The recent DESI Baryon Acoustic Oscillation measurements have led to tight upper limits on
the neutrino mass sum, potentially in tension with oscillation constraints requiring $\sum m …

The bimodal distribution of the observed duration of gamma-ray bursts (GRBs) has led to the
identification of two distinct progenitors; compact star mergers, comprising either two neutron …

Abstract Gamma-ray bursts (GRBs), as they are observed at high redshift (z= 9.4), are vital to
cosmological studies and investigating Population III stars. To tackle these studies, we need …

We present photometric and spectroscopic observations of the extraordinary gamma-ray
burst (GRB) 221009A in search of an associated supernova. Some past GRBs have shown …

The division of gamma-ray bursts (GRBs) into different classes, other than the 'short'and
'long', has been an active field of research. We investigate whether GRBs can be classified …

The existence of a secondary (in addition to compact object mergers) source of heavy
element (r-process) nucleosynthesis, the core-collapse of rapidly rotating and highly …

We analyse two distinct samples of gamma-ray bursts (GRBs), with and without radio
afterglow emission. We use an updated sample of 211 GRBs and find, in agreement with …

We present the semi-analytical light curve modelling of 13 supernovae associated with
gamma-ray bursts (GRB-SNe) along with two relativistic broad-lined (Ic-BL) SNe without …

A rapidly spinning, millisecond magnetar is widely considered one of the most plausible
power sources for gamma-ray burst-associated supernovae (GRB-SNe). Recent studies …

The binary-driven hypernova (BdHN) model proposes long gamma-ray bursts (GRBs)
originate in binaries composed of a carbon–oxygen (CO) star and a neutron star (NS) …