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20152026
most citedLow-energy Spectra of Gamma-ray Bursts from Cooling Electrons

72 citations · 387 across the 32 of their papers we have counts for

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Showing 2018 · astro-ph.HEShow all

8 papers · 2 filters

astro-ph.HE2018

Polarization with a 3-dimensional Mixed Magnetic Field and Its Application to GRB 170817A

Mi-Xiang Lan, Jin-Jun Geng, Xue-Feng Wu +1

A large-scale ordered magnetic field plays a very important role in the formation and acceleration of a gamma-ray burst (GRB) jet. During the GRB prompt phase, some dissipation pro…

astro-ph.HE2018

Probing Magnetic Fields of GRB X-ray Flares with Polarization Observations

Jin-Jun Geng, Yong-Feng Huang, Xue-Feng Wu +2

X-ray flares, lasting for s in the X-ray band, are often observed following gamma-ray bursts (GRBs). The physical origin of X-ray flares is still unknown merely w…

astro-ph.HE2018

Fast Radio Bursts from the collapse of Strange Star Crusts

Yue Zhang, Jin-Jun Geng, Yong-Feng Huang

Fast radio bursts (FRBs) are transient radio sources at cosmological distances. No counterparts in other bands have been observed for { non-repeating FRBs}. Here we suggest the col…

astro-ph.HE2018

Brightening X-ray/Optical/Radio Emission of GW170817/SGRB 170817A: Results of an Electron-Positron Wind from the Central Engine?

Jin-Jun Geng, Zi-Gao Dai, Yong-Feng Huang +4

Recent follow-up observations of the binary neutron star (NS) merging event GW170817/SGRB 170817A reveal that its X-ray/optical/radio emissions are brightening continuously up to $…

astro-ph.HE2018

Bimodal distribution of short gamma-ray bursts: evidence for two distinct types of short gamma-ray bursts

Y. B. Yu, L. B. Li, B. Li +2

Recently, GRB 170817A was confirmed to be associated with GW 170817, which was produced by a neutron star - neutron star merger. It indicates that at least some short gamma-ray bur…

astro-ph.HE2018

A Model of Fast Radio Bursts: Collisions Between Episodic Magnetic Blobs

Long-Biao Li, Yong-Feng Huang, Jin-Jun Geng +1

Fast radio bursts (FRBs) are bright radio pulses from the sky with millisecond durations and Jansky-level flux densities. Their origins are still largely uncertain. Here we suggest…