Determination of the Astrophysically Relevant ~6Li(n,γ)~7Li Cross Sections from the ~7Li(~6Li,~7Li)~6Li Elastic-Transfer Reaction

Angular distributions for the ~7(Li)(~6(Li),~7(Li))~6(Li) Li elastic-transfer reaction have been measured with the Q3D magnetic spectrograph at the HI-13 tandem accelerator of Beijing, China. The neutron spectroscopic factors of 7Li are derived by comparing the calculated differential cross sections, which are obtained through the distorted-wave Born approximation (DWBA) calculation, to the experimental data. And these spectroscopic factors are then used to deduce the direct capture cross sections in 6Li(n,γ)7 Li at energies of astrophysical relevance.     

Measurement of ~(25)Mg(~7Li,~6He)~(26)Al Angular Distribution

<正>In order to study the 58keV resonance in ~(25)Mg(p,γ)~(26)Al reaction,the measurement of the~(25)Mg(~7Li,~6 He)~(26) Al*_(6.364)reaction was carried out by using a 31.5 MeV ~7Li beam from the HI-13tandem accelerator,Beijing.The 200 enA 7Li beam impinged on ~(25)MgO,~(24)MgO and ~(12)C target,     

~2H(~6He,~7Li)n反应角分布和~7Li的质子谱因子

在中国原子能科学研究院HI-13串列加速器次级束流线上,使用6He次级束首次测量了质心系能量为9.1 MeV的2H(6He,7Li)n反应角分布,并用扭曲波波恩近似(DWBA)进行理论分析,导出了7Li的质子谱因子为0.40±0.02。     

Measurement of ~7Be(d,~3He)~6Li Angular Distribution

正The baryon density can be deduced from the Wilkinson microwave anisotropy probe(WMAP),and the ~6Li and ~7Li abundance can then be computed by the standard Big Bang nucleosynthesis model~([1]).Surprisingly,the primordial ~7Li abundances of astronomical observations are only     

Measurement of One Proton Transfer Reaction ~(208)Pb(~7Li,~6He)~(209)Bi in Deep Sub-barrier Region

<正>Due to the limit of the intensity and quality of the radioactive ion beam(RIB),it is a difficult task to extract the optical model potentials(OMPs)of halo nuclear systems directly from the elastic scattering measurement.In view of this fact,the transfer reaction was tried to be used as an alternative method to extract and stud-     

~7Be(d,~3He)~6Li and Its Effect on Primordial Lithium Abundance

<正>The ~6Li,~7Li abundance can be computed by the[standard Big Bang nucleosynthesis model[1].Surprisingly,the primordial ~7Li abundances of astronomical observations are only about 1/3of the model calculation,while the primordial ~6Li abundances observed by astronomical observa-     

Isospin Distribution of Fragments in Reaction ~(96)Ru ~(96)Ru, ~(96)Ru ~(96)Zr,~(96)Zr ~(96)Ru,and ~(96)Zr ~(96)Zr at Beam Energy 400 AMeV

The isospin distribution of particles and fragments in collisions 96Ru 96Ru, 96Ru 96Zr, 96Zr 96Ru, and 96Zr 96Zr at beam energy 400 AMeV is studied with isospin dependent QMD model. We find the rapidity distribution of difference between neutron-proton number in neutron rich nucleus-nucleus collisions at intermediate energies is sensitive to the isospin dependent part of nuclear potential. The study of the N/Z ratio of nucleons, light charged particles (LCP) and intermediate mass fragments (IMF) shows that the isospin dependent part of nuclear potential drives IMF to be more isospin symmetric and emitted nucleons to be more neutron rich. We also study the time evolution of the isospin distribution     

Model-based cross section calculations on production of ~(43,34)Sc,~(45)Ti,~(51)Cr,~(54)Mn,and ~(55)Fe radioisotopes

A cross section database on excitation functions of reactions produced by charged particles is essential for many areas of nuclear research. Particularly, accurate knowledge on nuclear cross sections for the cyclotron production of radioisotopes is very important for nuclear medicine. In the present paper, the cross section calculations for the production of~(43),~(34)Sc,~(45)Ti,~(51)Cr,~(54)Mn, and~(55) Fe radioisotopes were carried out by the use of ALICE/ASH code using the Fermi gas model, Kataria Ramamurthy Fermi gas model, and superfluid nuclear model for nuclear level density. Thereby, these model calculations were compared with the available measured data.     

我国膳食中~(90)Sr、~(137)Cs、~(226)Ra、~(228)Ra、~(210)Pb 和~(210)Po含量及其所致内照射剂量

作为1990年全国总膳食调查的放射性物质部分,本文报道了组成我国膳食的各类食品中~(90)Sr、~(137)Cs、~(226)Ra、~(228)Ra、~(210)Pb 和~(210)Po 含量的测定结果;按调查所得膳食组成和食品中核素含量,估算了我国居民(成年男子)当前这些核素经食入所致年摄入量和待积有效剂量当量。结果表明,每年食入所致总待积有效剂量当量约为0.24 mSv,贡献较大的食品是蔬菜、水产品和谷类,贡献较大的核素为~(210)Pb、~(210)Po 和~(228)Ra。这些结果更新了我国膳食中这些核素的资料,补充了来自饮水的数据。文中还讨论了我国膳食组成的地区差异及其对居民摄入量和所致内照射剂量的影响。     

Global Phenomenological Optical Model Potential for ~(6,7,8)Li Projectiles

<正>The optical model is one of the most fundamental theoretical models in nuclear reaction theory.The key point of the optical model is how to give the optical model potential.The global phenomenological optical model potential for ~6Li,~7Li,~8Li projectiles are obtained by simultaneously fitting the experimental data of the reaction cross sections and elastic scattering     

Study of Optical Potential of Weakly Bound System ~7Li+~(63)Cu

正The angular distributions of the elastic scattering of weakly bound nuclear systems of~7Li+~(63)Cu were measured at energy around the Coulomb barrier,to extract and study the optical model potential(OMP)of this weakly bound system.For the weakly-bound nucleus ~7Li,there are large amount of elastic scattering data.However,     

^176Hf（n,2n）^175Hf和^185Re（n,2n）^184Re^m,g反应截面研究

用中国原子能科学研究院ＨＩ－１３串列加速器,高压倍加器和北京大学４．５ＭＶ静电加速器分别获得能量为１０－１２,１４和１８ＭｅＶ的中子,了＾１７６Ｈｆ（ｎ,２ｎ）和＾１８５Ｒｅ（ｎ,２ｎ）的反应堆面,并与现有的实验数据作了比较,初步搞清了分歧的主要原因和激发函数的走向。     

~(107)Ag(d,2n)~(107)Cd和~(109)Ag(d,2n)~(109)Cd反应的激发函数

用13.4MeV的氘束轰击天然银迭靶,银箔前后用铝箔作捕集减能膜。实验确定了~(107)Ag(d,2n)~(107)Cd和~(109)Ag(d,2n)~(109)Cd反应的激发函数,同时作了理论计算。由结果可见,实验值与理论值吻合得很好。     

Differential Cross Section Measurement for ~6Li(n,t)~4He Reaction at 3.67 and 4.42 MeV

Using a gridded ionization chamber, the differential cross sections for ~6Li(n,t)~4He reaction were measured at 3.67 and 4.42 MeV. The neutrons were produced with D(d,n)~3He reaction. Absolute neutron flux was determined through ~(238)U(n,f) and H(n,p) reaction. The result at 3.67 MeV is almost 90 degree symmetry but it is obviously forward peaked at 4.42 MeV in the center of mass system.     

Product yields for the photofission of ~(232)Th,~(234,238)U,~(237)Np,and ~(239,240,242)Pu actinides at various incident photon energies

Photofission fragments mass yield for~(232)Th,~(234;238) U,~(237) Np, and~(239;240;242) Pu isotopes are investigated.The calculations are done using a developed approach based on Gorodisskiy's phenomenological formalism. The Gorodisskiy's method is developed to be applied for the neutron-induced fission. Here we revised it for application to photofission. The effect of emitted neutron prior to fission on the fission fragment mass yields has also been studied. The peak-to-valley ratio is extracted for the240 Pu isotope as a function of energy. Obtained results of the present formalism are compared with the available experimental data. Satisfactory agreement is achieved between the results of present approach and the experimental data.     

岩石中稀土元素中子活化分析时Na、Sc、Fe Cr等干扰元素的去除

稀土元素的分离、分析,在地球化学、宇宙化学、环境化学等学科中起着极为重要的作用。近年来,国内外利用高分辨率γ谱仪中子活化分析法测定岩石中稀土元素的报道很多,虽然对放射化学分析流程都在不同程度上有所改进,但对超基性岩石中大量存在的~(24)Na、~(46)Sc、~(59)Fe和~(51)Cr等核素的去除,解决被测元素γ谱之间相互干扰(包括重峰干扰和康普顿本底干扰)     

^179Hf（n,2n）^178Hf^m2和^209Bi（n,2n）^208Bi反应截面的测量

用活化法测量相对于~(93)Nb(n,2n)~(92)Nb~m反应的~(179)Hf(n,2n)~(178)Hf~(m2)的反应截面和相对于~(27)Al(n,2n)~(24)Na反应的~(209)Bi(n,2n)~(208)Bi的反应截面。在中子能量为14.4 MeV处~(179)Hf(n,2n)~(178)Hf~(m2)反应的测量截面为(6.04±0.32)×10~(-31)m~2。在中子能量为14.6 MeV处~(209)Bi(n,2n)~(208)Bi反应的测量截面为(2279±173)×10~(31)m~2。在这些测量中,中子能量是用~(90)Zr(n,2n)~(89)Zr~(m+8)反应和~(93)Nb(n,2n)~(92)Nb~m反应的截面比法测定的。     

武汉市空气中~(238)U、~(226)Ra、~(232)Th放射性浓度估算

本文报道武汉市空气中~(238)U、~(226)Ra、~(232)Th 放射性浓度的估算结果。空气中~(238)U、~(226)Ra、~(232)Th 的放射性浓度是根据地面空气中铀、镭、钍的主要天然来源是土壤粒子的再悬浮的假定,通过调查测量武汉市土壤中天然放射性核素含量和空气中含尘量,经计算后确定的。我们于1984年4—10月在武汉地区采集了60个土壤样品,调查测量了土壤中天然放射性核素含量,并根据在1981—1985年间采集的7346个空气粉尘样品测得的空气中含尘量,估算出武汉市空气中~(238)U、~(226)Ra 和~(232)Th 放射性浓度的五年平均值分别为24.0、18.9和28.7nBq/L。五年中以1983年的平均值最高,分别为30.4、23.9和36.2nBq/L。以1984和1985年的数据为例,空气中~(238)U、(226)Ra、~(232)Th 放射性浓度呈明显的季节性变化,两年中均以冬季为最高,夏季最低。在武汉市六个城区中,空气中~(238)U、~(226)Ra、~(232)Th 的放射性浓度,以青山区最高,武昌区最低。     

人骨骼中~(228)Th、~(230)Th和~(232)Th含量的同时测定

本文介绍了用α谱仪同时测定人骨骼中~(228)Th、~(230)Th和~(232)Th含量的方法。样品用浓 HNO_3和 H_2O_3湿灰化,草酸钙共沉淀载带、CL-5208萃淋树脂和743阳离子交换树脂联合分离后,电沉积制源,在低温半导体α谱仪上测量。该方法对~(234)Th的全程回收率为95.0±1.7%,对铀和镭的去污系数分别为6.3×10~4和1.5×10~3,对~(228)Th、~(230)Th、~(232)Th 的探测下限分别为0.432、0.135和0.108Bq/kg(鲜重)。