Introduction to the number of $e$-folds in slow-roll inflation

Fuente: arXiv
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Main Authors: Di Marco, Alessandro, Orazi, Emanuele, Pradisi, Gianfranco
Format: Preprint
Published: 2024
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author Di Marco, Alessandro
Orazi, Emanuele
Pradisi, Gianfranco
author_facet Di Marco, Alessandro
Orazi, Emanuele
Pradisi, Gianfranco
contents In this review, a pedagogical introduction to the concepts of slow-roll inflationary Universe and number of $e$-folds is provided. In particular, the differences between the basic notion of number of $e$-folds ($N_e$), total number of $e$-folds ($N_T$) and number of $e$-folds before the end of inflation ($N$), are outlined. The proper application of the number of $e$-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.
format Preprint
id arxiv_https___arxiv_org_abs_2408_01854
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Introduction to the number of $e$-folds in slow-roll inflation
Di Marco, Alessandro
Orazi, Emanuele
Pradisi, Gianfranco
Cosmology and Nongalactic Astrophysics
General Relativity and Quantum Cosmology
High Energy Physics - Theory
In this review, a pedagogical introduction to the concepts of slow-roll inflationary Universe and number of $e$-folds is provided. In particular, the differences between the basic notion of number of $e$-folds ($N_e$), total number of $e$-folds ($N_T$) and number of $e$-folds before the end of inflation ($N$), are outlined. The proper application of the number of $e$-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.
title Introduction to the number of $e$-folds in slow-roll inflation
topic Cosmology and Nongalactic Astrophysics
General Relativity and Quantum Cosmology
High Energy Physics - Theory
url https://arxiv.org/abs/2408.01854