77 citations · 300 across the 14 of their papers we have counts for
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Anisotropic Ejecta from Binary Neutron Star Mergers: Self-Consistent Main Thermal and Late-Time Radio Emission of NS-Powered Kilonovae
Jia-Xiang Chen, Shao-Ze Li
The interaction between the fast-moving ejecta and the interstellar medium can produce long-lasting radio signals after binary neutron star mergers. Searching for such radio signal…
Double Neutron Star Mergers: Are Late-time Radio Signals Overestimated?
Shao-Ze Li, Yun-Wei Yu, He Gao +1
The coalescence of binary neutron stars can yield the expulsion of a fast-moving, quasi-isotropic material, which may induce thermal radiation and give rise to kilonova emission. M…
Magnetar wind-driven shock breakout emission after double neutron star mergers: The effect of the anisotropy of the merger ejecta
Guang-Lei Wu, Yun-Wei Yu, Shao-Ze Li
A rapidly rotating and highly magnetized remnant neutron star (NS; magnetar) could survive from a merger of double NSs and drive a powerful relativistic wind. The early interaction…
The evolution effects of radius and moment of inertia for rapidly rotating neutron stars
Lin Lan, He Gao, Shunke Ai +1
A newly born millisecond magnetar is thought to be the central engine of some gamma-ray bursts (GRBs), especially those that present long-lasting X-ray plateau emissions. By solvin…
A powerful e^{+-} outflow driven by a proto-strange quark star
Shao-Ze Li, Yun-Wei Yu, He Gao +2
An electron-positron layer can cover the surface of a bare strange star (SS), the electric field in which can excite the vacuum and drive a pair wind by taking away the heat of the…
The evolution of a newborn millisecond magnetar with a propeller-recycling disk
Shao-Ze Li, Yun-Wei Yu, He Gao +1
A rapidly rotating and highly magnetized neutron star (NS) could be formed from the explosive phenomena such as superluminous supernovae and gamma-ray bursts. This newborn NS can s…
Studying newborn neutron stars by the transient emission after stellar collapses and compact binary mergers
Yun-Wei Yu, Aming Chen, Zi-Gao Dai +3
The formation of neutron stars (NSs), both from collapses of massive stars and mergers of compact objects, can be usually indicated by bright transients emitted from explosively-ej…
What Powered the Optical Transient AT2017gfo Associated with GW170817?
Shao-Ze Li, Liang-Duan Liu, Yun-Wei Yu +1
The groundbreaking discovery of the optical transient AT2017gfo associated with GW170817 opens a unique opportunity to study the physics of double neutron star (NS) mergers. We arg…
A statistical study of super-luminous supernovae in the magnetar engine model and implications for their connection with gamma-ray bursts and hypernovae
Yun-Wei Yu, Jin-Ping Zhu, Shao-Ze Li +2
By fitting the bolometric light curves of 31 super-luminous supernovae (SLSNe) with the magnetar engine model, we derive the ejecta masses and magnetar parameters for these SLSNe.…
A possible relation between flare activity in superluminous supernovae and gamma-ray bursts
Yun-Wei Yu, Shao-Ze Li
Significant undulations appear in the light curve of a recently discovered super-luminous supernova (SLSN) SN 2015bn after the first peak, while the underlying profile of the light…
Shock breakout driven by the remnant of a neutron star binary merger: An X-ray precursor of mergernova emission
Shao-Ze Li, Yun-Wei Yu
A supra-massive neutron star (NS) spinning extremely rapidly could survive from a merger of NS-NS binary. The spin-down of this remnant NS that is highly magnetized would power the…
Constraints on millicharged particles by neutron stars
Xi Huang, Xiao-Ping Zheng, Wei-Hua Wang +1
We have constrained the charge-mass () phase space of millicharged particles through the simulation of the rotational evolution of neutron stars, where an extra slow…
Rapidly Evolving and Luminous Transients Driven by Newly Born Neutron Stars
Yun-Wei Yu, Shao-Ze Li, Zi-Gao Dai
We provide a general analysis on the properties of emitting material of some rapidly evolving and luminous transients discovered recently with the Pan-STARRS1 Medium Deep Survey. I…