36 citations · 205 across the 14 of their papers we have counts for
14 papers
Gamma-ray Burst Empirical Correlation between Peak Luminosity and Peak Energy in The ICMART Model
Xueying Shao, He Gao
Internal-Collision-induced Magnetic Reconnection and Turbulence (ICMART) model is a widely accepted model for explaining how high-magnetization jets produce gamma-ray burst (GRB) p…
Long-term radio monitoring of the fast X-ray transient EP240315a: evidence for a relativistic jet
R. Ricci, E. Troja, Y. Yang +7
The recent launch of Einstein Probe (EP) in early 2024 opened up a new window onto the transient X-ray sky, allowing for real-time discovery and follow-up of fast X-ray transients…
Polarization Signature of Companion-Fed Supernovae Arising from BH-NS/BH Progenitor Systems
Xudong Wen, He Gao, Shunke Ai +3
The formation of black hole-neutron star (BH-NS) or BH-BH systems may be accompanied with special supernova (SN) signals, due to the accretion feedback from the companion BH. The a…
Model constraints based on the IceCube neutrino non-detection of GRB 221009A
Shunke Ai, He Gao
GRB 221009A is a bright Gamma-ray burst (GRB) with isotropic energy being larger than . Its fairly low redshift makes it a promising candidate for high energy…
Prospects of strongly lensed fast radio bursts: Simultaneous measurement of post-Newtonian parameter and Hubble constant
Ran Gao, Zhengxiang Li, He Gao
Strong gravitational lensing effect is a powerful tool to probe cosmological models and gravity theories. Recently, the time-delay cosmography from strong lensing and the stellar k…
GRB 211211A: a Prolonged Central Engine under a Strong Magnetic Field Environment
He Gao, Wei-Hua Lei, Zi-Pei Zhu
Recently, a kilonova-associated gamma-ray burst (GRB 211211A), whose light curve consists of a precursor (0.2 s), a hard spiky emission (10 s), and a soft long extended…
The Peculiar Precursor of a Gamma-Ray Burst from a Binary Merger Involving a Magnetar
Shuo Xiao, Yan-Qiu Zhang, Zi-Pei Zhu +42
The milestone discovery of GW 170817-GRB 170817A-AT 2017gfo has shown that gravitational wave (GW) could be produced during the merger of neutron star-neutron star/black hole and t…
The Number of Possible CETIs within Our Galaxy and the Communication Probability among These CETIs
Wenjie Song, He Gao
As the only known intelligent civilization, human beings are always curious about the existence of other communicating extraterrestrial intelligent civilizations (CETIs). Based on…
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…
What binary systems are the most likely sources for periodically repeating FRBs?
Xianfei Zhang, He Gao
The newly discovered 16.35 days period for repeating FRB 180916.J0158+65 provides an essential clue for understanding the sources and emission mechanism of repeating FRBs. Many mod…
G4.8+6.2, a possible kilonova remnant?
Yu Liu, Yuan-Chuan Zou, Bing Jiang +3
Kilonova explosions typically release erg in kinetic energy, which is sufficient to constitute a kilonova remnant (KNR); however, it has not yet been confirmed. I…
Effects of Lorentz breaking on the accretion onto a Schwarzschild-like black hole
Rong-Jia Yang, He Gao, Yaoguang Zheng +1
We formulate and solve the problem of spherically symmetric, steady state, adiabatic accretion onto a Schwarzschild-like black hole obtained recently. We derive the general analyti…
Long-Term Postmerger Simulations of Binary Neutron Star Coalescence: Formation of Toroidal Remnants and Gravitational Wave Afterglow
Xuefeng Zhang, Zhoujian Cao
It has been estimated that a significant proportion of binary neutron star merger events produce long-lived massive remnants supported by differential rotation and subject to rotat…