Abstract

We examine, within the framework of the interacting boson model, the structural evolution along the excitation energy across the saddle points of potential wells in a finite nuclear system, and its connection with excited-state quantum phase transitions (ESQPTs). We find that transitions between $\ensuremath{\gamma}$-rigid and $\ensuremath{\gamma}$-soft shapes occur as a function of angular momentum, $L$, analogous to the Jacobi transitions occurring in rotating stars. Empirical evidence of these transitions is found in the rotational spectra of $^{156--162}\mathrm{Gd}$.

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