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사범대학
과학교육과
Journal papers
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Experimental challenge to nuclear physics problems in the νp-process
Title
Experimental challenge to nuclear physics problems in the νp-process
Authors
Kubono S.
;
Binh D.N.
;
Hayakawa S.
;
Hashimoto T.
;
Kahl D.M.
;
Yamaguchi H.
;
Wakabayashi Y.
;
Teranishi T.
;
Iwasa N.
;
Komatsubara T.
;
Kato S.
;
Chen A.
;
Cherubini S.
;
Choi S.H.
;
Hahn I.S.
;
He J.J.
;
Khiem L.H.
;
Lee C.S.
;
Kwon Y.K.
;
Wanajo S.
;
Janka H.-T.
Ewha Authors
한인식
SCOPUS Author ID
한인식
Issue Date
2012
Journal Title
AIP Conference Proceedings
ISSN
0094-243X
Citation
AIP Conference Proceedings vol. 1484, pp. 189 - 196
Indexed
SCOPUS
Document Type
Conference Paper
Abstract
Astrophysical stellar reactions at extremely high temperatures involve a variety of problems both in nuclear reactions and nuclear structures. Specifically, the problems in the νpprocess were discussed in this talk based on our recent experimental results with low-energy RI beams and a simulation study. The νp-process is one of the key processes for investigating the mechanism of type II supernovae, and the process could be possibly responsible for "the excess production" of p-nuclei around mass 90-100. Alpha cluster resonances have been discovered experimentally to play a crucial role for the stellar (α, p) reactions just above the alpha threshold. Neutron induced reactions in the proton-rich nuclear regions in the νp-process are also suggested to play an important role, which involve nuclear structures of high level density at high excitation energies, probably giant resonances. The discussion also covered the p-nuclei production through the νp-process at around mass 100. © 2012 American Institute of Physics.
DOI
10.1063/1.4763394
ISBN
9780735410961
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