Modular invariant inflation and reheating
Gui-Jun Ding, Si-Yi Jiang, Yong Xu, Wenbin Zhao
TL;DR
The paper presents a minimal framework where modular symmetry, specifically the finite group $\Gamma_3\cong A_4$, organizes both the lepton flavor sector and early-universe cosmology through a common modulus field that acts as the inflaton. Neutrino masses arise via Type-I seesaw with modular form–determined Yukawas, while inflation proceeds along a modular-invariant trajectory stabilized near fixed points, yielding a flat potential and predictions of $r=\mathcal{O}(10^{-7})$ and $\alpha=\mathcal{O}(-10^{-3})$, with $n_s$ in the Planck range. Reheating is generated from the same modular expansions that govern flavor, with inflaton decays dominantly to right-handed neutrinos; the resulting $T_{\text{rh}}$ can satisfy BBN bounds for sufficiently large $m_\phi$, but non-thermal leptogenesis is challenging in this small-field setup. The work demonstrates that modular symmetry can cohesively address flavor, inflation, and reheating, and points to large-field modular inflation as a promising direction to potentially connect these aspects to the observed BAU.
Abstract
We use modular symmetry as an organizing principle that attempts to simultaneously address the lepton flavor puzzle, inflation, and post-inflationary reheating. We demonstrate this approach using the finite modular group $A_4$ in the lepton sector. In our model, neutrino masses are generated via the Type-I see-saw mechanism, with modular symmetry dictating the form of the Yukawa couplings and right-handed neutrino masses. The modular field also drives inflation, providing an excellent fit to recent Cosmic Microwave Background (CMB) observations. The corresponding prediction for the tensor-to-scalar ratio is very small, $r \sim \mathcal{O}(10^{-7})$, while the prediction for the running of the spectral index, $α\sim -\mathcal{O}(10^{-3})$, could be tested in the near future. An appealing feature of the setup is that the inflaton-matter interactions required for reheating naturally arise from the expansion of relevant modular forms. Although the corresponding inflaton decay rates are suppressed by the Planck scale, the reheating temperature can still be high enough to ensure successful Big Bang nucleosynthesis. The same couplings responsible for reheating can also contribute to generating baryon asymmetry of the Universe through non-thermal leptogenesis. However, the contribution is negligibly small in the current inflationary setup.
