https://doi.org/10.1140/epja/s10050-026-01806-7
Regular Article - Experimental Physics
Lifetimes of negative parity states in
Dy
1
Department of Physics and Astronomy, University of Notre Dame, 46556, Notre Dame, IN, USA
2
Department of Physics, North Carolina A&T State University, 27411, Greensboro, NC, USA
3
Department of Physics, University of Wisconsin–La Crosse, 54601, La Crosse, WI, USA
4
Department of Physics and Astronomy, Mississippi State University, 39762, Starkville, MS, USA
5
Department of Chemistry, University of Kentucky, 40506, Lexington, KY, USA
6
Department of Physics and Astronomy, University of Kentucky, 40506, Lexington, KY, USA
a
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Received:
16
October
2025
Accepted:
30
January
2026
Published online:
3
April
2026
Abstract
Lifetimes of excited states in
Dy were measured using the (n,n’
) reaction with the Doppler-Shift Attenuation Method (DSAM) at the University of Kentucky’s Accelerator Laboratory. A total of eighteen level lifetimes were obtained, including eleven negative-parity states, seven of which are new. These measurements significantly expand the experimental database of transition probabilities for negative-parity bands in the well-deformed rare earth region of nuclei. The extracted B(E1) and B(E2) values reveal enhanced interband E1 (
or
) W.u. and E2 strengths (several W.u.) between negative- and positive parity bands, particularly for the Kπ = 21,2- bands decaying to the the K
band, consistent with signatures of octupole-quadrupole coupling. In contrast, the K
and K
bands, which exhibit strong E1 transitions to the ground state band, are indicative of octupole-vibrational excitations built on the deformed ground state. Comparison of transition rates with Alaga rules supports this interpretation and distinguishes collective excitations from likely quasi-particle states. These new results establish
Dy as the most extensively characterized rare-earth nucleus for negative parity lifetimes and provide critical experimental benchmarks for theoretical models.
Communicated by Silvia Leoni.
© The Author(s) 2026
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