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《中国物理C》（英文）编辑部
2024年10月30日
Chinese Physics C> 2017, Vol. 41> Issue(5) : 054104 DOI: 10.1088/1674-1137/41/5/054104

Quenching of neutron spectroscopic factors of radioactive carbon isotopes with knockout reactions within a wide energy range

  • 1.

      School of Physics and State Key Laboratory of Nuclear Physics and Technology, Peking University, Beijing 100871, China

  • 2.

      School of Physics and Nuclear Energy Engineering, Beihang University, Beijing 100191, China

  • 3.

     School of Physics and Nuclear Energy Engineering, Beihang University, Beijing 100191, China

  • 4.

     Beijing Key Laboratory of Advanced Nuclear Materials and Physics, Beihang University, Beijing 100191, China

  • The quenching factors of one-neutron spectroscopic factors, which are ratios of theoretical to experimental one-neutron removal cross sections, are studied for the carbon isotopes 15-19C, with 12C and 9Be targets within incident energies from around 50 to 900 MeV/nucleon. The resulting values of quenching factors do not show strong energy dependence within such an energy range. The average values of the these quenching factors agree well with the systematics in [J.A. Tostevin and A. Gade, Phys. Rev. C, 90 057602 (2014)], which was established for a large set of radioactive nuclei with different masses below 305 MeV/nucleon.
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  • References

    [1] G. J. Kramer, H. P. Blok, and L. Lapiks, Nucl. Phys. A, 679: 267 (2001)
    [2] N. K. Glendenning, Annu. Rev. Nucl. Sci., 13: 191 (1963)
    [3] C. Barbieri, Phys. Rev. Lett., 103: 202502 (2009)
    [4] N. K. Timofeyuk, Phys. Rev. Lett.,103: 242501 (2009)
    [5] N. K. Timofeyuk, Phys. Rev. C, 81: 064306 (2010)
    [6] R. J. Charity, L. G. Sobotka, and W. H. Dickhoff, Phys. Rev. Lett., 97: 162503 (2006)
    [7] F. Flavigny, A. Gillibert, L. Nalpas et al, Phys. Rev. Lett., 110: 122503 (2013)
    [8] J. P. Schiffer, C. R. Hoffman, B. P. Kay et al, Phys. Rev. Lett., 108: 022501 (2012)
    [9] B. P. Kay, J. P. Schiffer, and S. J. Freeman, Phys. Rev. Lett., 111: 042502 (2013)
    [10] Jenny Lee, M. B. Tsang, D. Bazin et al, Phys. Rev. Lett., 104: 112701 (2010)
    [11] A. Gade, D. Bazin, C. M. Campbell et al, Phys. Rev. Lett., 93: 042501 (2004)
    [12] A. Gade, P. Adrich, D. Bazin et al, Phys. Rev. C, 77: 044306 (2008)
    [13] J. A. Tostevin and A. Gade, Phys. Rev. C, 90: 057602 (2014)
    [14] E. C.Simpson and J. A.Tostevin, Phys. Rev. C, 79: 024616 (2009)
    [15] De-Qing FANG, T. Yamaguchi, T. ZHENG et al, High Energy Physics and Nuclear Physics, 28: 93 (2004) (in Chinese)
    [16] Cui-E WU , Yan-Lin YE, Dong-Xing JIANG et al, High Energy Physics and Nuclear Physics, 29: 1052 (2005) (in Chinese)
    [17] De-Qing FANG, Yao FU, Xiao-Yan SUN et al, Chin. Phys. C, 33: 197 (2009)
    [18] Lin-Hui LV, Yan-Lin YE, Dong-Xing JIANG et al, Chin. Phys. C, 35: 891 (2011)
    [19] Yan-Lin YE, Lin-Hui LV, Zhong-Xin CAO, and Jun XIAO, Chin. Phys. C, 36: 127 (2012)
    [20] E. Sauvan et al, Phys. Rev. C, 69: 044603 (2004)
    [21] A. E. L. Dierperink and T. de Forest, Jr., Phys. Rev. C, 10: 543 (1974)
    [22] C. A. Bertulani and A. Gade, Comput. Phys. Commun., 175: 372-380 (2006)
    [23] L. Ray, Phys. Rev. C, 20: 1857 (1979)
    [24] S. M. Lenzi et al, Phys. Rev. C, 38: 2086 (1988)
    [25] W. Horiuchi et al, Phys. Rev. C, 75: 044607 (2007)
    [26] C. Perrin et al, Phys. Rev. Lett., 49: 1905 (1982)
    [27] H. Y. Zhang et al, Nucl. Phys. A, 707: 303 (2002)
    [28] D. Q. Fang et al, Phys. Rev. C, 61: 064311 (2000)
    [29] S. Kox et al, Phys. Rev. C, 35: 1678 (1987)
    [30] T. Zheng et al, Nucl. Phys. A, 709: 103 (2002)
    [31] J. Jaros et al, Phys. Rev. C, 18: 2273 (1978)
    [32] M. Takechi et al, Eur. Phys. J. A, 25 s01: 217 (2005)
    [33] M. Takechi et al, Phys. Rev. C, 79: 061601(R) (2009)
    [34] A. Ozawa, T. Suzuki, and I. Tanihata, Nucl. Phys. A, 693: 32 (2001).
    [35] B. A. Brown, Phys. Rev. C, 58: 220 (1998)
    [36] Jenny Lee, J. A. Tostevin, B. A. Brown et al, Phys. Rev. C, 73: 044608 (2006)
    [37] D. Y. Pang, Y. L. Ye, and F. R. Xu, Phys. Rev. C, 83: 064619 (2011)
    [38] Y. P. Xu and D. Y. Pang, Phys. Rev. C, 87: 044605 (2013)
    [39] D. T. Khoa, Phys. Rev. C, 63: 034007 (2001)
    [40] D. T. Khoa, Phys. Rev. C, 63:034007 (2001)
    [41] D. Y. Pang, Y. L. Ye, and F. R. Xu, J. Phys. G: Nucl. Part. Phys., 39: 095101 (2012)
    [42] H. De Vries, C. W. De Jager, and C. De Vries, At. Data Nucl. Data Tables, 36: 495 (1987)
    [43] D. Y. Pang, Y. L. Ye, and F. R. Xu, J. Phys. G:Nucl. Part. Phys., 39:095101 (2012)
    [44] C. Yuan, T. Suzuki, T. Otsuka, F. Xu, and N. Tsunoda, Phys.Rev. C, 85: 064324 (2012)
    [45] H. De Vries, C. W. De Jager and C. De Vries, At. Data Nucl. Data Tables 36:495 (1987)
    [46] B. A. Brown, A. Etchegoyan, and W. D. M. Rae, OXBASH ,Oxford, Buenos-Aires, Michigan State, Shell Model Program, Michigan State University Cyclotron Laboratory Report No. 524 (1986)
    [47] C. Yuan, T. Suzuki, T. Otsuka, F. Xu, and N. Tsunoda, Phys.Rev. C, 85:064324 (2012)
    [48] E. K. Warburton and B. A. Brown, Phys. Rev. C, 46: 923 (1992)
    [49] B. A. Brown, A. Etchegoyan, and W. D. M. Rae, OXBASH,Oxford, Buenos-Aires, Michigan State, Shell Model Program, Michigan State University Cyclotron Laboratory Report No.524 (1986)
    [50] C. Rodrguez-Tajes et al, Phys. Rev. C, 82: 024305 (2010)
    [51] E. K. Warburton and B. A. Brown, Phys. Rev. C, 46:923 (1992)
    [52] C. Rodrguez-Tajes et al, Phys. Rev. C, 82:024305 (2010)
    [53] B. A. Brown, P. G. Hansen, B. M. Sherrill, and J. A. Tostevin, Phys. Rev. C, 65: 061601(R) (2002)
    [54] B. A. Brown, P. G. Hansen, B. M. Sherrill, and J. A. Tostevin, Phys. Rev. C, 65:061601(R) (2002)
    [55] J.R. Terry et al, Phys. Rev. C, 69: 054306 (2004)
    [56] J.R. Terry et al, Phys. Rev. C, 69:054306 (2004)
    [57] V. Maddalena et al, Phys. Rev. C, 63: 024613 (2001)
    [58] D. Bazin et al, Phys. Rev. C, 57: 2156 (1998)
    [59] V. Maddalena et al, Phys. Rev. C, 63:024613 (2001)
    [60] D. Bazin et al, Phys. Rev. C, 57:2156 (1998)
    [61] N. Kobayashi et al, Phys. Rev. C, 86: 054604 (2012)
    [62] N. Kobayashi et al, Phys. Rev. C, 86:054604 (2012)
    [63] D. Cortina-Gil et al, Eur. Phys. J. A, 10: 49 (2001)
    [64] T. Suzuki and T. Otsuka, Phys. Rev. C, 78: 061301(R) (2008). C, 87:044605 (2013)
    [65] D. Cortina-Gil et al, Eur. Phys. J. A, 10:49 (2001)
    [66] T. Suzuki and T. Otsuka, Phys. Rev. C, 78:061301(R) (2008).

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Chao Wen, Yi-Ping Xu, Dan-Yang Pang and Yan-Lin Ye. Quenching of neutron spectroscopic factors of radioactive carbon isotopes with knockout reactions within a wide energy range[J]. Chinese Physics C, 2017, 41(5): 054104. doi: 10.1088/1674-1137/41/5/054104
Chao Wen, Yi-Ping Xu, Dan-Yang Pang and Yan-Lin Ye. Quenching of neutron spectroscopic factors of radioactive carbon isotopes with knockout reactions within a wide energy range[J]. Chinese Physics C, 2017, 41(5): 054104.  doi: 10.1088/1674-1137/41/5/054104 shu
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Received: 2016-11-14
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    Supported by National Natural Science Foundation of China (1275018, U1432247) and National Key Research and Development Program (2016YFA0400502)

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Quenching of neutron spectroscopic factors of radioactive carbon isotopes with knockout reactions within a wide energy range

    Corresponding author: Yan-Lin Ye,
  • 1.  School of Physics and State Key Laboratory of Nuclear Physics and Technology, Peking University, Beijing 100871, China
  • 2.  School of Physics and Nuclear Energy Engineering, Beihang University, Beijing 100191, China
  • 3. School of Physics and Nuclear Energy Engineering, Beihang University, Beijing 100191, China
  • 4. Beijing Key Laboratory of Advanced Nuclear Materials and Physics, Beihang University, Beijing 100191, China
  • Received Date: 2016-11-14
  • Available Online: 2017-05-05
Fund Project:  Supported by National Natural Science Foundation of China (1275018, U1432247) and National Key Research and Development Program (2016YFA0400502)

Abstract: The quenching factors of one-neutron spectroscopic factors, which are ratios of theoretical to experimental one-neutron removal cross sections, are studied for the carbon isotopes 15-19C, with 12C and 9Be targets within incident energies from around 50 to 900 MeV/nucleon. The resulting values of quenching factors do not show strong energy dependence within such an energy range. The average values of the these quenching factors agree well with the systematics in [J.A. Tostevin and A. Gade, Phys. Rev. C, 90 057602 (2014)], which was established for a large set of radioactive nuclei with different masses below 305 MeV/nucleon.

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