1991
DOI: 10.1007/bf01282938
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Low energy orbital magnetic dipole excitations of heavy nonspherical nuclei

Abstract: To clarify the physical nature of the orbital magnetic dipole excitations discussed widely in the past few years, a semiclassical model is presented and the nuclei a56Gd and 164Dy are investigated microscopically. The semiclassical model involves a consistent treatment of vibrational and rotational degrees of freedom; the microscopic results are obtained in quasiparticle-random-phase approximation (QRPA) with a realistic effective interaction. The results disagree with the picture of scissors modes or rotation… Show more

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Cited by 37 publications
(71 citation statements)
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“…This agrees with the conclusion of the papers [14,15]: classically (i.e., without Fermi surface deformation) the scissors mode is a zero energy mode.…”
Section: Isovector Eigenfrequenciessupporting
confidence: 92%
“…This agrees with the conclusion of the papers [14,15]: classically (i.e., without Fermi surface deformation) the scissors mode is a zero energy mode.…”
Section: Isovector Eigenfrequenciessupporting
confidence: 92%
“…Also the J=4 + state has not been found. There is additional information obtained by looking at 10 C and 10 B. In 10 C, which is the mirror nucleus of 10 Be, the 2 10 Li has recently been produced by Kryger et al [15] and studied by M. Zinser et al [16].…”
Section: The Experimental Situationmentioning
confidence: 99%
“…In even even nuclei, all of which have J=0 + ground sates, the scissors modes have quantum numbers J=1 strength for 0 Ä 2 transitions (alternately that orbital B(M1) is proportional to $ 2 , where $ is the deformation parameter). Another topic of interest is the possibility of finding scissors mode strength at about 2 | excitations as has been emphasized by Speth and Zawischa [9,10]. This follows from the fact that there is considerable B(E2) strength in that vicinity i.e.…”
Section: Introductionmentioning
confidence: 97%
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