Bi-maximal Neutrino Mixing Pattern Reexamined
Zhi-zhong Xing

TL;DR
This paper revisits the bi-maximal neutrino mixing pattern, proposing a simple extension that incorporates small couplings and large CP violation, aligning with key solar neutrino solutions.
Contribution
It introduces a minimal extension to the bi-maximal mixing model, enabling compatibility with solar neutrino observations and CP violation effects.
Findings
Compatible with vacuum and large-angle MSW solar solutions
Allows large CP violation in neutrino oscillations
Provides a more flexible neutrino mixing framework
Abstract
I propose a simple extension of the bi-maximal neutrino mixing pattern, allowing slight coupling between solar and atmospheric neutrino oscillations as well as large CP violation. The new scenario is compatible with either the vacuum oscillation solution or the large-angle MSW solution to the solar neutrino
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.
