欢迎登录材料期刊网

材料期刊网

高级检索

在双核模型框架下, 用数值解主方程方法计算了超重核的熔合几率. 明确描述了包含能量、角动量和碎片形变弛豫的相对运动, 并与核子扩散过程相耦合. 因此, 用微观方法推导出的核子跃迁几率是与时间相关的. 所计算的以Pb为靶的冷熔合超重核形成截面和以48Ca为弹核的热熔合超重核形成激发函数与已知的实验值在合理的范围内符合.

In the dinuclear system conception, the master equation is solved numerically to calculate the fusion probabilities of super-heavy nuclei. The relative motion concerning the energy, the angular momentum and the fragment deformation relaxations is explicitly treated to couple with the diffusion process. The nucleon transition probabilities, which are derived microscopically, are related with the energy dissipation of the relative motion, thus they are time-dependent. The formation cross sections of the super-heavy nuclei from Pb-based cold fusion and excitation functions from 48Ca induced hot fusion are reasonably consistent with known experimental data.

参考文献

[1] Hofmann S.Rep Prog Phys,1998,61:636.
[2] Oganessian Yu Ts,Yeremin A V,Popeko A G,et al.Nature,1999,400:242.
[3] Bjornholm S,Swiatecki W J.Nucl Phys,1982,A391:471.
[4] Aritomo Y,Wada T,Ohta M.Phys Rev,1999,C59:796.
[5] Cherepanov E A,Volkov V V,Antonenko N V,et al.Nucl Phys,1996,A459:145.
[6] Adamian G G,Antonenko N V,Scheid W.Nucl Phys,1997,A618:176.
[7] Zagrebaev V L.Phys Rev,2001,C64:034 606; Phys Rev,2003,C67:R061 601; Phys Rev,2002,C65:014 607.
[8] Zagrebaev V L.Phys Rev,2001,C64:034 606; Phys Rev,2003,C67:R061 601; Phys Rev,2002,C65:014 607.
[9] Zagrebaev V L.Phys Rev,2001,C64:034 606; Phys Rev,2003,C67:R061 601; Phys Rev,2002,C65:014 607.
[10] Shen Caiwann,Kosenko Grigori,Abe Yasuhisa.Phys Rev,2002,C59:061 602(R).
[11] Smolanczuk Robert.Phys Rev,1999,C59:2 634.
[12] Norenberg W.Phys Lett,1974,B53:289.
[13] Ayik S,Schuermann B,Norenberg W.Z Phys,1976,A277:299;Z Phys,1976,A279:145; Schuermann B,Norenberg W,Simbel M.Z Phys,1978,A286:263.
[14] Ayik S,Schuermann B,Norenberg W.Z Phys,1976,A277:299;Z Phys,1976,A279:145; Schuermann B,Norenberg W,Simbel M.Z Phys,1978,A286:263.
[15] Ayik S,Schuermann B,Norenberg W.Z Phys,1976,A277:299;Z Phys,1976,A279:145; Schuermann B,Norenberg W,Simbel M.Z Phys,1978,A286:263.
[16] Adamian G G,Antonenko N V,Scheid W,et al.Nucl Phys,1998,A633:409.
[17] Antonenko N V,Cherepanov E A,Nasirov A V,et al.Phys Lett,1993,B319:425; Phys Rev,1995,C51:2 634.
[18] Antonenko N V,Cherepanov E A,Nasirov A V,et al.Phys Lett,1993,B319:425; Phys Rev,1995,C51:2 634.
[19] Adamian G G,Antonenko N V,Scheid W,et al.Nucl Phys,1997,A627:361.
[20] Li W F,Wang N,Li J F,et al.Euro Phys Lett,2003,64:750.
[21] Li Wenfei,Wang Nan,Jia Fei,et al.J Phys,2006,G32:1 143.
[22] Feng Zhaoqing,Jin Genming,Fu Fen,et al.Nucl Phys,2006,A771:50.
[23] Wolschin G,Norenberg W.Z Phys,1978,A284:209.
[24] Moller P,Nix J R,Myers W D,et al.Atom Data and Nuclear Data Tables,1995,59:185.
[25] Wong C Y.Phys Rev Lett,1973,73:766.
[26] Li Qingfeng,Zuo Wei,Li Wenfei,et al.Euro Phys J,2005,A24:223.
[27] Adamian G G,Antonenko N V,Scheid W.Phys Rev,2003,C68:034 601.
[28] Grange P,Li Junqing,Weidenmüller H A.Phys Rev,1983,C27:2 063.
[29] Bohr N,Wheeler J A.Phys Rev,1939,56:426.
[30] Adamian G G,Antonenko N V,Ivanova S P,et al.Phys Rev,2000,C62,064 303.
[31] Vandenbosch R,Huizenga J.Nuclear Fission.New York,London:Academic Press,1973.
[32] Zagrebaev V I,Aritomo Y,Itkis M G,et al.Phys Rev,2001,C65:014 607.
[33] Zhang W,Zhang S S,Zhang S Q,et al.Chin Phys Lett,2003,20:1 694.
[34] Jackson J D.Can J Phys,1956,34:767.
[35] Adamian G G,Antonenko N V,Scheid W.Nucl Phys,2000,A678:24.
[36] Denisov V Yu,Hofmann S.Phys Rev,2000,C61:034 606.
[37] Smolańczuk R.Phys Rev,2001,C63:044 607.
[38] Adamian G G,Antonenko N V,Diaz-Torres A,et al.AIP Conf Proc,2001,561:421.
[39] Gregorich K E,Ginter T N,Loveland W,et al.Euro Phys J,2003,A18:633.
[40] Oganessian Yu Ts,Utyonkoy V K,Lobanov Yu V,et al.Phys Rev,2004,C69:021 601(R); Phys Rev,2004,C70:064 609.
[41] Oganessian Yu Ts,Utyonkoy V K,Lobanov Yu V,et al.Phys Rev,2004,C69:021 601(R); Phys Rev,2004,C70:064 609.
上一张 下一张
上一张 下一张
计量
  • 下载量()
  • 访问量()
文章评分
  • 您的评分:
  • 1
    0%
  • 2
    0%
  • 3
    0%
  • 4
    0%
  • 5
    0%