Study of stellar reactions in explosive hydrogen burning with CRIB

S. Kubono; T. Teranishi; M. Notani; H. Yamaguchi; A. Saito; J. J. He; M. Wakabayashi; H. Fujikawa; G. Amadio; H. Baba; T. Fukuchi; S. Shimoura; S. Michimasa; S. Nishimura; M. Nishimura; Y. Gono; A. Odahara; S. Kato; J. Y. Moon; J. H. Lee; C. S. Lee; J. C. Kim; K. I. Hahn; T. Ishikawa; T. Hashimoto; H. Ishiyama; Y. X. Watanabe; M. H. Tanaka; H. Miyatake; Zs Fülöp; V. Guimarães; R. Lichtenthaler

doi:10.1016/j.nuclphysa.2005.05.132

Study of stellar reactions in explosive hydrogen burning with CRIB

S. Kubono, T. Teranishi, M. Notani, H. Yamaguchi, A. Saito, J. J. He, M. Wakabayashi, H. Fujikawa, G. Amadio, H. Baba, T. Fukuchi, S. Shimoura, S. Michimasa, S. Nishimura, M. Nishimura, Y. Gono, A. Odahara, S. Kato, J. Y. Moon, J. H. LeeC. S. Lee, J. C. Kim, K. I. Hahn, T. Ishikawa, T. Hashimoto, H. Ishiyama, Y. X. Watanabe, M. H. Tanaka, H. Miyatake, Zs Fülöp, V. Guimarães, R. Lichtenthaler

Experimental Particle Physics

Research output: Contribution to journal › Article › peer-review

2 Citations (Scopus)

Abstract

With using low-energy RI beams from an in-flight RIB separator, CRIB, the most crucial stellar reaction ¹⁴O(α,p)¹⁷F for the onset of the high-temperature rp-process was directly investigated and the transitions through the states at around 6.2 MeV in ¹⁸Ne were first observed, confirming the importance predicted before. The (α,p) reaction leading to the first excited state in ¹⁷F was also found to have a large contribution. A proton resonance search experiment of ²³Mg + p was also discussed, which is a part of our series of resonance search studies relevant to the early stage of the rp-process.

Original language	English
Pages (from-to)	733-736
Number of pages	4
Journal	Nuclear Physics A
Volume	758
Issue number	1-4 SPEC. ISS.
DOIs	https://doi.org/10.1016/j.nuclphysa.2005.05.132
Publication status	Published - Jul 25 2005

All Science Journal Classification (ASJC) codes

Nuclear and High Energy Physics

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10.1016/j.nuclphysa.2005.05.132

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Kubono, S., Teranishi, T., Notani, M., Yamaguchi, H., Saito, A., He, J. J., Wakabayashi, M., Fujikawa, H., Amadio, G., Baba, H., Fukuchi, T., Shimoura, S., Michimasa, S., Nishimura, S., Nishimura, M., Gono, Y., Odahara, A., Kato, S., Moon, J. Y., ... Lichtenthaler, R. (2005). Study of stellar reactions in explosive hydrogen burning with CRIB. Nuclear Physics A, 758(1-4 SPEC. ISS.), 733-736. https://doi.org/10.1016/j.nuclphysa.2005.05.132

Kubono, S, Teranishi, T, Notani, M, Yamaguchi, H, Saito, A, He, JJ, Wakabayashi, M, Fujikawa, H, Amadio, G, Baba, H, Fukuchi, T, Shimoura, S, Michimasa, S, Nishimura, S, Nishimura, M, Gono, Y, Odahara, A, Kato, S, Moon, JY, Lee, JH, Lee, CS, Kim, JC, Hahn, KI, Ishikawa, T, Hashimoto, T, Ishiyama, H, Watanabe, YX, Tanaka, MH, Miyatake, H, Fülöp, Z, Guimarães, V & Lichtenthaler, R 2005, 'Study of stellar reactions in explosive hydrogen burning with CRIB', Nuclear Physics A, vol. 758, no. 1-4 SPEC. ISS., pp. 733-736. https://doi.org/10.1016/j.nuclphysa.2005.05.132

@article{98c7e8454fda4f9987da5459061510f5,

title = "Study of stellar reactions in explosive hydrogen burning with CRIB",

abstract = "With using low-energy RI beams from an in-flight RIB separator, CRIB, the most crucial stellar reaction 14O(α,p)17F for the onset of the high-temperature rp-process was directly investigated and the transitions through the states at around 6.2 MeV in 18Ne were first observed, confirming the importance predicted before. The (α,p) reaction leading to the first excited state in 17F was also found to have a large contribution. A proton resonance search experiment of 23Mg + p was also discussed, which is a part of our series of resonance search studies relevant to the early stage of the rp-process.",

author = "S. Kubono and T. Teranishi and M. Notani and H. Yamaguchi and A. Saito and He, {J. J.} and M. Wakabayashi and H. Fujikawa and G. Amadio and H. Baba and T. Fukuchi and S. Shimoura and S. Michimasa and S. Nishimura and M. Nishimura and Y. Gono and A. Odahara and S. Kato and Moon, {J. Y.} and Lee, {J. H.} and Lee, {C. S.} and Kim, {J. C.} and Hahn, {K. I.} and T. Ishikawa and T. Hashimoto and H. Ishiyama and Watanabe, {Y. X.} and Tanaka, {M. H.} and H. Miyatake and Zs F{\"u}l{\"o}p and V. Guimar{\~a}es and R. Lichtenthaler",

year = "2005",

month = jul,

day = "25",

doi = "10.1016/j.nuclphysa.2005.05.132",

language = "English",

volume = "758",

pages = "733--736",

journal = "Nuclear Physics A",

issn = "0375-9474",

publisher = "Elsevier",

number = "1-4 SPEC. ISS.",

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TY - JOUR

T1 - Study of stellar reactions in explosive hydrogen burning with CRIB

AU - Kubono, S.

AU - Teranishi, T.

AU - Notani, M.

AU - Yamaguchi, H.

AU - Saito, A.

AU - He, J. J.

AU - Wakabayashi, M.

AU - Fujikawa, H.

AU - Amadio, G.

AU - Baba, H.

AU - Fukuchi, T.

AU - Shimoura, S.

AU - Michimasa, S.

AU - Nishimura, S.

AU - Nishimura, M.

AU - Gono, Y.

AU - Odahara, A.

AU - Kato, S.

AU - Moon, J. Y.

AU - Lee, J. H.

AU - Lee, C. S.

AU - Kim, J. C.

AU - Hahn, K. I.

AU - Ishikawa, T.

AU - Hashimoto, T.

AU - Ishiyama, H.

AU - Watanabe, Y. X.

AU - Tanaka, M. H.

AU - Miyatake, H.

AU - Fülöp, Zs

AU - Guimarães, V.

AU - Lichtenthaler, R.

PY - 2005/7/25

Y1 - 2005/7/25

N2 - With using low-energy RI beams from an in-flight RIB separator, CRIB, the most crucial stellar reaction 14O(α,p)17F for the onset of the high-temperature rp-process was directly investigated and the transitions through the states at around 6.2 MeV in 18Ne were first observed, confirming the importance predicted before. The (α,p) reaction leading to the first excited state in 17F was also found to have a large contribution. A proton resonance search experiment of 23Mg + p was also discussed, which is a part of our series of resonance search studies relevant to the early stage of the rp-process.

AB - With using low-energy RI beams from an in-flight RIB separator, CRIB, the most crucial stellar reaction 14O(α,p)17F for the onset of the high-temperature rp-process was directly investigated and the transitions through the states at around 6.2 MeV in 18Ne were first observed, confirming the importance predicted before. The (α,p) reaction leading to the first excited state in 17F was also found to have a large contribution. A proton resonance search experiment of 23Mg + p was also discussed, which is a part of our series of resonance search studies relevant to the early stage of the rp-process.

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UR - http://www.scopus.com/inward/citedby.url?scp=20944436381&partnerID=8YFLogxK

U2 - 10.1016/j.nuclphysa.2005.05.132

DO - 10.1016/j.nuclphysa.2005.05.132

M3 - Article

AN - SCOPUS:20944436381

SN - 0375-9474

VL - 758

SP - 733

EP - 736

JO - Nuclear Physics A

JF - Nuclear Physics A

IS - 1-4 SPEC. ISS.

ER -

Study of stellar reactions in explosive hydrogen burning with CRIB

Abstract

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