2024-03-28T20:37:46Zhttp://digital.csic.es/dspace-oai/requestoai:digital.csic.es:10261/1410382022-05-19T10:04:35Zcom_10261_135com_10261_4col_10261_388
2016-12-01T10:34:16Z
urn:hdl:10261/141038
Backbending region study in 160,162Dy using incomplete fusion reactions
Jungclaus, Andrea
Binder, B.
Dietrich, A.
Härtlein, T.
Bauer, H.
Gund, Ch.
Pansegrau, D.
Schwalm, D.
Egido, J.L.
Sun, Y.
Bazzacco, D.
De Angelis, G.
Farnea, E.
Gadea, Andrés
Lunardi, S.
Napoli, D.R.
Rossi-Alvarez, C.
Ur, C.
Hagemann, G. B.
Federal Ministry of Education and Research (Germany)
German Research Foundation
18 págs.; 17 figs.; 3 tabs. ; PACS number(s): 23.20.Lv, 23.20.En, 27.70.1q, 21.60.Cs
The incomplete fusion reactions 7Li→158,160Gd at beam energies of 8 MeV/nucleon have been used to study the first band crossing region in the heavy stable Dy isotopes 160,162Dy. The γ rays were detected in the GASP spectrometer in coincidence with fast charged particles detected in the ISIS silicon ball. We succeeded to observe the first backbending in 162Dy at a crossing frequency of ℏ ω ≈ 350 keV, a value much higher than expected from other nuclei in this mass region. Moreover, for the first time in a nucleus with a very large interaction strength, the yrare band in 160Dy could be established up to rather high spin (I= 20ℏ) allowing for a precise determination of the interaction strength between the ground state and the Stockholm band, |Vg-S| = 219(2) keV. Together with |Vg-S| = 14(2) kev determined for the corresponding interaction in 162Dy, a full oscillation of the strengths from one node to the next could be observed within an isotopic chain. In addition to the ground state and Stockholm bands, many other known bands in the two nuclei were considerably extended to higher spin and the experimental results are compared to calculations within the projected shell model. ©2002 The American Physical Society
2016-12-01T10:34:16Z
2016-12-01T10:34:16Z
2002-07-26
2016-12-01T10:34:17Z
artículo
Physical Review C - Nuclear Physics 66: 143121-1431218 (2002)
http://hdl.handle.net/10261/141038
10.1103/PhysRevC.66.014312
http://dx.doi.org/10.13039/501100002347
http://dx.doi.org/10.13039/501100001659
eng
Publisher's version
http.//dx.doi.org/10.1103/PhysRevC.66.014312
Sí
openAccess
American Physical Society