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 ((Formula presented.)), total number of e-folds ((Formula presented.)) 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.

DI MARCO, A., Orazi, E., Pradisi, G. (2024). Introduction to the Number of e-Folds in Slow-Roll Inflation. UNIVERSE, 10(7) [10.3390/universe10070284].

Introduction to the Number of e-Folds in Slow-Roll Inflation

Alessandro Di Marco
Membro del Collaboration Group
;
Emanuele Orazi
Membro del Collaboration Group
;
Gianfranco Pradisi
2024-01-01

Abstract

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 ((Formula presented.)), total number of e-folds ((Formula presented.)) 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.
2024
Pubblicato
Rilevanza internazionale
Review
Esperti anonimi
Settore PHYS-02/A - Fisica teorica delle interazioni fondamentali, modelli, metodi matematici e applicazioni
English
Con Impact Factor ISI
cosmology
early universe cosmology
inflation
number of e-folds
https://www.mdpi.com/2218-1997/10/7/284
DI MARCO, A., Orazi, E., Pradisi, G. (2024). Introduction to the Number of e-Folds in Slow-Roll Inflation. UNIVERSE, 10(7) [10.3390/universe10070284].
DI MARCO, A; Orazi, E; Pradisi, G
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/2108/394714
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