TY - GEN
T1 - Gamow-Teller transitions and β-decay half-life in proton rich pf-shell nuclei
AU - Fujita, Y.
AU - Adachi, T.
AU - Blank, B.
AU - Von Brentano, P.
AU - Berg, G. P.A.
AU - Fujita, H.
AU - Fujita, K.
AU - Hatanaka, K.
AU - Nakanishi, K.
AU - Negret, A.
AU - Popescu, L.
AU - Rubio, B.
AU - Shimbara, Y.
AU - Shimizu, Y.
AU - Tameshige, Y.
AU - Tamii, A.
AU - Yosoi, M.
AU - Zell, K. O.
PY - 2010
Y1 - 2010
N2 - 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. In the β-decay study of these unstable pf-shell nuclei, half-lives can be measured rather accurately. On the other hand, in high-resolution (3He, t) charge-exchange reactions at 0°, individual GT transitions up to high excitations can be studied. Assuming the isospin symmetry for the strengths of Tz = ±2 → ±1 analogous GT transitions, we present a "merged analysis" for the determination of GT transition strengths starting from proton-rich Tz = -2 nuclei. We applied this analysis to the A = 52, T = 2 system, and it was found that the GT transitions and the properties of the 52Ni β decay can be understood better by combining the mirror GT strength distribution obtained from the 52Cr(3He, t) reaction.
AB - 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. In the β-decay study of these unstable pf-shell nuclei, half-lives can be measured rather accurately. On the other hand, in high-resolution (3He, t) charge-exchange reactions at 0°, individual GT transitions up to high excitations can be studied. Assuming the isospin symmetry for the strengths of Tz = ±2 → ±1 analogous GT transitions, we present a "merged analysis" for the determination of GT transition strengths starting from proton-rich Tz = -2 nuclei. We applied this analysis to the A = 52, T = 2 system, and it was found that the GT transitions and the properties of the 52Ni β decay can be understood better by combining the mirror GT strength distribution obtained from the 52Cr(3He, t) reaction.
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U2 - 10.1063/1.3455955
DO - 10.1063/1.3455955
M3 - Conference contribution
AN - SCOPUS:77954602396
SN - 9780735407848
T3 - AIP Conference Proceedings
SP - 297
EP - 300
BT - Tours Symposium on Nuclear Physics and Astrophysics - VII
T2 - 7th Tours Symposium on Nuclear Physics and Astrophysics
Y2 - 16 November 2009 through 20 November 2009
ER -