Sextic potential for γγ-rigid prolate nuclei

preprint2015arXivOpen access

Abstract

The equation of the Bohr-Mottelson Hamiltonian with a sextic oscillator potential is solved for γγ-rigid prolate nuclei. The associated shape phase space is reduced to three variables which are exactly separated. The angular equation has the spherical harmonic functions as solutions, while the ββ equation is brought to the quasi-exactly solvable case of the sextic oscillator potential with a centrifugal barrier. The energies and the corresponding wave functions are given in closed form and depend, up to a scaling factor, on a single parameter. The 0+0^{+} and 2+2^{+} states are exactly determined, having an important role in the assignment of some ambiguous states for the experimental ββ bands. Due to the special properties of the sextic potential, the model can simulate, by varying the free parameter, a shape phase transition from a harmonic to an anharmonic prolate ββ-soft rotor crossing through a critical point. Numerical applications are performed for 39 nuclei: 98−108^{98-108}Ru, 100,102^{100,102}Mo, 116−130^{116-130}Xe, 132,134^{132,134}Ce, 146−150^{146-150}Nd, 150,152^{150,152}Sm, 152,154^{152,154}Gd, 154,156^{154,156}Dy, 172^{172}Os, 180−196^{180-196}Pt, 190^{190}Hg and 222^{222}Ra. The best candidates for the critical point are found to be 104^{104}Ru and 120,126^{120,126}Xe, followed closely by 128^{128}Xe, 172^{172}Os, 196^{196}Pt and 148^{148}Nd.

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