Structure of 136Sn and the Z = 50 magicity

The first excited state in the neutron-rich tin isotope Sn has been identified at 682(13) keV by measuring -rays in coincidence with the one proton removal channel from Sb. This value is higher than those known for heavier even-even isotones, indicating the shell closure. It compares well to the fir...

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Published in:Progress of theoretical and experimental physics Vol. 2014; no. 2; p. 23
Main Authors: Wang, He, Aoi, Nori, Takeuchi, Satoshi, Matsushita, Masafumi, Doornenbal, Pieter, Motobayashi, Tohru, Steppenbeck, David, Yoneda, Kenichiro, Baba, Hidetada, Dombrádi, Zsolt, Kobayashi, Kota, Kondo, Yosuke, Lee, Jenny, Liu, Hong-Na, Minakata, Ryogo, Nishimura, Daiki, Otsu, Hideaki, Sakurai, Hiroyoshi, Sohler, Dora, Sun, Ye-Lei, Tian, Zheng-Yang, Tanaka, Ryuki, Vajta, Zsolt, Yang, Zai-Hong, Yamamoto, Tetsuya, Ye, Yan-Lin, Yokoyama, Rin
Format: Journal Article
Language:English
Published: Oxford University Press 01-02-2014
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Summary:The first excited state in the neutron-rich tin isotope Sn has been identified at 682(13) keV by measuring -rays in coincidence with the one proton removal channel from Sb. This value is higher than those known for heavier even-even isotones, indicating the shell closure. It compares well to the first excited state of the lighter tin isotope Sn, which may suggest that the seniority scheme also holds for Sn. Our result confirms the trend of lower excitation energies of even-even tin isotopes beyond compared to the known values in between the two doubly magic nuclei Sn and Sn.
ISSN:2050-3911
2050-3911
DOI:10.1093/ptep/ptu003