6533b837fe1ef96bd12a31cd

RESEARCH PRODUCT

The dark(er) side of inflation

Gabriela Barenboim

subject

High Energy Physics - PhenomenologyGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)FOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysics

description

We present a new approach to quintessential inflation, in which both dark energy and inflation are explained by the evolution of a single scalar field. We start from a simple scalar potential with both oscillatory and exponential behavior.We employ the conventional reheating mechanism of new inflation, in which the scalar decays to light fermions with a decay width that is proportional to the scalar mass. Because our scalar mass is proportional to the Hubble rate, this gives adequate reheating at early times while shutting off at late times to preserve quintessence and satisfy nucleosynthesis constraints.

https://dx.doi.org/10.48550/arxiv.hep-ph/0605111