Theoretical study on production cross sections of exotic actinide nuclei in multinucleon transfer reactions

  • Within the dinuclear system (DNS) model, the multinucleon transfer reactions 129,136Xe + 248Cm, 112Sn + 238U, and 144Xe + 248Cm are investigated. The production cross sections of primary fragments are calculated with the DNS model. By using a statistical model, we investigate the influence of charged particle evaporation channels on production cross sections of exotic nuclei. It is found that for excited neutron-deficient nuclei the charged particle evaporation competes with neutron emission and plays an important role in the cooling process. The production cross sections of several exotic actinide nuclei are predicted in the reactions 112Sn + 238U and 136,144Xe + 248Cm. Considering the beam intensities, the collisions of 136,144Xe projectiles with a 248Cm target for producing neutron-rich nuclei with Z=92-96 are investigated.
      PCAS:
    • 25.40.Hs(Transfer reactions)
    • 25.70.-z(Low and intermediate energy heavy-ion reactions)
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    [31] L. Zhu, Z. Q. Feng, and F. S. Zhang, J. Phys. G:Nucl. Part. Phys., 42:085102(2015)
    [32] G. G. Adamian, N. V. Antonenko, and A. S. Zubov, Phys. Rev. C, 71:034603(2005)
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    [39] N. Wang and L. Guo, Phys. Lett. B, 760:236(2016)
    [40] C. Li, F. Zhang, J. Li, L. Zhu, J. Tian, N. Wang, and F. S. Zhang, Phys. Rev. C, 93:014618(2016)
    [41] R. Yanez and W. Loveland, Phys. Rev. C, 91:044608(2015)
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    [43] N. Vonta et al, Phys. Rev. C, 94:064611(2016)
    [44] H. M. Devaraja et al, Phys. Lett. B, 748:199(2015)
    [45] L. Zhu, et al, Phys. Rev. C, 90:014612(2014)
    [46] L. Zhu, et al, Chin. Phys. C, 40:124105(2016)
    [47] X. J. Bao, Y. Gao, J. Q. Li, and H. F. Zhang, Phys. Rev. C, 91:064612(2015)
    [48] X. J. Bao, Y. Gao, J. Q. Li, and H. F. Zhang, Phys. Rev. C, 92:034612(2015)
    [49] N. Wang, E. G. Zhao, W. Scheid, and S. G. Zhou, Phys. Rev. C, 85:041601(R) (2012)
    [50] Z. Q. Feng, G. M. Jin, J. Q. Li, and W. Scheid, Phys. Rev. C, 76:044606(2007)
    [51] J. Hong, G. G. Adamian, and N. V. Antonenko, Phys. Lett. B, 764:42-48(2017)
    [52] W. Nrenberg, Z. Phys. A, 274:241-250(1975)
    [53] S. Ayik, B. Schrmann, and W. Nrenberg, Z. Phys. A, 277:299-310(1976)
    [54] P. Mller, J.R. Nix, W. D. Myers, and W. J. Swiatecki, At. Data Nucl. Data Tables, 59:185(1995)
    [55] L. Zhu et al, Phys. Rev. C, 93:064610(2016)
    [56] X. J. Bao, S. Q. Guo, H. F. Zhang, and J. Q. Li, J. Phys. G:Nucl. Part. Phys., 43:125105(2016)
    [57] C. Y. Wong, Phys. Rev. Lett., 31:766(1973)
    [58] J. Q. Li and G. Wolschin, Phys. Rev. C, 27:590(1983)
    [59] A. S. Zubov, G. G. Adamian, N. V. Antonenko, S. P. Ivanova, and W. Scheid, Phys. Rev. C, 68:014616(2003)
    [60] J. D. Jackson, Can. J. Phys, 34:(1956) 767
    [61] V. F. Weisskopf, Phys. Rev., 52:295(1937)
    [62] V. F. Weisskopf and D. H. Ewing, Phys. Rev., 57:472(1940)
    [63] N. Bohr and J. A. Wheeler, Phys. Rev., 56:426(1939)
    [64] S. Cohen and W.J. Swiatecki, Ann. Phys., 22:406(1963)
    [65] H. A. Bethe, Phys. Rev., 50:332(1936)
    [66] W. Loveland, Phys. Rev. C, 76:014612(2007)
  • [1] M. Thoennessen, Rep. Prog. Phys., 76:056301(2013)
    [2] V. V. Volkov, Phys. Rep., 44:93(1978)
    [3] H. Freiesleben and J. V. Kratz, Phys. Rep., 106:1(1984)
    [4] J. V. Kratz, W. Loveland, and K. J. Moody, Nucl. Phys. A, 944:117(2015)
    [5] K. D. Hildenbrand, H. Freiesleben, F. Phlhofer, W. F. W. Schneider, R. Bock, D. v. Harrach, and H. J. Specht, Phys. Rev. Lett., 39:1065(1977)
    [6] M. Schdel et al, Phys. Rev. Lett., 41:469(1978)
    [7] M. Schdel et al, Phys. Rev. Lett., 48:852(1982)
    [8] K. J. Moody et al, Phys. Rev. C, 33:1315(1986)
    [9] R. B. Welch and K. J. Moody et al, Phys. Rev. C, 35:204(1987)
    [10] D. C. Rafferty, et al, Phys. Rev. C, 94:024607(2016)
    [11] W. Loveland, A. M. Vinodkumar, D. Peterson, and J. P. Greene, Phys. Rev. C, 83:044610(2011)
    [12] J. V. Kratz, M. Schdel, and H. W. Gggeler, Phys. Rev. C, 88:054615(2013)
    [13] A. Vogt et al, Phys. Rev. C, 92:024619(2015)
    [14] L. Chen et al, Phys. Lett. B, 691:234(2010)
    [15] J. Kurcewicz et al, Phys. Lett. B, 717:371(2012)
    [16] E. M. Kozulin et al, Phys. Rev. C, 89:014614(2014)
    [17] M. V. Pajtler et al, Nucl. Phys. A, 941:273(2015)
    [18] W. Krlas et al, Nucl. Phys. A, 832:170(2010)
    [19] E. M. Kozulin et al, Phys. Rev. C, 86:044611(2012)
    [20] J. S. Barrett et al, Phys. Rev. C, 91:064615(2015)
    [21] Y. X. Watanabe et al, Phys. Rev. Lett., 115:172503(2015)
    [22] V. Zagrebaev and W. Greiner, Phys. Rev. Lett., 101:122701(2008)
    [23] Z. Q. Feng, G. M. Jin, and J. Q. Li, Phys. Rev. C, 80:067601(2009)
    [24] Z. Q. Feng, Phys. Rev. C, 95:024615(2017).
    [25] L. Zhu et al, Phys. Lett. B, 767:437(2017)
    [26] L. Zhu, et al, Phys. Rev. C, 94:054606(2016)
    [27] L. Zhu, et al, Phys. Rev. C, 95:044608(2017)
    [28] L. Zhu, et al, Nucl. Phys. A, 964:93(2017)
    [29] L. Zhu, et al, Phys. Rev. C, 96:024606(2017)
    [30] G. G. Adamian, N. V. Antonenko, and D. Lacroix, Phys. Rev. C, 82:064611(2010)
    [31] L. Zhu, Z. Q. Feng, and F. S. Zhang, J. Phys. G:Nucl. Part. Phys., 42:085102(2015)
    [32] G. G. Adamian, N. V. Antonenko, and A. S. Zubov, Phys. Rev. C, 71:034603(2005)
    [33] Yu. E. Penionzhkevich, G. G. Adamian, and N. V. Antonenko, Phys. Lett. B, 621:119(2005)
    [34] D. J. Kedziora and C. Simenel, Phys. Rev. C, 81:044613(2010)
    [35] K. Sekizawa and K. Yabana, Phys. Rev. C, 93:054616(2016)
    [36] K. Sekizawa, Phys. Rev. C, 96:014615(2017)
    [37] Y. Iwata, T. Otsuka, J. A. Maruhn, and N. Itagaki, Phys. Rev. Lett., 104:252501(2010)
    [38] K. Zhao, Z. Li, Y. Zhang, N. Wang, Q. Li, C. Shen, Y. Wang, and X. Wu, Phys. Rev. C, 94:024601(2016)
    [39] N. Wang and L. Guo, Phys. Lett. B, 760:236(2016)
    [40] C. Li, F. Zhang, J. Li, L. Zhu, J. Tian, N. Wang, and F. S. Zhang, Phys. Rev. C, 93:014618(2016)
    [41] R. Yanez and W. Loveland, Phys. Rev. C, 91:044608(2015)
    [42] C. Golabek and C. Simenel, Phys. Rev. Lett., 103:042701(2009)
    [43] N. Vonta et al, Phys. Rev. C, 94:064611(2016)
    [44] H. M. Devaraja et al, Phys. Lett. B, 748:199(2015)
    [45] L. Zhu, et al, Phys. Rev. C, 90:014612(2014)
    [46] L. Zhu, et al, Chin. Phys. C, 40:124105(2016)
    [47] X. J. Bao, Y. Gao, J. Q. Li, and H. F. Zhang, Phys. Rev. C, 91:064612(2015)
    [48] X. J. Bao, Y. Gao, J. Q. Li, and H. F. Zhang, Phys. Rev. C, 92:034612(2015)
    [49] N. Wang, E. G. Zhao, W. Scheid, and S. G. Zhou, Phys. Rev. C, 85:041601(R) (2012)
    [50] Z. Q. Feng, G. M. Jin, J. Q. Li, and W. Scheid, Phys. Rev. C, 76:044606(2007)
    [51] J. Hong, G. G. Adamian, and N. V. Antonenko, Phys. Lett. B, 764:42-48(2017)
    [52] W. Nrenberg, Z. Phys. A, 274:241-250(1975)
    [53] S. Ayik, B. Schrmann, and W. Nrenberg, Z. Phys. A, 277:299-310(1976)
    [54] P. Mller, J.R. Nix, W. D. Myers, and W. J. Swiatecki, At. Data Nucl. Data Tables, 59:185(1995)
    [55] L. Zhu et al, Phys. Rev. C, 93:064610(2016)
    [56] X. J. Bao, S. Q. Guo, H. F. Zhang, and J. Q. Li, J. Phys. G:Nucl. Part. Phys., 43:125105(2016)
    [57] C. Y. Wong, Phys. Rev. Lett., 31:766(1973)
    [58] J. Q. Li and G. Wolschin, Phys. Rev. C, 27:590(1983)
    [59] A. S. Zubov, G. G. Adamian, N. V. Antonenko, S. P. Ivanova, and W. Scheid, Phys. Rev. C, 68:014616(2003)
    [60] J. D. Jackson, Can. J. Phys, 34:(1956) 767
    [61] V. F. Weisskopf, Phys. Rev., 52:295(1937)
    [62] V. F. Weisskopf and D. H. Ewing, Phys. Rev., 57:472(1940)
    [63] N. Bohr and J. A. Wheeler, Phys. Rev., 56:426(1939)
    [64] S. Cohen and W.J. Swiatecki, Ann. Phys., 22:406(1963)
    [65] H. A. Bethe, Phys. Rev., 50:332(1936)
    [66] W. Loveland, Phys. Rev. C, 76:014612(2007)
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Get Citation
Long Zhu. Theoretical study on production cross sections of exotic actinide nuclei in multinucleon transfer reactions[J]. Chinese Physics C, 2017, 41(12): 124102. doi: 10.1088/1674-1137/41/12/124102
Long Zhu. Theoretical study on production cross sections of exotic actinide nuclei in multinucleon transfer reactions[J]. Chinese Physics C, 2017, 41(12): 124102.  doi: 10.1088/1674-1137/41/12/124102 shu
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Received: 2017-08-18
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    Supported by National Natural Science Foundation of China (11605296) and Natural Science Foundation of Guangdong Province, China (2016A030310208)

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Theoretical study on production cross sections of exotic actinide nuclei in multinucleon transfer reactions

  • 1. Sino-French Institute of Nuclear Engineering and Technology, Sun Yat-sen University, Zhuhai 519082, China
Fund Project:  Supported by National Natural Science Foundation of China (11605296) and Natural Science Foundation of Guangdong Province, China (2016A030310208)

Abstract: Within the dinuclear system (DNS) model, the multinucleon transfer reactions 129,136Xe + 248Cm, 112Sn + 238U, and 144Xe + 248Cm are investigated. The production cross sections of primary fragments are calculated with the DNS model. By using a statistical model, we investigate the influence of charged particle evaporation channels on production cross sections of exotic nuclei. It is found that for excited neutron-deficient nuclei the charged particle evaporation competes with neutron emission and plays an important role in the cooling process. The production cross sections of several exotic actinide nuclei are predicted in the reactions 112Sn + 238U and 136,144Xe + 248Cm. Considering the beam intensities, the collisions of 136,144Xe projectiles with a 248Cm target for producing neutron-rich nuclei with Z=92-96 are investigated.

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