Preprint Article Version 1 Preserved in Portico This version is not peer-reviewed

Production of Tachyonic Neutrino in Matter

Version 1 : Received: 4 December 2019 / Approved: 5 December 2019 / Online: 5 December 2019 (11:14:58 CET)

How to cite: Nanni, L. Production of Tachyonic Neutrino in Matter. Preprints 2019, 2019120067. Nanni, L. Production of Tachyonic Neutrino in Matter. Preprints 2019, 2019120067.


Recently, a new theory based on superluminal tunnelling has been proposed to explain the transition of highly energetic neutrinos propagating in matter to tachyonic states. In this work, we determine the possible mechanisms that lead neutrinos into a superluminal realm based on the assumption that ultrarelativistic particles travelling in matter lose part of their energy with the emission of Bremsstrahlung radiation. The obtained photons, in turn, can create neutrino-antineutrino pairs, one or both of which can be superluminal. We also prove that pair creation may occur with neutrino flavour oscillation provided that only one of them is a space-like particle. This suggests that mass oscillation and superluminal behaviour could be related phenomena. Finally, using the generalised Lorentz transformations, we formulate the Lagrangian of the kinematically allowed scattering processes. The structure of this Lagrangian is consistent with the formalism of the Standard Model. Based on this Lagrangian, at least one of the particles forming the pair must always be subluminal. The possibility that the pair creation process is mediated by a dark photon is also discussed.


superluminal neutrino; quantum tunnelling; mass oscillation; generalised Lorentz transformations


Physical Sciences, Optics and Photonics

Comments (0)

We encourage comments and feedback from a broad range of readers. See criteria for comments and our Diversity statement.

Leave a public comment
Send a private comment to the author(s)
* All users must log in before leaving a comment
Views 0
Downloads 0
Comments 0
Metrics 0

Notify me about updates to this article or when a peer-reviewed version is published.
We use cookies on our website to ensure you get the best experience.
Read more about our cookies here.