Study of stellar reactions in explosive hydrogen burning with CRIB

Kubono, Shigeru*; Teranishi, Takashi*; Notani, Masahiro*; Yamaguchi, Hidetoshi*; Saito, Akito*; He, J. J.*; Wakabayashi, Yasuo*; Fujikawa, Hisashi*; Amadio, G.*; Baba, Hidetada*; Fukuchi, Tomonori*; Shimoura, Susumu*; Michimasa, Shinichiro*; Nishimura, Shunji*; Nishimura, Mitsuki*; Gono, Yasuyuki*; Odahara, Atsuko*; Kato, Seigo*; Moon, J. Y.*; Lee, J. H.*; Lee, C. S.*; Kim, J. C.*; Hahn, K. I.*; Ishikawa, Tomoko*; Hashimoto, Takashi; Ishiyama, Hironobu*; Watanabe, Yutaka*; Tanaka, Masahiko*; Miyatake, Hiroari; Frp, Zs.*; Guimares, V.*; Lichtenthaler, R.*

With using $^{17}F$ RNB from CRIB, proton inelastic scattering was observed. From this experiment, some resonance parameters have been deduced for the key reaction, $^{14}O(alpha,p)^{17}F$ at the explosive hydrogen burning stage in stars. Proton inelastic scattering of $^{23}Mg$ are also reported.

Language	:	English
Journal	:	Nuclear Physics A
Volume	:	758
Number	:
Pages	:	p.733 - 736
Publication Year/Month	:	2005/07
Meeting title	:	8th International Symposium on Nuclei in the Cosmos
Held date	:	2004/07
Location (city)	:	Vancouver
Location (country)	:	Canada
Patent information	:
PDF	:
Paper URL	:	https://doi.org/10.1016/j.nuclphysa.2005.05.132
DOI for research data	:
Keywords	:	no keyword
Research Facility	:
Press Release	:
Article of JAEA R&D Review	:
Cooperating Institute	:

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Registration No. : BB20071619
JAEA Abstracts No. :
Paper Submission No. : 3091

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