Reheating, Multifield Inflation and the Fate of the Primordial Observables
Godfrey Leung, Ewan R. M. Tarrant, Christian T. Byrnes, Edmund J., Copeland

TL;DR
This paper investigates how the reheating process after two-field inflation influences primordial observables like non-Gaussianity and spectral index, highlighting the importance of reheating physics in interpreting cosmological data.
Contribution
It provides a numerical analysis of reheating effects on curvature perturbations and demonstrates the sensitivity of non-Gaussianity to reheating details in two-field inflation models.
Findings
f_NL can remain non-zero if initial non-Gaussianity exists.
f_NL is sensitive to reheating timescale, especially in certain potentials.
n_s remains relatively insensitive to decay rate variations.
Abstract
We study the effects of perturbative reheating on the evolution of the curvature perturbation \zeta, in two-field inflation models. We use numerical methods to explore the sensitivity of f_NL, n_s and r to the reheating process, and present simple qualitative arguments to explain our results. In general, if a large non-Gaussian signal exists at the start of reheating, it will remain non zero at the end of reheating. Unless all isocurvature modes have completely decayed before the start of reheating, we find that the non-linearity parameter, f_NL, can be sensitive to the reheating timescale, and that this dependence is most appreciable for `runaway' inflationary potentials that only have a minimum in one direction. For potentials with a minimum in both directions, f_NL can also be sensitive to reheating if a mild hierarchy exists between the decay rates of each field. Within the class of…
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.
