Feeding of superdeformed bands: The mechanism and constraints on band energies and the well depth
T. LauritsenArgonne National Laboratory, Argonne, Illinois 60439Ph. BenetArgonne National Laboratory, Argonne, Illinois 60439T. L. KhooArgonne National Laboratory, Argonne, Illinois 60439K. BeardArgonne National Laboratory, Argonne, Illinois 60439I. AhmadArgonne National Laboratory, Argonne, Illinois 60439M. P. CarpenterArgonne National Laboratory, Argonne, Illinois 60439P. J. DalyArgonne National Laboratory, Argonne, Illinois 60439M. W. DrigertArgonne National Laboratory, Argonne, Illinois 60439U. GargArgonne National Laboratory, Argonne, Illinois 60439P. B. FernandezArgonne National Laboratory, Argonne, Illinois 60439R. V. F. JanssensArgonne National Laboratory, Argonne, Illinois 60439E. F. MooreArgonne National Laboratory, Argonne, Illinois 60439F. L. H. WolfsArgonne National Laboratory, Argonne, Illinois 60439D. YeArgonne National Laboratory, Argonne, Illinois 60439
1992en
ABI
Аннотация
Entry distributions leading to normal and superdeformed (SD) states in $^{192}\mathrm{Hg}$ have been measured. A model, based on Monte Carlo simulations of \ensuremath{\gamma} cascades, successfully reproduces the entry distribution for SD states, as well as all other known observables connected with the population of SD states. Comparison of experimental and model results, together with the measured SD entry distribution, suggest that the SD band lies 3.3--4.3 MeV above the normal yrast line when it decays around spin 10 and that the SD well depth is 3.5--4.5 MeV at spin 40.
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