Abstract

A standing problem in neutrino physics is the consistent and universal definition of oscillating neutrino states as coherent superpositions of massive neutrino states. This problem is solved in a quantum field theoretical framework of neutrino mixing developed in analogy with the Nambu–Jona–Lasinio model for the dynamical generation of nucleon masses. The massive neutrino states are Bogoliubov quasiparticles and their vacuum is a condensate of “Cooper pairs” of massless flavour neutrinos. Their superpositions as oscillating neutrino states have intrinsic quantum coherence by construction. In this quantization framework, the standard phenomenological flavour neutrino states and oscillation probability formula are validated in the ultrarelativistic approximation.

Highlights

  • The discovery of neutrino oscillations [1,2] is the most prominent achievement of physics beyond the Standard Model

  • A standing problem in neutrino physics is the consistent and universal definition of oscillating neutrino states as coherent superpositions of massive neutrino states. This problem is solved in a quantum field theoretical framework of neutrino mixing developed in analogy with the Nambu–Jona–Lasinio model for the dynamical generation of nucleon masses

  • Neutrino oscillations were predicted long ago [3,4,5,6] and their standard theoretical description has been developed in the framework of quantum mechanics [7,8,9,10,11,12]

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Summary

Introduction

The discovery of neutrino oscillations [1,2] is the most prominent achievement of physics beyond the Standard Model. This phenomenon signals the fact that neutrinos are massive and they mix coherently, in contrast with the Standard Model massless neutrinos. For simplicity and clarity of the exposition, we shall consider throughout this paper the mixing of two families of Dirac neutrinos. The propagating massive states develop a time-dependent phase difference, such that an electron neutrino is turned, after a macroscopic distance of propagation, into a muon neutrino. Where E is the energy of the neutrinos in the beam and L is the distance between the neutrino production and detection

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Phenomenological definitions of flavour neutrino states
Universal oscillating neutrino states
Massive neutrinos as Bogoliubov quasiparticles
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Oscillating neutrino states and their transition probability
Outlook
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Full Text
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