Study of inelastic contribution in the 7Be + p scattering experiment at CRIB

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

doi:10.1063/1.2234426

Study of inelastic contribution in the ⁷Be + p scattering experiment at CRIB

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

SCI - Physics

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

Abstract

The ⁷Be(p,γ)⁸B reaction is undoubtfully important to the understanding of the solar model. As a step in the direction of improving the accuracy of the S₁₇ astrophysical factor, a study of the ⁷Be + p scattering was performed with the thick target method at the CRIB facility. In addition to its astrophysical significance, this reaction is also useful to clarify the nuclear structure of ⁸B. A primary beam of ⁷Li and a hydrogen gas target were used to produce a ⁷Be secondary beam at 7.69 MeV/u. This was the first time in which γ-rays were measured in coincidence with protons, and we have successfully measured the inelastic contribution to the scattering cross section.

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	362-364
Number of pages	3
DOIs	https://doi.org/10.1063/1.2234426
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: 2005 Nov 8 → 2005 Nov 11

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	05/11/8 → 05/11/11

Keywords

Nucleosynthesis
Proton resonant scattering
Solar neutrinos

ASJC Scopus subject areas

Physics and Astronomy(all)

Access to Document

10.1063/1.2234426

Cite this

Amadio, G., Yamaguchi, H., He, J. J., Saito, A., Wakabayashi, Y., Fujikawa, H., Kubono, S., Khiem, L. H., Kwon, Y. K., Teranishi, T., Nishimura, S., Niikura, M., Togano, Y., Iwasa, N., & Inafuku, S. (2006). Study of inelastic contribution in the ⁷Be + p scattering experiment at CRIB. 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. 362-364). (AIP Conference Proceedings; Vol. 847). https://doi.org/10.1063/1.2234426

Study of inelastic contribution in the ⁷Be + p scattering experiment at CRIB. / Amadio, G.; Yamaguchi, H.; 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. 362-364 (AIP Conference Proceedings; Vol. 847).

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

Amadio, G, Yamaguchi, H, He, JJ, Saito, A, Wakabayashi, Y, Fujikawa, H, Kubono, S, Khiem, LH, Kwon, YK, Teranishi, T, Nishimura, S, Niikura, M, Togano, Y, Iwasa, N & Inafuku, S 2006, Study of inelastic contribution in the ⁷Be + p scattering experiment at CRIB. 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. 362-364, 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, 05/11/8. https://doi.org/10.1063/1.2234426

Amadio G, Yamaguchi H, He JJ, Saito A, Wakabayashi Y, Fujikawa H et al. Study of inelastic contribution in the ⁷Be + p scattering experiment at CRIB. 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. 2006. p. 362-364. (AIP Conference Proceedings). https://doi.org/10.1063/1.2234426

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

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AU - Amadio, G.

AU - Yamaguchi, H.

AU - He, J. J.

AU - Saito, A.

AU - Wakabayashi, Y.

AU - Fujikawa, H.

AU - Kubono, S.

AU - Khiem, L. H.

AU - Kwon, Y. K.

AU - Teranishi, T.

AU - Nishimura, S.

AU - Niikura, M.

AU - Togano, Y.

AU - Iwasa, N.

AU - Inafuku, S.

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N2 - The 7Be(p,γ)8B reaction is undoubtfully important to the understanding of the solar model. As a step in the direction of improving the accuracy of the S17 astrophysical factor, a study of the 7Be + p scattering was performed with the thick target method at the CRIB facility. In addition to its astrophysical significance, this reaction is also useful to clarify the nuclear structure of 8B. A primary beam of 7Li and a hydrogen gas target were used to produce a 7Be secondary beam at 7.69 MeV/u. This was the first time in which γ-rays were measured in coincidence with protons, and we have successfully measured the inelastic contribution to the scattering cross section.

AB - The 7Be(p,γ)8B reaction is undoubtfully important to the understanding of the solar model. As a step in the direction of improving the accuracy of the S17 astrophysical factor, a study of the 7Be + p scattering was performed with the thick target method at the CRIB facility. In addition to its astrophysical significance, this reaction is also useful to clarify the nuclear structure of 8B. A primary beam of 7Li and a hydrogen gas target were used to produce a 7Be secondary beam at 7.69 MeV/u. This was the first time in which γ-rays were measured in coincidence with protons, and we have successfully measured the inelastic contribution to the scattering cross section.

KW - Nucleosynthesis

KW - Proton resonant scattering

KW - Solar neutrinos

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