Cosmological Signatures of Neutrino Seesaw Mechanism

TL;DR

This paper proposes a novel cosmological approach to detect neutrino seesaw signatures via inflaton decay modulated by Higgs fluctuations, potentially observable in large-scale structure surveys.

Contribution

It introduces a new method linking inflaton decay, Higgs modulation, and neutrino seesaw to produce measurable non-Gaussian signatures in the universe.

Findings

Large parameter space of neutrino seesaw can be probed by upcoming surveys.

Primordial non-Gaussianities provide signatures of the seesaw mechanism.

Higgs modulated reheating offers a new observational window.

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 Letter, we propose a new approach to study cosmological signatures of neutrino seesaw through the interaction between inflaton and right-handed neutrinos that 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 Higgs field that 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 find that these surveys have the potential to probe a large portion of the neutrino seesaw parameter space, opening up a new window for testing the high scale seesaw mechanism.