Astronomy and Astrophysics – Astrophysics
Scientific paper
2005-10-21
JCAP 0601:011,2006
Astronomy and Astrophysics
Astrophysics
12 pages, 3 figures
Scientific paper
10.1088/1475-7516/2006/01/011
Previous authors have calculated the mass function of primordial black holes only on scales which are well outside the horizon at the end of inflation. Here we extend the calculation to sub-horizon scales, on which the density perturbation never becomes classical. Regarding the formation of black holes as a `measurement' of the (high peaks) of the density perturbation, we estimate a mass function by assuming that black holes form as soon as inflation ends, in those rare regions where the Bardeen potential exceeds a threshold value of $Psi_c\simeq 0.5$.
Lyth David H.
Malik Karim A.
Sasaki Misao
Zaballa Ignacio
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