RT Journal Article
T1 Nuclear astrophysics with radioactive ions at FAIR
A1 Álvarez Rodríguez, Raquel
A1 Fraile Prieto, Luis Mario
A1 López Herraiz, Joaquín
A1 Martínez Pérez, María Cristina
A1 Moreno Díaz, Óscar
A1 Udías Moinelo, José Manuel
AB 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.
PB IOP Publishing Ltd
SN 1742-6588
YR 2016
FD 2016
LK https://hdl.handle.net/20.500.14352/24369
UL https://hdl.handle.net/20.500.14352/24369
LA eng
NO ©IOP Publishing Ltd.Artículo escrito por más de 10 autores.Nuclear Physics in Astrophysics Conference (NPA) (6. 2013. Lisboa, Portugal).This project was supported by the HGF Young Investigators Project VH-NG-327, EMMI, H4F, HGS-HIRe, JINA, NAVI, DFG and ATHENA.
NO HGF Young Investigators
NO EMMI
NO HGS-HIRe
NO H4F
NO JINA
NO NAVI
NO DFG
NO ATHENA.
DS Docta Complutense
RD 6 abr 2025