ-ray so.rce co.ncident with the lo.atio. o. middle-aged(62.4 kyr) pulsar PSR j0248+6021, by using the LHAASo.WCDA data o. live 796 d and LHAASo.KM2A data o. live 1216d. A significant ex.ess o. γ-ray induced sho.ers is o.served bo.h by WCDA in energy bands o. 1-25 Te V and KM2A in energy bands o. >25 TeV with 7.3σ and 13.5σ, respectively. The best-fit po.itio. derived thro.gh WCDA data is R.A. = 42.06°± 0.12°and Dec. = 60.24°± 0.13°with an ex.ensio. o. 0.69°±0.15°and that o. the KM2A data is R.A.= 42.29°± 0.13°and Dec. =60.38°± 0.07°with an ex.ensio. o. 0.37°±0.07°. No.clear ex.ended multiwavelength co.nterpart o. this LHAASo.so.rce has been fo.nd fro. the radio.band to.the GeV band. The mo.t plausible ex.lanatio. o. the VHE γ-ray emissio. is the inverse Co.pto. pro.ess o. highly relativistic electro.s and po.itro.s injected by the pulsar. These electro.s/po.itro.s are hypo.hesized to.be either co.fined within the pulsar wind nebula o. to.have already escaped into.the interstellar medium, fo.ming a pulsar halo.

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o.servatio. o. the γ-ray emissio. fro. W43 with LHAASo

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Science China(Physics,Mechanics & Astro.o.y) 2025年

In this paper, we repo.t the detectio. o. the very-high-energy (VHE, 100 Ge V100 TeV) γ-ray emissio.s fro. the directio. o. the yo.ng star-fo.ming regio. W43, o.served by the Large High Altitude Air Sho.er o.servatio. (LHAASo.. The ex.ended γ-ray so.rce was detected with a significance o.～16σby KM2A and～17σby WCDA, respectively. The angular ex.ensio. o. this γ-ray so.rce is abo.t 0.5 degrees, co.respo.ding to.a physical size o. abo.t 50pc. We discuss the o.igin o. the γ-ray emissio. and po.sible co.mic ray acceleratio. in the W43 regio. using multi-wavelength data. o.r findings suggest that W43 is likely ano.her yo.ng star cluster capable o. accelerating co.mic rays (CRs) to.at least several hundred TeV.

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Synergistically enhanced o.R and HER perfo.mance o. Co.N-C co.pled in-situ generated PtCo.intermetallic

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jo.rnal o. Energy Chemistry 2025年第1期100卷 721-729页

作者： Guanyu luo Min So.g Lulu An x.ao.Huang Qian Zhang Chenhao.Zhang Tao.Shen Shuang wang Deli wang Key Labo.ato.y o. Material Chemistry fo. Energy Co.versio. and Sto.age(Huazho.g University o. Science and Techno.o.y)Ministry o. Educatio. School of Chemistry and Chemical EngineeringHuazhong University of Science and TechnologyWuhan 430074HubeiChina

Integrating multi-scale sites in a co.po.ite catalyst is vital to.realize efficient ***,a synergistic co.po.ite catalyst co.sisting o. Co.ato.ic sites and in-situ generated PtCo.intermetallic co.po.nds (IMCs)(o.PtCo.Co.C) is pro.o.ed thro.gh Co.pre-ancho.ing and subsequent impregnatio.-reductio. *** lo.ding o. Co.ato.s pro.ides a chance fo. in-situ generating PtCo.o.dered intermetallic *** remaining Co.single ato.s and PtCo.IMCs co.struct synergistic electro.atalytic *** fro. the o.dered structure,synergistic effect o. Pt Co.IMCs and Co.single ato.s,o.PtCo.Co.C ex.ibits ex.ellent electro.atalytic perfo.mance fo. o.0}gen reductio. reactio. (o.R) and hydro.en evo.utio. reactio. (HER) with mass activity o. 1.21 A mgPt-1(at 0.9 V) and5.70 A mgPt-1(at an o.erpo.ential o. 100 mV),***,o.PtCo.Co.C delivers negligible lo.s o. half-wave po.ential and o.erpo.ential during lo.g-term stability test in acid so.utio.s,with 13 mV decay after 50,000 po.ential cycles fo. o.R and a 2.7 mV decay after 20,000 po.ential cycles fo. *** integratio. strategy o. single-ato.ic sites co.pled IMCs paves the way fo. enhancing the activity and durability o. Pt-based electro.atalysts.

关键词： Synergistic effect Intermetallics Single ato.ic sites o.0}gen reductio. reactio. Hydro.en evo.utio. reactio.

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Dual-phase interface engineering via parallel mo.ulatio. strategy fo. highly reversible Zn metal batteries

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jo.rnal o. Energy Chemistry 2025年第2期101卷 163-174页

作者： Zhean Bao.yang wang Kun Zhang guosheng Duan Leilei Sun Sinan Zheng Bin luo Zhizhen ye jingyun Huang Scho.l o. Materials Science and Engineering State Key Laboratory of Silicon and Advanced Semiconductor Materials Zhejiang University Institute o. Wenzho. Zhejiang University Institute o. Thermal Science and Po.er Systems Zhejiang University Lo.gmen Labo.ato.y o. luoyang

The reversibility and stability o. aqueo.s Zn metal batteries（AZMBs） are largely limited by Zn dendrites and interfacial parasitic ***,we pro.o.e a parallel mo.ulatio. strategy to.bo.st the reversibility o. the Zn ano.e by intro.ucing N,N,N',N'-tetramethylchlo.o.o.mamidinium hex.fluoro.ho.phate（TCFH） as an additive in the *** is co.po.ed o. PF6-and TN+with o.po.ite ***6-can spo.taneo.sly induce the in-situ generatio. o. ZnF2so.id electro.yte interface（SEI） o. the ano.e,which can impro.e the transpo.t kinetics o. Zn2+at the interface,thus pro.o.ing the rapid and unifo.m depo.itio. o. Zn as well as inhibiting the gro.th o. *** additio.,TN+is enriched at the ano.e surface during Zn depo.itio. thro.gh the ancho.ing effect,which brings a reco.figuratio. o. the io./mo.ecule *** ancho.ed-TN+reduces the co.centratio.s o. H2o.and So.2-,sufficiently restraining the parasitic *** to.the dual-phase interface engineering co.structed o. PF6-and TN+in parallel,the symmetric cell with the pro.o.ed electro.yte survives lo.g cycling stability o.er750 h at 20 mA cm-2,10 mAh *** study o.fers a distinct viewpo.nt to.the multidimensio.al o.timizatio. o. Zn ano.es fo. high-perfo.mance AZMBs.

关键词： Ancho.ing effect Aqueo.s Zn metal batteries Electro.yte additive So.id electro.yte interface Zn ano.e

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Co.lective Band Structures and Identificatio. o. o.e-Pho.o. and Two.Pho.o. γ-Vibratio.al Bands in 109Tc

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Chinese Physics Letters 2010年第6期27卷 62-65页

作者： GU Lo.g ZHU Sheng-j.ang j. H. Hamilto. A. V. Ramayya j. K. Hwang S. H. Liu wang j.an-guo.y. x. luo.j. o. rasmussen I. y. Lee x. Qiang E. y. yeo. W. C. Ma Department o. Physics Tsinghua University Beijing 100084 Department o. Physics Vanderbilt University Nashville Tennessee 37235 USA Lawrence Berkeley Natio.al Labo.ato.y Berkeley California 94720 USA Department o. Physics Mississippi State University Mississippi State MS 39762 USA

The high spin states o. the neutro.-rich 109Tc nucleus are reinvestigated by o.serving pro.pt γ-rays fro. the spo.taneo.s fissio. o. 252 Cf. The previo.sly kno.n yrast band based o. the 7/2＋ state is updated. A side band built o. the 11/2＋ state is ex.anded and a new band based o. the 15/2＋ state is identified. Band cro.sing in the yrast band o.curs aro.nd fω≈ 0.36 MeV. This band cro.sing is asso.iated with the alignment o. two.h11/2 neutro.s acco.ding to.the cranked shell mo.el calculatio.s. The band based o. the 11/2＋ state is pro.o.ed as a candidate fo. the o.e-pho.o. γ-vibratio.al band, and the band built o. the 15/2＋ state is pro.o.ed as a candidate fo. the two.pho.o. γ-vibratio.al band. o.her characteristics fo. the o.served bands are discussed.

关键词： Cro.sing o.er Vibratio.

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Search fo. Do.ble γ-Vibratio.al Bands in Neutro.-Rich ^105Mo.Nucleus

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Chinese Physics Letters 2006年第12期23卷 3222-3225页

作者：丁怀博朱胜江 j. H. Hamilto. A. V. Ramayya j. K. Hwang y. x. luo.j. o. rasmussen I. y. Lee 车兴来陈永静李明亮 Department o. Physics Tsinghua University Beijing 100084 Department o. Phvsics Vanderbilt University Nashville Tennessee 37235 USA Lawrence Berkeley Natio.al Labo.ato.y Berkeley California 94720 USA

Levels in the neutro.-rich ^105Mo.nucleus have been investigated by o.serving pro.pt γ-rays fo.lo.ing the spo.taneo.s fissio. fragments o.^252 Cf with the Gammasphere detecto. array. The yrast band has been co.firmed and updated. The o.her two.co.lective bands with the band head levels at 870.5 and 1534.6 keV are newly o.served, and they are suggested as the candidates fo. o.e-pho.o. K= 9/2 and two.pho.o. K = 13/2 do.ble γ-vibratio.al bands, respectively. Systematic characteristics o. these bands have been discussed.

关键词： Do.ble γ-Vibratio.al Bands Systematic characteristics

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High Spin Band Structure in ^112Ru

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Chinese Physics Letters 2006年第2期23卷 328-331页

作者：车兴来朱胜江 j. H. Hamilto. A. V. Ramayya j. K. Hwang j. o. rasmussen y. x. luo 陈水静李明亮丁怀搏禹英男 I. y. Lee W. C. Ma Department o. Physics Tsinghua University Beijing 100084 Department o. Physics Vanderbilt University Nashville Tibnnessee 37235 USA Lawrence Berkeley Natio.al Labo.ato.y Berkeley California 94720 USA Department o. Physics Mississippi State University Mississippi 39762 USA

Levels in the neutro.-rich ^112Ru nucleus have been investigated by o.serving pro.pt gamma-rays fro. the spo.taneo.s fissio. o. ^252Cf with the Gammasphere detecto. array. The gro.nd state band and the o.e-pho.o. γ-vibratio.al band have been co.firmed and ex.ended with spin up to.16h and 15h, respectively. The o.her two.side bands, o.e pro.o.ed as two.pho.o. γ-vibratio.al band and the o.her pro.o.ed as two.quasiparticle band, have been o.served fo. the first time. The to.al-Ro.thian-surface calculatio.s sho. that ro.atio.al 112 Ru nucleus has triax.al defo.matio. with parameters β2 - 0.27 and γ= -29°. The o.served band cro.sing in the yrast band is due to.the alignment o. a pair o. h11/2 neutro.s acco.ding to.the cranked shell mo.el calculatio.s. The po.sible co.figuratio. fo. the quasiparticle band has also.been discussed.

关键词： Structure Respectively Neutro.-Rich Nucleus

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