Proton resonance scattering of 7Be

H. Yamaguchi; A. Saito; J. J. He; Y. Wakabayashi; G. Amadio; H. Fujikawa; S. Kubono; L. H. Khiem; Y. K. Kwon; M. Niikura; T. Teranishi; S. Nishimura; Y. Togano; N. Iwasa; K. Inafuku

doi:10.1063/1.2234413

Proton resonance scattering of ⁷Be

H. Yamaguchi, A. Saito, J. J. He, Y. Wakabayashi, G. Amadio, H. Fujikawa, S. Kubono, L. H. Khiem, Y. K. Kwon, M. Niikura, T. Teranishi, S. Nishimura, Y. Togano, N. Iwasa, K. Inafuku

Experimental Particle Physics

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

2 Citations (Scopus)

Abstract

We have studied the proton resonance scattering of ⁷Be by using a pure ⁷Be beam produced at CRIB (CNS Radioactive Ion Beam separator; CNS stands for Center of Nuclear Study, University of Tokyo). The excitation function of ⁸B was measured up to the excitation energy of 6.8 MeV, with the thick-target method. The excited states of ⁸B higher than 3.5 MeV were not known by the past experiments. This proton elastic scattering is also of importance in relation with the ⁷Be(p,γ) ⁸B reaction, which is a key reaction in the standard solar model.

Original language	English
Title of host publication	ORIGIN OF MATTER AND EVOLUTION OF GALAXIES
Subtitle of host publication	International Symposium on Origin of Matter and Evolution of Galaxies 2005: New Horizon of Nuclear Astrophysics and Cosmology
Pages	275-280
Number of pages	6
DOIs	https://doi.org/10.1063/1.2234413
Publication status	Published - 2006
Event	ORIGIN OF MATTER AND EVOLUTION OF GALAXIES: International Symposium on Origin of Matter and Evolution of Galaxies 2005: New Horizon of Nuclear Astrophysics and Cosmology - Tokyo, Japan Duration: Nov 8 2005 → Nov 11 2005

Publication series

Name	AIP Conference Proceedings
Volume	847
ISSN (Print)	0094-243X
ISSN (Electronic)	1551-7616

Other

Other	ORIGIN OF MATTER AND EVOLUTION OF GALAXIES: International Symposium on Origin of Matter and Evolution of Galaxies 2005: New Horizon of Nuclear Astrophysics and Cosmology
Country/Territory	Japan
City	Tokyo
Period	11/8/05 → 11/11/05

All Science Journal Classification (ASJC) codes

Physics and Astronomy(all)

Access to Document

10.1063/1.2234413

Cite this

Yamaguchi, H., Saito, A., He, J. J., Wakabayashi, Y., Amadio, G., Fujikawa, H., Kubono, S., Khiem, L. H., Kwon, Y. K., Niikura, M., Teranishi, T., Nishimura, S., Togano, Y., Iwasa, N., & Inafuku, K. (2006). Proton resonance scattering of ⁷Be. In ORIGIN OF MATTER AND EVOLUTION OF GALAXIES: International Symposium on Origin of Matter and Evolution of Galaxies 2005: New Horizon of Nuclear Astrophysics and Cosmology (pp. 275-280). (AIP Conference Proceedings; Vol. 847). https://doi.org/10.1063/1.2234413

Proton resonance scattering of ⁷Be. / Yamaguchi, H.; Saito, A.; He, J. J. et al.
ORIGIN OF MATTER AND EVOLUTION OF GALAXIES: International Symposium on Origin of Matter and Evolution of Galaxies 2005: New Horizon of Nuclear Astrophysics and Cosmology. 2006. p. 275-280 (AIP Conference Proceedings; Vol. 847).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

Yamaguchi, H, Saito, A, He, JJ, Wakabayashi, Y, Amadio, G, Fujikawa, H, Kubono, S, Khiem, LH, Kwon, YK, Niikura, M, Teranishi, T, Nishimura, S, Togano, Y, Iwasa, N & Inafuku, K 2006, Proton resonance scattering of ⁷Be. in ORIGIN OF MATTER AND EVOLUTION OF GALAXIES: International Symposium on Origin of Matter and Evolution of Galaxies 2005: New Horizon of Nuclear Astrophysics and Cosmology. AIP Conference Proceedings, vol. 847, pp. 275-280, ORIGIN OF MATTER AND EVOLUTION OF GALAXIES: International Symposium on Origin of Matter and Evolution of Galaxies 2005: New Horizon of Nuclear Astrophysics and Cosmology, Tokyo, Japan, 11/8/05. https://doi.org/10.1063/1.2234413

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abstract = "We have studied the proton resonance scattering of 7Be by using a pure 7Be beam produced at CRIB (CNS Radioactive Ion Beam separator; CNS stands for Center of Nuclear Study, University of Tokyo). The excitation function of 8B was measured up to the excitation energy of 6.8 MeV, with the thick-target method. The excited states of 8B higher than 3.5 MeV were not known by the past experiments. This proton elastic scattering is also of importance in relation with the 7Be(p,γ) 8B reaction, which is a key reaction in the standard solar model.",

author = "H. Yamaguchi and A. Saito and He, {J. J.} and Y. Wakabayashi and G. Amadio and H. Fujikawa and S. Kubono and Khiem, {L. H.} and Kwon, {Y. K.} and M. Niikura and T. Teranishi and S. Nishimura and Y. Togano and N. Iwasa and K. Inafuku",

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AU - Yamaguchi, H.

AU - Saito, A.

AU - He, J. J.

AU - Wakabayashi, Y.

AU - Amadio, G.

AU - Fujikawa, H.

AU - Kubono, S.

AU - Khiem, L. H.

AU - Kwon, Y. K.

AU - Niikura, M.

AU - Teranishi, T.

AU - Nishimura, S.

AU - Togano, Y.

AU - Iwasa, N.

AU - Inafuku, K.

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N2 - We have studied the proton resonance scattering of 7Be by using a pure 7Be beam produced at CRIB (CNS Radioactive Ion Beam separator; CNS stands for Center of Nuclear Study, University of Tokyo). The excitation function of 8B was measured up to the excitation energy of 6.8 MeV, with the thick-target method. The excited states of 8B higher than 3.5 MeV were not known by the past experiments. This proton elastic scattering is also of importance in relation with the 7Be(p,γ) 8B reaction, which is a key reaction in the standard solar model.

AB - We have studied the proton resonance scattering of 7Be by using a pure 7Be beam produced at CRIB (CNS Radioactive Ion Beam separator; CNS stands for Center of Nuclear Study, University of Tokyo). The excitation function of 8B was measured up to the excitation energy of 6.8 MeV, with the thick-target method. The excited states of 8B higher than 3.5 MeV were not known by the past experiments. This proton elastic scattering is also of importance in relation with the 7Be(p,γ) 8B reaction, which is a key reaction in the standard solar model.

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