Please use this identifier to cite or link to this item:
logo share SHARE logo core CORE BASE
Visualizar otros formatos: MARC | Dublin Core | RDF | ORE | MODS | METS | DIDL | DATACITE

Nuclear astrophysics with radioactive ions at FAIR

AuthorsReifarthl, R.; Álvarez-Pol, H.; Álvarez-Rodríguez, 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 CSIC ORCID; Galaviz, D. CSIC ORCID; Machado, J.; Martinez Perez, M.; Moreno, Óscar; Nácher, Enrique CSIC ORCID CVN; Parkar, V.; Paradela, C.; Perea, Ángel CSIC ORCID; Pereira, J.; Ribeiro, Guillermo; Rodriguez Frutos, T.; Rodriguez Vignote, J.; Sanchez del Río Saez, J.; Sanchez-Rosado, J.; Sarriguren, Pedro CSIC ORCID; Silva, J.; Tengblad, Olof CSIC ORCID ; Volknandt, M.
Issue Date2016
PublisherInstitute of Physics Publishing
CitationJournal of Physics: Conference Series 665: 052110 (2016)
AbstractThe 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.
DescriptionR. Reifarth et al: ; 12 págs.; 9 figs.; Open Access funded by Creative Commons Atribution Licence 3.0 ; Nuclear Physics in Astrophysics VI (NPA6)
Publisher version (URL)
Identifiersdoi: 10.1088/1742-6596/665/1/012044
issn: 1742-6588
Appears in Collections:(CFMAC-IEM) Artículos

Files in This Item:
File Description SizeFormat
Nuclear astrophysics.pdf3,85 MBAdobe PDFThumbnail
Show full item record
Review this work


checked on Nov 23, 2021

Google ScholarTM




WARNING: Items in Digital.CSIC are protected by copyright, with all rights reserved, unless otherwise indicated.