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XU Xing, WANG Meng, ZHANG Yuhu, SHUAI Peng, XU Hushan, TU Xiaolin, ZHOU Xiaohong, CHEN Ruijiu, CHEN Xiangcheng, FU Chaoyi, GE Zhuang, HUANG Wenjia, LAM Yek-wah, LI Hongfu, LIU Junhao, SUN Mingze, XING Yuanming, YAN Xinliang, ZENG Qi, ZHANG Peng, XIAO Guoqing, ZHAN Wenlong. Shell Evolution Study for New Magic Number N =32 via Isochronous Mass Spectrometry[J]. Nuclear Physics Review, 2016, 33(2): 156-159. DOI: 10.11804/NuclPhysRev.33.02.156
Citation: XU Xing, WANG Meng, ZHANG Yuhu, SHUAI Peng, XU Hushan, TU Xiaolin, ZHOU Xiaohong, CHEN Ruijiu, CHEN Xiangcheng, FU Chaoyi, GE Zhuang, HUANG Wenjia, LAM Yek-wah, LI Hongfu, LIU Junhao, SUN Mingze, XING Yuanming, YAN Xinliang, ZENG Qi, ZHANG Peng, XIAO Guoqing, ZHAN Wenlong. Shell Evolution Study for New Magic Number N =32 via Isochronous Mass Spectrometry[J]. Nuclear Physics Review, 2016, 33(2): 156-159. DOI: 10.11804/NuclPhysRev.33.02.156
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Shell Evolution Study for New Magic Number N =32 via Isochronous Mass Spectrometry

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  • Recent results and progress of mass measurements of neutron-rich nuclei utilizing Isochronous Mass Spectrometry (IMS) based on the HIRFL-CSR complex at Lanzhou are reported. The nuclei of interest were produced through projectile fragmentation of primary 86Kr ions at a realistic energy of 460.65 MeV/u. After in-flight separation by the fragment separator RIBLL2, the fragments were injected and stored in the experimental storage ring CSRe, and their masses were determined from measurements of their revolution times. The re-determined masses were compared and evaluated with other mass measurements, and the impact of these evaluated masses on the shell evolution study is discussed.
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