Boomerang mechanism explaining the excess radio background
arXiv:2509.03441 · doi:10.1103/ncv3-jtnp
Abstract
We propose a boomerang mechanism for the explanation of the excess radio background detected by ARCADE 2. In an early stage of the Universe, at a temperature in the range --, a fraction of relic neutrinos is resonantly converted into dark neutrinos by mixing induced by a pre-existing lepton asymmetry. Dark neutrinos decay much later into a dark-standard photon state and a dark fermion, with a lifetime longer than the age of the Universe, as required by a solution to the excess radio background. This scenario circumvents the upper bound on the neutrino magnetic moment but still implies a testable lower bound.
9 pages, 4 figures; v3: matches version published in PRD;
References in corpus (23)
- Right-Handed Neutrinos at LHC and the Mechanism of Neutrino Mass Generation
- Dark photon limits: a handbook
- Results from the Baksan Experiment on Sterile Transitions (BEST)
- Microwave Background Constraints on Mixing of Photons with Hidden Photons
- Pseudo-Dirac Neutrinos in the New Standard Model
- Reconciling the CAST and PVLAS Results
- Indications for a Nonzero Lepton Asymmetry from Extremely Metal-Poor Galaxies
- Naturally Light Dirac and Pseudo-Dirac Neutrinos from Left-Right Symmetry
- SN1987A still shining: A Quest for Pseudo-Dirac Neutrinos
- Soft logarithms in processes with heavy quarks
- Neutrino Electromagnetic Properties
- Revisiting pseudo-Dirac neutrino scenario after recent solar neutrino data
- Probing Pseudo-Dirac Neutrinos with Astrophysical Sources at IceCube
- A search for an eV-scale sterile neutrino using improved high-energy event reconstruction in IceCube
- DUNE potential as a New Physics probe
- Solar Neutrinos at DARWIN
- Constraining super-light sterile neutrinos at Borexino and KamLAND
- Relic neutrino decay solution to the excess radio background
- Pseudo-Dirac Neutrinos and Relic Neutrino Matter Effect on the High-energy Neutrino Flavor Composition
- Dual-Baseline Search for Active-to-Sterile Neutrino Oscillations in NOvA
- Constraining the pseudo-Dirac nature of neutrinos using astrophysical neutrino flavor data
- A Large Twist Limit for Any Operator
- The optical system of the Tenerife Microwave Spectrometer: a window for observing the 10-20 GHz sky spectra