Gamow-Teller transitions starting from Tz=+3/2 nucleus 47Ti

E. Ganioǧlu; H. Fujita; Y. Fujita; T. Adachi; A. Algora; M. Csatlos; J. Deaven; E. Estevez; C. Guess; J. Gulyás; K. Hatanaka; K. Hirota; D. Ishikawa; A. Krasznahorkay; H. Matsubara; R. Meharchand; F. Molina; H. Okamura; H. J. Ong; G. Perdikakis; B. Rubio; C. Scholl; G. Susoy; T. Suzuki; A. Tamii; J. Thies; R. G.T. Zegers; J. Zenihiro

doi:10.1063/1.3628368

Gamow-Teller transitions starting from T_z=+3/2 nucleus ⁴⁷Ti

E. Ganioǧlu, H. Fujita, Y. Fujita, T. Adachi, A. Algora, M. Csatlos, J. Deaven, E. Estevez, C. Guess, J. Gulyás, K. Hatanaka, K. Hirota, D. Ishikawa, A. Krasznahorkay, H. Matsubara, R. Meharchand, F. Molina, H. Okamura, H. J. Ong, G. PerdikakisB. Rubio, C. Scholl, G. Susoy, T. Suzuki, A. Tamii, J. Thies, R. G.T. Zegers, J. Zenihiro

研究成果: 書籍/レポートタイプへの寄稿 › 会議への寄与

抄録

Gamow-Teller (GT) transitions are mediated by the στ operator. Owing to its simplicity and also its spin-isospin nature, GT transitions play key roles in the studies of nuclear structure as well as astro-nuclear processes. In violent neutrino-induced reactions at the core-collapse stage of type II supernovae, Gamow-Teller (GT) transitions starting from stable as well as unstable pf-shell nuclei play important roles. We study GT transitions starting from ⁴⁷Ti in a high-resolution (³He,t) charge-exchange reactions at 0° and at an intermediate incident energy of 140 MeV/nucleon at Research Center for Nuclear Physics (RCNP), Osaka. Individual GT transitions up to high excitations were observed. Assuming the isospin symmetry for the strengths of T_z=±3/2→±1/2 analogous GT transitions, we can deduce the detailed strength distribution starting from mirror unstable nucleus ⁴⁷Mn.

本文言語	英語
ホスト出版物のタイトル	Frontiers in Nuclear Structure, Astrophysics, and Reactions, FINUSTAR 3
ページ	126-130
ページ数	5
DOI	https://doi.org/10.1063/1.3628368
出版ステータス	出版済み - 2011
外部発表	はい
イベント	3rd International Conference on Frontiers in Nuclear Structure, Astrophysics, and Reactions, FINUSTAR 3 - Rhodes, ギリシャ継続期間: 23-08-2010 → 27-08-2010

出版物シリーズ

名前	AIP Conference Proceedings
巻	1377
ISSN（印刷版）	0094-243X
ISSN（電子版）	1551-7616

会議

会議	3rd International Conference on Frontiers in Nuclear Structure, Astrophysics, and Reactions, FINUSTAR 3
国/地域	ギリシャ
City	Rhodes
Period	23-08-10 → 27-08-10

All Science Journal Classification (ASJC) codes

物理学および天文学一般

文献へのアクセス

10.1063/1.3628368

他のファイルとリンク

引用スタイル

Ganioǧlu, E., Fujita, H., Fujita, Y., Adachi, T., Algora, A., Csatlos, M., Deaven, J., Estevez, E., Guess, C., Gulyás, J., Hatanaka, K., Hirota, K., Ishikawa, D., Krasznahorkay, A., Matsubara, H., Meharchand, R., Molina, F., Okamura, H., Ong, H. J., ... Zenihiro, J. (2011). Gamow-Teller transitions starting from T_z=+3/2 nucleus ⁴⁷Ti. In Frontiers in Nuclear Structure, Astrophysics, and Reactions, FINUSTAR 3 (pp. 126-130). (AIP Conference Proceedings; Vol. 1377). https://doi.org/10.1063/1.3628368

@inproceedings{9532578ed24745f282dfed07cdefd472,

title = "Gamow-Teller transitions starting from Tz=+3/2 nucleus 47Ti",

abstract = "Gamow-Teller (GT) transitions are mediated by the στ operator. Owing to its simplicity and also its spin-isospin nature, GT transitions play key roles in the studies of nuclear structure as well as astro-nuclear processes. In violent neutrino-induced reactions at the core-collapse stage of type II supernovae, Gamow-Teller (GT) transitions starting from stable as well as unstable pf-shell nuclei play important roles. We study GT transitions starting from 47Ti in a high-resolution (3He,t) charge-exchange reactions at 0° and at an intermediate incident energy of 140 MeV/nucleon at Research Center for Nuclear Physics (RCNP), Osaka. Individual GT transitions up to high excitations were observed. Assuming the isospin symmetry for the strengths of Tz=±3/2→±1/2 analogous GT transitions, we can deduce the detailed strength distribution starting from mirror unstable nucleus 47Mn.",

author = "E. Ganioǧlu and H. Fujita and Y. Fujita and T. Adachi and A. Algora and M. Csatlos and J. Deaven and E. Estevez and C. Guess and J. Guly{\'a}s and K. Hatanaka and K. Hirota and D. Ishikawa and A. Krasznahorkay and H. Matsubara and R. Meharchand and F. Molina and H. Okamura and Ong, {H. J.} and G. Perdikakis and B. Rubio and C. Scholl and G. Susoy and T. Suzuki and A. Tamii and J. Thies and Zegers, {R. G.T.} and J. Zenihiro",

year = "2011",

doi = "10.1063/1.3628368",

language = "English",

isbn = "9780735409378",

series = "AIP Conference Proceedings",

pages = "126--130",

booktitle = "Frontiers in Nuclear Structure, Astrophysics, and Reactions, FINUSTAR 3",

note = "3rd International Conference on Frontiers in Nuclear Structure, Astrophysics, and Reactions, FINUSTAR 3 ; Conference date: 23-08-2010 Through 27-08-2010",

}

Ganioǧlu, E, Fujita, H, Fujita, Y, Adachi, T, Algora, A, Csatlos, M, Deaven, J, Estevez, E, Guess, C, Gulyás, J, Hatanaka, K, Hirota, K, Ishikawa, D, Krasznahorkay, A, Matsubara, H, Meharchand, R, Molina, F, Okamura, H, Ong, HJ, Perdikakis, G, Rubio, B, Scholl, C, Susoy, G, Suzuki, T, Tamii, A, Thies, J, Zegers, RGT & Zenihiro, J 2011, Gamow-Teller transitions starting from T_z=+3/2 nucleus ⁴⁷Ti. in Frontiers in Nuclear Structure, Astrophysics, and Reactions, FINUSTAR 3. AIP Conference Proceedings, vol. 1377, pp. 126-130, 3rd International Conference on Frontiers in Nuclear Structure, Astrophysics, and Reactions, FINUSTAR 3, Rhodes, ギリシャ, 23-08-10. https://doi.org/10.1063/1.3628368

TY - GEN

T1 - Gamow-Teller transitions starting from Tz=+3/2 nucleus 47Ti

AU - Ganioǧlu, E.

AU - Fujita, H.

AU - Fujita, Y.

AU - Adachi, T.

AU - Algora, A.

AU - Csatlos, M.

AU - Deaven, J.

AU - Estevez, E.

AU - Guess, C.

AU - Gulyás, J.

AU - Hatanaka, K.

AU - Hirota, K.

AU - Ishikawa, D.

AU - Krasznahorkay, A.

AU - Matsubara, H.

AU - Meharchand, R.

AU - Molina, F.

AU - Okamura, H.

AU - Ong, H. J.

AU - Perdikakis, G.

AU - Rubio, B.

AU - Scholl, C.

AU - Susoy, G.

AU - Suzuki, T.

AU - Tamii, A.

AU - Thies, J.

AU - Zegers, R. G.T.

AU - Zenihiro, J.

PY - 2011

Y1 - 2011

N2 - Gamow-Teller (GT) transitions are mediated by the στ operator. Owing to its simplicity and also its spin-isospin nature, GT transitions play key roles in the studies of nuclear structure as well as astro-nuclear processes. In violent neutrino-induced reactions at the core-collapse stage of type II supernovae, Gamow-Teller (GT) transitions starting from stable as well as unstable pf-shell nuclei play important roles. We study GT transitions starting from 47Ti in a high-resolution (3He,t) charge-exchange reactions at 0° and at an intermediate incident energy of 140 MeV/nucleon at Research Center for Nuclear Physics (RCNP), Osaka. Individual GT transitions up to high excitations were observed. Assuming the isospin symmetry for the strengths of Tz=±3/2→±1/2 analogous GT transitions, we can deduce the detailed strength distribution starting from mirror unstable nucleus 47Mn.

AB - Gamow-Teller (GT) transitions are mediated by the στ operator. Owing to its simplicity and also its spin-isospin nature, GT transitions play key roles in the studies of nuclear structure as well as astro-nuclear processes. In violent neutrino-induced reactions at the core-collapse stage of type II supernovae, Gamow-Teller (GT) transitions starting from stable as well as unstable pf-shell nuclei play important roles. We study GT transitions starting from 47Ti in a high-resolution (3He,t) charge-exchange reactions at 0° and at an intermediate incident energy of 140 MeV/nucleon at Research Center for Nuclear Physics (RCNP), Osaka. Individual GT transitions up to high excitations were observed. Assuming the isospin symmetry for the strengths of Tz=±3/2→±1/2 analogous GT transitions, we can deduce the detailed strength distribution starting from mirror unstable nucleus 47Mn.

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U2 - 10.1063/1.3628368

DO - 10.1063/1.3628368

M3 - Conference contribution

AN - SCOPUS:81555212744

SN - 9780735409378

T3 - AIP Conference Proceedings

SP - 126

EP - 130

BT - Frontiers in Nuclear Structure, Astrophysics, and Reactions, FINUSTAR 3

T2 - 3rd International Conference on Frontiers in Nuclear Structure, Astrophysics, and Reactions, FINUSTAR 3

Y2 - 23 August 2010 through 27 August 2010

ER -