학술논문

Nuclear astrophysics with radioactive ions at FAIR
Document Type
Author
Reifarthl, R.Altstadt, S.Goebell, K.Heftrich, T.Heil, M.Koloczek, A.Langer, C.Plag, R.Pohl, M.Sonnabend, K.Weigand, M.Adachi, T.Aksouh, F.Al-Khalili, J.AlGarawi, M.AlGhamdi, S.Alkhazov, G.Alkhomashi, N.Alvarez-Pol, H.Alvarez-Rodriguez, R.Andreev, V.Andrei, B.Atar, L.Aumann, T.Adeichikov, V.Bacri, C.Bagchi, S.Barbieri, C.Beceiro, S.Beck, C.Beinrucker, C.Belier, G.Bemmerer, D.Bendel, M.Benlliure, J.Benzoni, G.Berjillos, R.Bertini, D.Bertulani, C.Bishop, S.Blasi, N.Bloch, T.Blumenfeld, Y.Bonaccorso, A.Boretzky, K.Botvina, A.Boudard, A.Boutachkov, P.Boztosun, I.Bracco, A.Brambilla, S.Briz Monago, J.Caamano, M.Caesar, C.Camera, F.Casarejos, E.Catford, W.Cederkall, J.Cederwall, B.Chartier, M.Chatillon, A.Cherciu, M.Chulkov, L.Coleman-Smith, P.Cortina-Gil, D.Crespi, F.Crespo, R.Cresswell, J.Csatlos, M.Dechery, F.Davids, B.Davinson, T.Derya, V.Detistov, P.Diaz Fernandez, P.DiJuliot, D.Dmitry, S.Dore, D.Duenas, J.Dupont, E.Egelhof, P.Egorova, I.Elekes, Z.Enders, J.Endres, J.Ershov, S.Ershova, O.Fernandez-Dominguez, B.Fetisov, A.Fiori, E.Fomichev, A.Fonseca, M.Fraile, L.Freer, M.Friese, J.Borge, M. G.Galaviz Redondo, D.Gannon, S.Garg, U.Gasparic, I.Gasques, L.Gastineau, B.Geissel, H.Gernhaeuser, R.Ghosh, T.Gilbert, M.Glorius, J.Golubev, P.Gorshkov, A.Gourishett, A.Grigorenko, L.Gulyas, J.Haiduc, M.Hammache, F.Harakeh, M.Hass, M.Heine, M.Hennig, A.Henriques, A.Herzberg, R.Holl, M.Ignatov, A.Ignatyuk, A.Ilieva, S.Ivanov, M.Iwasa, N.Jakobsson, B.Johansson, H.Jonson, B.Joshi, P.Junghans, A.Jurado, B.Koerner, G.Kalantar, N.Kanungo, R.Kelic-Heil, A.Kezzar, K.Khan, E.Khanzadeev, A.Kiselev, O.Kogimtzis, M.Koerper, D.Kraeckmann, S.Kroell, T.Kruecken, R.Krasznahorkay, A.Kratz, J.Kresan, D.Krings, T.Krumbholz, A.Krupko, S.Kulessa, R.Kumar, S.Kurz, N.Kuzmin, E.Labiche, M.Langanke, K.Lazarus, I.Le Bleis, T.Lederer, C.Lemasson, A.Lemmon, R.Liberati, V.Litvinov, Y.Loeher, B.Lopez Herraiz, J.Muenzenberg, G.Machado, J.Maev, E.Mahata, K.Mancusi, D.Marganiec, J.Martinez Perez, M.Marusov, V.Mengoni, D.Million, B.Morcelle, V.Moreno, O.Movsesyan, A.Nacher, E.Najafi, M.Nakamura, T.Naqvi, F.Nikolski, E.Nilsson, T.Nociforo, C.Nolan, P.Novatsky, B.Nyman, G.Ornelas, A.Palit, R.Pandit, S.Panin, V.Paradela, C.Parkar, V.Paschalis, S.Pawlowski, P.Perea, A.Pereira, J.Petrache, C.Petri, M.Pickstone, S.Pietralla, N.Pietri, S.Pivovarov, Y.Potlog, P.Prokofiev, AlexanderRastrepina, G.Rauscher, T.Ribeiro, G.Ricciardi, M.Richter, A.Rigollet, C.Riisager, K.Rios, A.Ritter, C.Frutos, T. RodriguezRodriguez Vignote, J.Roeder, M.Romig, C.Rossi, D.Roussel-Chomaz, P.Rout, P.Roy, S.Soederstroem, P.Sarkar, M. SahaSakuta, S.Salsac, M.Sampson, J.del Rio Saez, J. SanchezSanchez Rosado, J.Sanjari, S.Sarriguren, P.Sauerwein, A.Savran, D.Scheidenberger, C.Scheit, H.Schmidt, S.Schmitt, C.Schnorrenberger, L.Schrock, P.Schwengner, R.Seddon, D.Sherrill, B.Shrivastava, A.Sidorchuk, S.Silva, J.Simon, H.Simpson, E.Singh, P.Slobodan, D.Sohler, D.Spieker, M.Stach, D.Stan, E.Stanoiu, M.Stepantsov, S.Stevenson, P.Strieder, F.Stuhl, L.Suda, T.Suemmerer, K.Streicher, B.Taieb, J.Takechi, M.Tanihata, I.Taylor, J.Tengblad, O.Ter-Akopian, G.Terashima, S.Teubig, P.Thies, R.Thoennessen, M.Thomas, T.Thornhill, J.Thungstrom, G.Timar, J.Togano, Y.Tomohiro, U.Tornyi, T.Tostevin, J.Townsley, C.Trautmann, W.Trivedi, T.Typel, S.Uberseder, E.Udias, J.Uesaka, T.Uvarov, L.Vajta, Z.Velho, P.Vikhrov, V.Volknandt, M.Volkov, V.von Neumann-Cose, P.von Schmid, M.Wagner, A.Wamers, F.Weick, H.Wells, D.Westerberg, LarsWieland, O.Wiescher, M.Wimmer, C.Wimmer, K.Winfield, J. S.Winkel, M.Woods, P.Wyss, R.Yakorev, D.Yavor, M.Cardona, J. ZamoraZartova, I.Zerguerras, T.Zgura, I.Zhdanov, A.Zhukov, M.Zieblinski, M.Zilges, A.Zuber, K.
Source
NUCLEAR PHYSICS IN ASTROPHYSICS VI (NPA6) Journal of Physics Conference Series.
Subject
Language
English
ISSN
1742-6588
Abstract
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 beta-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.