In this paper, we discuss the constraints on the reheating temperature supposing an early postreheating cosmological phase dominated by one or more simple scalar fields produced from inflaton decay and decoupled from matter and radiation. In addition, we explore the combined effects of the reheating and nonstandard scalar field phases on the inflationary number of e-foldings.

Di Marco, A., Pradisi, G., Cabella, P. (2018). Inflationary scale, reheating scale, and pre-BBN cosmology with scalar fields. PHYSICAL REVIEW D, 98(12) [10.1103/PhysRevD.98.123511].

Inflationary scale, reheating scale, and pre-BBN cosmology with scalar fields

Pradisi G.;Cabella P.
2018-12-13

Abstract

In this paper, we discuss the constraints on the reheating temperature supposing an early postreheating cosmological phase dominated by one or more simple scalar fields produced from inflaton decay and decoupled from matter and radiation. In addition, we explore the combined effects of the reheating and nonstandard scalar field phases on the inflationary number of e-foldings.
13-dic-2018
Pubblicato
Rilevanza internazionale
Articolo
Esperti anonimi
Settore FIS/02 - FISICA TEORICA, MODELLI E METODI MATEMATICI
English
Con Impact Factor ISI
https://journals.aps.org/prd/abstract/10.1103/PhysRevD.98.123511
Di Marco, A., Pradisi, G., Cabella, P. (2018). Inflationary scale, reheating scale, and pre-BBN cosmology with scalar fields. PHYSICAL REVIEW D, 98(12) [10.1103/PhysRevD.98.123511].
Di Marco, A; Pradisi, G; Cabella, P
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/2108/218896
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