activity
20072026
most citedCandidate MKiD nucleus 106Rh in triaxial relativistic mean-field approach with time-odd fields

60 citations · 188 across the 11 of their papers we have counts for

collaborators

11 papers

nucl-th2026

coupling of single-particle orbitals in octupole deformed nuclei

XuDong Wang, Bin Qi, Shouyu Wang +1

Conventionally, octupole deformation in nuclei has been attributed to strong couplings between opposite-parity single-particle orbitals. In this work, we demonstrate that th…

nucl-th2022★ 15 cited

Influence of moments of inertia on transverse wobbling mode in odd-mass nuclei

Hui Zhang, Bin Qi, Xu Dong Wang +2

The reported transverse wobbling band in odd-mass Pd has been reinvestigated by the triaxial particle rotor model. Employing different parameter sets of moment of inertia (…

nucl-th2020★ 14 cited

Influence of triaxial deformation on wobbling motion in even-even nuclei

Bin Qi, Hui Zhang, Shou Yu Wang +1

The influence of triaxial deformation on the purely collective form of wobbling motion in even-even nuclei are discussed based on the triaxial rotor model. It is found that the…

nucl-ex2020★ 21 cited

Recent progress in multiple chiral doublet bands

Shou-Yu Wang

The recent progress of multiple chiral doublet bands (MD) is reviewed for both experimental and theoretical sides. In particular, the experimental findings, theoretical predicti…

nucl-th2019★ 8 cited

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy

Nai-Bo Zhang, Bin Qi, Shou-Yu Wang

The constraints on tidal deformability of neutron stars are first extracted from GW170817 by LIGO and Virgo Collaborations but the relation between radius and tidal deforma…

astro-ph.CO2018★ 5 cited

The maximum mass of dark matter existing in compact stars based on the self-interacting fermionic model

X. D. Wang, B. Qi, N. B. Zhang +1

By assuming that only gravitation acts between dark matter (DM) and normal matter (NM), we studied DM admixed neutron stars (DANSs) using the two-fluid TOV equations. The NM and DM…