activity
20242026
collaborators

14 papers

astro-ph.HE2026

Short-duration GRB 250221A Afterglow Driven by Two-Component Jets from the merger of a compact star

Xiao Tian, Hou-Jun Lü, Xiao-Xuan Liu +4

GRB 250221A is a short gamma-ray burst (GRB) at redshift , with a duration of 1.8 s and no extended emission in either Swift/Burst Alert Telescope or Konus-Wind bands. A r…

astro-ph.HE2026

Identifying the poynting-flux-dominated outflow of Fermi GRBs with non-thermal spectrum and its energy-resolved light curve fitting

Xue-Zhao Chang, HouJun Lü, Zhao-Wei Du +2

The jet compositions of gamma-ray bursts (GRBs) are very important to understand the energy dissipation and radiation mechanisms, but it remains an open question in GRB physics. In…

astro-ph.HE2025

Evidence for the transition from thermal to non-thermal emission in the prompt emission of GRB 161117A

Xue-Zhao Chang, HouJun Lü, Jia-Ming Chen +1

GRB 161117A is a long-duration GRB with three main overlapping peaks. By analyzing the time-resolved spectra of its data observed with the Gamma-Ray Burst Monitor (GBM) on board th…

astro-ph.HE2025

Probing the Nature of High-Redshift Long GRB 250114A and Its Magnetar Central Engine

Wen-Yuan Yu, Hou-Jun Lü, Xiao Tian +2

GRB 250114A is a long-duration gamma-ray burst (GRB) which triggered the Swift/BAT with a spectroscopic high-redshift at . The light curve of the prompt emission is comp…

astro-ph.HE2025

The color evolution of magnetar-powered kilonova emission in merging neutron star-neutron star systems

Suo-Ning Wang, Hou-Jun Lü, Xiao-Xuan Liu +3

The first direct detection of the gravitational wave (GW) event GW170817 and its electromagnetic (EM) counterpart open a new window for studying of multi-messenger astronomy. Howev…

astro-ph.HE2025

Signature of a magnetar central engine with precession motion in the X-ray emission of GRB 220711B

Ying-Ze Shan, Xing Yang, Hou-Jun Lü +6

The -ray light curve of long-duration GRB 220711B, is characterized by a multi-peaked structure with a duration lasting 105 seconds. More interestingly, the X-ray afterglo…

astro-ph.HE2025

Neutron Star-White Dwarf Merger as One Possible Optional Source of Kilonova-like Emission: Implications for GRB 211211A

Xiao-Xuan Liu, Hou-Jun Lü, Qiu-Hong Chen +2

Long-duration GRB 211211A, which lacked an associated supernova at such a low redshift , but was associated with a possible kilonova emission, has attracted great attentio…

astro-ph.HE2025

Constraining the Nuclear Equation of State of neutron star via high-frequency quasi-periodic oscillation in short gamma-ray bursts

Jun-Xiang Huang, Hou-Jun Lü, En-Wei Liang

The determination of the equation of state (EOS) of a neutron star (NS) and its maximum mass is very important for understanding the formation and properties of NSs under extreme c…

astro-ph.HE2025

Discovery of high-frequency quasi-periodic oscillation in short-duration gamma-ray bursts

Xing Yang, Hou-Jun Lü, Jared Rice +1

Rapidly rotating newborn magnetars, which originate from binary neutron star (NS) mergers and serve as the central engines of short gamma-ray bursts (GRBs), may leave some imprints…

astro-ph.HE2025

Constraining the Cosmic-ray Energy Based on Observations of Nearby Galaxy Clusters by LHAASO

The LHAASO Collaboration, Zhen Cao, F. Aharonian +323

Galaxy clusters act as reservoirs of high-energy cosmic rays (CRs). As CRs propagate through the intracluster medium, they generate diffuse -rays detectable by arrays such as LH…

astro-ph.HE2024

Neutrino constraints and detection prospects from gamma-ray bursts with different jet compositions

Yang-Dong-Jun Ou, Hou-Jun Lü, Xue-Zhao Chang +2

The prompt emission mechanism of gamma-ray bursts (GRBs) is a long-standing open question, and GRBs have been considered as potential sources of high-energy neutrinos. Despite many…

astro-ph.HE2024

Shear Particle Acceleration in Structured Gamma-Ray Burst Jets: I. Physical Origin of the Band Function and Application to GRBs 090926A, 131108A, and 160509A

Zi-Qi Wang, Xiao-Li Huang, En-Wei Liang

The radiation physics of gamma-ray bursts (GRBs) remains an open question. Based on the simulation analysis and recent observations, it was proposed that GRB jets are composed of a…

astro-ph.HE2024

The thermal emission in short GRBs with extended emission observed by Fermi/GBM

Xue-Zhao Chang, Hou-Jun Lü, Xing Yang +2

Short gamma-ray bursts (SGRBs) with extended emission (EE) are composed of initial main emission (ME) with a short-hard spike, followed by a long-lasting EE. Whether the ME and EE…

astro-ph.HE2024

A Comprehensive Analysis of Text-Book-Version Afterglow Light curves of Gamma-Ray Bursts and Implication for Universal Radiation Physics of Baryonic Jets

Lu-Lu Zhang, Shu-Qing Zhong, Li-Ping Xin +1

The standard external shock model in the thin-shell scenario predicts an onset bump in the early optical afterglow light curves of gamma-ray bursts (GRBs). We collect such a textbo…