output
20062024
most citedObservation of a near-threshold structure in the recoil-mass spectra in

192 citations

Showing astro-ph.HEShow all

13 papers · 1 filter

astro-ph.HE20237 cited

Statistical Properties of X-Ray Bursts from SGR J1935+2154 Detected by Insight-HXMT

Wen-Long Zhang, Xiu-Juan Li, Yu-Peng Yang +5

As one class of the most important objects in the universe, magnetars can produce a lot of different frequency bursts including X-ray bursts. In \cite{2022ApJS..260...24C}, 75 X-ra…

astro-ph.HE202312 cited

Evidence for self-organized criticality phenomena in prompt phase of short gamma-ray bursts

Xiu-Juan Li, Wen-Long Zhang, Shuang-Xi Yi +2

The prompt phase of gamma-ray burst (GRB) contains essential information regarding the physical nature and central engine, which are as yet unknown. In this paper, we investigate t…

astro-ph.HE202219 cited

Hypercritical Accretion for Black Hole High Spin in Cygnus X-1

Ying Qin, Xinwen Shu, Shuangxi Yi +1

Recent observations of AdLIGO and Virgo have shown that the spin measurements in binary black hole (BH) systems are typically small, which is consistent with the predictions by the…

astro-ph.HE202112 cited

Constraining Properties of GRB Central Engines with X-ray flares

Shuang-Xi Yi, Wei Xie, Shuai-Bing Ma +2

X-ray flares in gamma-ray bursts (GRBs) are believed to be generated by the late activities of central engine, and thus provide an useful tool to diagnose the properties of central…

astro-ph.HE202015 cited

Testing Blandford-Znajek mechanism in black hole hyperaccretion flows for long-duration gamma-ray bursts

Mei Du, Shuang-Xi Yi, Tong Liu +2

Long-duration gamma-ray bursts (GRBs) are generally related to the core-collapse of massive stars. In the collapsar scenario, a rotating stellar-mass black hole (BH) surrounded by…

astro-ph.HE202070 cited

The Optical Luminosity-Time Correlation for More Than 100 Gamma-Ray Burst Afterglows

M. G. Dainotti, S. Livermore, D. A. Kann +7

Gamma-Ray Bursts (GRBs) are fascinating events due to their panchromatic nature. Their afterglow emission is observed from sub-TeV energies to radio wavelengths. We investigate GRB…