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DOE OSTI · 21388577

Semiclassical shell structure in rotating Fermi systems

Magner, A G·Sitdikov, A S·Khamzin, A A·Bartel, J
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Abstract

The collective moment of inertia is derived analytically within the cranking model for any rotational frequency of the harmonic-oscillator potential well and at a finite temperature. Semiclassical shell-structure components of the collective moment of inertia are obtained for any potential by using the periodic-orbit theory. We found semiclassically their relation to the free-energy shell corrections through the shell-structure components of the rigid-body moment of inertia of the statistically equilibrium rotation in terms of short periodic orbits. The shell effects in the moment of inertia exponentially disappear with increasing temperature. For the case of the harmonic-oscillator potential, one observes a perfect agreement of the semiclassical and quantum shell-structure components of the free energy and the moment of inertia for several critical bifurcation deformations and several temperatures.

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73 NUCLEAR PHYSICS AND RADIATION PHYSICSAPPROXIMATIONSBIFURCATIONCALCULATION METHODSCORRECTIONSCRANKING MODELDEFORMATIONENERGYEQUILIBRIUMFREE ENERGYHARMONIC OSCILLATORSMATHEMATICAL MODELSMOMENT OF INERTIANUCLEAR DEFORMATIONNUCLEAR MODELSORBITSPERIODICITYPHYSICAL PROPERTIESSEMICLASSICAL APPROXIMATIONTHERMODYNAMIC PROPERTIESVARIATIONS

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Magner, A G, Sitdikov, A S, Khamzin, A A, Bartel, J. 2010-06-15. Semiclassical shell structure in rotating Fermi systems. https://doi.org/10.1103/physrevc.81.064302

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