Cosmological signatures of neutrino seesaw mechanism
Year: 2025
Type: article
Abstract: The tiny neutrino masses are most naturally explained by seesaw mechanism through singlet right-handed neutrinos, which can further explain the matter-antimatter asymmetry in the Universe. In this work, we propose a new approach to study cosmological signatures of neutrino seesaw through the interaction between inflaton and right-handed neutrinos, which respects the shift symmetry. In our framework, after inflation the inflaton predominantly decays into right-handed neutrinos and its decay rate is modulated by the fluctuations of the Higgs field, which act as the source of curvature perturbations. This gives a new realization of Higgs modulated reheating, and it produces primordial non-Gaussian signatures that can be measured by the forthcoming large-scale structure surveys. We demonstrate, for the first time, that the measurements of non-Gaussianity by these surveys can probe the neutrino seesaw scale and have the potential to constrain a large portion of the seesaw parameter space, opening up a new window for directly testing the high-scale seesaw mechanism.
DOI: 10.1103/b7hv-3h2p
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: hybrid
Funders: National Natural Science Foundation of China, Sun Yat-sen University, Ministry of Education, India, Shanghai Jiao Tong University, Science, Technology and Innovation Commission of Shenzhen Municipality, National Key Research and Development Program of China, Fundamental Research Funds for the Central Universities
OpenAlex ID: W4415757207
