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Report No.
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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; F$"u$r$"o$p, Zs.*; Guimar$~a$es, 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.

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Category:Physics, Nuclear

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