~(12)C~(6+)离子辐射对细胞存活增殖及模拟失重和辐射对家蚕卵发育的影响

目的:观察重离子辐射后人骨肉瘤细胞MG-63、人胚胎皮肤成纤维细胞ESF-1和人胚胎肝正常细胞HEL-1的生存和增殖情况,及重离子辐射和模拟失重环境处理后家蚕卵的孵化和发育情况,初步探讨重离子辐射对细胞及复合环境对家蚕卵的一些生物学效应.方法:利用超导磁体模拟失重环境,利用重离子加速器产生12C6+离子,用不同剂量辐射细胞和家蚕卵,检测在重离子辐射后细胞的存活和克隆形成能力及复合条件下家蚕卵的发育情况.结果:HEL-1细胞在0.1Gy时存活率已经开始降低,且随辐射剂量的增大这种影响也增加,到1.5Gy时存活率降低50%.ESF-1细胞在1.5Gy时存活率下降约20%,但辐射对骨肉瘤MG-63细胞的存活率影响不大.HEL-1和ESF-1细胞受到0.1Gy的辐射后克隆形成能力就明显降低90.2%和79.1%,而MG-63细胞一直保持较高的克隆形成率,直到1.5Gy时迅速降低75%.家蚕的出蚁率随辐射剂量的增大而降低,到30Gy时出蚁率降到2.22%.当辐射剂量为0～10Gy时,家蚕卵在两种不同重力条件下的孵化率没有明显差异.但当辐射剂量增加到15,20和30Gy时,失重环境明显促进了家蚕卵的孵化.另外,失重环境下家蚕卵的孵化时间比正常条件下缩短约3d左右.同时,高剂量的辐射处理会延迟家蚕幼虫的生长.结论:重离子辐射降低了细胞的存活和增殖能力,同时影响了家蚕从受精卵到幼虫的发育,降低了出蚁率.失重环境可以缩短家蚕卵的孵化时间

JUNO Sensitivity on Proton Decay p→νˉK+p\to \bar\nu K^+ Searches

The Jiangmen Underground Neutrino Observatory (JUNO) is a large liquid scintillator detector designed to explore many topics in fundamental physics. In this paper, the potential on searching for proton decay in $p\to \bar\nu K^+$ mode with JUNO is investigated.The kaon and its decay particles feature a clear three-fold coincidence signature that results in a high efficiency for identification. Moreover, the excellent energy resolution of JUNO permits to suppress the sizable background caused by other delayed signals. Based on these advantages, the detection efficiency for the proton decay via $p\to \bar\nu K^+$ is 36.9% with a background level of 0.2 events after 10 years of data taking. The estimated sensitivity based on 200 kton-years exposure is $9.6 \times 10^{33}$ years, competitive with the current best limits on the proton lifetime in this channel

JUNO sensitivity on proton decay p → ν K + searches*

The Jiangmen Underground Neutrino Observatory (JUNO) is a large liquid scintillator detector designed to explore many topics in fundamental physics. In this study, the potential of searching for proton decay in the $p\to \bar{\nu} K^+$ mode with JUNO is investigated. The kaon and its decay particles feature a clear three-fold coincidence signature that results in a high efficiency for identification. Moreover, the excellent energy resolution of JUNO permits suppression of the sizable background caused by other delayed signals. Based on these advantages, the detection efficiency for the proton decay via $p\to \bar{\nu} K^+$ is 36.9% ± 4.9% with a background level of $0.2\pm 0.05({\rm syst})\pm$$0.2({\rm stat})$ events after 10 years of data collection. The estimated sensitivity based on 200 kton-years of exposure is $9.6 \times 10^{33}$ years, which is competitive with the current best limits on the proton lifetime in this channel and complements the use of different detection technologies