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Level densities of silicon-28, titanium-46, chromium-52 and nickel-60 from Ericson fluctuations.

机译:埃里克森波动引起的硅28,钛46,铬52和镍60的能级密度。

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Ericson fluctuations in the differential cross sections are investigated for the compound reactions 27Al(p , n0)27Si, 45Sc(p, n 4)45Ti,45Sc( p, n5)45Ti, 51V(p, n0 )51Cr and 53 Ni(p, n0)59 Co. The excitation functions vary rapidly and irregularly with energy in a form that depends on the mass number A; for low A the fluctuations are stretched in energy while the opposite is observed for medium A nuclei.; Level widths in the compound nuclei 28Si, 46Ti, 52Cr and 60Ni are extracted from the analysis of the differential cross sections by the Fourier method and a nonlinear fit to the ln A2k+B2k > distribution. The neutron spectra for each reaction were measured at least at three backward angles but the coherence width Γ > does not show a strong angular dependence. The results then were weighted obtaining: Γ > = (33 ± 5) keV for 28Si at U = 18.9 MeV; Γ > = (5.9 ± 4) keV for 46 Ti at U = 15.5 MeV; Γ > = (9.6 ± 4) keV for 52Cr at U = 13.5 MeV and Γ > = (6.9 ± 4) keV for 60Ni at U = 12.9 MeV.; Nuclear level densities for the above nuclei were extracted by relating the average level spacing DJπ to the average level width ΓJ π using the fluctuation theory. The level density equation obtained by this procedure depends in general on the transmission coefficients, the density of levels in the residual nuclei and the spin cutoff parameter on the compound nucleus. Local optical model parameters (OMP) were preferred to global ones in order to find the transmission coefficients, this was the case in general for (p,p) reactions and in some cases for (α,α) reactions, however given the lack of OMP for neutrons we resorted to global systematics. For the present analysis the density of levels in the residual nuclei are model independent except for (p,p) reactions in 27 Al and 45Sc. This is due to the low excitations in the residual nuclei for the kinetic energy of the projectiles involved in the experiment and also because in the range of analysis TnlTplT al . For the spin cutoff we assumed a 100% solid sphere dependency on the excitation energy. Level density parameters of Al-Quraishi were employed to evaluate level densities in other ranges of energies for widths obtained by fluctuation measurements from database compilations.; Reasonable agreements are found with level density compilations based in the Fermi gas formalism of Al-Quraishi and Huang for 28 Si, 46Ti and 52 Cr but the comparison diverges for 60Ni for which additional measurements are required in order to clarify the observed discrepancies. The level density parameters that best describe the data are a = 3.57
机译:研究了复合反应 27 Al p n 的微分截面的Ericson涨落。 0 27 Si 45 Sc p ,< italic> n 4 45 Ti 45 Sc n 5 45 Ti 51 V p n 0 51 Cr 53 Ni p n 0 59 。激发函数随能量的大小迅速而不规则地变化,其形式取决于质量数A;对于低A而言,能量的波动被拉伸,而对于中等A核则相反。复合原子 28 Si 46 Ti 52 Cr 60 Ni ln math> A 2 k + B 2 k 并未显示出强烈的角度依赖性。然后对结果进行加权获得:对于U = 18.9 MeV的 28 Si ,<Γ> =(33±5)keV; U = 15.5 MeV时 46 Ti 的<Γ> =(5.9±4)keV; 52 Cr 13.5 MeV时<Γ> =(9.6±4)keV, 60在<Γ> =(6.9±4)keV super> Ni ,U = 12.9 MeV。通过将平均水平间距 D J π与平均水平宽度Γ J π使用涨落理论。通过此过程获得的能级密度方程式通常取决于透射系数,残留原子核中能级密度和复合核上的自旋截止参数。为了找到透射系数,局部光学模型参数(OMP)比全局参数更可取,这通常是(p,p)反应的情况,在某些情况下是(α,α)反应的情况,但是由于缺少中子的OMP我们求助于全球系统学。在本分析中,除了 27 Al 45 < italic> Sc 。这是由于参与实验的弹丸的动能在残余核中的激发较低,而且是由于在分析范围内 T n l < / inf T p l a l 。对于自旋截止,我们假设固体球对激励能量的依赖性为100%。 Al-Quraishi的能级密度参数用于评估其他能量范围内的能级密度,该能级密度用于通过数据库汇编中的波动测量获得的宽度。根据Al-Quraishi和Huang的费米气体形式论对 28 Si 46 Ti的能级密度汇编找到了合理的协议 52 Cr ,但是对于 60 Ni 的比较却有所不同,为此需要额外的测量澄清观察到的差异。最能描述数据的水平密度参数为 a = 3.57

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