Coulomb dissociation of 27P for study of 26Si(p, γ)27P reaction

Y. Togano; T. Gomi; T. Motobayashi; Y. Ando; N. Aoi; H. Baba; K. Demichi; Z. Elekes; N. Fukuda; Zs Fülöp; U. Futakami; H. Hasegawa; Y. Higurashi; K. Ieki; N. Imai; M. Ishihara; K. Ishikawa; N. Iwasa; H. Iwasaki; S. Kanno; Y. Kondo; T. Kubo; S. Kubono; M. Kunibu; K. Kurita; Y. U. Matsuyama; S. Michimasa; T. Minemura; M. Miura; H. Murakami; T. Nakamura; M. Notani; S. Ota; A. Saito; M. Serata; S. Shimoura; T. Sugimoto; E. Takeshita; S. Takeuchi; K. Ue; K. Yamada; Y. Yanagisawa; K. Yoneda; A. Yoshida

doi:10.1063/1.2234414

Coulomb dissociation of ²⁷P for study of ²⁶Si(p, γ)²⁷P reaction

Y. Togano, T. Gomi, T. Motobayashi, Y. Ando, N. Aoi, H. Baba, K. Demichi, Z. Elekes, N. Fukuda, Zs Fülöp, U. Futakami, H. Hasegawa, Y. Higurashi, K. Ieki, N. Imai, M. Ishihara, K. Ishikawa, N. Iwasa, H. Iwasaki, S. KannoY. Kondo, T. Kubo, S. Kubono, M. Kunibu, K. Kurita, Y. U. Matsuyama, S. Michimasa, T. Minemura, M. Miura, H. Murakami, T. Nakamura, M. Notani, S. Ota, A. Saito, M. Serata, S. Shimoura, T. Sugimoto, E. Takeshita, S. Takeuchi, K. Ue, K. Yamada, Y. Yanagisawa, K. Yoneda, A. Yoshida

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

Abstract

The Coulomb dissociation of the proton-rich nuclei ²⁷P was studied experimentally using a ²⁷P beam at 57 MeV/nucleon with a lead target. The γ decay widths of the low-lying excited states in ²⁷P were deduced. The resonant capture reaction rate of stellar ²⁶Si(p,γ)²⁷P through these states was estimated using the measured γ decay width. The astrophysical implications derived from the estimated reaction rate is discussed.

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	281-286
Number of pages	6
DOIs	https://doi.org/10.1063/1.2234414
State	Published - 2006
Externally published	Yes
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: 8 Nov 2005 → 11 Nov 2005

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	8/11/05 → 11/11/05

Keywords

20≤A≤3
Coulomb excitation
Nucleosynthesis in novae
Reaction induced by unstable nuclei
Supernovae and other explosive environments

Access to Document

10.1063/1.2234414

Cite this

Togano, Y., Gomi, T., Motobayashi, T., Ando, Y., Aoi, N., Baba, H., Demichi, K., Elekes, Z., Fukuda, N., Fülöp, Z., Futakami, U., Hasegawa, H., Higurashi, Y., Ieki, K., Imai, N., Ishihara, M., Ishikawa, K., Iwasa, N., Iwasaki, H., ... Yoshida, A. (2006). Coulomb dissociation of ²⁷P for study of ²⁶Si(p, γ)²⁷P reaction. 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. 281-286). (AIP Conference Proceedings; Vol. 847). https://doi.org/10.1063/1.2234414

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title = "Coulomb dissociation of 27P for study of 26Si(p, γ)27P reaction",

abstract = "The Coulomb dissociation of the proton-rich nuclei 27P was studied experimentally using a 27P beam at 57 MeV/nucleon with a lead target. The γ decay widths of the low-lying excited states in 27P were deduced. The resonant capture reaction rate of stellar 26Si(p,γ)27P through these states was estimated using the measured γ decay width. The astrophysical implications derived from the estimated reaction rate is discussed.",

keywords = "20≤A≤3, Coulomb excitation, Nucleosynthesis in novae, Reaction induced by unstable nuclei, Supernovae and other explosive environments",

author = "Y. Togano and T. Gomi and T. Motobayashi and Y. Ando and N. Aoi and H. Baba and K. Demichi and Z. Elekes and N. Fukuda and Zs F{\"u}l{\"o}p and U. Futakami and H. Hasegawa and Y. Higurashi and K. Ieki and N. Imai and M. Ishihara and K. Ishikawa and N. Iwasa and H. Iwasaki and S. Kanno and Y. Kondo and T. Kubo and S. Kubono and M. Kunibu and K. Kurita and Matsuyama, {Y. U.} and S. Michimasa and T. Minemura and M. Miura and H. Murakami and T. Nakamura and M. Notani and S. Ota and A. Saito and M. Serata and S. Shimoura and T. Sugimoto and E. Takeshita and S. Takeuchi and K. Ue and K. Yamada and Y. Yanagisawa and K. Yoneda and A. Yoshida",

year = "2006",

doi = "10.1063/1.2234414",

language = "英語",

isbn = "0735403422",

series = "AIP Conference Proceedings",

pages = "281--286",

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",

}

Togano, Y, Gomi, T, Motobayashi, T, Ando, Y, Aoi, N, Baba, H, Demichi, K, Elekes, Z, Fukuda, N, Fülöp, Z, Futakami, U, Hasegawa, H, Higurashi, Y, Ieki, K, Imai, N, Ishihara, M, Ishikawa, K, Iwasa, N, Iwasaki, H, Kanno, S, Kondo, Y, Kubo, T, Kubono, S, Kunibu, M, Kurita, K, Matsuyama, YU, Michimasa, S, Minemura, T, Miura, M, Murakami, H, Nakamura, T, Notani, M, Ota, S, Saito, A, Serata, M, Shimoura, S, Sugimoto, T, Takeshita, E, Takeuchi, S, Ue, K, Yamada, K, Yanagisawa, Y, Yoneda, K & Yoshida, A 2006, Coulomb dissociation of ²⁷P for study of ²⁶Si(p, γ)²⁷P reaction. 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. 281-286, 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, 8/11/05. https://doi.org/10.1063/1.2234414

Coulomb dissociation of ²⁷P for study of ²⁶Si(p, γ)²⁷P reaction. / Togano, Y.; Gomi, T.; Motobayashi, T. 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. 281-286 (AIP Conference Proceedings; Vol. 847).

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

TY - GEN

T1 - Coulomb dissociation of 27P for study of 26Si(p, γ)27P reaction

AU - Togano, Y.

AU - Gomi, T.

AU - Motobayashi, T.

AU - Ando, Y.

AU - Aoi, N.

AU - Baba, H.

AU - Demichi, K.

AU - Elekes, Z.

AU - Fukuda, N.

AU - Fülöp, Zs

AU - Futakami, U.

AU - Hasegawa, H.

AU - Higurashi, Y.

AU - Ieki, K.

AU - Imai, N.

AU - Ishihara, M.

AU - Ishikawa, K.

AU - Iwasa, N.

AU - Iwasaki, H.

AU - Kanno, S.

AU - Kondo, Y.

AU - Kubo, T.

AU - Kubono, S.

AU - Kunibu, M.

AU - Kurita, K.

AU - Matsuyama, Y. U.

AU - Michimasa, S.

AU - Minemura, T.

AU - Miura, M.

AU - Murakami, H.

AU - Nakamura, T.

AU - Notani, M.

AU - Ota, S.

AU - Saito, A.

AU - Serata, M.

AU - Shimoura, S.

AU - Sugimoto, T.

AU - Takeshita, E.

AU - Takeuchi, S.

AU - Ue, K.

AU - Yamada, K.

AU - Yanagisawa, Y.

AU - Yoneda, K.

AU - Yoshida, A.

PY - 2006

Y1 - 2006

N2 - The Coulomb dissociation of the proton-rich nuclei 27P was studied experimentally using a 27P beam at 57 MeV/nucleon with a lead target. The γ decay widths of the low-lying excited states in 27P were deduced. The resonant capture reaction rate of stellar 26Si(p,γ)27P through these states was estimated using the measured γ decay width. The astrophysical implications derived from the estimated reaction rate is discussed.

AB - The Coulomb dissociation of the proton-rich nuclei 27P was studied experimentally using a 27P beam at 57 MeV/nucleon with a lead target. The γ decay widths of the low-lying excited states in 27P were deduced. The resonant capture reaction rate of stellar 26Si(p,γ)27P through these states was estimated using the measured γ decay width. The astrophysical implications derived from the estimated reaction rate is discussed.

KW - 20≤A≤3

KW - Coulomb excitation

KW - Nucleosynthesis in novae

KW - Reaction induced by unstable nuclei

KW - Supernovae and other explosive environments

UR - http://www.scopus.com/inward/record.url?scp=33846349460&partnerID=8YFLogxK

U2 - 10.1063/1.2234414

DO - 10.1063/1.2234414

M3 - 会議への寄与

AN - SCOPUS:33846349460

SN - 0735403422

SN - 9780735403420

T3 - AIP Conference Proceedings

SP - 281

EP - 286

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 -

Togano Y, Gomi T, Motobayashi T, Ando Y, Aoi N, Baba H et al. Coulomb dissociation of ²⁷P for study of ²⁶Si(p, γ)²⁷P reaction. 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. 281-286. (AIP Conference Proceedings). doi: 10.1063/1.2234414