Radiatively Corrected Hybrid Inflation: Parameter Scans and Machine Learning with ACT and Future CMB Experiments
Waqas Ahmed, Saleh O. Allehabi, Mansoor Ur Rehman

TL;DR
This paper studies a hybrid inflation model with right-handed neutrinos, showing quantum corrections align predictions with observations, and employs machine learning to efficiently explore the model's parameter space.
Contribution
It demonstrates how quantum corrections modify the inflation potential to match data and applies machine learning for parameter space analysis in cosmological models.
Findings
Quantum corrections flatten the potential, leading to a red-tilted spectral index.
Approximately 15% of the parameter space satisfies current experimental constraints.
Machine learning achieves high accuracy (87.5% to 98.9%) in predicting viable parameters.
Abstract
We investigate a realistic non-supersymmetric hybrid inflation model incorporating right-handed neutrinos and assess its viability in light of recent cosmological observations. At tree level, the inflaton potential yields a blue-tilted scalar spectrum, which is disfavored by current data from Planck and ACT that instead support a red tilt. We show that including one-loop quantum corrections, arising from generic couplings required for reheating, significantly modifies the potential, flattening it at large field values. This leads to a red-tilted spectral index () and a suppressed tensor-to-scalar ratio , both consistent with observational constraints. To ensure theoretical control, we focus on sub-Planckian field values, where the effective field theory description remains valid. The coupling of the inflaton to right-handed neutrinos naturally facilitates efficient reheating…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
