Abstract
I present two inflationary universe models in which density fluctuations with a sharp peak on a specific scale are produced. When that scale reenters the Hubble radius in the subsequent radiation-dominated era, significant amount of primordial black holes can be produced that may be identified with massive compact halo objects with mass ∼ 0.5M⊙ observed through gravitational microlensing experiments.
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CITATION STYLE
APA
Yokoyama, J. (1999). Formation of primordial black holes in inflationary cosmology. Progress of Theoretical Physics Supplement, (136), 338–352. https://doi.org/10.1143/PTPS.136.338
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