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Neutron and Alpha Structure in Neutron Deficient Nuclei in Astrophysics

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【作者】 S.Kubono何建军H.YamaguchiD.M.KahlS.HayakawaT.TeranishiS.CheribiniM.GulinoY.K.KwonT.HashimotoY.WakabayashiN.IwasaS.KatoT.KomatsubaraD.N.BinhL.H.KhiemN.N.DuyT.KawabataC.SpitaleriG.G.RapisardaM.La CognataL.LamiaR.G.PizzoneS.RomanoA.CocN.de SerevilleF.HammacheG.KissS.Bishop

【Author】 S.Kubono;HE Jianjun;H.Yamaguchi;D.M.Kahl;S.Hayakawa;T.Teranishi;S.Cheribini;M.Gulino;Y.K.Kwon;T.Hashimoto;Y.Wakabayashi;N.Iwasa;S.Kato;T.Komatsubara;D.N.Binh;L.H.Khiem;N.N.Duy;T.Kawabata;C.Spitaleri;G.G.Rapisarda;M.La Cognata;L.Lamia;R.G.Pizzone;S.Romano;A.Coc;N.de Sereville;F.Hammache;G.Kiss;S.Bishop;Institute of Modern Physics,Chinese Academy of Sciences;RIKEN Nishina Center;Center for Nuclear Study,University of Tokyo;Department of Physics,Kyushu University;Laboratori Nazionali del Sud,Istituto Nazionale di Fisica Nucleare;Institute for Basic Science,70,Yuseong-daero 1689-gil;RIKEN Nishina Center,2-1 Hirosawa;Department of Physics,Tohoku University;Department of Physics,Yamagata University;Institute of Physics,Vietnam Academy for Science and Technology;Department of Physics,Kyoto University;IN2P3;Institute for Nuclear Research (MTA-ATOMKI);TUM;

【机构】 Institute of Modern Physics,Chinese Academy of SciencesRIKEN Nishina CenterCenter for Nuclear Study,University of TokyoDepartment of Physics,Kyushu UniversityLaboratori Nazionali del Sud,Istituto Nazionale di Fisica NucleareInstitute for Basic Science,70,Yuseong-daero 1689-gilRIKEN Nishina Center,2-1 HirosawaDepartment of Physics,Tohoku UniversityDepartment of Physics,Yamagata UniversityInstitute of Physics,Vietnam Academy for Science and TechnologyDepartment of Physics,Kyoto UniversityIN2P3Institute for Nuclear Research (MTA-ATOMKI)TUM

【摘要】 The paper includes discussions on the important role of neutron and alpha configurations in proton-rich nuclei in nuclear astrophysics in terms of nucleosynthesis under extremely high-temperature hydrogenburning conditions. The νp-process, which is supposed to take place at the very early epoch of type II supernovae, has considerable neutrons and alphas together with protons. The alpha-induced reactions on proton-rich unstable nuclei in the light mass regions is expected to play a crucial role, but very few of them were investigated well yet because of the experimental difficulties. Specifically, I report our recent experimental effort for the breakout process from the pp-chain region,7Be(α, γ)11C(α,p)14N under the νp-process. The neutron-induced reactions on proton-rich nuclei, which is even more a challenging subject, were investigated previously for very few nuclei. One possible experimental method is the Trojan Horse Method(THM). We successfully have applied THM to the 18F(n,α)14N reaction study with an unstable beam of 18F.

【Abstract】 The paper includes discussions on the important role of neutron and alpha configurations in proton-rich nuclei in nuclear astrophysics in terms of nucleosynthesis under extremely high-temperature hydrogenburning conditions. The νp-process, which is supposed to take place at the very early epoch of type II supernovae, has considerable neutrons and alphas together with protons. The alpha-induced reactions on proton-rich unstable nuclei in the light mass regions is expected to play a crucial role, but very few of them were investigated well yet because of the experimental difficulties. Specifically, I report our recent experimental effort for the breakout process from the pp-chain region,7Be(α, γ)11C(α,p)14N under the νp-process. The neutron-induced reactions on proton-rich nuclei, which is even more a challenging subject, were investigated previously for very few nuclei. One possible experimental method is the Trojan Horse Method(THM). We successfully have applied THM to the 18F(n,α)14N reaction study with an unstable beam of 18F.

【基金】 Japan Society for the Promotion of Science(JSPS)Research(KAKENHI)(26287058)
  • 【文献出处】 原子核物理评论 ,Nuclear Physics Review , 编辑部邮箱 ,2016年02期
  • 【分类号】P14;O571
  • 【下载频次】6
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