Properties of heavy ion interaction potentials calculated in the energy density formalism
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Nuclear potentials model for heavy-ion reactions
2019, New AstronomyCitation Excerpt :The evidence such as calculations related to fusion barrier distribution, logarithmic derivative L(E) and astrophysical S(E) factors shows that all experiments measure the fusion cross sections (Canto et al., 2006; Aguilera et al., 1995; Silva et al. 1977) and then extract useful information about the fusion barriers by using theoretical models. Under these situations, a large number of theoretical models and potentials have been introduced to describe the heavy ion fusion reaction (Dutt and Puri, 2010;Blocki et al., 1977; Residorf, 1994; Myers and Swiatecki, 2000; Bass, 1974, 1977; Christensen and Winther, 1976; Winther 1995; Denisov, 2002; Royer et al. 2009; Gupta et al., 1993; Ngo et al., 1975; Denisov and Pilipenko, 2007; Umar and Oberacker, 2008). In the theoretical approaches, the coupling effects between the relative motion of the participant nuclei and their intrinsic degrees of freedom strongly enhances the fusion probability and resulting in the fusion cross sections at near and below Coulomb barrier energies (Balantekin and Takigawa, 1998; Dasgupta et al., 1998; Beckerman, 1988; Steadman and Rhoades-Brown, 1986; Stokstad et al., 1980; Leigh et al., 1995; Montagnoli et al. 2013).
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Laboratoire associé au CNRS.