Low-energy radioactive ion beam production of 22Mg

N. N. Duy, S. Kubono, H. Yamaguchi, D. Kahl, Y. Wakabayashi, Takashi Teranishi, N. Iwasa, Y. K. Kwon, L. H. Khiem, Y. H. Kim, J. S. Song, J. Hu, Y. Ayyad

研究成果: ジャーナルへの寄稿記事

抄録

The 22Mg nucleus plays an important role in nuclear astrophysics, specially in the 22Mg(α,p)25Al and proton capture 22Mg(p,γ)23Al reactions. It is believed that 22Mg is a waiting point in the αp-process of nucleosynthesis in novae. We proposed a direct measurement of the 22Mg+α resonance reaction in inverse kinematics using a radioactive ion (RI) beam. A 22Mg beam of 3.73 MeV/u was produced at CRIB (Center for Nuclear Study (CNS) low-energy RI Beam) facility of the University of Tokyo located at RIKEN (Japan) in 2011. In this paper we present the results about the production of the 22Mg beam used for the direct measurement of the scattering reaction 22Mg(α,α) 22Mg, and the stellar reaction 22Mg(α,p) 25Al in the energy region concerning an astrophysical temperature of T9=1-3 GK.

元の言語英語
ページ(範囲)99-101
ページ数3
ジャーナルNuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
723
DOI
出版物ステータス出版済み - 6 10 2013

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Ion beams
Nucleosynthesis
ion beams
Astrophysics
Inverse kinematics
Protons
Scattering
inverse kinematics
nuclear astrophysics
novae
energy
nuclear fusion
Japan
astrophysics
Temperature
nuclei
protons
scattering
temperature

All Science Journal Classification (ASJC) codes

  • Nuclear and High Energy Physics
  • Instrumentation

これを引用

Low-energy radioactive ion beam production of 22Mg. / Duy, N. N.; Kubono, S.; Yamaguchi, H.; Kahl, D.; Wakabayashi, Y.; Teranishi, Takashi; Iwasa, N.; Kwon, Y. K.; Khiem, L. H.; Kim, Y. H.; Song, J. S.; Hu, J.; Ayyad, Y.

:: Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, 巻 723, 10.06.2013, p. 99-101.

研究成果: ジャーナルへの寄稿記事

Duy, NN, Kubono, S, Yamaguchi, H, Kahl, D, Wakabayashi, Y, Teranishi, T, Iwasa, N, Kwon, YK, Khiem, LH, Kim, YH, Song, JS, Hu, J & Ayyad, Y 2013, 'Low-energy radioactive ion beam production of 22Mg', Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, 巻. 723, pp. 99-101. https://doi.org/10.1016/j.nima.2013.05.026
Duy, N. N. ; Kubono, S. ; Yamaguchi, H. ; Kahl, D. ; Wakabayashi, Y. ; Teranishi, Takashi ; Iwasa, N. ; Kwon, Y. K. ; Khiem, L. H. ; Kim, Y. H. ; Song, J. S. ; Hu, J. ; Ayyad, Y. / Low-energy radioactive ion beam production of 22Mg. :: Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment. 2013 ; 巻 723. pp. 99-101.
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abstract = "The 22Mg nucleus plays an important role in nuclear astrophysics, specially in the 22Mg(α,p)25Al and proton capture 22Mg(p,γ)23Al reactions. It is believed that 22Mg is a waiting point in the αp-process of nucleosynthesis in novae. We proposed a direct measurement of the 22Mg+α resonance reaction in inverse kinematics using a radioactive ion (RI) beam. A 22Mg beam of 3.73 MeV/u was produced at CRIB (Center for Nuclear Study (CNS) low-energy RI Beam) facility of the University of Tokyo located at RIKEN (Japan) in 2011. In this paper we present the results about the production of the 22Mg beam used for the direct measurement of the scattering reaction 22Mg(α,α) 22Mg, and the stellar reaction 22Mg(α,p) 25Al in the energy region concerning an astrophysical temperature of T9=1-3 GK.",
author = "Duy, {N. N.} and S. Kubono and H. Yamaguchi and D. Kahl and Y. Wakabayashi and Takashi Teranishi and N. Iwasa and Kwon, {Y. K.} and Khiem, {L. H.} and Kim, {Y. H.} and Song, {J. S.} and J. Hu and Y. Ayyad",
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AU - Duy, N. N.

AU - Kubono, S.

AU - Yamaguchi, H.

AU - Kahl, D.

AU - Wakabayashi, Y.

AU - Teranishi, Takashi

AU - Iwasa, N.

AU - Kwon, Y. K.

AU - Khiem, L. H.

AU - Kim, Y. H.

AU - Song, J. S.

AU - Hu, J.

AU - Ayyad, Y.

PY - 2013/6/10

Y1 - 2013/6/10

N2 - The 22Mg nucleus plays an important role in nuclear astrophysics, specially in the 22Mg(α,p)25Al and proton capture 22Mg(p,γ)23Al reactions. It is believed that 22Mg is a waiting point in the αp-process of nucleosynthesis in novae. We proposed a direct measurement of the 22Mg+α resonance reaction in inverse kinematics using a radioactive ion (RI) beam. A 22Mg beam of 3.73 MeV/u was produced at CRIB (Center for Nuclear Study (CNS) low-energy RI Beam) facility of the University of Tokyo located at RIKEN (Japan) in 2011. In this paper we present the results about the production of the 22Mg beam used for the direct measurement of the scattering reaction 22Mg(α,α) 22Mg, and the stellar reaction 22Mg(α,p) 25Al in the energy region concerning an astrophysical temperature of T9=1-3 GK.

AB - The 22Mg nucleus plays an important role in nuclear astrophysics, specially in the 22Mg(α,p)25Al and proton capture 22Mg(p,γ)23Al reactions. It is believed that 22Mg is a waiting point in the αp-process of nucleosynthesis in novae. We proposed a direct measurement of the 22Mg+α resonance reaction in inverse kinematics using a radioactive ion (RI) beam. A 22Mg beam of 3.73 MeV/u was produced at CRIB (Center for Nuclear Study (CNS) low-energy RI Beam) facility of the University of Tokyo located at RIKEN (Japan) in 2011. In this paper we present the results about the production of the 22Mg beam used for the direct measurement of the scattering reaction 22Mg(α,α) 22Mg, and the stellar reaction 22Mg(α,p) 25Al in the energy region concerning an astrophysical temperature of T9=1-3 GK.

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