Can Dirac neutrinos destabilize $\mathcal{Z}_2$ domain wall network?
Debasish Borah, Partha Kumar Paul, Narendra Sahu

TL;DR
This paper proposes a mechanism where Dirac neutrino masses induce explicit $ ext{Z}_2$ symmetry breaking radiatively, leading to domain wall decay and a gravitational wave signal, linking neutrino physics with cosmological observations.
Contribution
It introduces a novel connection between Dirac neutrino mass generation and domain wall destabilization via radiative effects, impacting gravitational wave predictions.
Findings
Radiative $ ext{Z}_2$ breaking scales inversely with the cube of the Dirac neutrino mass.
Gravitational wave spectrum scales with the sixth power of the Dirac neutrino mass.
Proposes that upcoming experiments can probe a wide range of Dirac seesaw scales.
Abstract
In particle physics model building, a discrete symmetry is often spontaneously broken for phenomenological reasons. When this breaking occurs dynamically in the early Universe, stable domain wall networks are formed, which can eventually dominate the cosmic energy density. To avoid this problem, explicit -breaking terms in the scalar potential are usually introduced in an ad hoc manner. In this Letter, we show that if the same symmetry is also responsible for generating light Dirac neutrino masses, such explicit breaking terms can instead arise radiatively from the particles involved in the Dirac mass generation. We find that the resulting bias term scales inversely with the cube of the Dirac neutrino mass, leading to a gravitational wave spectrum proportional to the sixth power of the Dirac neutrino mass. This establishes a nontrivial…
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Taxonomy
TopicsNeutrino Physics Research · Noncommutative and Quantum Gravity Theories · Quantum Mechanics and Non-Hermitian Physics
