Physics Letters B (Mar 2020)

Restoration of the natural E(1/21+) - E(3/21+) energy splitting in odd-K isotopes towards N = 40

  • Y.L. Sun,
  • A. Obertelli,
  • P. Doornenbal,
  • C. Barbieri,
  • Y. Chazono,
  • T. Duguet,
  • H.N. Liu,
  • P. Navrátil,
  • F. Nowacki,
  • K. Ogata,
  • T. Otsuka,
  • F. Raimondi,
  • V. Somà,
  • Y. Utsuno,
  • K. Yoshida,
  • N. Achouri,
  • H. Baba,
  • F. Browne,
  • D. Calvet,
  • F. Château,
  • S. Chen,
  • N. Chiga,
  • A. Corsi,
  • M.L. Cortés,
  • A. Delbart,
  • J.-M. Gheller,
  • A. Giganon,
  • A. Gillibert,
  • C. Hilaire,
  • T. Isobe,
  • T. Kobayashi,
  • Y. Kubota,
  • V. Lapoux,
  • T. Motobayashi,
  • I. Murray,
  • H. Otsu,
  • V. Panin,
  • N. Paul,
  • W. Rodriguez,
  • H. Sakurai,
  • M. Sasano,
  • D. Steppenbeck,
  • L. Stuhl,
  • Y. Togano,
  • T. Uesaka,
  • K. Wimmer,
  • K. Yoneda,
  • O. Aktas,
  • T. Aumann,
  • L.X. Chung,
  • F. Flavigny,
  • S. Franchoo,
  • I. Gašparić,
  • R.-B. Gerst,
  • J. Gibelin,
  • K.I. Hahn,
  • D. Kim,
  • T. Koiwai,
  • Y. Kondo,
  • P. Koseoglou,
  • J. Lee,
  • C. Lehr,
  • B.D. Linh,
  • T. Lokotko,
  • M. MacCormick,
  • K. Moschner,
  • T. Nakamura,
  • S.Y. Park,
  • D. Rossi,
  • E. Sahin,
  • D. Sohler,
  • P.-A. Söderström,
  • S. Takeuchi,
  • H. Törnqvist,
  • V. Vaquero,
  • V. Wagner,
  • S. Wang,
  • V. Werner,
  • X. Xu,
  • H. Yamada,
  • D. Yan,
  • Z. Yang,
  • M. Yasuda,
  • L. Zanetti

Journal volume & issue
Vol. 802

Abstract

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We report on the first γ-ray spectroscopy of 51,53K produced via the 52,54Ca(p,2p) reactions at ∼250 MeV/nucleon. Unambiguous final-state angular-momentum assignments were achieved for beam intensities down to few particles per second by using a new technique based on reaction vertex tracking combined with a thick liquid-hydrogen target. Through γ-ray spectroscopy and exclusive parallel momentum distribution analysis, 3/2+ ground states and 1/2+ first excited states in 51,53K were established quantifying the natural ordering of the 1d3/2 and 2s1/2 proton-hole states that are restored at N = 32 and 34. State-of-the-art ab initio calculations and shell-model calculations with improved phenomenological effective interactions reproduce the present data and predict consistently the increase of the E(1/21+) - E(3/21+) energy differences towards N = 40. Keywords: Spectroscopy, Shell evolution, 51K, 53K