Measurement of 25Al+p resonant elastic scattering for studying the 25Al(p,γ)26Si

Y. K. Kwon, C. S. Lee, H. S. Jung, J. Y. Moon, J. H. Lee, C. C. Yun, S. Kubono, H. Yamaguchi, T. Hashimoto, D. Kahl, S. Hayakawa, Seonho Choi, M. J. Kim, Y. H. Kim, Y. K. Kim, J. S. Park, E. J. Kim, C. B. Moon, T. Teranishi, Y. WakabayashiN. Iwasa, T. Yamada, Y. Togano, S. Kato, S. Cherubini, G. G. Rapisarda

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Abstract

Proton resonant states in 26Si have been studied by the resonant elastic scattering of 25Al+p with a 25Al radioactive ion beam at 2.863 MeV/nucleon bombarding a thick H2 gas target with the inverse kinematics method at the low-energy RI beam facility CRIB (CNS Radioactive Ion Beam separator), University of Tokyo. The properties of these resonance states are important to better determine the production rates of 25Al(p,γ)26Si reaction, which is one of the astrophysically important nuclear reactions to understand the production of the ground state of 26Al, the emitter of its characteristic 1.809-MeV gamma-ray, under the explosive stellar environments such as novae and X-ray bursts. In this work, several resonances above the proton threshold level have been observed with a high statistics and background free through a covered the range of excitation energies from Ex ∼ 6.8 to 8.2 MeV.

Original languageEnglish
Title of host publicationOrigin of Matter and Evolution of Galaxies 2011
Pages365-368
Number of pages4
DOIs
Publication statusPublished - Dec 1 2012
EventInternational Symposium on Origin of Matter and Evolutions of Galaxies 2011, OMEG 2011 - Wako, Japan
Duration: Nov 14 2011Nov 17 2011

Publication series

NameAIP Conference Proceedings
Volume1484
ISSN (Print)0094-243X
ISSN (Electronic)1551-7616

Other

OtherInternational Symposium on Origin of Matter and Evolutions of Galaxies 2011, OMEG 2011
CountryJapan
CityWako
Period11/14/1111/17/11

Fingerprint

protons
elastic scattering
ion beams
scattering
ions
inverse kinematics
novae
separators
emitters (equipment)
ion
energy
kinematics
nuclear reactions
gamma radiation
explosive
bursts
emitters
X-radiation
statistics
gases

All Science Journal Classification (ASJC) codes

  • Physics and Astronomy(all)

Cite this

Kwon, Y. K., Lee, C. S., Jung, H. S., Moon, J. Y., Lee, J. H., Yun, C. C., ... Rapisarda, G. G. (2012). Measurement of 25Al+p resonant elastic scattering for studying the 25Al(p,γ)26Si. In Origin of Matter and Evolution of Galaxies 2011 (pp. 365-368). (AIP Conference Proceedings; Vol. 1484). https://doi.org/10.1063/1.4763422

Measurement of 25Al+p resonant elastic scattering for studying the 25Al(p,γ)26Si. / Kwon, Y. K.; Lee, C. S.; Jung, H. S.; Moon, J. Y.; Lee, J. H.; Yun, C. C.; Kubono, S.; Yamaguchi, H.; Hashimoto, T.; Kahl, D.; Hayakawa, S.; Choi, Seonho; Kim, M. J.; Kim, Y. H.; Kim, Y. K.; Park, J. S.; Kim, E. J.; Moon, C. B.; Teranishi, T.; Wakabayashi, Y.; Iwasa, N.; Yamada, T.; Togano, Y.; Kato, S.; Cherubini, S.; Rapisarda, G. G.

Origin of Matter and Evolution of Galaxies 2011. 2012. p. 365-368 (AIP Conference Proceedings; Vol. 1484).

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Kwon, YK, Lee, CS, Jung, HS, Moon, JY, Lee, JH, Yun, CC, Kubono, S, Yamaguchi, H, Hashimoto, T, Kahl, D, Hayakawa, S, Choi, S, Kim, MJ, Kim, YH, Kim, YK, Park, JS, Kim, EJ, Moon, CB, Teranishi, T, Wakabayashi, Y, Iwasa, N, Yamada, T, Togano, Y, Kato, S, Cherubini, S & Rapisarda, GG 2012, Measurement of 25Al+p resonant elastic scattering for studying the 25Al(p,γ)26Si. in Origin of Matter and Evolution of Galaxies 2011. AIP Conference Proceedings, vol. 1484, pp. 365-368, International Symposium on Origin of Matter and Evolutions of Galaxies 2011, OMEG 2011, Wako, Japan, 11/14/11. https://doi.org/10.1063/1.4763422
Kwon YK, Lee CS, Jung HS, Moon JY, Lee JH, Yun CC et al. Measurement of 25Al+p resonant elastic scattering for studying the 25Al(p,γ)26Si. In Origin of Matter and Evolution of Galaxies 2011. 2012. p. 365-368. (AIP Conference Proceedings). https://doi.org/10.1063/1.4763422
Kwon, Y. K. ; Lee, C. S. ; Jung, H. S. ; Moon, J. Y. ; Lee, J. H. ; Yun, C. C. ; Kubono, S. ; Yamaguchi, H. ; Hashimoto, T. ; Kahl, D. ; Hayakawa, S. ; Choi, Seonho ; Kim, M. J. ; Kim, Y. H. ; Kim, Y. K. ; Park, J. S. ; Kim, E. J. ; Moon, C. B. ; Teranishi, T. ; Wakabayashi, Y. ; Iwasa, N. ; Yamada, T. ; Togano, Y. ; Kato, S. ; Cherubini, S. ; Rapisarda, G. G. / Measurement of 25Al+p resonant elastic scattering for studying the 25Al(p,γ)26Si. Origin of Matter and Evolution of Galaxies 2011. 2012. pp. 365-368 (AIP Conference Proceedings).
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abstract = "Proton resonant states in 26Si have been studied by the resonant elastic scattering of 25Al+p with a 25Al radioactive ion beam at 2.863 MeV/nucleon bombarding a thick H2 gas target with the inverse kinematics method at the low-energy RI beam facility CRIB (CNS Radioactive Ion Beam separator), University of Tokyo. The properties of these resonance states are important to better determine the production rates of 25Al(p,γ)26Si reaction, which is one of the astrophysically important nuclear reactions to understand the production of the ground state of 26Al, the emitter of its characteristic 1.809-MeV gamma-ray, under the explosive stellar environments such as novae and X-ray bursts. In this work, several resonances above the proton threshold level have been observed with a high statistics and background free through a covered the range of excitation energies from Ex ∼ 6.8 to 8.2 MeV.",
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AU - Lee, J. H.

AU - Yun, C. C.

AU - Kubono, S.

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AU - Teranishi, T.

AU - Wakabayashi, Y.

AU - Iwasa, N.

AU - Yamada, T.

AU - Togano, Y.

AU - Kato, S.

AU - Cherubini, S.

AU - Rapisarda, G. G.

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N2 - Proton resonant states in 26Si have been studied by the resonant elastic scattering of 25Al+p with a 25Al radioactive ion beam at 2.863 MeV/nucleon bombarding a thick H2 gas target with the inverse kinematics method at the low-energy RI beam facility CRIB (CNS Radioactive Ion Beam separator), University of Tokyo. The properties of these resonance states are important to better determine the production rates of 25Al(p,γ)26Si reaction, which is one of the astrophysically important nuclear reactions to understand the production of the ground state of 26Al, the emitter of its characteristic 1.809-MeV gamma-ray, under the explosive stellar environments such as novae and X-ray bursts. In this work, several resonances above the proton threshold level have been observed with a high statistics and background free through a covered the range of excitation energies from Ex ∼ 6.8 to 8.2 MeV.

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