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izvor podataka: crosbi

Nuclear astrophysics with radioactive ions at FAIR (CROSBI ID 230901)

Prilog u časopisu | izvorni znanstveni rad | međunarodna recenzija

Reifarth, R. ; Altstadt, S. ; Göbel, K. ; Heftrich, T. ; Heil, M. ; Koloczek, A. ; Langer, C. ; Plag, R. ; Pohl, M. ; Sonnabend, K. et al. Nuclear astrophysics with radioactive ions at FAIR // Journal of physics. Conference series, 665 (2016), 1; 012044, 12. doi: 10.1088/1742-6596/665/1/012044

Podaci o odgovornosti

Reifarth, R. ; Altstadt, S. ; Göbel, K. ; Heftrich, T. ; Heil, M. ; Koloczek, A. ; Langer, C. ; Plag, R. ; Pohl, M. ; Sonnabend, K. ; Weigand, M. ; ... ; Gašparić, Igor ; ... ; Zuber, K.

engleski

Nuclear astrophysics with radioactive ions at FAIR

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.

r-process nucleosynthesis ; weak-interaction rates ; s-process ; stars ; supernovae ; light

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Podaci o izdanju

665 (1)

2016.

012044

12

objavljeno

1742-6588

1742-6596

10.1088/1742-6596/665/1/012044

Povezanost rada

Fizika

Poveznice
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