A dynamical inflaton coupled to strongly interacting matter
Christian Ecker, Elias Kiritsis, Wilke van der Schee

TL;DR
This paper models the early universe's reheating process by coupling inflationary dynamics with a strongly interacting quantum field theory using holography, revealing a sequence from inflation to thermalized QFT domination.
Contribution
It introduces a self-consistent holographic framework coupling Einstein-inflaton equations with strongly coupled QFT to study cosmological reheating.
Findings
The coupled system produces an inflating universe transitioning to a reheating phase.
The universe eventually becomes dominated by a thermalized strongly interacting QFT.
The model demonstrates a realistic sequence of early universe evolution stages.
Abstract
According to the inflationary theory of cosmology, most elementary particles in the current universe were created during a period of reheating after inflation. In this work we self-consistently couple the Einstein-inflaton equations to a strongly coupled quantum field theory (QFT) as described by holography. We show that this leads to an inflating universe, a reheating phase and finally a universe dominated by the QFT in thermal equilibrium.
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Taxonomy
TopicsCosmology and Gravitation Theories · Black Holes and Theoretical Physics · Solar and Space Plasma Dynamics
