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

SCI - Physics

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

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: 2005 Nov 8 → 2005 Nov 11

Publication series

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

Conference

Conference	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

Astrophysical S-factor
Proton resonance scattering
Solar neutrino problem

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

@inproceedings{f73305bb09154ed3acd4e060b4973d3a,

title = "Proton resonance scattering of 7Be",

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.",

keywords = "Astrophysical S-factor, Proton resonance scattering, Solar neutrino problem",

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",

year = "2006",

doi = "10.1063/1.2234413",

language = "English",

isbn = "0735403422",

series = "AIP Conference Proceedings",

pages = "275--280",

booktitle = "ORIGIN OF MATTER AND EVOLUTION OF GALAXIES",

note = "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 ; Conference date: 08-11-2005 Through 11-11-2005",

}

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, 05/11/8. 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 › peer-review

TY - GEN

T1 - Proton resonance scattering of 7Be

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.

PY - 2006

Y1 - 2006

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.

KW - Astrophysical S-factor

KW - Proton resonance scattering

KW - Solar neutrino problem

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SN - 9780735403420

T3 - AIP Conference Proceedings

SP - 275

EP - 280

BT - ORIGIN OF MATTER AND EVOLUTION OF GALAXIES

T2 - 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

Y2 - 8 November 2005 through 11 November 2005

ER -