Effect of dead carbon on the C-14 dating of the speleothem

IEECAS SKLLQG

洞穴次生碳酸盐中“死碳”对~(14)C法测年的影响

IEECAS SKLLQG

15.14 MeV/u ~(136)Xe离子引起的单粒子效应(英文)

研究了 1 5.1 4MeV/u136 　Xe离子在不同批次的 3 2k× 8bits静态存储器中所引起的单粒子效应 .获得了单粒子翻转和单粒子闭锁截面与入射角度的依赖关系 .将单粒子效应截面与灵敏区中沉积的能量相联系 ,而不是线性能量转移(LET)值 .估计了灵敏体积的深度和死层的厚度 .

28.7MeV/u的~(14,16,18)O+~(7,9)Be反应中的同位素分布研究

用同位旋相关的Boltzmann Langevin方程研究了在入射能量为2 8 7MeV/u下 ,不同弹核 14O ,16 O和 18O轰击不同靶核 7Be和 9Be的反应 ,计算了生成碎片的产生截面 ,发现用丰中子 (缺中子 )炮弹或丰中子 (缺中子 )靶进行反应 ,所得到的产物均有丰中子 (缺中子 )的碎片出现 .同位素分布宽度和峰位与入射体系密切相关 ,产生碎片的电荷数越接近入射弹核的电荷数 ,则同位素分布的宽度越大 ,峰位偏离β稳定线值越远 ,其同位旋效应越明显 .

低能~(14)N~(+1)离子微剂量学研究

叙述了用圆柱型流气式组织等效正比计数器测定用Ｋ－２００ｋＶ低能重离子加速器加速的能量为６６—１１９ｋｅＶ的１４Ｎ+１离子穿过４μｍ厚的ＰＥＴ（Ｃ８０Ｈ８Ｏ４）薄膜后的微剂量谱、径向剂量分布等微剂量学参数。测定了穿过４μｍ厚的ＰＥＴ（Ｃ８０Ｈ８Ｏ４）薄膜后的１４Ｎ＋１离子的单次事件剂量平均比能马Ｚ１Ｄ随离子能量和强度的变化曲线。并与用ＴＩＲＭ９２Ｍｏｎｔｅ　Ｃａｒｌｏ程序计算的１４Ｎ＋１离子在ＰＥＴ材料中的射程一能量曲线进行了比较和讨论。

Measurement of the inelastic branch of the O-14(alpha, p)F-17 reaction: Implications for explosive burning in novae and x-ray bursters

A measurement of the inelastic component of the key astrophysical resonance in the 14O(α,p)17F reaction for burning and breakout from hot carbon-nitrogen-oxygen (CNO) cycles is reported. The inelastic component is found to be comparable to the ground-state branch and will enhance the 14O(α,p)17F reaction rate. The current results for the reaction rate confirm that the 14O(α,p)17F reaction is unlikely to contribute substantially to burning and breakout from the CNO cycles under novae conditions. The reaction can, however, contribute strongly to the breakout from the hot CNO cycles under the more extreme conditions found in x-ray bursters.

A new axial injection beam line of the SFC

A new axial beam injection system is designed and being constructed at the HIRFL. It consists of 2 GLASSER lenses, 1 dipole, 5 quadrupoles and 3 solenoids. There are two beam line branches for 14.5GHz ECR ion source and 18.5GHz super conducting ECR ion source. Both transverse and longitudinal beam optics are improved in contrast with the old one. The layout, beam optics calculation results and further improved design are given.

Measurement of the inelastic branch of the stellar O-14(alpha,p)F-17 reaction occurring in the explosive burning in Novae and X-ray busters

The inelastic component of the key astrophysical resonance (1(-), E-x=6.15 MeV) in the O-14(alpha,p)F-17 reaction has been studied by using the resonant scattering of F-17+p. The experiment was done at REX-ISOLDE CERN with the Miniball setup. The thick target method in inverse kinematics was utilized in the present experiment where a 44.2 MeV F-17 beam bombarded a similar to 40 mu m thick (CH2)(n) target. The inelastic scattering protons in coincidence with the de-excited 495 keV gamma rays have been clearly seen and they are from the inelastic branch to the first excited state in F-17 following decay of the 1(-) resonance in Ne-18. Some preliminary results are reported.