Connecting early and late universe by $f(R)$ gravity
Salvatore Capozziello, Mariafelicia De Laurentis, Orlando Luongo

TL;DR
This review explores how $f(R)$ gravity can unify descriptions of the early inflationary universe and the current dark energy-driven acceleration, highlighting its potential as a geometric framework for cosmology.
Contribution
It provides a concise overview of $f(R)$ gravity's role in modeling both early and late universe accelerated phases, emphasizing its fundamental physics motivations and main components.
Findings
$f(R)$ gravity can describe both inflation and dark energy.
The paper summarizes key aspects of $f(R)$ inflation and quintessence.
It outlines the main ingredients of $f(R)$ cosmography.
Abstract
Inflation and dark energy are two of the most relevant aspects of modern cosmology. These different epochs provide the universe is passing through accelerated phases soon after the Big-Bang and at present stage of its evolution. In this review paper, we discuss that both eras can be, in principle, described by a geometric picture, under the standard of gravity. We give the fundamental physics motivations and outline the main ingredients of inflation, quintessence and cosmography. This wants to be a quick summary of paradigm without claiming of completeness.
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