6533b830fe1ef96bd1297cea

RESEARCH PRODUCT

Revisiting pseudo-Dirac neutrinos

Jukka MaalampiJukka MaalampiK.r.s. BalajiAnna Kalliomäki

subject

PhysicsNuclear and High Energy PhysicsParticle physics010308 nuclear & particles physicsDirac (video compression format)Operator (physics)Physics beyond the Standard ModelDark matterHigh Energy Physics::PhenomenologyFOS: Physical sciencesContext (language use)01 natural sciencesCosmologyMAJORANAHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesHigh Energy Physics::ExperimentNeutrino010306 general physics

description

We study the pseudo-Dirac mixing of left and right-handed neutrinos in the case where the Majorana masses M_L and M_R are small when compared with the Dirac mass, M_D. The light Majorana masses could be generated by a non-renormalizable operator reflecting effects of new physics at some high energy scale. In this context, we obtain a simple model independent closed bound for M_D. A phenomenologically consistent scenario is achieved with M_L,M_R ~ 10^{-7} eV and M_D ~ 10^{-5}-10^{-4} eV. This precludes the possibility of positive mass searches in the planned future experiments like GENIUS or in tritium decay experiments. If on the other hand, GENIUS does observe a positive signal for a Majorana mass \geq 10^{-3} eV, then with very little fine tuning of neutrino parameters, the scale of new physics could be in the TeV range, but pseudo-Dirac scenario in that case is excluded. We briefly discuss the constraints from cosmology when a fraction of the dark matter is composed of nearly degenerate neutrinos.

https://dx.doi.org/10.48550/arxiv.hep-ph/0110314