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Nuclear astrophysics with radioactive ions at FAIR
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2016 (Engelska)Ingår i: NUCLEAR PHYSICS IN ASTROPHYSICS VI (NPA6), Institute of Physics Publishing (IOPP), 2016, 012044Konferensbidrag, Publicerat paper (Refereegranskat)
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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 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.

Ort, förlag, år, upplaga, sidor
Institute of Physics Publishing (IOPP), 2016. 012044
Serie
Journal of Physics Conference Series, ISSN 1742-6588 ; 665
Nationell ämneskategori
Astronomi, astrofysik och kosmologi
Identifikatorer
URN: urn:nbn:se:kth:diva-182871DOI: 10.1088/1742-6596/665/1/012044ISI: 000368236600044Scopus ID: 2-s2.0-84962624605OAI: oai:DiVA.org:kth-182871DiVA: diva2:906470
Konferens
6th Nuclear Physics in Astrophysics Conference (NPA), MAY 19-24, 2013, Hungarian Acad Sci, Inst Nucl Res, Lisbon, PORTUGAL
Anmärkning

QC 20160224

Tillgänglig från: 2016-02-24 Skapad: 2016-02-23 Senast uppdaterad: 2016-02-24Bibliografiskt granskad

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Cederwall, Bo

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Cederwall, BoWyss, Ramon
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Skolan för teknikvetenskap (SCI)KTH
Astronomi, astrofysik och kosmologi

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