arXiv · 1209.5630
Explanation for the low flux of high energy astrophysical muon-neutrinos
Abstract
We consider the possibility that some exotic neutrino property is responsible for reducing the muon neutrino flux at high energies from distant neutrino sources; specifically, we consider (i) neutrino decay and (ii) neutrinos being pseudo-Dirac particles. This would provide a mechanism for the lack of high energy muons in the Icecube detector.
Explore related subjects
Keep this discovery
Sandip Pakvasa, Anjan Joshipura, Subhendra Mohanty. 2012-09-25. Explanation for the low flux of high energy astrophysical muon-neutrinos. https://doi.org/10.1103/physrevlett.110.171802
Cite the original work for its findings. Save a collection to share your selection of sources.