Classicality of primordial fluctuations and Primordial Black Holes

Details Classicality of primordial fluctuations and Primordial Black Holes Classicality of primordial fluctuations and Primordial Black Holes

2001-09-21

arxiv.org/abs/astro-ph/0109388v2

Int.J.Mod.Phys. D10 (2001) 927

Astronomy and Astrophysics

Astrophysics

uses LaTeX, 8 pages; one ref. added; to appear in Int. J. of Mod. Physics D

Scientific paper

10.1142/S021827180100161X

The production of Primordial Black Holes (PBH) from inflationary perturbations provides a physical process where the effective classicality of the fluctuations does not hold for certain scales. For adiabatic perturbations produced during inflation, this range of scales corresponds to PBH with masses $M\ll 10^{15}$ g. For PBH with masses $M\sim M_H(t_e)$, the horizon mass at the end of inflation, the generation process during the preheating stage could be classical as well, in contrast to the formation of PBH on these scales by adiabatic inflationary perturbations. For the non evaporated PBH, the generation process is essentially classical.

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