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20062026
most citedNeutrino-dominated accretion flows as the central engine of gamma-ray bursts

154 citations · 2.5k across the 92 of their papers we have counts for

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Showing 2018Show all

7 papers · 1 filter

astro-ph.HE2018★ 24 cited

Black hole hyperaccretion inflow-outflow model. II. Long-duration gamma-ray bursts and supernova bumps

Cui-Ying Song, Tong Liu

Long-duration gamma-ray bursts (LGRBs) associated with supernovae (SNe) are possibly born out of the death of a massive star. After the star collapses, a stellar-mass black hole (B…

astro-ph.HE2018★ 43 cited

Multi-color blackbody emission in GRB 081221

Shu-Jin Hou, Bin-Bin Zhang, Yan-Zhi Meng +9

The radiation mechanism of the prompt emission of gamma-ray bursts (GRBs) remains an open question. Although their spectra are usually well fitted with the empirical Band function,…

astro-ph.HE2018★ 1 cited

A lower occurrence rate of bright X-ray flares in SN-GRBs than GRBs: evidence of energy partitions?

Hui-Jun Mu, Wei-Min Gu, Jirong Mao +6

The occurrence rates of bright X-ray flares in z<1 gamma-ray bursts (GRBs) with or without observed supernovae (SNe) association were compared. Our Sample I: the z<1 long GRBs (LGR…

astro-ph.HE2018★ 7 cited

Central Engine-Powered Bright X-ray Flares in Short Gamma-Ray Bursts: A Hint of Black Hole-Neutron Star Merger?

Hui-Jun Mu, Wei-Min Gu, Jirong Mao +3

Short gamma-ray bursts may originate from the merger of double neutron stars (NS) or that of a black hole (BH) and an NS. We propose that the bright X-ray flare related to the cent…

astro-ph.HE2018★ 12 cited

First Electromagnetic Pulse Associated with a Gravitational-Wave Event: Profile, Duration, and Delay

Da-Bin Lin, Tong Liu, Jie Lin +3

We study the first electromagnetic pulse after the gravitational wave chirp signal, focusing on the profile and duration. It is found that the light curve, especially the steep dec…

astro-ph.HE2018★ 4 cited

Compact binary merger and kilonova: outflows from remnant disc

Tuan Yi, Wei-Min Gu, Tong Liu +3

Outflows launched from a remnant disc of compact binary merger may have essential contribution to the kilonova emission. Numerical calculations are conducted in this work to study…