Journal
JOURNAL OF HIGH ENERGY PHYSICS
Volume -, Issue 4, Pages -Publisher
SPRINGER
DOI: 10.1007/JHEP04(2022)105
Keywords
Baryo-and Leptogenesis; Supersymmetry; Cosmology of Theories BSM; Early Universe Particle Physics
Categories
Funding
- JSPS KAKENHI [20H05851, 20K22344, 21K13910]
- World Premier International Research Center Initiative (WPI Initiative), MEXT, Japan
- JSPS [20J12415]
- Natural Science Foundation of China [12150610465]
- Leading Initiative for Excellent Young Researchers, MEXT, Japan
- Grants-in-Aid for Scientific Research [21K13910, 20J12415, 20K22344] Funding Source: KAKEN
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In this study, a supersymmetric Nelson-Barr mechanism is shown to naturally accommodate the Affleck-Dine baryogenesis within a CP-invariant Lagrangian. The model also addresses the strong CP problem and the baryon asymmetric Universe. Furthermore, it solves the electroweak naturalness problem and predicts the existence of dark matter, making it a compelling paradigm beyond the Standard Model.
Spontaneous CP violation, such as the Nelson-Barr (NB) mechanism, is an attractive scenario for addressing the strong CP problem while realizing the observed phase of the Cabibbo-Kobayashi-Maskawa (CKM) quark-mixing matrix. However, not only the CKM phase but also the baryon asymmetric Universe requires sources of CP violation. In this study, we show that a supersymmetric NB mechanism can naturally accommodate the Affleck-Dine (AD) baryogenesis within a CP-invariant Lagrangian. The model provides flat directions associated with new heavy quarks. Focusing on one of the directions, we find that the correct baryon asymmetry is obtained with a sufficiently low reheating temperature which does not cause the gravitino problem. Some parameter space is consistent with the gravitino dark matter. We assess radiative corrections to the strong CP phase induced by gauge-mediated supersymmetry breaking and CP-violating heavy fields and show that the strong CP problem is solved in a viable parameter space where the visible sector supersymmetric particles must be lighter than O(100) TeV. Even in the case that they are heavier than the TeV scale, our model predicts the neutron electric dipole moment within the reach of the near future experiments. Our model addresses the electroweak naturalness problem, strong CP problem, baryon asymmetric Universe, and dark matter. Then, the model may give a new compelling paradigm of physics beyond the Standard Model.
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