Nuclear astrophysics with radioactive ions at FAIR

Nuclear astrophysics with radioactive ions at FAIR (2013)

Authors:
- Reifarth, R
- Gasques, Leandro Romero
Autor USP: GASQUES, LEANDRO ROMERO - IF
Unidade: IF
Subjects: REAÇÕES NUCLEARES; ASTROFÍSICA; ÍONS PESADOS
Language: Inglês
Abstract: 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 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 o er 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.
Imprenta:
- Publisher place: São Paulo
- Date published: 2013

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ABNT

REIFARTH, R; GASQUES, Leandro Romero. Nuclear astrophysics with radioactive ions at FAIR. [S.l: s.n.], 2013.
APA

Reifarth, R., & Gasques, L. R. (2013). Nuclear astrophysics with radioactive ions at FAIR. São Paulo.
NLM

Reifarth R, Gasques LR. Nuclear astrophysics with radioactive ions at FAIR. 2013 ;
Vancouver

Reifarth R, Gasques LR. Nuclear astrophysics with radioactive ions at FAIR. 2013 ;