The creation of radiation and the relic of inflaton potential
Yu-Chung Chen

TL;DR
This paper proposes a new model where radiation is produced through inflaton interactions with an effective frictional force, leading to two universe expansion types and a relic inflaton potential acting as a cosmological constant.
Contribution
It introduces a novel perspective on inflaton-radiation interaction via effective friction, explaining universe expansion behaviors and the persistence of inflaton potential as a relic cosmological constant.
Findings
Type I universe reaches a uniform rolling phase with continuous particle creation.
Type II universe's inflaton becomes static, leaving a relic potential as a cosmological constant.
Inflaton potential can survive as a relic, influencing late-time cosmic acceleration.
Abstract
Recently, we have performed research on the subject of the cosmological constant problem. The scenario is based on two postulates for inflationary theory: one is that inflaton can interact with radiation (relativistic particles); the other is that radiation will be created continuously during and after the epoch of inflation. According to these postulates and from a "macroscopic perspective", we discover that radiation can be viewed as a product of the interaction between and some "effective kinetic frictional force" that exists in inflaton dynamics. Deducing and surmising from "effective friction", we obtain conclusions of two special types of expanding universe: A Type I universe will finally enter an expanding course after a special time with uniformly rolling due to the balance between , 3H(t)\dot{\phi}(t_{*}) and the…
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Taxonomy
TopicsCosmology and Gravitation Theories · Solar and Space Plasma Dynamics · Galaxies: Formation, Evolution, Phenomena
