activity
20242026
collaborators

7 papers

astro-ph.HE2026

Impact of Neutrino Flavour Conversion on the Diffuse Neutrino Background from Neutrino-dominated Accretion Flows

Yun-Feng Wei, Tong Liu

Neutrino-dominated accretion flows (NDAFs) are believed to form during the fallback accretion phase of some core-collapse supernovae (CCSNe). Such systems produce copious neutrino…

astro-ph.HE2026

Impact of disk magnetic fields on the propagation of stellar-scale jets in the magnetically arrested accretion disks of active galactic nuclei

Bao-Quan Huang, Tong Liu, Jian-Fu Zhang

It is widely recognized that active galactic nucleus (AGN) disks host numerous massive stars and compact objects. Stellar-scale jets triggered by collapses of massive stars and mer…

astro-ph.HE2026

Imprints of gravitational waves from magnetar spindown in GRB X-ray afterglows

Shu-Jin Hou, Rui Xue, Fang-Kun Peng +3

Given that newborn magnetars are considered potential central engines of gamma-ray bursts (GRBs), there is strong motivation to identify gravitational wave (GW) signatures within G…

astro-ph.HE2025

Hyperaccretion-driven relativistic jets from massive collapsars in active galactic nucleus disks

Yun-Feng Wei, Tong Liu, Bao-Quan Huang

The observable characteristics of gamma-ray bursts (GRBs) embedded in the accretion disk of active galactic nuclei (AGNs) are mainly determined by the jet propagation within the di…

astro-ph.HE2025

Anisotropy of core-collapse supernovae effected by AGN disks

Jiao-Zhen She, Tong Liu, Bao-Quan Huang +4

Active galactic nucleus (AGN) disk provide dense environments to influence on the star formation, evolution, and migration. In AGN disks, pressure gradients and migration accelerat…

astro-ph.HE2025

A Neutron Capture Explanation for the 10 MeV Emission Line Seen in GRB 221009A

Jiahuan Zhu, Hua Feng, Tong Liu

The brightest ever gamma-ray burst (GRB) 221009A displays a significant emission line component around 10 MeV. As the GRB central engine is neutron-rich, we propose that the emissi…