Dependence of the cross sections for Ir isotopes on the values of Qgg in the heavy ion collision

¹⁹⁷Au were irradiated with 47 MeV/u ¹²C ions. Iridium was produced via the multinucleon transfer reactions in bombardments of ¹⁹⁷Au with ¹²C. and was separated radiochemically from Au and the mixture of the reaction products. The γ radioactivities of Ir isotopes were measured by using a HPGe detector. The production cross sections of Ir isotopes were determined from activities of Ir isotopes at the end of bombardment and the other relative data. It has been found that the cross sections for neutron-rich isotopes of iridium show an exponential dependence on the values of Q_gg. Our experimental results also demonstrate lack of correlation between the cross sections and Q_gg in the case of neutron-deficient isotopes of iridium. The fact can be explained from that neutron-rich isotopes of iridium were produced in the deep inelastic transfer reactions.     

新重丰中子同位素239Pa

用50MeV/u ¹⁸O离子同天然铀靶反应产生了新重丰中子同位素²³⁹Pa.用放射化学法从反应产物中分离Pa活性,通过观测²³⁹Pa及子体²³⁹U衰变所得到的结果显示:首次合成和鉴别了新重丰中子核素²³⁹Pa,并测定出²³⁹Pa的半衰期为106±30min.     

HIRFL上合成的第一个新核素—208Hg

本文简述在中科院近物所HIRFL上发现的第一个新核素208Hg的合成和鉴别,兼论利用HIRFL提供的中能重离子束开展远离β稳定线核素合成和衰变研究的优势、困难以及拟采用的物理和技术路线。 The synthesis and identification of the first discovered new nuclide 208Hg on HIRFL(Heavy Ion Research Facility of Lanzhou) were described. In this paper the superiorities, difficultiesas well as the physical and technical line about the synthesis and decay study for the nuclides far fromβ-stability line to be made at HIRFL were discussed.     

239Pa可能对天体物理研究产生一点影响

扼要介绍利用重计时对的核宇宙年代学来进行宇宙年龄估计的方法. 简单叙述²³⁹Pa的异常长的半衰期对于宇宙年龄估计的影响.     

175Er的衰变纲图

用14MeV中子照射天然Yb靶,通过¹⁷⁶Yb(n,2p)¹⁷⁵Er反应产生了新的重丰中子同位素¹⁷⁵Er,借助X-γ,γ-γ符合测量方法,首次鉴别出了¹⁷⁵Er,并测得其半衰期为(1.2±0.3)min.同时还观察到了¹⁷⁵Er衰变所发射的8条新γ射线,建立了¹⁷⁵Er的部分γ衰变纲图,从中指定了¹⁷⁵Tm的一个基态转动带.     

~(73)Br的衰变研究

以~(64)Zn(~(12)C,2np)~(73)Br反应得到~(73)Br,经过氦喷嘴传输系统和快速化学分离后进行了γ单谱、γ-γ,符合和角关联测量,得到了~(73)Br的27条γ射线能量和相对强度,其中102.1、137.2、166.2、249.0、345.5、363.8、381.5、385.7和390.2keV9条γ射线以及192.4、537.4和574.1keV 3条能级为本工作首次测得.建立了~(73)Br的衰变纲图,由logft值和角关联系数测量值推测了90.4keV能级的自旋.     

230Acβ延发裂变的观测

搜索了230Ac β延发裂变. 由60MeV/u18O离子照射232Th,通过多核子转移反应产生230Ra. 经放射化学分离和薄的230Raβ- 230 Ac源的制备,获得了108个230Ac原子. 该源对云母裂变径迹探测器曝光. 借助于所测的γ能谱和两个裂变事件,鉴别了β延发裂变核230Ac,得到了它的β延发裂变几率为(1.19±0.85)×10-8.     

重丰中子核237Th半衰期的测量

通过60MeV/u的¹⁸O离子束轰击天然铀靶,利用多核子转移反应并由放射化学分离方法准备了²³⁷Th的存在,测得它的半衰期为(4.69±0.60)min.这个新的值不仅与我们较早获得的(5.0±0.9)min值一致,而且提高了实验精度.     

新重丰中子同位素175Er的合成和γ衰变

用14MeV中子轰击天然镜靶,通过¹⁷⁶Yb(n,2p)¹⁷⁵Er反应,首次合成了新同位素¹⁷⁵Er.利用γ(X)谱学方法,对¹⁷⁵Er的活性进行了观测,发现了能量为76.5,120.9,123.7,128.5,227.3,234.0,281.4,1167.5keV半衰期为1.2±0.3min的八条新γ射线,并指定为¹⁷⁵Er的β-衰变.建立了¹⁷⁵Er的部分衰变纲图.     

266Bh的α衰变性质研究(英文)

报道了利用兰州重离子研究装置提供的26Mg重离子束流轰击243Am靶产生和鉴别已知超重核素266Bh的实验结果。利用转轮收集探测装置依靠母子核遗传关系通过观测Bh同位素与其子核Db和Lr之间的α-α关联事件来鉴别266Bh。实验中观测到266Bh的α能量为（9.03 ± 0.08）MeV， 与日本理化学研究所在合成113号元素中第一个衰变链中观测到266Bh的α能量为9.07 MeV相近。 266Bh的半衰期为0.66+0.59-0.26 s， 从实验得到的Qα也符合Z=107的Qα随中子数变化的系统性。The isotope of 266Bh was produced and identified definitely in bombardments of 243Am target with 162 MeV 26Mg ions at HIRFL. Identification was made by observation of correlated α particle decays between the Bh isotopes and their Db and Lr daughters using a rotating wheel system. The measured α energy for 266Bh is (9.03±0.08) MeV, and this value close to the 9.07 MeV for 266Bh observed in the first chain of element 113 at RIKEN. The half life of 266Bh is 0.66+0.59 -0.26 s. The Qα value derived from this experiment fits well into the general trend in a “Qα N systematics” for the isotopes with Z = 107.