Starburst galaxies, which are known as 'reservoirs' of high-energy cosmic-rays, can
represent an important high-energy neutrino 'factory'contributing to the diffuse neutrino flux …

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 …

Milagro observations have found bright, diffuse TeV emission concentrated along the
galactic plane of the Milky Way. The intensity and spectrum of this emission is difficult to …

A recent analysis of cosmic ray air showers observed at the Pierre Auger Observatory
indicates that nearby starburst galaxies (SBGs) might be the cause of∼ 10% of the Ultra …

High-energy astrophysical neutrinos, with TeV--PeV energies, offer unique insight into
astrophysics and particle physics. Their incoming directions and flavor composition--ie, the …

We present new theoretical modeling to predict the luminosity and spectrum of gamma-ray
and neutrino emission of a star-forming galaxy, from the star formation rate (ψ), gas mass (M …

The discovery of extraterrestrial neutrinos in the∼ 30 TeV–PeV energy range by IceCube
provides new constraints on high energy astrophysics. An important background to the …

The exact sources of high-energy neutrinos detected by the IceCube neutrino observatory
still remain a mystery. For the first time, this work explores the hypothesis that galaxy …

We perform the first one-point fluctuation analysis of the high-energy neutrino sky. This
method reveals itself to be especially suited to contemporary neutrino data, as it allows to …

The origin of diffuse high-energy neutrinos from TeV to PeV energies detected by IceCube
Observatory remains a mystery. In our previous work, we have shown that hadronuclear (pp) …