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Nuclear astrophysics with radioactive ions at FAIR
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2016 (English)In: Journal of Physics: Conference Series, Vol. 665, no 1, article id 012044Article in journal (Refereed) Published
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Abstract [en]

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, β-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.

Place, publisher, year, edition, pages
2016. Vol. 665, no 1, article id 012044
National Category
Physical Sciences
Identifiers
URN: urn:nbn:se:miun:diva-27845DOI: 10.1088/1742-6596/665/1/012044ISI: 000368236600044Scopus ID: 2-s2.0-84962624605OAI: oai:DiVA.org:miun-27845DiVA, id: diva2:934775
Conference
6th Nuclear Physics in Astrophysics, NPA 2013; Lisbon; Portugal; 19 May 2013 through 24 May 2013; Code 119707
Note

Conference Paper

Available from: 2016-06-09 Created: 2016-06-09 Last updated: 2017-08-09Bibliographically approved

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CiteExportLink to record
Permanent link

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Cite
Citation style
  • apa
  • ieee
  • modern-language-association-8th-edition
  • vancouver
  • Other style
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  • de-DE
  • en-GB
  • en-US
  • fi-FI
  • nn-NO
  • nn-NB
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  • Other locale
More languages
Output format
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  • asciidoc
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