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Nuclear astrophysics with radioactive ions at FAIR

Reifarthl, R.; Altstadt, S.; Goebell, K.; Heftrich, T.; Heil, M.; Koloczek, A.; Langer, C.; Plag, R.; Pohl, M. and Sonnabend, K., et al. (2016) 6th Nuclear Physics in Astrophysics Conference (NPA) In Journal of Physics: Conference Series 665. p.012044-012044
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... (More)
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. (Less)
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Journal of Physics: Conference Series
volume
665
pages
012044 - 012044
publisher
IOP Publishing
conference name
6th Nuclear Physics in Astrophysics Conference (NPA)
external identifiers
  • wos:000368236600044
  • scopus:84962624605
ISSN
1742-6588
1742-6596
DOI
10.1088/1742-6596/665/1/012044
language
English
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yes
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90acb9ff-2b4a-4c96-a22b-74a1ddd4a4e4 (old id 8748079)
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2016-02-23 09:17:32
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2017-02-05 03:21:26
@inproceedings{90acb9ff-2b4a-4c96-a22b-74a1ddd4a4e4,
  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.},
  author       = {Reifarthl, R. and Altstadt, S. and Goebell, K. and Heftrich, T. and Heil, M. and Koloczek, A. and Langer, C. and Plag, R. and Pohl, M. and Sonnabend, K. and Weigand, M. and Adachi, T. and Aksouh, F. and Al-Khalili, J. and AlGarawi, M. and AlGhamdi, S. and Alkhazov, G. and Alkhomashi, N. and Alvarez-Pol, H. and Alvarez-Rodriguez, R. and Andreev, V. and Andrei, B. and Atar, L. and Aumann, T. and Avdeichikov, Vladimir and Bacri, C. and Bagchi, S. and Barbieri, C. and Beceiro, S. and Beck, C. and Beinrucker, C. and Belier, G. and Bemmerer, D. and Bendel, M. and Benlliure, J. and Benzoni, G. and Berjillos, R. and Bertini, D. and Bertulani, C. and Bishop, S. and Blasi, N. and Bloch, T. and Blumenfeld, Y. and Bonaccorso, A. and Boretzky, K. and Botvina, A. and Boudard, A. and Boutachkov, P. and Boztosun, I. and Bracco, A. and Brambilla, S. and Briz Monago, J. and Caamano, M. and Caesar, C. and Camera, F. and Casarejos, E. and Catford, W. and Cederkäll, Joakim and Cederwall, B. and Chartier, M. and Chatillon, A. and Cherciu, M. and Chulkov, L. and Coleman-Smith, P. and Cortina-Gil, D. and Crespi, F. and Crespo, R. and Cresswell, J. and Csatlos, M. and Dechery, F. and Davids, B. and Davinson, T. and Derya, V. and Detistov, P. and Diaz Fernandez, P. and DiJulio, Douglas and Dmitry, S. and Dore, D. and Duenas, J. and Dupont, E. and Egelhof, P. and Egorova, I. and Elekes, Z. and Enders, J. and Endres, J. and Ershov, S. and Ershova, O. and Fernandez-Dominguez, B. and Fetisov, A. and Fiori, E. and Fomichev, A. and Fonseca, M. and Fraile, L. and Freer, M. and Friese, J. and Borge, M. G. and Galaviz Redondo, D. and Gannon, S. and Garg, U. and Gasparic, I. and Gasques, L. and Gastineau, B. and Geissel, H. and Gernhaeuser, R. and Ghosh, T. and Gilbert, M. and Glorius, J. and Golubev, Pavel and Gorshkov, A. and Gourishett, A. and Grigorenko, L. and Gulyas, J. and Haiduc, M. and Hammache, F. and Harakeh, M. and Hass, M. and Heine, M. and Hennig, A. and Henriques, A. and Herzberg, R. and Holl, M. and Ignatov, A. and Ignatyuk, A. and Ilieva, S. and Ivanov, M. and Iwasa, N. and Jakobsson, Bo and Johansson, H. and Jonson, B. and Joshi, P. and Junghans, A. and Jurado, B. and Koerner, G. and Kalantar, N. and Kanungo, R. and Kelic-Heil, A. and Kezzar, K. and Khan, E. and Khanzadeev, A. and Kiselev, O. and Kogimtzis, M. and Koerper, D. and Kraeckmann, S. and Kroell, T. and Kruecken, R. and Krasznahorkay, A. and Kratz, J. and Kresan, D. and Krings, T. and Krumbholz, A. and Krupko, S. and Kulessa, R. and Kumar, S. and Kurz, N. and Kuzmin, E. and Labiche, M. and Langanke, K. and Lazarus, I. and Le Bleis, T. and Lederer, C. and Lemasson, A. and Lemmon, R. and Liberati, V. and Litvinov, Y. and Loeher, B. and Lopez Herraiz, J. and Muenzenberg, G. and Machado, J. and Maev, E. and Mahata, K. and Mancusi, D. and Marganiec, J. and Martinez Perez, M. and Marusov, V. and Mengoni, D. and Million, B. and Morcelle, V. and Moreno, O. and Movsesyan, A. and Nacher, E. and Najafi, M. and Nakamura, T. and Naqvi, F. and Nikolski, E. and Nilsson, T. and Nociforo, C. and Nolan, P. and Novatsky, B. and Nyman, G. and Ornelas, A. and Palit, R. and Pandit, S. and Panin, V. and Paradela, C. and Parkar, V. and Paschalis, S. and Pawlowski, P. and Perea, A. and Pereira, J. and Petrache, C. and Petri, M. and Pickstone, S. and Pietralla, N. and Pietri, S. and Pivovarov, Y. and Potlog, P. and Prokofiev, A. and Rastrepina, G. and Rauscher, T. and Ribeiro, G. and Ricciardi, M. and Richter, A. and Rigollet, C. and Riisager, K. and Rios, A. and Ritter, C. and Frutos, T. Rodriguez and Rodriguez Vignote, J. and Roeder, M. and Romig, C. and Rossi, D. and Roussel-Chomaz, P. and Rout, P. and Roy, S. and Soederstroem, P. and Sarkar, M. Saha and Sakuta, S. and Salsac, M. and Sampson, J. and del Rio Saez, J. Sanchez and Sanchez Rosado, J. and Sanjari, S. and Sarriguren, P. and Sauerwein, A. and Savran, D. and Scheidenberger, C. and Scheit, H. and Schmidt, S. and Schmitt, C. and Schnorrenberger, L. and Schrock, P. and Schwengner, R. and Seddon, D. and Sherrill, B. and Shrivastava, A. and Sidorchuk, S. and Silva, J. and Simon, H. and Simpson, E. and Singh, P. and Slobodan, D. and Sohler, D. and Spieker, M. and Stach, D. and Stan, E. and Stanoiu, M. and Stepantsov, S. and Stevenson, P. and Strieder, F. and Stuhl, L. and Suda, T. and Suemmerer, K. and Streicher, B. and Taieb, J. and Takechi, M. and Tanihata, I. and Taylor, J. and Tengblad, O. and Ter-Akopian, G. and Terashima, S. and Teubig, P. and Thies, R. and Thoennessen, M. and Thomas, T. and Thornhill, J. and Thungstrom, G. and Timar, J. and Togano, Y. and Tomohiro, U. and Tornyi, T. and Tostevin, J. and Townsley, C. and Trautmann, W. and Trivedi, T. and Typel, S. and Uberseder, E. and Udias, J. and Uesaka, T. and Uvarov, L. and Vajta, Z. and Velho, P. and Vikhrov, V. and Volknandt, M. and Volkov, V. and von Neumann-Cose, P. and von Schmid, M. and Wagner, A. and Wamers, F. and Weick, H. and Wells, D. and Westerberg, L. and Wieland, O. and Wiescher, M. and Wimmer, C. and Wimmer, K. and Winfield, J. S. and Winkel, M. and Woods, P. and Wyss, R. and Yakorev, D. and Yavor, M. and Cardona, J. Zamora and Zartova, I. and Zerguerras, T. and Zgura, I. and Zhdanov, A. and Zhukov, M. and Zieblinski, M. and Zilges, A. and Zuber, K.},
  booktitle    = {Journal of Physics: Conference Series},
  issn         = {1742-6588},
  language     = {eng},
  pages        = {012044--012044},
  publisher    = {IOP Publishing},
  title        = {Nuclear astrophysics with radioactive ions at FAIR},
  url          = {http://dx.doi.org/10.1088/1742-6596/665/1/012044},
  volume       = {665},
  year         = {2016},
}