The origin of high-energy cosmic rays, and their behavior in astrophysical sources, remains
an open question. Recently, new ways to address this question have been made possible …

The IceCube collaboration pioneered the detection of Script O (PeV) neutrino events and the
identification of astrophysical sources of high-energy neutrinos. In this study, we explore …

The flavor composition of TeV--PeV astrophysical neutrinos, ie, the proportion of neutrinos of
different flavors in their flux, is a versatile probe of high-energy astrophysics and …

The decay of asymmetric dark matter (ADM) can lead to distinct neutrino signatures
characterized by an asymmetry between neutrinos and antineutrinos. In the high-energy …

The three Standard Model neutrinos can have Majorana mass or strictly Dirac mass, but
both scenarios are practically indistinguishable in neutrino oscillation experiments. If they …

We show that high-energy astrophysical neutrinos produced in the cores of heavily
obscured active galactic nuclei (AGNs) can undergo strong matter effects, thus significantly …

The in-ice or in-water Cherenkov neutrino telescope such as IceCube has already proved its
power in measuring the Glashow resonance by searching for the bump around …

The IceCube collaboration pioneered the detection of O (PeV) neutrino events and the
identification of astrophysical sources of high-energy neutrinos. In this study, we explore …

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 …

In the past decades, many experiments have been built to detect neutrinos and learn about
their properties. An example is IceCube, which, with its extraordinary volume, measured a …