Energy-independent new physics in the flavour ratios of high-energy astrophysical neutrinos

DOI10.1007/JHEP04(2010)066zbMath1272.83091arXiv1001.4878WikidataQ59254748 ScholiaQ59254748MaRDI QIDQ367776

Mohammad Hasan, M. Dambrine, H. S. Yoon

Publication date: 16 September 2013

Published in: Journal of High Energy Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1001.4878

zbMATH Keywords

discrete and finite symmetriesbeyond standard modelneutrino physics

Mathematics Subject Classification ID

Unified quantum theories (81V22) Relativistic cosmology (83F05) Symmetry breaking in quantum theory (81R40) Finite-dimensional groups and algebras motivated by physics and their representations (81R05) Weak interaction in quantum theory (81V15) Radiative transfer in astronomy and astrophysics (85A25)

Related Items (2)

Neutrinos from cosmic accelerators including magnetic field and flavor effects ⋮ SUSY renormalization group effects in ultra high energy neutrinos

Uses Software

• MACRO detector

Cites Work

• An analysis of cosmic neutrinos: flavor composition at source and neutrino mixing parameters
• HIGH ENERGY ASTROPHYSICAL NEUTRINO FLUX AND MODIFIED DISPERSION RELATIONS
• INTRINSIC AND OSCILLATED ASTROPHYSICAL NEUTRINO FLAVOR RATIOS REVISITED

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