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新型硅胶-聚合胺树脂从氯化钴电解液中深度净化除铜 总被引:1,自引:0,他引:1
SP-C是一种新型硅胶-聚合胺复合材料树脂,对铜具有较好的选择吸附性能.本文研究了该树脂在模拟氯化钴电解液中深度净化除铜工艺.在Co2 ~80g/L、Cu2 0.5g/L~2.0g/L、pH 2~4、温度20℃~60℃的氯化钴电解液中,考察了该树脂对铜的吸附性能.结果表明,随料液pH增大以及温度升高,铜的交换容量增大;料液Cu2 浓度对交换容量影响较小;最佳吸附条件为:料液pH 4、接触时间30min,温度60℃.对比研究了盐酸、硫酸两种解析液,硫酸显示出更好的解析效果,最佳解析条件为H2SO4 2mol/L、解析接触时间40min.最佳工艺条件下,每亳升湿树脂对铜的工作交换容量及饱和交换容量分别0.439mol和0.508mol,铜的解析液峰值浓度为28g/L. 相似文献
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In the framework of the relativistic mean field theory including the hyperon-hyperon(YY) interactions,protoneutron stars with a weakly interacting light U boson are studied. The U-boson leads to the increase of the star maximum mass. The modification to the maximum mass by the U-boson with the strong YY interaction is larger than that with the weak YY interaction. The maximum mass of the protoneutron star is less sensitive to the U-boson than that of the neutron star. The inclusion of the U-boson narrows down the mass window for the hyperonized protoneutron stars. As g~2/μ~2 increases, the species of hyperons, which can appear in a stable protoneutron star decrease. The rotation frequency, the red shift, the momentum of inertia and the total neutrino fraction of PSR J1903-0327 are sensitive to the U-boson and change with g~2/μ~2 in an approximate linear trend. The possible way to constrain the coupling constants of the U-boson is discussed. 相似文献
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SP-C是一种新型硅胶-聚合胺复合材料树脂,对铜具有较好的选择吸附性能.本文研究了该树脂在模拟氯化钴电解液中深度净化除铜工艺.在Co2 ~80g/L,Cu2 0.5g/L~2.0g/L、pH2~4、温度20℃~60℃的氯化钴电解液中,考察了该树脂对铜的吸附性能.结果表明,随料液pH增大以及温度升高,铜的交换容量增大:料液Cu2 浓度对交换容量影响较小;最佳吸附条件为:料液pH 4、接触时间30min,温度60℃.对比研究了盐酸、硫酸两种解析液,硫酸显示出更好的解析效果,最佳解析条件为H2SO42mol/L、解析接触时间40min.最佳工艺条件下,每毫升湿树脂对铜的工作交换容量及饱和交换容量分别为0.439mol和0.508mol,铜的解析液峰值浓度为28g/L. 相似文献
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在相对论平均场理论(RMFT)框架内,使用GL91参数组结合超核数据和大质量中子星的观测数据限定超子标量耦合参数Xσ=0.59~1.0,用慢转近似计算了大质量中子星和前中子星的转动惯量。当Xσ从0.59增加到1.0,中子星(前中子星)的最大转动惯量增幅达89%(60%)。在同样的变化范围内,用Crab的观测数据,计算得到中子星(前中子星)的最大能量损失(dE/dt)的增幅为44%(25%),最大磁场增幅为48%(38%)。相比于前中子星,中子星的性质对超子参数更为敏感。当Xσ从0.59增加到1.0,PSR J0348+0432的转动惯量和dE/dt的增幅均为14%,而磁场减幅为10%。如果天文观测能够给出中子星转动惯量的上限,或者同时精确测量中子星的质量和转动惯量,能帮助人们进一步限定超子参数。In the framework of the relativistic mean field theory(RMFT) with GL91 cets, the momentum of inertia (I) of slowly rotating neutron stars is studied by perturbative approach. The scalar hyperon coupling should lie in the range of Xσ=0.59~1.0 to be compatible with massive neutron stars. As Xσ increases from 0.59 to 1.0, the maximum momentum of inertia(Imax) of neutron (protoneutron) stars increases by 89% (60%). According to the data of Crab, the maximum energy loss(dE/dt) of neutron (protoneutron) stars will increase by 44%(25%)and the maximum magnetic field (B) will increase by 48%(38%). I and dE/dt of PSR J0348+0432 both increase by 14%, while B decreases by 10% as Xσ increases from 0.59 to 1.0. So if the upper bound of I, or the accurate values of both the mass and I of neutron stars could be provided by the astronomical observations, the hyperon couplings should be further constrained in the future. 相似文献
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