Prediction of the CP Phase δCP in Neutrino Oscillation and an Axion-less Solution to the Strong CP Problem

Abstract A model of the axion-less solution to the strong CP problem has recently been constructed based on the $\bf T^2/\mathbb {Z}_3$ orbifold in six-dimensional space-time. We extend, in this paper, the model to include the lepton sector with three right-handed neutrinos (RHNs). A crucial point in the extended model is that we have only one CP-violating phase and thus the CP phase in neutrino oscillation can be predicted by the CP phase in the Cabibbo–Kobayashi–Maskawa (CKM) matrix. The CP phase $\delta _{\mathrm{ CP}}$ in the Pontecorvo–Maki–Nakagawa–Sakata matrix (PMNS) matrix is predicted as $\delta _{\mathrm{ CP}}\simeq 192^\circ \!-\! 195^\circ$, which can be tested in near-future experiments. We also discuss the effective mass $m_{\beta \beta }$ responsible for the neutrinoless double beta decay of the nucleus, which is predicted as $m_{\beta \beta } \simeq 8 \!-\! 11$ meV. We consider leptogenesis and confirm that our model generates the right sign of the baryon asymmetry if the first family RHN is the lightest among the heavy RHNs.

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Publication Details

Journal
Progress of Theoretical and Experimental Physics
Published
2025-02-22
DOI
https://doi.org/10.1093/ptep/ptae177
Primary Topic
Dark Matter and Cosmic Phenomena
Type
article
Field-Weighted Citation Impact
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article

Prediction of the CP Phase δCP in Neutrino Oscillation and an Axion-less Solution to the Strong CP Problem

Tsutomu T. Yanagida, M. Tanimoto
Progress of Theoretical and Experimental Physics
Dark Matter and Cosmic Phenomena
article

Prediction of the CP Phase δCP in Neutrino Oscillation and an Axion-less Solution to the Strong CP Problem

Tsutomu T. Yanagida, M. Tanimoto
article en

Abstract

Abstract A model of the axion-less solution to the strong CP problem has recently been constructed based on the $\bf T^2/\mathbb {Z}_3$ orbifold in six-dimensional space-time. We extend, in this paper, the model to include the lepton sector with three right-handed neutrinos (RHNs). A crucial point in the extended model is that we have only one CP-violating phase and thus the CP phase in neutrino oscillation can be predicted by the CP phase in the Cabibbo–Kobayashi–Maskawa (CKM) matrix. The CP phase $\delta _{\mathrm{ CP}}$ in the Pontecorvo–Maki–Nakagawa–Sakata matrix (PMNS) matrix is predicted as $\delta _{\mathrm{ CP}}\simeq 192^\circ \!-\! 195^\circ$, which can be tested in near-future experiments. We also discuss the effective mass $m_{\beta \beta }$ responsible for the neutrinoless double beta decay of the nucleus, which is predicted as $m_{\beta \beta } \simeq 8 \!-\! 11$ meV. We consider leptogenesis and confirm that our model generates the right sign of the baryon asymmetry if the first family RHN is the lightest among the heavy RHNs.

Progress of Theoretical and Experimental PhysicsVol. 2025(3)
Kavli Institute for the Physics and Mathematics of the Universe (JP), Shanghai Jiao Tong University (CN), Kavli Institute for the Physics and Mathematics of the Universe (JP), Institute of Natural Science (KP), Niigata University (JP), The University of Tokyo (JP)
Openalex Percentile: Top 98%
Dark Matter and Cosmic Phenomena
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