Author pages are created from data sourced from our academic publisher partnerships and public sources.
- Publications
- Influence
Share This Author
The association of GRB 060218 with a supernova and the evolution of the shock wave
- S. Campana, V. Mangano, N. White
- PhysicsNature
- 31 August 2006
TLDR
Low-Luminosity Gamma-Ray Bursts as a Unique Population: Luminosity Function, Local Rate, and Beaming Factor
- E. Liang, Bing Zhang, F. Virgili, Z. Dai
- Physics
- 8 May 2006
Swift BAT has detected ~200 long-duration GRBs, with redshift measurements for ~50 of them. We derive the luminosity function (?HL) and the local event rate (?) of the conventional high-luminosity…
Afterglow Emission from Highly Collimated Jets with Flat Electron Spectra: Application to the GRB 010222 Case?
We derive light curves of the afterglow emission from highly collimated jets if the power-law index (p )o f the electron energy distribution is above 1 but below 2. We find the following: (1) Below…
The Observer's Guide to the Gamma-Ray Burst-Supernova Connection
- Z. Cano, Shan-Qin Wang, Z. Dai, Xue-Feng Wu
- Physics
- 12 April 2016
We present a detailed report of the connection between long-duration gamma-ray bursts (GRBs) and their accompanying supernovae (SNe). The discussion presented here places emphasis on how…
X-ray Flares from Postmerger Millisecond Pulsars
- Z. Dai, X. Y. Wang, X. Wu, B. Zhang
- PhysicsScience
- 23 February 2006
TLDR
Gamma-ray burst afterglows: effects of radiative corrections and non-uniformity of the surrounding medium
The afterglow of a gamma-ray burst (GRB) is commonly thought to be the result of continuous deceleration of a relativistically expanding fireball in the surrounding medium. Assuming that the…
Gamma-ray bursts and afterglows from rotating strange starsand neutron stars
We here discuss a new model of $\gamma$-ray bursts (GRBs) based on differentially rotating strange stars. Strange stars in this model and differentially rotating neutron stars in the…
Overall Evolution of Jetted Gamma-ray Burst Ejecta
- Y. F. Huang, L. Gou, Z. Dai, T. Lu
- Physics
- 27 October 1999
Whether gamma-ray bursts are highly beamed or not is a very difficult but important problem that we are confronted with. Some theorists suggest that beaming effect usually leads to a sharp break in…
The afterglow of GRB 990123 and a dense medium
Recent observations show that the temporal decay of the R-band afterglow from GRB 990123 steepened about 2.5 days after the burst. We here propose a possible explanation for such a steepening: a…
A GENERIC DYNAMICAL MODEL OF GAMMA-RAY BURST REMNANTS
- Y. F. Huang, Z. Dai, T. Lu
- Physics
- 24 June 1999
The conventional generic model is deemed to explain the dynamics of $\gamma$-ray burst remnants very well, no matter whether they are adiabatic or highly radiative. However, we find that for…
...
1
2
3
4
5
...