How Robust is the N=34 Subshell Closure? First Spectroscopy of 52Ar
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creator | Liu, H.N Obertelli, A Doornenbal, P Bertulani, C. A Hagen, G Holt, J. D Jansen, G. R Morris, T. D Schwenk, A Stroberg, R Achouri, N Baba, H Browne, F Calvet, D Château, F Chen, S Chiga, N Corsi, A Cortés, M. L Delbart, A Gheller, J.-M Giganon, A Gillibert, A Hilaire, C Isobe, T Kobayashi, T Kubota, Y Lapoux, V Motobayashi, T Murray, I Otsu, H Panin, V Paul, N Rodriguez, W Sakurai, H Sasano, M Steppenbeck, D Stuhl, L Sun, Y. L Togano, Y Uesaka, T Wimmer, K Yoneda, K Aktas, O Aumann, T Chung, L.X Flavigny, F Franchoo, S Gašparić, I Gerst, R.-B Gibelin, J Hahn, K. I Kim, D Koiwai, T Kondo, Y Koseoglou, P Lee, J Lehr, C Linh, B.D Lokotko, T MacCormick, M Moschner, K Nakamura, T Park, S. Y Rossi, D Sahin, Eda Sohler, D Söderström, P.-A Takeuchi, S Törnqvist, H Vaquero, V Wagner, V Wang, S Werner, V Xu, X Yamada, H Yan, D Yang, Z Yasuda, M Zanetti, L |
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title | How Robust is the N=34 Subshell Closure? First Spectroscopy of 52Ar |
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