11–13 May 2026
University of Pittsburgh
US/Eastern timezone

Gravitational Waves from an A4 Neutrino Mass Model

11 May 2026, 16:30
15m
David Lawrence Hall 203, University of Pittsburgh

David Lawrence Hall 203, University of Pittsburgh

Gravitational Waves and Particle Physics Gravitational Waves

Speaker

Cameron Moffett-Smith

Description

The $A_4$ flavor symmetry has provided tremendous insight into the flavor structure of the lepton sector of the Standard Model, predicting a very good approximation to neutrino mixing angles called tri-bimaximal mixing (TBM). $A_4$ is spontaneously broken by a scalar called the flavon, and when this happens a number of degenerate vacua can form, resulting in so-called domain walls. These objects are not observed and hence need to be annihilated. This is usually done by explicitly breaking $A_4$ by adding a bias term to the scalar potential. In this paper, we construct a new model invariant under $A_4 \times \mathbb{Z}_4$ which creates cosmologically viable domain walls, lifts the degeneracy of the vacuum giving a natural mechanism for domain walls to annihilate, as well as predicts realistic neutrino mixing angles; all utilizing cross couplings between flavons. The annihilation of the domain walls, with proper choice of wall tension and the consequent bias term, leads to a gravitational wave signal that is potentially detectable in near future gravitational wave experiments, and interestingly intersects with the observed Pulsar Timing Array signal.

Authors

Cameron Moffett-Smith Prof. Mu-Chun Chen (University of California - Irvine)

Presentation materials

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