A phenomenological model is presented to explain the light curves of gamma-ray bursts. Gamma-rays are produced in a narrow beam which sweeps through space due to the precession of a slaved accretion disc. The light curve expected from such a precessing luminosity cone can explain the complex temporal behavior of bright gamma-ray bursts
International audienceWe present hydrodynamic simulations of the hot cocoon produced when a relativi...
International audienceWe develop a model to explain the flaring activity in gamma-ray burst X-ray af...
We calculate light-curves for Gamma-Ray Burst afterglows when material ejected in the explosion is c...
We present an internal shock model with external characteristics for explaining the complicated ligh...
Aims.An extreme Kerr black hole (BH) surrounded by a precessing disk is invoked to explain the light...
An extreme Kerr black hole (BH) surrounded by a precessing disk is invoked to explain the light curv...
Recent observations suggest that gamma ray bursts (GRBs) and their afterglows are produced by highly...
Abstract. The variability of Gamma Ray Bursts (GRBs) light curves at the beginning of GRB event can ...
Because it has been widely accepted that a relativistic description has to be used for modeling all ...
It is widely believed that gamma-ray bursts are produced by a jet-like outflows directed towards the...
We introduce a simple model to explain the time-reversed and stretched residuals in gamma-ray burst ...
The physical origin of the >0.1 GeV emission detected from gamma-ray bursts (GRBs) by the Fermi sate...
We carry out a theoretical investigation of jet propagation in Gamma Ray Bursts and examine the jitt...
We selected a sample of 33 gamma-ray bursts detected by Swift, with known redshift and optical extin...
Abstract Optical and radio afterglows arising from shocks by relativistic conical ejecta running int...
International audienceWe present hydrodynamic simulations of the hot cocoon produced when a relativi...
International audienceWe develop a model to explain the flaring activity in gamma-ray burst X-ray af...
We calculate light-curves for Gamma-Ray Burst afterglows when material ejected in the explosion is c...
We present an internal shock model with external characteristics for explaining the complicated ligh...
Aims.An extreme Kerr black hole (BH) surrounded by a precessing disk is invoked to explain the light...
An extreme Kerr black hole (BH) surrounded by a precessing disk is invoked to explain the light curv...
Recent observations suggest that gamma ray bursts (GRBs) and their afterglows are produced by highly...
Abstract. The variability of Gamma Ray Bursts (GRBs) light curves at the beginning of GRB event can ...
Because it has been widely accepted that a relativistic description has to be used for modeling all ...
It is widely believed that gamma-ray bursts are produced by a jet-like outflows directed towards the...
We introduce a simple model to explain the time-reversed and stretched residuals in gamma-ray burst ...
The physical origin of the >0.1 GeV emission detected from gamma-ray bursts (GRBs) by the Fermi sate...
We carry out a theoretical investigation of jet propagation in Gamma Ray Bursts and examine the jitt...
We selected a sample of 33 gamma-ray bursts detected by Swift, with known redshift and optical extin...
Abstract Optical and radio afterglows arising from shocks by relativistic conical ejecta running int...
International audienceWe present hydrodynamic simulations of the hot cocoon produced when a relativi...
International audienceWe develop a model to explain the flaring activity in gamma-ray burst X-ray af...
We calculate light-curves for Gamma-Ray Burst afterglows when material ejected in the explosion is c...
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