Magicity versus Superfluidity around O28 viewed from the Study of F30

Author:

Kahlbow J.12ORCID,Aumann T.134,Sorlin O.5,Kondo Y.6,Nakamura T.6,Nowacki F.7,Revel A.58,Achouri N. L.8,Al Falou H.9,Atar L.1,Baba H.2,Boretzky K.3,Caesar C.13,Calvet D.10,Chae H.11,Chiga N.2,Corsi A.10,Delaunay F.8,Delbart A.10,Deshayes Q.8,Dombrádi Z.12,Douma C. A.13,Elekes Z.12,Gašparić I.142,Gheller J.-M.10,Gibelin J.8,Gillibert A.10,Harakeh M. N.313,Hirayama A.6,Holl M.13,Horvat A.13,Horváth Á.15,Hwang J. W.16,Isobe T.2,Kalantar-Nayestanaki N.13,Kawase S.17,Kim S.16,Kisamori K.2,Kobayashi T.18,Körper D.3,Koyama S.19,Kuti I.12,Lapoux V.10,Lindberg S.20,Marqués F. M.8,Masuoka S.21,Mayer J.22,Miki K.23,Murakami T.24,Najafi M.13,Nakano K.17,Nakatsuka N.24,Nilsson T.20,Obertelli A.10,Orr N. A.8,Otsu H.2,Ozaki T.6,Panin V.2,Paschalis S.1,Rossi D. M.13,Saito A. T.6,Saito T.19,Sasano M.2,Sato H.2,Satou Y.16,Scheit H.1,Schindler F.1,Schrock P.21,Shikata M.6,Shimada K.6,Shimizu Y.2,Simon H.3,Sohler D.12,Stuhl L.252,Takeuchi S.6,Tanaka M.26,Thoennessen M.23,Törnqvist H.13,Togano Y.6,Tomai T.6,Tscheuschner J.1,Tsubota J.6,Uesaka T.2,Wang H.2,Yang Z.2,Yasuda M.6,Yoneda K.2,

Affiliation:

1. Technische Universität Darmstadt

2. RIKEN Nishina Center

3. GSI Helmholtzzentrum für Schwerionenforschung

4. Helmholtz Forschungsakademie Hessen für FAIR

5. Grand Accélérateur National d’Ions Lourds (GANIL)

6. Tokyo Institute of Technology

7. Université de Strasbourg

8. Université de Caen Normandie

9. Lebanese University

10. Université Paris-Saclay

11. IBS

12. HUN-REN Institute for Nuclear Research

13. University of Groningen

14. Ruđer Bošković Institute

15. Eötvös Loránd University

16. Seoul National University

17. Kyushu University

18. Tohoku University

19. Unversity of Tokyo

20. Chalmers Tekniska Högskola

21. University of Tokyo

22. Universität zu Köln

23. Michigan State University

24. Kyoto University

25. Institute for Basic Science

26. Osaka University

Abstract

The neutron-rich unbound fluorine isotope F2130 has been observed for the first time by measuring its neutron decay at the SAMURAI spectrometer (RIBF, RIKEN) in the quasifree proton knockout reaction of Ne31 nuclei at 235MeV/nucleon. The mass and thus one-neutron-separation energy of F30 has been determined to be Sn=472±58(stat)±33(sys)keV from the measurement of its invariant-mass spectrum. The absence of a sharp drop in Sn(F30) shows that the “magic” N=20 shell gap is not restored close to O28, which is in agreement with our shell-model calculations that predict a near degeneracy between the neutron d and fp orbitals, with the 1p3/2 and 1p1/2 orbitals becoming more bound than the 0f7/2 one. This degeneracy and reordering of orbitals has two potential consequences: O28 behaves like a strongly superfluid nucleus with neutron pairs scattering across shells, and both F29,31 appear to be good two-neutron halo-nucleus candidates. Published by the American Physical Society 2024

Funder

Deutsche Forschungsgemeinschaft

Technische Universität Darmstadt

GSI Helmholtzzentrum für Schwerionenforschung

RIKEN

Tokyo Institute of Technology

Japan Society for the Promotion of Science

Agence Nationale de la Recherche

Helmholtz International Center for FAIR

Hrvatska Zaklada za Znanost

National Science Foundation

Institute for Basic Science

Ministry of Education, Culture, Sports, Science and Technology

National Research, Development and Innovation Fund of Hungary

Franco-Japanese LIA-International Associated Laboratory for Nuclear Structure Problems

Publisher

American Physical Society (APS)

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