Gamma-ray bursts (GRBs) are divided into two populations,; long GRBs that derive from the
core collapse of massive stars (for example, ref.) and short GRBs that form in the merger of …

It is generally believed that long-duration gamma-ray bursts (GRBs) are associated with
massive star core collapse, whereas short-duration GRBs are associated with mergers of …

The mechanism responsible for the prompt emission of gamma‐ray bursts (GRBs) is still a
debated issue. The prompt phase‐related GRB correlations can allow discriminating among …

For decades, gamma-ray bursts (GRBs) have been broadly divided into long-and short-
duration bursts, lasting more or less than 2 s, respectively. However, this dichotomy does not …

Gamma-ray bursts (GRBs) serve as powerful probes of the early universe, with their
luminous afterglows revealing the locations and physical properties of star-forming galaxies …

On 9 October 2022, the Large High Altitude Air Shower Observatory (LHAASO) reported the
observation of the very early TeV afterglow of the brightest-of-all-time gamma-ray burst …

Gamma-ray bursts (GRBs) have been phenomenologically classified into long and short
populations based on the observed bimodal distribution of duration. Multi-wavelength and …

Abstract Several correlations among Gamma-Ray Bursts (GRBs) quantities, both in the
prompt and afterglow emissions, have been established during the last decades, thus …

The majority of short gamma-ray bursts (SGRBs) are thought to originate from the merger of
compact binary systems collapsing directly to form a black hole. However, it has been …

Well-sampled optical light curves of 146 gamma-ray bursts (GRBs) are compiled from the
literature. By empirical fitting, we identify eight possible emission components and …