Study of $$N=50$$ gap evolution around $$Z=32$$: new structure information for $${}^{82}$$Ge
-
Published:2023-07-11
Issue:7
Volume:59
Page:
-
ISSN:1434-601X
-
Container-title:The European Physical Journal A
-
language:en
-
Short-container-title:Eur. Phys. J. A
Author:
Thisse D.ORCID, Lebois M., Verney D., Wilson J. N., Jovančević N., Rudigier M., Canavan R., Etasse D., Adsley P., Algora A., Babo M., Belvedere K., Benito J., Benzoni G., Blazhev A., Boso A., Bottoni S., Bunce M., Chakma R., Cieplicka-Oryńczak N., Courtin S., Cortés M. L., Davies P., Delafosse C., Fallot M., Fornal B., Fraile L., Gjestvang D., Gottardo A., Guadilla V., Gerst R. -B., Häfner G., Hauschild K., Heine M., Henrich C., Homm I., Hommet J., Ibrahim F., Iskra Ł. W., Ivanov P., Jazrawi S., Korgul A., Koseoglou P., Kröll T., Kurtukian-Nieto T., Meur L. Le, Leoni S., Ljungvall J., Lopez-Martens A., Lozeva R., Matea I., Miernik K., Nemer J., Oberstedt S., Paulsen W., Piersa-Silkowska M., Poklepa W., Popovitch Y., Porzio C., Qi L., Ralet D., Regan P. H., Reygadas-Tello D., Rezynkina K., Sánchez-Tembleque V., Siem S., Schmitt C., Söderström P. -A., Solak K., Sürder C., Tocabens G., Vedia V., Warr N., Wasilewska B., Wiederhold J., Yavahchova M., Zeiser F., Ziliani S.
Funder
Narodowe Centrum Nauki Department for Business, Energy and Industrial Strategy, UK Government Science and Technology Facilities Council University of Surrey UK Nuclear Data Network Deutsche Forschungsgemeinschaft Romanian Ministry of Research, Innovation and Digitalization Bundesministerium für Bildung und Forschung European Union - HORIZON2020
Publisher
Springer Science and Business Media LLC
Subject
Nuclear and High Energy Physics
Reference33 articles.
1. Ch. Engelmann, F. Ameil, P. Armbruster, M. Bernas, S. Czajkowski, Ph. Dessagne, C. Donzaud, H. Geissel, A. Heinz, Z. Janas, C. Kozhuharov, Ch. Miehe, G. Munzenberg, M. Pfutzner, C. Rohl, W. Schwab, C. Stephan, K. Summerer, L. Tassan-Got, B. Voss, Production and identification of heavy Ni isotopes: evidence for the doubly magic nucleus $$^{78} _{28}$$Ni. Z. Phys. A 352, 351 (1995) 2. R. Taniuchi, C. Santamaria, P. Doornenbal, A. Obertelli, K. Yoneda, G. Authelet, H. Baba, D. Calvet, F. Château, A. Corsi, A. Delbart, J.-M. Gheller, A. Gillibert, J.D. Holt, T. Isobe, V. Lapoux, M. Matsushita, J. Menéndez, S. Momiyama, T. Motobayashi, M. Niikura, F. Nowacki, K. Ogata, H. Otsu, T. Otsuka, C. Péron, S. Péru, A. Peyaud, E.C. Pollacco, A. Poves, J.-Y. Roussé, H. Sakurai, A. Schwenk, Y. Shiga, J. Simonis, S.R. Stroberg, S. Takeuchi, Y. Tsunoda, T. Uesaka, H. Wang, F. Browne, L.X. Chung, Z. Dombradi, S. Franchoo, F. Giacoppo, A. Gottardo, K. Hadyńska-Klęk, Z. Korkulu, S. Koyama, Y. Kubota, J. Lee, M. Lettmann, C. Louchart, R. Lozeva, K. Matsui, T. Miyazaki, S. Nishimura, L. Olivier, S. Ota, Z. Patel, E. Şahin, C. Shand, P.-A. Söderström, I. Stefan, D. Steppenbeck, T. Sumikama, D. Suzuki, Z. Vajta, V. Werner, J. Wu, Z.Y. Xu, $${}^{78}$$Ni revealed as a doubly magic stronghold against nuclear deformation. Nature 569(7754), 53–58 (2019) 3. J. Hakala, S. Rahaman, V.-V. Elomaa, T. Eronen, U. Hager, A. Jokinen, A. Kankainen, I.D. Moore, H. Penttilä, S. Rinta-Antila, J. Rissanen, A. Saastamoinen, T. Sonoda, C. Weber, J. Äystö, Evolution of the N=50 Shell Gap Energy towards $$^{78}\rm Ni $$. Phys. Rev. Lett. 101, 052502 (2008) 4. S. Baruah, G. Audi, K. Blaum, M. Dworschak, S. George, C. Guénaut, U. Hager, F. Herfurth, A. Herlert, A. Kellerbauer, H.-J. Kluge, D. Lunney, H. Schatz, L. Schweikhard, C. Yazidjian, Mass measurements beyond the major $$r$$-process waiting point $$^{80}\rm Zn $$. Phys. Rev. Lett. 101, 262501 (2008) 5. Y. H. Zhang, Zs. Podolyàk, G. de Angelis, A. Gadea, C. Ur, S. Lunardi, N. Marginean, C. Rusu, R. Schwengner, Th. Kröll, D. R. Napoli, R. Menegazzo, D. Bazzacco, E. Farnea, S. Lenzi, T. Martinez, M. Axiotis, D. Tonev, W. Gelletly, S. Langdown, P. H. Regan, J. J. Valiente Dobon, W. von Oertzen, B. Rubio, B. Quintana, N. Medina, R. Broda, D. Bucurescu, M. Ionescu-Bujor, A. Iordachescu, Stability of the N=50 shell gap in the neutron-rich Rb, Br, Se, and Ge isotones. Phys. Rev. C, 70, 024301 (2004)
|
|