Neutrino Pair Emission from Excited Atoms
arXiv:hep-ph/0611362 · doi:10.1103/PhysRevD.75.113007
Abstract
We explore a possibility of measuring the magnitude and the Majorana nature of neutrino masses, by using a novel process of neutrino pair emission from excited atoms. Except lepton number non-conserving processes, the neutrino pair () emission is the unique process to distinguish the Majorana neutrino from the Dirac neutrino. The small energy difference between atomic levels makes it easier to measure small neutrino masses as indicated by neutrino oscillation experiments. The crucial point is how to enhance the rate of pair emission without enhancing the radiative decay. We have in mind two particular cases; (1) laser irradiated pair emission from metastable atoms, and (2) microwave irradiated emission from circular Rydberg states. A new mechanism of the parametric amplification to enhance the neutrino pair emission is pointed out when Rydberg atoms are irradiated by microwave, while the radiative process may be inhibited by the cavity QED effect. A great variety of measurable neutrino parameters and a variety of experimental methods are conceivable.
56 pages, 1 figure added showing the rate. 2 notes added in the end. Several typos are corected from the previous version
Cited by in corpus (15)
- Predicting the Values of the Leptonic CP Violation Phases
- Limits on the cosmic neutrino background
- Experimental method of detecting relic neutrino by atomic de-excitation
- Solitons and Precision Neutrino Mass Spectroscopy
- Inferring the nature of active neutrinos: Dirac or Majorana?
- Probing Light Mediators in the Radiative Emission of Neutrino Pair
- Effect of Relic Neutrino on Neutrino Pair Emission from Metastable Atoms
- Unique Probe of Neutrino Electromagnetic Moments with Radiative Pair Emission
- Radiative Emission of Neutrino Pairs in Atoms and Light Sterile Neutrinos
- Practical Dirac Majorana confusion theorem: Issues and Applicability
- Disentangle Neutrino Electromagnetic Properties with Atomic Radiative Pair Emission
- Neutrino-2008: Where are we? Where are we going?
- Parity violating radiative emission of neutrino pair in heavy alkaline earth atoms of even isotopes
- Parity violating magnetization at neutrino pair emission using trivalent lanthanoid ions
- Probing Cosmic Neutrino Background through Parametric Fluorescence