105 citations · 468 across the 18 of their papers we have counts for
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A new subclass of gamma-ray burst originating from compact binary merger
Chen-Wei Wang, Wen-Jun Tan, Shao-Lin Xiong +15
Type I gamma-ray bursts (GRBs) are believed to originate from compact binary merger usually with duration less than 2 seconds for the main emission. However, recent observations of…
One Fits All: A Unified Synchrotron Model Explains GRBs with FRED-Shaped Pulses
Zhen-Yu Yan, Jun Yang, Xiao-Hong Zhao +2
The analysis of gamma-ray burst (GRB) spectra often relies on empirical models lacking a distinct physical explanation. Previous attempts to couple physical models with observed da…
Significant cocoon emission and photosphere duration stretching in GRB 211211A: a burst from a neutron star - black hole merger
Yan-Zhi Meng, Xiangyu Ivy Wang, Zi-Ke Liu
The radiation mechanism (thermal photosphere or magnetic synchrotron) and the progenitor of gamma-ray burst (GRB) are under hot debate. Recently discovered, the prompt long-duratio…
Synchrotron Radiation Dominates the Extremely Bright GRB 221009A
Jun Yang, Xiao-Hong Zhao, Zhenyu Yan +30
The brightest Gamma-ray burst, GRB 221009A, has spurred numerous theoretical investigations, with particular attention paid to the origins of ultra-high energy TeV photons during t…
GRB 220408B: A Three-Episode Burst from a Precessing Jet
Zijian Zhang, Yihan Yin, Chenyu Wang +27
Jet precession has previously been proposed to explain the apparently repeating features in the light curves of a few gamma-ray bursts (GRBs). In this {\it Letter}, we further appl…
The Hardness-intensity Correlation of Photospheric Emission from a Structured Jet for Gamma-Ray Bursts
Xin-Ying Song, Yan-Zhi Meng
For many gamma-ray bursts (GRBs), hardness-intensity correlation (HIC) can be described by a power-law function, , where is the peak energy of $νF…