Astrophysical neutrinos are excellent probes of astroparticle physics and high-energy
physics. With energies far beyond solar, supernovae, atmospheric, and accelerator …

Gamma-ray bursts (GRBs) have long been considered a possible source of high-energy
neutrinos. While no correlations have yet been detected between high-energy neutrinos and …

The Askaryan Radio Array (ARA) is an ultrahigh energy (UHE,> 10 17 eV) neutrino detector
designed to observe neutrinos by searching for the radio waves emitted by the relativistic …

The brightest long gamma-ray burst (GRB) detected so far by the Swift-BAT and Fermi-GBM
telescopes, GRB 221009A, provides an unprecedented opportunity for understanding the …

Some afterglow light curves of gamma-ray bursts (GRBs) exhibit very complex temporal and
spectral features, such as a sudden intensity jump about one hour after the prompt emission …

Gamma-ray bursts (GRBs) are the most luminous electromagnetic burst in the Universe.
They occur when a rapidly rotating massive star collapses or a binary neutron star merges …

Synchrotron radiation from a decelerating blastwave is a widely accepted model of radio to
X-ray afterglow emission from gamma-ray bursts (GRBs). GeV gamma-ray emission …

Abstract The ANtarctic Impulsive Transient Antenna (ANITA) long-duration balloon
experiment is sensitive to interactions of ultrahigh-energy (E> 10 18 eV) neutrinos in the …

We explore the possibility that high-energy (HE) neutrinos produced from choked jets can be
annihilated with low-energy neutrinos emitted from the accretion disk around a black hole in …

The electron antinuetrino flux limits are presented for the brightest gamma-ray burst (GRB) of
all time, GRB221009A, over a range of 1.8-200 MeV using the Kamioka Liquid Scintillator …