We apply the synchro-curvature mechanism instead of the synchrotron one to explain the spectra of gamma-ray bursts (hereafter, GRBs), especially those with both a turnoff point and high energy excess, which are often explained by combining with some other processes. We fit several spectra and get very good results. Our mechanism can give more detailed descriptions of the magnetic fields and strict constraints on the formation mechanism, thus it is helpful for understanding the physical processes in GRBs
Relativistic blast wave models of Gamma Ray Bursts (GRB) predict the spectrum of the emitted synchro...
Context. Gamma-ray burst emission in the prompt phase is often interpreted as synchrotron ...
We propose a model for the spectral formation of gamma-ray burst (GRB) prompt emission, where the ph...
We apply the synchro-curvature mechanism instead of the synchrotron one to explain the spectra of ga...
The extreme physical conditions of Gamma Ray Bursts can constitute a useful observational laboratory...
AbstractThe extreme physical conditions of Gamma Ray Bursts can constitute a useful observational la...
Context. We study the sharpness of the time-resolved prompt emission spectra of gamma-ray bursts (GR...
Gamma-ray bursts (GRBs) are the most energetic electromagnetic sources in the Universe, releasing 10...
Although much progress has been made in our understanding of gamma-ray bursts (GRBs) and their after...
We discuss here constraints on the particle acceleration models from the observed gamma-ray bursts s...
Detailed information on the physical parameters in the sources of cosmological Gamma-Ray Bursts (GRB...
Detailed information on the physical parameters in the sources of cosmological Gamma-Ray Bursts (GRB...
Context. The peak energy (Ep) exhibited during the prompt emission phase of gamma-ray bursts (GRBs) ...
International audienceContext. Gamma-ray burst emission in the prompt phase is often interpreted as ...
Observations from BATSE show that the spectra of gamma-ray bursts are very wide, which cannot be des...
Relativistic blast wave models of Gamma Ray Bursts (GRB) predict the spectrum of the emitted synchro...
Context. Gamma-ray burst emission in the prompt phase is often interpreted as synchrotron ...
We propose a model for the spectral formation of gamma-ray burst (GRB) prompt emission, where the ph...
We apply the synchro-curvature mechanism instead of the synchrotron one to explain the spectra of ga...
The extreme physical conditions of Gamma Ray Bursts can constitute a useful observational laboratory...
AbstractThe extreme physical conditions of Gamma Ray Bursts can constitute a useful observational la...
Context. We study the sharpness of the time-resolved prompt emission spectra of gamma-ray bursts (GR...
Gamma-ray bursts (GRBs) are the most energetic electromagnetic sources in the Universe, releasing 10...
Although much progress has been made in our understanding of gamma-ray bursts (GRBs) and their after...
We discuss here constraints on the particle acceleration models from the observed gamma-ray bursts s...
Detailed information on the physical parameters in the sources of cosmological Gamma-Ray Bursts (GRB...
Detailed information on the physical parameters in the sources of cosmological Gamma-Ray Bursts (GRB...
Context. The peak energy (Ep) exhibited during the prompt emission phase of gamma-ray bursts (GRBs) ...
International audienceContext. Gamma-ray burst emission in the prompt phase is often interpreted as ...
Observations from BATSE show that the spectra of gamma-ray bursts are very wide, which cannot be des...
Relativistic blast wave models of Gamma Ray Bursts (GRB) predict the spectrum of the emitted synchro...
Context. Gamma-ray burst emission in the prompt phase is often interpreted as synchrotron ...
We propose a model for the spectral formation of gamma-ray burst (GRB) prompt emission, where the ph...