Observational information on high-energy astrophysical neutrinos is being continuously
collected by the IceCube observatory. However, the sources of the neutrinos are still …

We present predictions for the interactions of energetic neutrinos with matter as they
propagate through Earth towards large-volume detectors. Our results are based on state-of …

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 …

Based on high quality surgery and scientific data, scientists and surgeons are committed to
protecting patients as well as healthcare staff and hereby provide this Guidance to address …

Tau neutrinos are expected to comprise roughly one third of both the astrophysical and
cosmogenic neutrino flux, but currently the flavor ratio is poorly constrained and the …

Tau neutrinos are unique cosmic messengers, especially at extreme energies. When they
undergo a charged-current interaction, the short lifetime of the produced tau gives rise to …

We scrutinize the paradigm that conventional long-duration gamma-ray bursts (GRBs) are
the dominant source of the ultrahigh energy cosmic rays (UHECRs) within the internal shock …

A bstract In scenarios with large extra dimensions (LEDs), the fundamental Planck scale can
be low enough that collisions between high-energy particles may produce microscopic black …

On 2017 September 22, a through-going muon that deposited 23.7 TeV was detected at the
IceCube telescope (Aartsen et al. 2017) in Antarctica, likely to be produced by a neutrino …

We present a semianalytical method for the calculation of coherent Askaryan radiation in
showers induced by neutrinos of any flavor in ice. We compare our results with those of a full …