Relic neutrino masses and the highest energy cosmic rays
- 1 June 2002
- journal article
- Published by Springer Nature in Journal of High Energy Physics
- Vol. 2002 (6) , 046
- https://doi.org/10.1088/1126-6708/2002/06/046
Abstract
No abstract availableKeywords
All Related Versions
This publication has 100 references indexed in Scilit:
- Constraints on the ultrahigh-energy photon flux using inclined showers from the Haverah Park arrayPhysical Review D, 2002
- A C++ code to solve the DGLAP equations applied to Ultra High Energy Cosmic RaysComputer Physics Communications, 2002
- In quest of neutrino masses atO(eV)scalePhysical Review D, 2002
- Expected signals in relic neutrino detectorsPhysical Review D, 2001
- Monte Carlo simulation for jet fragmentation in SUSY QCDPhysical Review D, 2001
- Ultrahigh energy neutrinos from hidden-sector topological defectsPhysical Review D, 2000
- Cosmic-ray neutrino annihilation on relic neutrinos revisited: a mechanism for generating air showers above the Greisen-Zatsepin-Kuzmin cutoffAstroparticle Physics, 1999
- Ultra–High‐Energy Neutrino Scattering onto Relic Light Neutrinos in the Galactic Halo as a Possible Source of the Highest Energy Extragalactic Cosmic RaysThe Astrophysical Journal, 1999
- Propagation of ultra high energy protons and gamma rays over cosmological distances and implications for topological defect modelsAstroparticle Physics, 1996
- High-energy-physics event generation with PYTHIA 5.7 and JETSET 7.4Computer Physics Communications, 1994