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

Author:

Di Marco Alessandro12ORCID,Orazi Emanuele3ORCID,Pradisi Gianfranco24ORCID

Affiliation:

1. Istituto Nazionale di Astrofisica, Istituto di Astrofisica e Planetologia Spaziali (INAF-IAPS), Via Fosso del Cavaliere, 100, 00133 Rome, Italy

2. Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Roma Tor Vergata, Via Della Ricerca Scientifica 1, 00133 Roma, Italy

3. Escola de Ciência e and International Institute of Physics, Federal University of Rio Grande do Norte, Campus Universitario, Lagoa Nova 59078-970, RN, Brazil

4. Dipartimento di Fisica, Università di Roma Tor Vergata, Via Della Ricerca Scientifica 1, 00133 Roma, Italy

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 (Ne), total number of e-folds (NT) 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.

Publisher

MDPI AG

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