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Gross shell structure at high spin in heavy nuclei

2003/11/20 by M. A. Deleplanque, S. Frauendorf, V.V. Pashkevich +5 · 26 citations
Physics and Astronomy · #Angular momentum #Astro and Planetary Science #Atomic physics #Classical mechanics #Condensed matter physics #Mass number #Materials science #Moment of inertia #Neutron #Neutron number #Neutron temperature #Nuclear physics #Nuclear physics research studies #Nuclear structure #Physics #Quantum #Quantum chaos and dynamical systems #Quantum mechanics #Semiclassical physics #Shell (structure) #Spin (aerodynamics) #Spins #Yrast #cond-mat.mes-hall #nucl-th #physics.atm-clus

paper · pdf · doi:10.1103/physrevc.69.044309

published in Physical Review C 69(4) (American Institute of Physics) · 40 pages total; 22 pages text, 19 figures sent as 27 .png files

arxiv created 2003/11/20 · openalex publication_date 2004/04/16 · arxiv updated 2014/11/18 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

Experimental nuclear moments of inertia at high spins along the yrast line have been determined for a large number of nuclei. They are found to systematically differ from the rigid-body values. The difference is attributed to shell effects which are well described by a rotating Woods-Saxon potential. The data and quantal calculations are interpreted by means of the semiclassical periodic orbit theory. From this new perspective, features in the moments of inertia as a function of neutron number and spin as well as their relation to the shell energies can be understood. Gross shell effects persist up to the highest angular momenta observed.

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