activity
20152026
most citedA statistical study of super-luminous supernovae in the magnetar engine model and implications for their connection with gamma-ray bursts and hypernovae

77 citations · 300 across the 14 of their papers we have counts for

collaborators

14 papers

astro-ph.HE2026

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…

astro-ph.HE2023

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…

astro-ph.HE2022

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…

astro-ph.HE2021★ 6 cited

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…

astro-ph.HE2021★ 3 cited

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…

astro-ph.HE2020★ 16 cited

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…

astro-ph.HE2019★ 2 cited

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…

astro-ph.HE2018★ 75 cited

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…

astro-ph.HE2017★ 77 cited

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.…

astro-ph.HE2016★ 23 cited

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…

astro-ph.HE2015★ 30 cited

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…

astro-ph.HE2015★ 3 cited

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…

astro-ph.HE2015★ 57 cited

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…

hep-ph2015★ 8 cited

Higgs boson production and decay at colliders as a probe of the Left-Right twin Higgs model

Jinzhong Han, Shaofeng Li, Bingfang Yang +1

In the framework of the Left-Right twin Higgs (LRTH) model, we consider the constrains from the latest search for high-mass dilepton resonances at the LHC and find that the heavy n…