Neutrino capture on tritium as a probe of flavor vacuum condensate and dark matter
arXiv:2205.09640 · doi:10.1016/j.physletb.2023.137776
Abstract
We show that the study of neutrino capture on tritium, for non-relativistic neutrinos, can allow to distinguish among the various neutrino models, eventually prove the quantum field theory condensation effects and permit to test the hypothesis according to which the flavor vacuum energy gives a contribution to the dark matter of the universe. Indeed, we show that the capture rate depends on the neutrino model considered, and that it brings an imprint of the flavor vacuum condensate. Experiments like PTOLEMY, designed to reveal the cosmic neutrino background, then can give an indication of the existence of the dark matter component induced by neutrino mixing.
11 pages, 2 figures
References in corpus (12)
- Neutrino mixing as a source of dark energy
- Einstein, Planck and Vera Rubin: relevant encounters between the Cosmological and the Quantum Worlds
- Dark energy and particle mixing
- Neutrinos in curved spacetimes: particle mixing and flavor oscillations
- Revealing neutrino nature and violation with decoherence effects
- Detecting the radiative decay of the cosmic neutrino background with line-intensity mapping
- The flavor vacuum in the expanding universe and dark matter
- Neutron Interferometry and axion like particles
- Probing dark matter and quantum field theory effects with Rydberg atoms
- Beyond the MSW effect: Neutrinos in a dense medium
- Boson mixing and flavor oscillations in curved space-time
- Precise Capture Rates of Cosmic Neutrinos and Their Implications on Cosmology
Cited by in corpus (3)
- Saez-Ballester gravity in Kantowski-Sachs Universe: a new reconstruction paradigm for Barrow Holographic Dark Energy
- Generalized interacting Barrow Holographic Dark Energy: cosmological predictions and thermodynamic considerations
- Lagrangian reconstruction of Barrow holographic dark energy in interacting tachyon model