Can new heavy gauge bosons be observed in ultra-high energy cosmic neutrino events?
arXiv:1401.6012 · doi:10.1103/PhysRevD.89.077702
Abstract
A wide range of models beyond the Standard Model predict charged and neutral resonances, generically called - and -bosons, respectively. In this paper we study the impact of such resonances on the deep inelastic scattering of ultra-high energy neutrinos as well as on the resonant charged current scattering (Glashow resonance). We find that the effects of such resonances can not be observed with the Pierre Auger Observatory or any foreseeable upgrade of it.
5 pages, 2 figures
References in corpus (8)
- QCDNUM: Fast QCD Evolution and Convolution
- Energy dependent neutrino flavor ratios from cosmic accelerators on the Hillas plot
- Search for Point-Like Sources of Ultra-High Energy Neutrinos at the Pierre Auger Observatory and Improved Limit on the Diffuse Flux of Tau Neutrinos
- LHC Higgs Signatures from Extended Electroweak Gauge Symmetry
- Ultrahigh Energy Neutrinos at the Pierre Auger Observatory
- Discovery and Identification of W' and Z' in SU(2) x SU(2) x U(1) Models at the LHC
- LHC phenomenology of general SU(2)xSU(2)xU(1) models
- Heavy Quark Production in the ACOT Scheme at NNLO and N3LO
Cited by in corpus (7)
- Probing New Physics at Future Tau Neutrino Telescopes
- Electroweak top-quark pair production at the LHC with bosons to NLO QCD in POWHEG
- Probing Heavy Sterile Neutrinos at Ultrahigh Energy Neutrino Telescopes via the Dipole Portal
- Hunting the Glashow Resonance with PeV Neutrino Telescopes
- Double and multiple bangs at tau neutrino telescopes: A novel probe of sphalerons with cosmogenic neutrinos
- Inferring astrophysical neutrino sources from the Glashow resonance
- Probing new physics with high-multiplicity events: UHE neutrinos at air-shower detector arrays