Stability of the N=50 shell gap in the neutron-rich Rb, Br, Se, and Ge isotones

  1. Zhang, Y.H.
  2. Podolyàk, Zs.
  3. De Angelis, G.
  4. Gadea, A.
  5. Ur, C.
  6. Lunardi, S.
  7. Marginean, N.
  8. Rusu, C.
  9. Schwengner, R.
  10. Kröll, Th.
  11. Napoli, D.R.
  12. Menegazzo, R.
  13. Bazzacco, D.
  14. Farnea, E.
  15. Lenzi, S.
  16. Martinez, T.
  17. Axiotis, M.
  18. Tonev, D.
  19. Gelletly, W.
  20. Langdown, S.
  21. Regan, P.H.
  22. Valiente Dobon, J.J.
  23. Von Oertzen, W.
  24. Rubio, B.
  25. Quintana, B.
  26. Medina, N.
  27. Broda, R.
  28. Bucurescu, D.
  29. Ionescu-Bujor, M.
  30. Iordachescu, A.
  31. Show all authors +
Journal:
Physical Review C - Nuclear Physics

ISSN: 0556-2813

Year of publication: 2004

Volume: 70

Issue: 2

Type: Article

DOI: 10.1103/PHYSREVC.70.024301 GOOGLE SCHOLAR

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