Nuclear astrophysics with radioactive ions at FAIR

6th Nuclear Physics in Astrophysics

物理学;天文学

Reifarth, R.^1 ; Altstadt, S.^1,2 ; Göbel, K.^1 ; Heftrich, T.^1,2 ; Heil, M.^2 ; Koloczek, A.^1,2 ; Langer, C.^1,2,60 ; Plag, R.^1,2 ; Pohl, M.^1 ; Sonnabend, K.^1 ; Weigand, M.^1 ; Adachi, T.^47 ; Aksouh, F.^5 ; Al-Khalili, J.^18 ; Algarawi, M.^5 ; Alghamdi, S.^5 ; Alkhazov, G.^3 ; Alkhomashi, N.^4 ; Alvarez-Pol, H.^6 ; Alvarez-Rodriguez, R.^7 ; Andreev, V.^3 ; Andrei, B.^8 ; Atar, L.^2 ; Aumann, T.^9 ; Avdeichikov, V.^10 ; Bacri, C.^11 ; Bagchi, S.^47 ; Barbieri, C.^18 ; Beceiro, S.^6 ; Beck, C.^12 ; Beinrucker, C.^1 ; Belier, G.^13 ; Bemmerer, D.^14 ; Bendel, M.^15 ; Benlliure, J.^6 ; Benzoni, G.^16 ; Berjillos, R.^17 ; Bertini, D.^2 ; Bertulani, C.^19 ; Bishop, S.^15 ; Blasi, N.^85 ; Bloch, T.^9 ; Blumenfeld, Y.^21 ; Bonaccorso, A.^22 ; Boretzky, K.^2 ; Botvina, A.^23 ; Boudard, A.^24 ; Boutachkov, P.^9 ; Boztosun, I.^25 ; Bracco, A.^85 ; Brambilla, S.^85 ; Monago, J. Briz^26 ; Caamano, M.^6 ; Caesar, C.^2 ; Camera, F.^85 ; Casarejos, E.^27 ; Catford, W.^18 ; Cederkall, J.^10 ; Cederwall, B.^28 ; Chartier, M.^31 ; Chatillon, A.^13 ; Cherciu, M.^32 ; Chulkov, L.^33 ; Coleman-Smith, P.^34 ; Cortina-Gil, D.^6 ; Crespi, F.^16 ; Crespo, R.^35 ; Cresswell, J.^31 ; Csatlós, M.^36 ; Déchery, F.^24 ; Davids, B.^37 ; Davinson, T.^38 ; Derya, V.^39 ; Detistov, P.^40 ; Fernandez, P. Diaz^6 ; Dijulio, D.^10 ; Dmitry, S.^33 ; Doré, D.^24 ; Dueñas, J.^17 ; Dupont, E.^24 ; Egelhof, P.^2 ; Egorova, I.^8 ; Elekes, Z.^14 ; Enders, J.^9 ; Endres, J.^39 ; Ershov, S.^8 ; Ershova, O.^1 ; Fernandez-Dominguez, B.^6 ; Fetisov, A.^3 ; Fiori, E.^41 ; Fomichev, A.^8 ; Fonseca, M.^1 ; Fraile, L.^7 ; Freer, M.^42 ; Friese, J.^15 ; Borge, M.G.^26 ; Redondo, D. Galaviz^44 ; Gannon, S.^31 ; Garg, U.^41,84 ; Gasparic, I.^9,86 ; Gasques, L.^45 ; Gastineau, B.^24 ; Geissel, H.^2 ; Gernhäuser, R.^15 ; Ghosh, T.^20 ; Gilbert, M.^1 ; Glorius, J.^1 ; Golubev, P.^10 ; Gorshkov, A.^8 ; Gourishetty, A.^46 ; Grigorenko, L.^8 ; Gulyas, J.^36 ; Haiduc, M.^32 ; Hammache, F.^11 ; Harakeh, M.^47 ; Hass, M.^48 ; Heine, M.^9 ; Hennig, A.^39 ; Henriques, A.^44 ; Herzberg, R.^31 ; Holl, M.^9 ; Ignatov, A.^9 ; Ignatyuk, A.^50 ; Ilieva, S.^9 ; Ivanov, M.^40 ; Iwasa, N.^51 ; Jakobsson, B.^10 ; Johansson, H.^49 ; Jonson, B.^49 ; Joshi, P.^52 ; Junghans, A.^14 ; Jurado, B.^53 ; Körner, G.^54 ; Kalantar, N.^47 ; Kanungo, R.^55 ; Kelic-Heil, A.^2 ; Kezzar, K.^5 ; Khan, E.^11 ; Khanzadeev, A.^3 ; Kiselev, O.^2 ; Kogimtzis, M.^34 ; Körper, D.^2 ; Kräckmann, S.^1 ; Kröll, T.^9 ; Krücken, R.^15 ; Krasznahorkay, A.^36 ; Kratz, J.^56 ; Kresan, D.^9 ; Krings, T.^57 ; Krumbholz, A.^9 ; Krupko, S.^8 ; Kulessa, R.^58 ; Kumar, S.^59 ; Kurz, N.^2 ; Kuzmin, E.^33 ; Labiche, M.^34 ; Langanke, K.^2 ; Lazarus, I.^34 ; Le Bleis, T.^15 ; Lederer, C.^1 ; Lemasson, A.^60 ; Lemmon, R.^34 ; Liberati, V.^30 ; Litvinov, Y.^2 ; Löher, B.^41 ; Herraiz, J. Lopez^7 ; Münzenberg, G.^2 ; Machado, J.^44

University of Frankfurt, Germany^1

GSI Darmstadt, Germany^2

PNPI Gatchina, Russia^3

Atomic Energy Research Institute, Saudi Arabia^4

King Saudi University, Saudi Arabia^5

University of Santiago de Compostela, Spain^6

Universidad Complutense de Madrid, Spain^7

JINR Dubna, Russia^8

TU Darmstadt, Germany

(10) Lund University, Sweden

(11) IPN Orsay, France

(12) IPHC-CNRS, UdS Strasbourg, France

(13) CEA Bruyères le Châtel, France

(14) Helmholtz-Zentrum Dresden-Rossendorf, Germany

(15) Technische Universität München, Germany

(16) INFN Milano, Italy

(17) University of Huelva, Spain

(18) University of Surrey, United Kingdom

(19) Texas A and M University-Commerce, United States

(20) VECC Kolkata, India

(21) CERN, Switzerland

(22) INFN Pisa, Italy

(23) INR RAS Moscow, Russia

(24) CEA Saclay, France

(25) Akdeniz University, Turkey

(26) CSIC Madrid, Spain

(27) Universidad de Vigo, Spain

(28) Royal Institute of Technology KTH Stockholm, Sweden

(29) SINP Kolkata, India

(30) University of the West of Scotland, United Kingdom

(31) University of Liverpool, United Kingdom

(32) Institute of Space Sciences, Romania

(33) NRC Kurchatov Institute Moscow, Russia

(34) STFC Daresbury Laboratory, United Kingdom

(35) Instituto Superior Tecnico, Portugal

(36) ATOMKI Debrecen, Hungary

(37) TRIUMF, Canada

(38) University of Edinburgh, United Kingdom

(39) University of Cologne, Germany

(40) INRNE BAS Sofia, Bulgaria

(41) Extreme Matter Institute, GSI Darmstadt, Germany

(42) University of Birmingham, United Kingdom

(43) University of Aarhus, Denmark

(44) University of Lisboa, Portugal

(45) University of Sao Paulo, Brazil

(46) Indian Institute of Technology Roorkee, India

(47) KVI/University of Groningen, Netherlands

(48) Weizmann Institute of Science Rehovot, Israel

(49) Chalmers University of Technology, Sweden

(50) IPPE Obninsk, Russia

(51) University of Tohoku, Japan

(52) University of York, United Kingdom

(53) CENBG, France

(54) NuPECC, Europe, France

(55) Saint Mary University, Canada

(56) University of Mainz, Germany

(57) SEMIKON Detector GmbH, Germany

(58) Jagiellonian University of Krakow, Poland

(59) University of Delhi, India

(60) NSCL/MSU, United States

(61) BARC Mumbai, India

(62) IFJ PAN Krakow, Poland

(63) University of Padova, Italy

(64) Federal Fluminense University, Brazil

(65) Tokyo Institute of Technology, Japan

(66) University of Yale, United States

(67) TIFR Mumbai, India

(68) CSNSM Orsay, France

(69) Polytechnic University of Tomsk, Russia

(70) Svedberg Laboratory, Sweden

(71) TU Dresden, Germany

(72) University of Basel, Switzerland

(73) RIKEN, Japan

(74) GANIL, France

(75) ESS Bilbao, Spain

(76) IFIN-HH Bucharest, Romania

(77) Ruhr University Bochum, Germany

(78) RCNP Osaka, Japan

(79) Beihang University, China

(80) Mid Sweden University, Sweden

(81) Uppsala University, Sweden

(82) IAI RAS St. Petersburg, Russia

(83) University of Stockholm, Sweden

(84) University of Notre Dame, United States

(85) INFN Rome, Italy

(86) RBI, Zagreb, Croatia^9

关键词: Facility for antiproton and ion research;    High yield;    Neutron capture;    Nuclear astro-physics;    Radioactive ions;    Reaction cross-sections;    Reaction data;    Time-reversed;   

Others  :  https://iopscience.iop.org/article/10.1088/1742-6596/665/1/012044/pdf
DOI  :  10.1088/1742-6596/665/1/012044

学科分类：天文学(综合)

来源: IOP

【 摘 要 】

The nucleosynthesis of elements beyond iron is dominated by neutron captures in the s and r processes. However, 32 stable, proton-rich isotopes cannot be formed during those processes, because they are shielded from the s-process flow and r-process, β-decay chains. These nuclei are attributed to the p and rp process. For all those processes, current research in nuclear astrophysics addresses the need for more precise reaction data involving radioactive isotopes. Depending on the particular reaction, direct or inverse kinematics, forward or time-reversed direction are investigated to determine or at least to constrain the desired reaction cross sections. The Facility for Antiproton and Ion Research (FAIR) will offer unique, unprecedented opportunities to investigate many of the important reactions. The high yield of radioactive isotopes, even far away from the valley of stability, allows the investigation of isotopes involved in processes as exotic as the r or rp processes.