2015
DOI: 10.5506/aphyspolb.46.657
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Gamow--Teller Excitations Studied by Weak and Strong Interactions

Abstract: Studying weak nuclear responses, especially the Gamow-Teller (GT) transitions starting from stable as well as unstable nuclei, provide crucial and critical information on nuclear structure. Therefore, the study of GT transitions is a key issue in nuclear physics and also nuclear-astrophysics. Under the assumption of isospin symmetry, it is expected that the structure of mirror nuclei and the GT transitions starting from their ground states are identical. We have studied the corresponding GT transitions startin… Show more

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Cited by 5 publications
(18 citation statements)
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“…A quenching factor q F =0.74 to the GamowTeller (GT) operator is employed to calculate the β -decay strength distribution. The modern GXPF1J interaction has recently been used to reproduce various experimental GamowTeller (GT) strengths in the region close to A = 52 [39]. The calculated results are shown in the right part of Fig.…”
mentioning
confidence: 81%
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“…A quenching factor q F =0.74 to the GamowTeller (GT) operator is employed to calculate the β -decay strength distribution. The modern GXPF1J interaction has recently been used to reproduce various experimental GamowTeller (GT) strengths in the region close to A = 52 [39]. The calculated results are shown in the right part of Fig.…”
mentioning
confidence: 81%
“…2. The J π assignments for the levels in 52 Co are inferred from the analogous states in the mirror nucleus 52 Mn [39]. By using the IMME, the mass excess of 52 Ni is predicted to be ME( 52 Ni) = −22699 (22) keV and the Q EC value of 52 Ni is thus deduced to be 11662(23) keV.…”
mentioning
confidence: 99%
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“…2. The J π assignments for the levels in 52 Co are inferred from the analogous states in the mirror nucleus 52 Mn [39]. By using the IMME, the mass excess of 52 Ni is predicted to be ME( 52 Ni) = −22699(22) keV and the Q EC value of 52 Ni is thus deduced to be 11662(23) keV.…”
Section: β -Decay Properties Of 52 Nimentioning
confidence: 99%
“…The absolute intensity of 42(10)% for the 2407-keV γ transition measured in 52 Co is much stronger than the 13.7(2)% 1352(10)-keV proton emission [26]. Hence, it is reasonable to assign the former as from the IAS in 52 Co with ME = −31426(10) keV, and the latter as from a 1 + state with ME = −31561(14) keV, which could be the analog 1 + state to the one identified in the mirror nucleus 52 Mn [38,39].…”
Section: Pos(inpc2016)025mentioning
confidence: 99%