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사범대학
과학교육과
Journal papers
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Direct measurement of the astrophysical reaction 14O(α,p)17F
Title
Direct measurement of the astrophysical reaction 14O(α,p)17F
Authors
Notani M.
;
Kubono S.
;
Teranishi T.
;
Yanagisawa Y.
;
Michimasa S.
;
Ue K.
;
He J.J.
;
Iwasaki H.
;
Baba H.
;
Tamaki M.
;
Minemura T.
;
Shimoura S.
;
Hokoiwa N.
;
Wakabayashi Y.
;
Sasaki T.
;
Fukuchi T.
;
Odahara A.
;
Gono Y.
;
Fulop Zs.
;
Lee E.K.
;
Hahn K.I.
;
Moon J.Y.
;
Yun C.C.
;
Lee J.H.
;
Lee C.S.
;
Kato S.
Ewha Authors
한인식
SCOPUS Author ID
한인식
Issue Date
2004
Journal Title
Nuclear Physics A
ISSN
0375-9474
Citation
Nuclear Physics A vol. 738, no. 1-4 SUPPL., pp. 411 - 415
Indexed
SCI; SCIE; SCOPUS
Document Type
Article
Abstract
The stellar reaction 14O(α,p)17F, that critically determines the onset of the hightemperature rp-process, has been studied through a direct measurement with a low-energy radioactive 14O beam and a gaseous helium target cooled down to 30 K. The reaction cross section was measured directly by means of a thick target technique in the energy range of Ec.m(l4O+α) = 0.8-3.8 MeV. The 14O(α,p)17F* reaction leading to the first excited state in 17F was clearly observed for the first time, suggesting an increase of about 50% for the stellar reaction rate through resonances at around 7.1 MeV in 18Ne. © 2004 Published by Elsevier B.V.
DOI
10.1016/j.nuclphysa.2004.04.076
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