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Nuclear Experiment

arXiv:1610.09772 (nucl-ex)
[Submitted on 31 Oct 2016]

Title:Identification of the Lowest $T=2$, $J^{π=}0^+$ Isobaric Analog State in $^{52}$Co and Its Impact on the Understanding of $β$-Decay Properties of $^{52}$Ni

Authors:X. Xu, P. Zhang, P. Shuai, R. J. Chen, X. L. Yan, Y. H. Zhang, M. Wang, Yu. A. Litvinov, H. S. Xu, T. Bao, X. C. Chen, H. Chen, C. Y. Fu, S. Kubono, Y. H. Lam, D.W. Liu, R. S. Mao, X.W. Ma, M. Z. Sun, X. L. Tu, Y. M. Xing, J. C. Yang, Y. J. Yuan, Q. Zeng, X. Zhou, X. H. Zhou, W. L. Zhan, S. Litvinov, K. Blaum, G. Audi, T. Uesaka, Y. Yamaguchi, T. Yamaguchi, A. Ozawa, B. H. Sun, Y. Sun, A. C. Dai, F. R. Xu
View a PDF of the paper titled Identification of the Lowest $T=2$, $J^{\pi=}0^+$ Isobaric Analog State in $^{52}$Co and Its Impact on the Understanding of $\beta$-Decay Properties of $^{52}$Ni, by X. Xu and 37 other authors
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Abstract:Masses of $^{52g,52m}$Co were measured for the first time with an accuracy of $\sim 10$ keV, an unprecedented precision reached for short-lived nuclei in the isochronous mass spectrometry. Combining our results with the previous $\beta$-$\gamma$ measurements of $^{52}$Ni, the $T=2$, $J^{\pi}=0^+$ isobaric analog state (IAS) in $^{52}$Co was newly assigned, questioning the conventional identification of IASs from the $\beta$-delayed proton emissions. Using our energy of the IAS in $^{52}$Co, the masses of the $T=2$ multiplet fit well into the Isobaric Multiplet Mass Equation. We find that the IAS in $^{52}$Co decays predominantly via $\gamma$ transitions while the proton emission is negligibly small. According to our large-scale shell model calculations, this phenomenon has been interpreted to be due to very low isospin mixing in the IAS.
Comments: Accepted for publication in PRL. 5 pages, 2figures
Subjects: Nuclear Experiment (nucl-ex)
Cite as: arXiv:1610.09772 [nucl-ex]
  (or arXiv:1610.09772v1 [nucl-ex] for this version)
  https://doi.org/10.48550/arXiv.1610.09772
arXiv-issued DOI via DataCite
Journal reference: Phys. Rev. Lett. 117, 182503 (2016)
Related DOI: https://doi.org/10.1103/PhysRevLett.117.182503
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From: Xing Xu [view email]
[v1] Mon, 31 Oct 2016 03:21:43 UTC (111 KB)
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