Astrophysical reaction rate of 30S(p, γ)31Cl studied by Coulomb dissociation

Y. Togano; T. Motobayashi; N. Aoi; H. Baba; S. Bishop; X. Cai; P. Doornenbal; D. Fang; T. Furukawa; K. Ieki; N. Iwasa; T. Kawabata; S. Kanno; N. Kobayashi; Y. Kondo; T. Kuboki; N. Kume; K. Kurita; M. Kurokawa; Y. G. Ma; Y. Matsuo; H. Murakami; M. Matsushita; T. Nakamura; K. Okada; S. Ota; Y. Satou; S. Shimoura; R. Shioda; K. N. Tanaka; S. Takeuchi; W. Tian; H. Wang; J. Wang; K. Yamada; Y. Yamada; K. Yoneda

Astrophysical reaction rate of ³⁰S(p, γ)³¹Cl studied by Coulomb dissociation

Y. Togano, T. Motobayashi, N. Aoi, H. Baba, S. Bishop, X. Cai, P. Doornenbal, D. Fang, T. Furukawa, K. Ieki, N. Iwasa, T. Kawabata, S. Kanno, N. Kobayashi, Y. Kondo, T. Kuboki, N. Kume, K. Kurita, M. Kurokawa, Y. G. MaY. Matsuo, H. Murakami, M. Matsushita, T. Nakamura, K. Okada, S. Ota, Y. Satou, S. Shimoura, R. Shioda, K. N. Tanaka, S. Takeuchi, W. Tian, H. Wang, J. Wang, K. Yamada, Y. Yamada, K. Yoneda

理学研究科・物理学専攻

研究成果: Conference article › 査読

抄録

The Coulomb dissociation of the proton-rich nucleus ³¹Cl was studied experimentally using a ³¹Cl beam at 58 MeV/nucleon with a lead target. The relative energy spectrum between ³⁰S ions and protons was obtained from the measured momentum vectors of the reaction products detected in coincidence by the invariant mass method. The first excited state in 31Cl was observed which is relevant to the resonant capture in the stellar ³⁰S(p, γ)³¹Cl reaction. Discussion for another observed state is also given.

本文言語	English
ジャーナル	Proceedings of Science
出版ステータス	Published - 2010
イベント	11th Symposium on Nuclei in the Cosmos, NIC 2010 - Heidelberg, Germany 継続期間: 2010 7 19 → 2010 7 23

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引用スタイル

Astrophysical reaction rate of ³⁰S(p, γ)³¹Cl studied by Coulomb dissociation. / Togano, Y.; Motobayashi, T.; Aoi, N.; Baba, H.; Bishop, S.; Cai, X.; Doornenbal, P.; Fang, D.; Furukawa, T.; Ieki, K.; Iwasa, N.; Kawabata, T.; Kanno, S.; Kobayashi, N.; Kondo, Y.; Kuboki, T.; Kume, N.; Kurita, K.; Kurokawa, M.; Ma, Y. G.; Matsuo, Y.; Murakami, H.; Matsushita, M.; Nakamura, T.; Okada, K.; Ota, S.; Satou, Y.; Shimoura, S.; Shioda, R.; Tanaka, K. N.; Takeuchi, S.; Tian, W.; Wang, H.; Wang, J.; Yamada, K.; Yamada, Y.; Yoneda, K.

In: Proceedings of Science, 2010.

研究成果: Conference article › 査読

Togano, Y, Motobayashi, T, Aoi, N, Baba, H, Bishop, S, Cai, X, Doornenbal, P, Fang, D, Furukawa, T, Ieki, K, Iwasa, N, Kawabata, T, Kanno, S, Kobayashi, N, Kondo, Y, Kuboki, T, Kume, N, Kurita, K, Kurokawa, M, Ma, YG, Matsuo, Y, Murakami, H, Matsushita, M, Nakamura, T, Okada, K, Ota, S, Satou, Y, Shimoura, S, Shioda, R, Tanaka, KN, Takeuchi, S, Tian, W, Wang, H, Wang, J, Yamada, K, Yamada, Y & Yoneda, K 2010, 'Astrophysical reaction rate of ³⁰S(p, γ)³¹Cl studied by Coulomb dissociation', Proceedings of Science.

Togano, Y. ; Motobayashi, T. ; Aoi, N. ; Baba, H. ; Bishop, S. ; Cai, X. ; Doornenbal, P. ; Fang, D. ; Furukawa, T. ; Ieki, K. ; Iwasa, N. ; Kawabata, T. ; Kanno, S. ; Kobayashi, N. ; Kondo, Y. ; Kuboki, T. ; Kume, N. ; Kurita, K. ; Kurokawa, M. ; Ma, Y. G. ; Matsuo, Y. ; Murakami, H. ; Matsushita, M. ; Nakamura, T. ; Okada, K. ; Ota, S. ; Satou, Y. ; Shimoura, S. ; Shioda, R. ; Tanaka, K. N. ; Takeuchi, S. ; Tian, W. ; Wang, H. ; Wang, J. ; Yamada, K. ; Yamada, Y. ; Yoneda, K. / Astrophysical reaction rate of ³⁰S(p, γ)³¹Cl studied by Coulomb dissociation. In: Proceedings of Science. 2010.

@article{d3e755949acd4e33b2f7fa250b23e8d5,

title = "Astrophysical reaction rate of 30S(p, γ)31Cl studied by Coulomb dissociation",

abstract = "The Coulomb dissociation of the proton-rich nucleus 31Cl was studied experimentally using a 31Cl beam at 58 MeV/nucleon with a lead target. The relative energy spectrum between 30S ions and protons was obtained from the measured momentum vectors of the reaction products detected in coincidence by the invariant mass method. The first excited state in 31Cl was observed which is relevant to the resonant capture in the stellar 30S(p, γ)31Cl reaction. Discussion for another observed state is also given.",

author = "Y. Togano and T. Motobayashi and N. Aoi and H. Baba and S. Bishop and X. Cai and P. Doornenbal and D. Fang and T. Furukawa and K. Ieki and N. Iwasa and T. Kawabata and S. Kanno and N. Kobayashi and Y. Kondo and T. Kuboki and N. Kume and K. Kurita and M. Kurokawa and Ma, {Y. G.} and Y. Matsuo and H. Murakami and M. Matsushita and T. Nakamura and K. Okada and S. Ota and Y. Satou and S. Shimoura and R. Shioda and Tanaka, {K. N.} and S. Takeuchi and W. Tian and H. Wang and J. Wang and K. Yamada and Y. Yamada and K. Yoneda",

year = "2010",

language = "English",

journal = "Proceedings of Science",

issn = "1824-8039",

publisher = "Sissa Medialab Srl",

note = "11th Symposium on Nuclei in the Cosmos, NIC 2010 ; Conference date: 19-07-2010 Through 23-07-2010",

}

TY - JOUR

T1 - Astrophysical reaction rate of 30S(p, γ)31Cl studied by Coulomb dissociation

AU - Togano, Y.

AU - Motobayashi, T.

AU - Aoi, N.

AU - Baba, H.

AU - Bishop, S.

AU - Cai, X.

AU - Doornenbal, P.

AU - Fang, D.

AU - Furukawa, T.

AU - Ieki, K.

AU - Iwasa, N.

AU - Kawabata, T.

AU - Kanno, S.

AU - Kobayashi, N.

AU - Kondo, Y.

AU - Kuboki, T.

AU - Kume, N.

AU - Kurita, K.

AU - Kurokawa, M.

AU - Ma, Y. G.

AU - Matsuo, Y.

AU - Murakami, H.

AU - Matsushita, M.

AU - Nakamura, T.

AU - Okada, K.

AU - Ota, S.

AU - Satou, Y.

AU - Shimoura, S.

AU - Shioda, R.

AU - Tanaka, K. N.

AU - Takeuchi, S.

AU - Tian, W.

AU - Wang, H.

AU - Wang, J.

AU - Yamada, K.

AU - Yamada, Y.

AU - Yoneda, K.

PY - 2010

Y1 - 2010

N2 - The Coulomb dissociation of the proton-rich nucleus 31Cl was studied experimentally using a 31Cl beam at 58 MeV/nucleon with a lead target. The relative energy spectrum between 30S ions and protons was obtained from the measured momentum vectors of the reaction products detected in coincidence by the invariant mass method. The first excited state in 31Cl was observed which is relevant to the resonant capture in the stellar 30S(p, γ)31Cl reaction. Discussion for another observed state is also given.

AB - The Coulomb dissociation of the proton-rich nucleus 31Cl was studied experimentally using a 31Cl beam at 58 MeV/nucleon with a lead target. The relative energy spectrum between 30S ions and protons was obtained from the measured momentum vectors of the reaction products detected in coincidence by the invariant mass method. The first excited state in 31Cl was observed which is relevant to the resonant capture in the stellar 30S(p, γ)31Cl reaction. Discussion for another observed state is also given.

UR - http://www.scopus.com/inward/record.url?scp=84887464943&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=84887464943&partnerID=8YFLogxK

M3 - Conference article

AN - SCOPUS:84887464943

JO - Proceedings of Science

JF - Proceedings of Science

SN - 1824-8039

T2 - 11th Symposium on Nuclei in the Cosmos, NIC 2010

Y2 - 19 July 2010 through 23 July 2010

ER -

Astrophysical reaction rate of 30S(p, γ)31Cl studied by Coulomb dissociation

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ASJC Scopus subject areas

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Astrophysical reaction rate of ³⁰S(p, γ)³¹Cl studied by Coulomb dissociation