Back to Search Start Over

94 β -Decay Half-Lives of Neutron-Rich Cs 55 to Ho 67 : Experimental Feedback and Evaluation of the r -Process Rare-Earth Peak Formation

Authors :
Wu, J.
Nishimura, S.
Lorusso, G.
Möller, P.
Ideguchi, E.
Regan, P.-H.
Simpson, G.S.
Söderström, P.-A.
Walker, P.M.
Watanabe, H.
Xu, Z.
Baba, H.
Browne, F.
Daido, R.
Doornenbal, P.
Fang, Y. F.
Gey, G.
Isobe, T.
Lee, P.S.
Liu, J.J.
Li, Z.
Korkulu, Z.
Patel, Z.
Phong, V.
Rice, S.
Sakurai, H.
Sinclair, L.
Sumikama, T.
Tanaka, M.
Yagi, A.
Ye, Y.L.
Yokoyama, R.
Zhang, G.X.
Alharbi, T.
Aoi, N.
Bello Garrote, F. L.
Benzoni, G.
Bruce, A.M.
Carroll, R.J.
Chae, K.Y.
Dombradi, Z.
Estrade, A.
Gottardo, A.
Griffin, C.J.
Kanaoka, H.
Kojouharov, I.
Kondev, F.G.
Kubono, S.
Kurz, N.
Kuti, I.
Lalkovski, S.
Lane, G.J.
Lee, E.J.
Lokotko, T.
Lotay, G.
Moon, C.-B.
Nishibata, H.
Nishizuka, I.
Nita, C.
Odahara, A.
Podolyák, Zs.
Roberts, Q.J.
Schaffner, H.
Shand, C.
Taprogge, J.
Terashima, S.
Vajta, Z.
Yoshida, S.
Institut Laue-Langevin (ILL)
ILL
Laboratoire de Physique Subatomique et de Cosmologie (LPSC)
Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Université Grenoble Alpes [2016-2019] (UGA [2016-2019])-Centre National de la Recherche Scientifique (CNRS)
Source :
Physical Review Letters, Physical Review Letters, American Physical Society, 2017, 118 (7), pp.072701 ⟨10.1103/PhysRevLett.118.072701⟩
Publication Year :
2017
Publisher :
HAL CCSD, 2017.

Abstract

International audience; The β-decay half-lives of 94 neutron-rich nuclei 144−151Cs, 146−154Ba, 148−156La, 150−158Ce, 153−160Pr, 156−162Nd, 159−163Pm, 160−166Sm, 161−168Eu, 165−170Gd, 166−172Tb, 169−173Dy, 172−175Ho, and two isomeric states 174mEr, 172mDy were measured at the Radioactive Isotope Beam Factory, providing a new experimental basis to test theoretical models. Strikingly large drops of β-decay half-lives are observed at neutron-number N=97 for 58Ce, 59Pr, 60Nd, and 62Sm, and N=105 for 63Eu, 64Gd, 65Tb, and 66Dy. Features in the data mirror the interplay between pairing effects and microscopic structure. r-process network calculations performed for a range of mass models and astrophysical conditions show that the 57 half-lives measured for the first time play an important role in shaping the abundance pattern of rare-earth elements in the solar system.

Details

Language :
English
ISSN :
00319007 and 10797114
Database :
OpenAIRE
Journal :
Physical Review Letters, Physical Review Letters, American Physical Society, 2017, 118 (7), pp.072701 ⟨10.1103/PhysRevLett.118.072701⟩
Accession number :
edsair.dedup.wf.001..1da11a071e9fffedc29c3f0bc5d40530
Full Text :
https://doi.org/10.1103/PhysRevLett.118.072701⟩