Bounds from primordial black holes with a near critical collapse initial mass function

Recent numerical evidence suggests that a mass spectrum of primordial black holes (PBHs) is produced as a consequence of near critical gravitational collapse. Assuming that these holes formed from the initial density perturbations seeded by inflation, we calculate model independent upper bounds on t...

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Veröffentlicht in:Physical Review, D D, 1999, Vol.60 (10), Article 103510
Hauptverfasser: Kribs, Graham D., Leibovich, Adam K., Rothstein, I. Z.
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Sprache:eng
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