Ultra High Energy Neutrino Astronomy
arXiv:astro-ph/0505220 · doi:10.1016/j.nuclphysbps.2005.07.062
Abstract
The short review of theoretical aspects of ultra high energy (UHE) neutrinos and superGZK neutrinos. The sources and diffuse fluxes of UHE neutrinos are discussed. Much attention is given to comparison of the cascade and cosmic ray upper bounds for diffuse neutrino fluxes. Cosmogenic neutrinos and neutrinos from the mirror mater are considered as superGZK neutrinos.
review given at 13th Int. Symposium on VHECR Interactions, Pylos, Sept. 2004
References in corpus (7)
- Experimental Limit on the Cosmic Diffuse Ultra-high Energy Neutrino Flux
- FORTE satellite constraints on ultra-high energy cosmic particle fluxes
- High-Energy Cosmic Rays from Gamma-Ray Bursts
- Fragmentation functions in SUSY QCD and UHECR spectra produced in top-down models
- Limits on diffuse fluxes of high energy extraterrestrial neutrinos with the AMANDA-B10 detector
- Bounds on the cosmogenic neutrino flux
- Neutrinos and gamma-rays of hadronic origin from AGN jets
Cited by in corpus (11)
- The Astrophysics of Ultrahigh Energy Cosmic Rays
- Cosmogenic Neutrinos: parameter space and detectabilty from PeV to ZeV
- High energy neutrino yields from astrophysical sources I: Weakly magnetized sources
- High energy neutrino yields from astrophysical sources II: Magnetized sources
- UHE neutrinos from superconducting cosmic strings
- Cosmic Strings in Hidden Sectors: 2. Cosmological and Astrophysical Signatures
- UHE neutrinos from Pop III stars: concept and constraints
- Probing Very High Energy Prompt Muon and Neutrino fluxes and the cosmic ray knee via Underground Muons
- Ultrahigh Energy Cosmic Rays and Neutrinos
- UHE neutrino astronomy and neutrino oscillations
- Astronomy with ultra high-energy particles