scholarly journals Nuclear spin scissors mode – experimental status

2018 ◽  
Vol 194 ◽  
pp. 04004
Author(s):  
Irina Molodtsova ◽  
Evgeny Balbutsev ◽  
Peter Schuck

A new type of nuclear collective motion - the spin scissors mode - was predicted seven years ago. Promising signs of its existence in 232Th were found. We perform a systematic analysis of experimental data on M1 excitations in rare-earth nuclei to find traces of the spin scissors mode in this area. Obvious signs of its existence are demonstrated.

2018 ◽  
Vol 194 ◽  
pp. 04005 ◽  
Author(s):  
Evgeny Balbutsev ◽  
Irina Molodtsova

The solution of TDHFB equations by Wigner Function Moments method with the isovectorisoscalar coupling taken into account leads to the prediction of the new type of nuclear spin scissors mode. It turns out that the lower group of M1 excitations in 164Dy, which is usually not included in the systematics of the scissors mode, can be quite naturally attributed to this new type of scissors.


2013 ◽  
Vol 88 (1) ◽  
Author(s):  
E. B. Balbutsev ◽  
I. V. Molodtsova ◽  
P. Schuck

2005 ◽  
Vol 14 (02) ◽  
pp. 197-213 ◽  
Author(s):  
N. BENHAMOUDA ◽  
N. H. ALLAL ◽  
M. FELLAH ◽  
M. R. OUDIH

The physical properties of the nuclear shape have been investigated through the charge square radius (<r2>) and the quadrupole (Q2) and hexadecapole (Q4) moments of the even–even neutron-rich rare-earth nuclei. The single-particle energies used are those of a deformed Woods–Saxon mean-field. The pairing effects have been included by means of an exact projection method. The model has been tested for the "ordinary" nuclei near the shell closure N = 82 and has correctly reproduced the experimental data and particularly the "Kink" effect. The study has then been extended to the neutron-rich nuclei and has shown a stability of the <r2> and Q2 results for N≃100 which may be attributed to the existence of a new magic number. On the other hand, a saturation of the prolate shape appears around N = 108 for the elements Nd , Sm and Gd and near N = 102 for the Dy , Er and Yb . These observations could not be confirmed by the investigation of the hexadecapole moment.


2014 ◽  
Vol 533 ◽  
pp. 012010
Author(s):  
E B Balbutsev ◽  
I V Molodtsova

2018 ◽  
Vol 97 (4) ◽  
Author(s):  
E. B. Balbutsev ◽  
I. V. Molodtsova ◽  
P. Schuck

1979 ◽  
Vol 40 (C5) ◽  
pp. C5-56-C5-57 ◽  
Author(s):  
E. Belorizky ◽  
Y. Berthier ◽  
R. A.B. Devine ◽  
P. M. Levy ◽  
J. J. Niez

2011 ◽  
Vol 312 (9) ◽  
pp. 092062 ◽  
Author(s):  
V Werner ◽  
N Cooper ◽  
M Bonett-Matiz ◽  
E Williams ◽  
J-M Régis ◽  
...  

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