Introduction to the number of $e$-folds in slow-roll inflation
Alessandro Di Marco, Emanuele Orazi, Gianfranco Pradisi

TL;DR
This paper provides a clear, pedagogical overview of the concept of the number of e-folds in slow-roll inflation, clarifying different definitions and their importance for inflationary predictions.
Contribution
It clarifies the distinctions between various notions of e-folds and discusses their proper application in inflationary cosmology.
Findings
Different definitions of e-folds are distinguished and explained.
Proper application of e-folds is crucial for accurate inflationary predictions.
The review emphasizes the role of e-folds as a time variable and a key parameter.
Abstract
In this review, a pedagogical introduction to the concepts of slow-roll inflationary Universe and number of -folds is provided. In particular, the differences between the basic notion of number of -folds (), total number of -folds () and number of -folds before the end of inflation (), are outlined. The proper application of the number of -folds before the end of inflation is discussed both as a time-like variable for the scalar field evolution and as a key parameter for computing inflationary predictions.
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