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From inflation to late acceleration: A new cosmological paradigm

TLDR
In this article, a new idea of deriving a cosmological term from an underlying theory has been proposed in order to explain the expansion history of the universe and obtain the scale factor with this derived cosmology term and demonstrate that it reflects all the characteristics of the expanding universe in different era.
Abstract
A new idea of deriving a cosmological term from an underlying theory has been proposed in order to explain the expansion history of the universe. We obtain the scale factor with this derived cosmological term and demonstrate that it reflects all the characteristics of the expanding universe in different era so as to result in a transition from inflation to late acceleration through intermediate decelerating phases by this single entity. We further discuss certain observational aspects of this paradigm.

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Citations
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Journal ArticleDOI

Mutated hilltop inflation: a natural choice for early universe

TL;DR: In this article, a model of hilltop inflation with a suitable potential for a single scalar field which falls in the wide class of hill-top inflation is proposed. But, the model is not suitable for the case of infinite fields.
References
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Book

Cosmological Inflation and Large-Scale Structure

TL;DR: This textbook is the first to provide a modern and unified overview of inflationary cosmology and carefully compares predictions with the latest observations, including those of the cosmic microwave background, the clustering and velocities of galaxies and the epoch of structure formation.
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