Photons coming from an opaque obstacle as a manifestation of heavy neutrino decays
arXiv:1804.10065 · doi:10.1103/PhysRevD.97.095021
Abstract
Within the framework of physics beyond the standard model we study the possibility that mesons produced in the atmosphere by the cosmic ray flux, decay to heavy Majorana neutrino and these mostly to photons in the low mass region. We study the photon flux produced by sterile Majorana neutrinos () decaying after passing through a massive and opaque object such as a mountain. In order to model the production of 's in the atmosphere and their decay to photons, we consider the interaction between the Majorana neutrinos and the standard matter as modeled by an effective theory. We then calculate the heavy neutrino flux originated by the decay of mesons in the atmosphere. The surviving photon flux, originated by decays, is calculated using transport equations that include the effects of Majorana neutrino production and decay.
arXiv comment21 pages, 6 figures, accepted by Phys. ReV. D. arXiv admin note: text overlap with arXiv:1609.07661
References in corpus (15)
- The Search for Heavy Majorana Neutrinos
- Neutrinos and Collider Physics
- A Search for Electron Neutrino Appearance at the Delta m**2 ~ 1 eV**2 Scale
- Unexplained Excess of Electron-Like Events From a 1-GeV Neutrino Beam
- Patterns of Deviation from the Standard Model
- Heavy neutrino signals at large hadron colliders
- Heavy Majorana Neutrinos in the Effective Lagrangian Description: Application to Hadron Colliders
- Global Constraints on a Heavy Neutrino
- Search for heavy neutrinos at Belle
- Combining Experimental and Cosmological Constraints on Heavy Neutrinos
- Bounds on heavy sterile neutrinos revisited
- Majorana neutrinos production at LHeC in an effective approach
- Majorana neutrino decay in an Effective Approach
- Effective Majorana neutrino decay
- Effects of Majorana Physics on the UHE Flux Traversing the Earth