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

Ultra-high-energy (UHE) cosmic neutrinos, with energies above 100~ PeV, could be finally
discovered in the near future. Measuring their flavor composition would reveal information …

The next generation gravitational wave (GW) detectors—Einstein Telescope (ET) and
Cosmic Explorer (CE)—will have distance horizons up to O (10) Gpc for detecting binary …

The origin of the observed diffuse neutrino flux is not yet known. Studies of the relative
flavour content of the neutrino flux detected at Earth can give information on the production …

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 …

We perform the fit to the structure function\(F_2\) data from HERA including terms due to the
resummation at small x. The equation for the unintegrated gluon density is solved …

The observation of ultra-high-energy EeV-energy cosmogenic neutrinos provides a direct
path to identifying the sources of the highest energy cosmic rays; searches have so far …

Ultrahigh-energy neutrinos (UHE $\nu $ s) can be used as a valuable probe of superheavy
dark matter above $\sim 10^ 9$ GeV, the latter being difficult to probe with collider and direct …

The IceCube collaboration pioneered the detection of $\mathcal {O}{(\text {PeV})} $ neutrino
events and the identification of astrophysical sources of high-energy neutrinos. In this study …

The IceCube collaboration pioneered the detection of $\mathcal {O}{(\text {PeV})} $ neutrino
events and the identification of astrophysical sources of high-energy neutrinos. In this study …