978 resultados para 129-800
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20 0 4年曾报道过利用4 0 Ca + 92 Mo融合蒸发反应产生了近质子滴线新核素12 9Pm ,并首次观测到它 (EC + β+)衰变产生的能量为 99keV的γ射线 .为了进一步确认上述指认 ,以下提供了三方面的新证据 :1)在 16 4— 190MeV能量范围内测量了 99keV衰变γ射线的激发函数 ;2 )进行了交叉反应36 Ar + 96 Ru的实验 ,观察到了相同的 99keV衰变γ射线 ;3)用Woods SaxonStrutinsky方法计算了12 9Pm的核势能面 ,其基态自旋宇称被预言为 5 / 2 - ,所以12 9Pm的 (EC + β+)衰变有利于馈送到子核12 9Nd的 5 / 2 - 的低位态 ,这也与前期报道相符 .
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IEECAS SKLLQG
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报道了用高电荷态离子1 2 9Xe30 + (15 0keV)轰击金属Ni表面 ,激发的 2 0 0— 10 0 0nmNiⅠ和NiⅡ的特征光谱线的实验结果 .实验结果表明 :用电荷态足够高的离子作光谱激发源 ,无需很强的束流强度 (nA量级 ) ,便可有效地产生原子和离子的复杂组态间跃迁所形成的可见光波段的特征谱线 ,特别是NiⅠ和NiⅡ偶极禁戒的电四极跃迁E2和磁偶极跃迁M1的特征光谱线 .通过分析发现 ,在禁戒跃迁的谱线中 ,有些是电子组态相同而原子态不同的偶极禁戒跃迁光谱线而且NiⅡ的 6 84 84nm谱线较强
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通过重离子引起的融合蒸发反应 92 Mo (40 Ca ,p2n)合成了稀土区未知核素 12 9Pm ,并且配合氦喷嘴快速带传输系统利用X γ符合方法对它进行了首次鉴别 .实验观测到了经 12 9Pm的 (EC +β+ )衰变产生的对应于子核 12 9Nd中 5 2 -→ 1 2 -跃迁的一条 99keVγ线 .根据这条 99keVγ线的时间衰变曲线 ,提取出 12 9Pm的半衰期为 (2 .4± 0 .6 )s .
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介绍了近代物理研究所自行研制的新型HIRFL 80 0低温泵。对其抽速、低温冷凝板和屏蔽板的热负荷进行了具体的分析和计算。肯定了新型HIRFL 80 0低温泵的设计方案
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利用 10 2MeV16O6+束轰击同位素靶117Sn ,通过熔合蒸发 4n反应产生核素12 9Ce.由氦喷嘴快速带传输系统将反应产物送到低本底区 .通过化学分离来制备待测的Ce样品 ,与此同时用16O束轰击117Sn的两种相邻的同位素靶118Sn和116Sn ,并比较上述 3种反应中的产物来进一步区分元素Ce的不同的同位素 .结果一种半衰期为 4.1min的活性被鉴定为12 9Ce.基于X -γ -t和γ -γ -t符合测量 ,建议了包括 5 1条射线在内的12 9Ce的 (EC/ β+)衰变纲图 .其中 ,12 9Ce基态直接馈送到12 9La基态的份额 ( 2 6± 7) %是用观测到的12 9La衰变的 2 78.6keV的γ射线的生长和衰变曲线估计出来的 .另外还给出了用La Kα X射线和6 8.2keVγ射线开门的γ谱以及典型的衰变γ射线的时间谱
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Using the slow highly charged ions Xe-129(q+) (q = 25, 26, 27; initial kinetic T-0 <= 4.65 keV/a.u.) to impact Au surface, the Au atomic M alpha characteristic X-ray spectrum is induced. The result shows that as long as the charge state of projectile is high enough, the heavy atomic characteristic X-ray can be effectively excited even though the incident beam is very weak (nA magnitude), and the X-ray yield per ion is in the order of 10(-8) and increases with the kinetic energy and potential energy of projectile. By measuring the Au M alpha-X-ray spectra, Au atomic N-level lifetime is estimated at about 1.33x10(-18) s based on Heisenberg uncertainty relation.
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Highly oriented pyrolytic graphite (HOPG) samples were irradiated by Xe ions of initial kinetic energy of 3 MeV/u. The irradiations were performed at temperatures of 500 and 800 K. Scanning tunneling microscopy (STM) images show that the tracks occasionally have elongated structures under high-temperature irradiation. The track creation yield at 800 K is by three orders of magnitude smaller compared to that obtained during room-temperature irradiation. STM and Raman spectra show that amorphization occurs in graphite samples irradiated at 500 K to higher fluences, but not at 800 K. The obtained experimental results clearly reveal that the irradiation under high temperature causes track annealing.
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Nd-129 was produced by irradiation of an enriched target of Ru-96 with a Ar-36 beam and studied by using a helium-jet fast tape transport system in combination with X-gamma and gamma-gamma coincidence measurements. A 2.6s isomer of Nd-129 was observed for the first time and tentatively proposed to be the configuration of 1/2[411].
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We studied the characteristic X-ray spectra produced by the interaction of highly charged ions of X-129(q+) (q =25, 26, 27) with surface of metallic Mo. The experimental result shows that highly charged ions can excite the characteristic X-ray spectra of L-shell of Mo when the beam' s intensity is not more than 120 nA. The X-ray yield of single ion reaches a quantitative level of 10(-8) and increases with the increment of the ion' s kinetic energy and ionic charge (potential energy). By measuring the X-ray spectra of Mo-L alpha(1) the M-level lifetime of Mo atom is estimated by using Heisenberg uncertainty relation.