Tachyonic Majorana neutrinos or neutrino spin-to-orbital angular momentum conversion in OPERA
M. Laveder, F. Tamburini, ((1) Department of Physics, Astronomy,, University of Padova, via Marzolo 8, Padova, Italy, INFN - Sezione di, Padova - (2) Department of Physics, Astronomy, University of Padova, via, Marzolo 8, Padova, Italy, CIVEN, Venezia)

TL;DR
This paper discusses the OPERA experiment's data supporting the existence of tachyonic Majorana neutrinos with imaginary mass and explores neutrino spin-to-orbital angular momentum conversion phenomena.
Contribution
It presents a phenomenological model of Majorana neutrinos with imaginary mass and compares simulation results with OPERA data, supporting tachyonic neutrino behavior.
Findings
Good agreement between simulations and OPERA data.
Confirmation of tachyonic behavior in neutrinos.
Discussion of spin-to-orbital angular momentum conversion.
Abstract
The new data release of OPERA - CNGS experiment, obtained with a shorter spill of protons, confirms the tachyionic behavior expected from the phenomenological model of a Majorana neutrino with a fictitious imaginary mass term acquired during the propagation in the Earth's crust, recently presented by us. We performed numerical simulations of neutrino event detections to compare the properties of these Majorana tachyons with the new OPERA results, finding a good agreement. The possibility of spin-to orbital angular momentum conversion that is expected to give a negative squared mass in a medium, is also briefly discussed.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Neutrino Physics Research · Particle physics theoretical and experimental studies
