Phys. Rev. A 66, 013206 (2002) [8 pages]

Scissor modes in triaxial metal clusters

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P.-G. Reinhard1 *, V. O. Nesterenko1,2 , E. Suraud3, S. El Gammal4, and W. Kleinig2,5
1Institut fur Theoretische Physik, Universität Erlangen, D-91058 Erlangen, Germany
2Bogoliubov Laboratory of Theoretical Physics, Joint Institute for Nuclear Research 141980, Dubna, Moscow Region, Russia
3Laboratoire de Physique Quantique, Université Paul Sabatier, 118 Route de Narbonne, 31062 Toulouse cedex, France
4Physics Department, Faculty of Science, El-Menoufia University, Shebin El-Kom, Egypt
5Institut für Analysis, Technische Universität Dresden, Dresden D-01062, Germany

Received 7 March 2002; published 24 July 2002

We study the scissor mode (orbital M1 excitations) in small Na clusters, triaxial metal clusters Na12 and Na16 and the close-to-spherical Na9+, all described in density-functional theory with detailed ionic background. The scissor modes built on spin-saturated ground and spin-polarized isomeric states are analyzed in virtue of both macroscopic collective and microscopic shell-model treatments. It is shown that the mutual destruction of Coulomb and the exchange-correlation parts of the residual interaction makes the collective shift small and the net effect can depend on details of the actual excited state. The cross-talk with dipole and spin-dipole modes is studied in detail. In particular, a strong cross-talk with spin-dipole negative-parity mode is found in the case of spin-polarized states. Triaxiality and ionic structure considerably complicate the scissor response, mainly at the expense of stronger fragmentation of the strength. Nevertheless, even in these complicated cases the scissor mode is mainly determined by the global deformation. The detailed ionic structure destroys the spherical symmetry and can cause finite M1 response (transverse optical mode) even in clusters with zero global deformation. But its strength turns out to be much smaller than for the genuine scissor modes in deformed systems.


©2002 The American Physical Society

URL: http://link.aps.org/doi/10.1103/PhysRevA.66.013206
DOI: 10.1103/PhysRevA.66.013206
PACS: 36.40.Gk, 36.40.Vz

* Email address: mpt218@theorie2.physik.uni-erlangen.de
Email address: nester@thsun1.jinr.ru

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