Unification of cosmological scalar fields
Abdel P\'erez-Lorenzana, Merced Montesinos, Tonatiuh Matos

TL;DR
This paper proposes a unified model where a single complex scalar field's real and imaginary parts drive early inflation and late acceleration of the universe, protected by an SO(1,1) symmetry, enabling successful potential construction.
Contribution
It introduces a novel unification of inflaton and phantom fields through a complex scalar with SO(1,1) symmetry, providing a new framework for cosmological scalar fields.
Findings
The model unifies early and late universe acceleration with a single complex scalar.
It demonstrates a matter-phantom duality transforming solutions.
The symmetry allows for successful potential construction.
Abstract
We present a model where early inflation and late accelerating expansion of the Universe are driven by the real and imaginary parts of a single complex scalar field, which we identified as inflaton and phantom field, respectively. This inflaton-phantom unification is protected by an internal SO(1,1) symmetry, with the two cosmological scalars appearing as the degrees of freedom of a sole fundamental representation. The unification symmetry allows to build successful potentials. We observe that our theory provides a matter-phantom duality, which transforms scalar matter cosmological solutions into phantom solutions and vice versa. We also suggest that a complete unification of all scalar fields of cosmological interest is yet possible under a similar footing.
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.
