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《中国物理C》(英文)编辑部
2024年10月30日

Shape coexistence close to N=50 in the neutron-rich isotope 80Ge investigated by IBM-2

  • The properties of the low-lying states, especially the relevant shape coexistence in 80Ge, close to one of most neutron-rich doubly magic nuclei at N=50 and Z=28, have been investigated within the framework of the proton-neutron interacting model (IBM-2). Based on the fact that the relative energy of the d neutron boson is different from that of the proton boson, the calculated energy levels of low-lying states and E2 transition strengths can reproduce the experimental data very well. Particularly, the first excited state 0+2, which is intimately related to the shape coexistence phenomenon, is reproduced quite nicely. The ρ2(E2, 02+→01+) transition strength is also predicted. The experimental data and theoretical results indicate that both collective spherical and γ-soft vibration structures coexist in 80Ge.
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  • [1] A. Poves, J. Phys. G:Nucl. Part. Phys., 43:020401(2016)
    [2] K. Heyde and J. L. Wood, Rev. Mod. Phys., 83:1467(2011)
    [3] A. Gade and S. N. Liddick, J. Phys. G:Nucl. Part. Phys., 43:024001(2016)
    [4] F. Nowacki, A. Poves, E. Caurier, and B. Bounthong, Phys. Rev. Lett., 117:272501(2016)
    [5] A. N. Andreyev, Nature, 405:430(2000)
    [6] A. G\ddotorgen and W. Korten, J. Phys. G:Nucl. Part. Phys., 43:024002(2016)
    [7] Y. X. Liu, S. Y. Yu, and Y. Sun, Sci. China-Phys. Mech. Astron., 58:112003(2015)
    [8] G. X. Dong, X. B. Wang, and S. Y. Yu, Sci. China-Phys. Mech. Astron., 58:112004(2015)
    [9] Z. J. Bai, X. M. Fu, C. F. Jiao, and F. R. Xu, Chin. Phys. C, 39:094101(2015)
    [10] J. Sun, T. Komatsubara, J. Q. Wang, H. Guo, X. Y. Hu, Y. J. Ma, Y. Z. Liu, and K. Furuno, Chin. Phys. C, 40:124001(2016)
    [11] F. Iachello, N. V. Zamfir, and R. F. Casten, Phys. Rev. Lett., 81:1191(1998)
    [12] Y. X. Liu, L. Z. Mu, and H. Q. Wei, Phys. Lett. B, 633:49(2006)
    [13] M. Hasegawa, K. Kaneko, T. Mizusaki, and Y. Sun, Phys. Lett. B, 656:51(2007)
    [14] Y. Sun et al, Phys. Rev. C, 80:054306(2009)
    [15] Y. X. Liu, Y. Sun, X. H. Zhou, Y. H. Zhang, S. Y. Yu, Y. C. Yang, H. Jin, Nucl. Phys. A, 858:11(2011)
    [16] Z. Z. Ren, Phys. Rev. C, 65:051304(2002)
    [17] G. Hagen, G. R. Jansen, and T. Papenbrock, Phys. Rev. Lett., 117:172501(2016)
    [18] A. Gottardo et al, Phys. Rev. Lett., 116:182501(2016)
    [19] E. Padilla-Rodal et al, Phys. Rev. Lett., 94:122501(2005)
    [20] S. F. Shen, S. J. Zheng, F. R. Xu, and R. Wyss, Phys. Rev. C, 84:044315(2011)
    [21] D. L. Zhang and B. G. Ding, Chin. Phys. Lett., 30:122101(2013)
    [22] D. L. Zhang, and C. F. Mu, Sci. China-Phys. Mech. Astron., 61:012012(2018)
    [23] M. Lettmann et al, Phys. Rev. C, 96:011301(2017)
    [24] H. Iwasaki et al, Phys. Rev. C, 78:021304(2008)
    [25] S. Mukhopadhyay et al, Phys. Rev. C, 95:014327(2017)
    [26] L. Guo, J. A. Maruhn, and P. G. Reinhard, Phys. Rev. C, 76:034317(2007)
    [27] P. Sarriguren, Phys. Rev. C, 91:044304(2015)
    [28] T. Nikić, P. Marević, and D. Vretenar, Phys. Rev. C, 89:044325(2014)
    [29] G. H. Bhat, W. A. Dar, J. A. Sheikh, and Y. Sun, Phys. Rev. C, 89:014328(2014)
    [30] D. Verney et al, Phys. Rev. C, 87:054307(2013)
    [31] S. T. Hsieh, H. C. Chiang, and D. S. Chuu, Phys. Rev. C, 46:195(1992)
    [32] F. Iachello, and A. Arima The Interacting Boson Model (Cambridge, England:Cambridge University Press, 1987)
    [33] P. D. Duval, D. Goutte, and M. Vergnes, Phys. Lett. B, 124:297(1983)
    [34] J. P. Elliott, J. A. Evans, V. S. Lac, and G. L. Long, Nucl. Phys. A, 609:1(1996)
    [35] K. Nomura et al, Phys. Rev. C, 95:064310(2017)
    [36] D. L. Zhang and B. G. Ding, Sci. China-Phys. Mech. Astron., 57:447(2014)
    [37] D. L. Zhang and C. F. Mu, Chin. Phys. Lett., 33:102102(2016)
    [38] D. L. Zhang and C. F. Mu, Sci. China-Phys. Mech. Astron., 59:682012(2016)
    [39] P. Cejner, J, Jolie, and R. F. Casten, Rev. Mod. Phys., 82:2155(2010)
    [40] G. Grdal et al, Phys. Rev. C, 88:014301(2013)
    [41] H. Rotter et al, Nucl. Phys. A, 514:401(1990)
    [42] H. Dejbakhsh, D. Latypov, G. Ajupova, and S. Shlomo, Phys. Rev. C, 46:2326(1992)
    [43] K. Nomura, T. Otsuka, N. Shimizu, and L. Guo, Phys. Rev. C, 83:041302(2011)
    [44] K. Nomura, T. Otsuka, and P. V.Isacker, J. Phys. G:Nucl. Part. Phys., 43:024008(2016)
    [45] D. L. Zhang and C. F. Mu, Sci. China-Phys. Mech. Astron., 60:042011(2017)
    [46] T. Otsuka and N. Yoshida, Program NPBOS, JAER-M Report, No.85(unpublished):(1985)
    [47] R. F. Casten and D. D. Warner, Rev. Mod. Phys., 60:389(1988)
    [48] D. L. Zhang, S. Q. Yuan, and B. G. Ding, Chin. Phys. Lett., 32:062101(2015)
    [49] W. D. Hamilton, A. Irback, and J. P. Elliott, Phys. Rev. Lett., 53:2469(1984)
    [50] J. Stachel, P. Van Isacker, and K. Heyde, Phys. Rev. C, 25:650(1982)
    [51] P. F. Mantica and W. B. Walters, Phys. Rev. C, 53:R2586(1996)
    [52] E. Bouchez et al, Phys. Rev. Lett., 90:082502(2003)
    [53] B. A.Brown, A. B. Garnsworthy, T. Kib\acuteedi, and A. E. Stuchbery, Phys. Rev. C, 95:011301(2017)
    [54] B. R. Barrett and T. Otsuka, Phys. Rev. C, 46:1735(1992)
    [55] A. Leviatan and D. Shapira, Phys. Rev. C, 93:051302(2016)
    [56] J. L. Wood, E. E. Zganjar, C. E. Coster, and K. Heyde, Nucl. Phys. A, 651:323(1999)
    [57] K. Kaneko, Y. Sun, and R. Wadsworth, Phys. Scr. 92:114008(2017)
    [58] Y. Tsunoda et al, Phys. Rev. C, 89:031301(R) (2014)
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Da-Li Zhang and Cheng-Fu Mu. Shape coexistence close to N=50 in the neutron-rich isotope 80Ge investigated by IBM-2[J]. Chinese Physics C, 2018, 42(3): 034101. doi: 10.1088/1674-1137/42/3/034101
Da-Li Zhang and Cheng-Fu Mu. Shape coexistence close to N=50 in the neutron-rich isotope 80Ge investigated by IBM-2[J]. Chinese Physics C, 2018, 42(3): 034101.  doi: 10.1088/1674-1137/42/3/034101 shu
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Received: 2017-10-23
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    Supported by National Natural Science Foundation of China (11475062, 11647306, 11147148)

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Shape coexistence close to N=50 in the neutron-rich isotope 80Ge investigated by IBM-2

    Corresponding author: Da-Li Zhang,
    Corresponding author: Cheng-Fu Mu,
  • 1. Department of Physics, Huzhou University, Huzhou 313000, China
Fund Project:  Supported by National Natural Science Foundation of China (11475062, 11647306, 11147148)

Abstract: The properties of the low-lying states, especially the relevant shape coexistence in 80Ge, close to one of most neutron-rich doubly magic nuclei at N=50 and Z=28, have been investigated within the framework of the proton-neutron interacting model (IBM-2). Based on the fact that the relative energy of the d neutron boson is different from that of the proton boson, the calculated energy levels of low-lying states and E2 transition strengths can reproduce the experimental data very well. Particularly, the first excited state 0+2, which is intimately related to the shape coexistence phenomenon, is reproduced quite nicely. The ρ2(E2, 02+→01+) transition strength is also predicted. The experimental data and theoretical results indicate that both collective spherical and γ-soft vibration structures coexist in 80Ge.

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