An analytic, parameter-free (up to overall scale factors) solution of the Bohr Hamiltonian involving axially symmetric quadrupole and octupole deformations, as well as an infinite well potential, is obtained, after separating variables in a way reminiscent of the Variable Moment of Inertia (VMI) concept. Normalized spectra and B(EL) ratios are found to agree with experimental data for 226 Ra and 226 Th, the nuclei known to lie closest to the border between octupole deformation and octupole vibrations in the light actinide region.
IntroductionCritical point symmetries [1,2] are attracting recently considerable interest, since they provide parameter-independent (up to overall scale factors) predictions supported by experiment [3,4,5,6]. The E(5) [1] and X(5) [2] critical point symmetries have been obtained from the Bohr Hamiltonian [7] after separating variables in different ways and using an infinite square well potential in the β (quadrupole) variable, the latter corresponding to the critical point of the transition from quadrupole vibrations [U(5)] to axial quadrupole deformation [SU(3)] [2]. A systematic study of phase transitions in nuclear collective models has been given in [8,9,10].In the present work a solution of the Bohr Hamiltonian aiming at the description of the transition from axial octupole deformation to octupole vibrations in the light actinides [11] is worked out. In the spirit of E(5) and X(5) the solution involves an infinite square well potential in the deformation variable and leads to parameter-free (up to overal scale factors) predictions for spectra and B(EL) transition rates. Both (axially symmetric) quadrupole and octupole deformations are taken into account, in order to describe low-lying negative parity states related to octupole deformation, known to occur in the light actinides [11]. Separation of variables is achieved in a novel way, reminiscent of the Variable Moment of Inertia (VMI) concept [12]. The parameter-free predictions of the model turn out to be