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Nuclear astrophysics with radioactive ions at FAIR

AutorReifarthl, R.; Alvarez-Pol, H.; Alvarez-Rodriguez, R.; Beceiro, S.; Benlliure, J.; Berjillos, R.; Briz Monago, J.; Caamano, M.; Cortina-Gil, D.; Casarejos, E.; Diaz Fernandez, P.; Dueñas, J.; Fernandez-Dominguez, B.; Fraile, L.; García Borge, María José ; Galaviz, D. ; Machado, J.; Martinez Perez, M.; Moreno, O.; Nácher, Enrique ; Parkar, V.; Paradela, C.; Perea, Ángel ; Pereira, J.; Ribeiro, Guillermo; Rodriguez Frutos, T.; Rodriguez Vignote, J.; Sanchez del Río Saez, J.; Sanchez-Rosado, J.; Sarriguren, Pedro ; Silva, J.; Tengblad, Olof ; Volknandt, M.
Fecha de publicación2016
EditorInstitute of Physics Publishing
CitaciónJournal of Physics: Conference Series 665: 052110 (2016)
ResumenThe 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 ow and r-process -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 oer 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.
DescripciónR. Reifarth et al: ; 12 págs.; 9 figs.; Open Access funded by Creative Commons Atribution Licence 3.0 ; Nuclear Physics in Astrophysics VI (NPA6)
Versión del editorhttp://doi.org/10.1088/1742-6596/665/1/012044
URIhttp://hdl.handle.net/10261/151854
DOI10.1088/1742-6596/665/1/012044
Identificadoresdoi: 10.1088/1742-6596/665/1/012044
issn: 1742-6588
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