
TL;DR
This paper proposes a unified model where a single scalar field accounts for both inflation and Dark Matter, using existing parameters without additional fine tuning, and explains how the field transitions from inflation to Dark Matter.
Contribution
It introduces a minimal unification scheme that combines inflation and Dark Matter using one scalar field with no extra parameters beyond standard inflation models.
Findings
Dark Matter produced at low energies without fine tuning
The model links Dark Matter properties to inflation parameters
Four parameters suffice for unification, matching existing models
Abstract
We present a model where inflation and Dark Matter takes place via a single scalar field phi. Without introducing any new parameters we are able unify inflation and Dark Matter using a scalar field phi that accounts for inflation at an early epoch while it gives a Dark Matter WIMP particle at low energies. After inflation our universe must be reheated and we must have a long period of radiation dominated before the epoch of Dark Matter. Typically the inflaton decays while it oscillates around the minimum of its potential. If the inflaton decay is not complete or sufficient then the remaining energy density of the inflaton after reheating must be fine tuned to give the correct amount of Dark Matter. An essential feature here, is that Dark Matter-Inflaton particle is produced at low energies without fine tuning or new parameters. This process uses the same coupling g as for the inflaton…
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.
