Study of proton resonance structure in 27P via resonant elastic scattering of 26Si+p

H. S. Jung; C. S. Lee; Y. K. Kwon; 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. Wakabayashi; N. Iwasa; T. Yamada; Y. Togano; S. Kato; S. Cherubini; G. G. Rapisarda

doi:10.1063/1.4763412

Study of proton resonance structure in ²⁷P via resonant elastic scattering of ²⁶Si+p

H. S. Jung, C. S. Lee, Y. K. Kwon, 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

School of Earth System Sciences

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

Abstract

A measurement of resonant elastic scattering of ²⁶Si+p was performed with a thick target using a ²⁶Si radioactive ion beam at the CRIB (CNS Radioactive Ion Beam separator) of the Center for Nuclear Study (CNS), the University of Tokyo. The excitation function of ²⁷P was measured successfully with the inverse kinematics method through a covered the range of excitation energies from E_x ∼ 2.3 to 3.8 MeV, providing information about the resonance structure of this nucleus. The properties of these resonances are important to better determine the production rates of ²⁶Si(p,g)²⁷P reaction, which is one of the astrophysically important nuclear reactions to understand the production of the ²⁶Al. Some new resonant states have been investigated, and determined their resonance parameters, such as excitation energies, proton partial widths, and spin-parities by R-matrix calculation.

Original language	English
Title of host publication	Origin of Matter and Evolution of Galaxies 2011
Pages	307-312
Number of pages	6
DOIs	https://doi.org/10.1063/1.4763412
State	Published - 2012
Event	International Symposium on Origin of Matter and Evolutions of Galaxies 2011, OMEG 2011 - Wako, Japan Duration: 14 Nov 2011 → 17 Nov 2011

Publication series

Name	AIP Conference Proceedings
Volume	1484
ISSN (Print)	0094-243X
ISSN (Electronic)	1551-7616

Conference

Conference	International Symposium on Origin of Matter and Evolutions of Galaxies 2011, OMEG 2011
Country/Territory	Japan
City	Wako
Period	14/11/11 → 17/11/11

Keywords

Si(p,γ) P reaction
Proton resonant scattering
Radioactive Ion beam

Access to Document

10.1063/1.4763412

Cite this

Jung, H. S., Lee, C. S., Kwon, Y. K., Moon, J. Y., Lee, J. H., Yun, C. C., Kubono, S., Yamaguchi, H., Hashimoto, T., Kahl, D., Hayakawa, S., Choi, S., Kim, M. J., Kim, Y. H., Kim, Y. K., Park, J. S., Kim, E. J., Moon, C. B., Teranishi, T., ... Rapisarda, G. G. (2012). Study of proton resonance structure in ²⁷P via resonant elastic scattering of ²⁶Si+p. In Origin of Matter and Evolution of Galaxies 2011 (pp. 307-312). (AIP Conference Proceedings; Vol. 1484). https://doi.org/10.1063/1.4763412

@inproceedings{f4da77f37f474f49984d3f8955902bb2,

title = "Study of proton resonance structure in 27P via resonant elastic scattering of 26Si+p",

abstract = "A measurement of resonant elastic scattering of 26Si+p was performed with a thick target using a 26Si radioactive ion beam at the CRIB (CNS Radioactive Ion Beam separator) of the Center for Nuclear Study (CNS), the University of Tokyo. The excitation function of 27P was measured successfully with the inverse kinematics method through a covered the range of excitation energies from Ex ∼ 2.3 to 3.8 MeV, providing information about the resonance structure of this nucleus. The properties of these resonances are important to better determine the production rates of 26Si(p,g)27P reaction, which is one of the astrophysically important nuclear reactions to understand the production of the 26Al. Some new resonant states have been investigated, and determined their resonance parameters, such as excitation energies, proton partial widths, and spin-parities by R-matrix calculation.",

keywords = "Si(p,γ) P reaction, Proton resonant scattering, Radioactive Ion beam",

author = "Jung, {H. S.} and Lee, {C. S.} and Kwon, {Y. K.} and Moon, {J. Y.} and Lee, {J. H.} and Yun, {C. C.} and S. Kubono and H. Yamaguchi and T. Hashimoto and D. Kahl and S. Hayakawa and Seonho Choi and Kim, {M. J.} and Kim, {Y. H.} and Kim, {Y. K.} and Park, {J. S.} and Kim, {E. J.} and Moon, {C. B.} and T. Teranishi and Y. Wakabayashi and N. Iwasa and T. Yamada and Y. Togano and S. Kato and S. Cherubini and Rapisarda, {G. G.}",

year = "2012",

doi = "10.1063/1.4763412",

language = "English",

isbn = "9780735410961",

series = "AIP Conference Proceedings",

pages = "307--312",

booktitle = "Origin of Matter and Evolution of Galaxies 2011",

note = "International Symposium on Origin of Matter and Evolutions of Galaxies 2011, OMEG 2011 ; Conference date: 14-11-2011 Through 17-11-2011",

}

Jung, HS, Lee, CS, Kwon, YK, 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, Study of proton resonance structure in ²⁷P via resonant elastic scattering of ²⁶Si+p. in Origin of Matter and Evolution of Galaxies 2011. AIP Conference Proceedings, vol. 1484, pp. 307-312, International Symposium on Origin of Matter and Evolutions of Galaxies 2011, OMEG 2011, Wako, Japan, 14/11/11. https://doi.org/10.1063/1.4763412

TY - GEN

T1 - Study of proton resonance structure in 27P via resonant elastic scattering of 26Si+p

AU - Jung, H. S.

AU - Lee, C. S.

AU - Kwon, Y. K.

AU - Moon, J. Y.

AU - Lee, J. H.

AU - Yun, C. C.

AU - Kubono, S.

AU - Yamaguchi, H.

AU - Hashimoto, T.

AU - Kahl, D.

AU - Hayakawa, S.

AU - Choi, Seonho

AU - Kim, M. J.

AU - Kim, Y. H.

AU - Kim, Y. K.

AU - Park, J. S.

AU - Kim, E. J.

AU - Moon, C. B.

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.

PY - 2012

Y1 - 2012

N2 - A measurement of resonant elastic scattering of 26Si+p was performed with a thick target using a 26Si radioactive ion beam at the CRIB (CNS Radioactive Ion Beam separator) of the Center for Nuclear Study (CNS), the University of Tokyo. The excitation function of 27P was measured successfully with the inverse kinematics method through a covered the range of excitation energies from Ex ∼ 2.3 to 3.8 MeV, providing information about the resonance structure of this nucleus. The properties of these resonances are important to better determine the production rates of 26Si(p,g)27P reaction, which is one of the astrophysically important nuclear reactions to understand the production of the 26Al. Some new resonant states have been investigated, and determined their resonance parameters, such as excitation energies, proton partial widths, and spin-parities by R-matrix calculation.

AB - A measurement of resonant elastic scattering of 26Si+p was performed with a thick target using a 26Si radioactive ion beam at the CRIB (CNS Radioactive Ion Beam separator) of the Center for Nuclear Study (CNS), the University of Tokyo. The excitation function of 27P was measured successfully with the inverse kinematics method through a covered the range of excitation energies from Ex ∼ 2.3 to 3.8 MeV, providing information about the resonance structure of this nucleus. The properties of these resonances are important to better determine the production rates of 26Si(p,g)27P reaction, which is one of the astrophysically important nuclear reactions to understand the production of the 26Al. Some new resonant states have been investigated, and determined their resonance parameters, such as excitation energies, proton partial widths, and spin-parities by R-matrix calculation.

KW - Si(p,γ) P reaction

KW - Proton resonant scattering

KW - Radioactive Ion beam

UR - http://www.scopus.com/inward/record.url?scp=84874518486&partnerID=8YFLogxK

U2 - 10.1063/1.4763412

DO - 10.1063/1.4763412

M3 - Conference contribution

AN - SCOPUS:84874518486

SN - 9780735410961

T3 - AIP Conference Proceedings

SP - 307

EP - 312

BT - Origin of Matter and Evolution of Galaxies 2011

T2 - International Symposium on Origin of Matter and Evolutions of Galaxies 2011, OMEG 2011

Y2 - 14 November 2011 through 17 November 2011

ER -