Cascades from ultra-high-energy neutrinos
astro-ph.HE, hep-ph
Submitted: 2026-08-31
Updated: 2026-08-31
Comments: 28 pages, 11 figures. To be submitted to JCAP. Comments are welcomed!
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Neutrino-driven Explosions
- The NuMoon experiment: first results
- Trinity: An Imaging Air Cherenkov Telescope to Search for Ultra-High-Energy Neutrinos
- Generation of TeV Photons by PeV Neutrinos in Dense Astrophysical Environments
- Observational strategies for ultrahigh-energy neutrinos: the importance of deep sensitivity for detection and astronomy
- Upper Bound on the Energy of Particles and Their Secondary Neutrinos
- Testing Heavy Dark Matter Decay as the Origin of KM3-230213A
- A search for photons with energies above $2{\times}10^{17}$ eV using hybrid data from the low-energy extensions of the Pierre Auger Observatory
- Cosmological implications of photon-flux upper limits at ultra-high energies in scenarios of Planckian-interacting massive particles for dark matter
- Automatized One-Loop Calculations in 4 and D dimensions
- FormCalc 9 and Extensions
- Recola2: REcursive Computation of One-Loop Amplitudes 2
- One-loop leading logarithms in electroweak radiative corrections, I. Results
- One-loop leading logarithms in electroweak radiative corrections: II. Factorization of collinear singularities
- One-loop electroweak Sudakov logarithms: a revisitation and automation
- Probing the Cosmic Neutrino Background and New Physics with TeV-Scale Astrophysical Neutrinos
- Precise predictions for multi-${\rm TeV}$ and ${\rm PeV}$ energy neutrino scattering rates
- Cuba - a library for multidimensional numerical integration
- Concurrent Cuba
Related papers
- Accreting Neutron Stars in Low-Mass X-ray Binaries
- Numerical Studies of Accretion Flows onto a Neutron Star Engulfed in a Massive Star
- Early panchromatic spectra reveal helium in the thermonuclear supernova 2024kce
- Multiwavelength Classification of Chandra Sources in Omega Centauri
- Impact of the equation of state on core collapse supernovae I: the low- T/W instability
- Secular Evolution of Quasiperiodic Eruptions: eRO-QPE2