Abstract
For the first time, the relativistic mean field (RMF) model is applied to the shears band recently observed in ${}_{37}^{84}\mathrm{Rb}.$ Signals of the appearance of the shears mechanism, such as smooth decreases of the shears angle and of the $B(M1)/B(E2)$ ratio while keeping the nearly constant tilt angle, are well reproduced. Thus it is shown that the microscopic RMF model can nicely describe the shears band in this nucleus.
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